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39 results on '"MASS-DISTRIBUTION"'

1. z ~ 2-9 galaxies magnified by the Hubble Frontier Field clusters: I. Source selection and surface density-magnification constraints from >2500 galaxies

Author: R. J. Bouwens, G. Illingworth, R. S. Ellis, P. Oesch, A. Paulino-Afonso, B. Ribeiro, and M. Stefanon
Subjects: DECOMPOSITION, Astrophysics - astrophysics of galaxies, LOW-LUMINOSITY GALAXIES, UNIVERSE, FOS: Physical sciences, Astronomy and Astrophysics, Galaxy clusters, SIZES, FAINT GALAXIES, EVOLUTION, Lyman-break galaxies, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), Strong gravitational lensing, DARK-MATTER, STRONG LENSING DATA, RECONSTRUCTION, Dwarf galaxies, MASS-DISTRIBUTION
Abstract: We assemble a large comprehensive sample of 2534 z~2, 3, 4, 5, 6, 7, 8, and 9 galaxies lensed by the six clusters from the Hubble Frontier Fields (HFF) program. Making use of the availability of multiple independent magnification models for each of the HFF clusters and alternatively treating one of the models as the "truth," we show that the median magnification factors from the v4 parametric models are typically reliable to values of 30 to 50, and in one case to 100. Using the median magnification factor from the latest v4 models, we estimate the UV luminosities of the 2534 lensed z~2-9 galaxies, finding sources as faint as -12.4 mag at z~3 and -12.9 mag at z~7. We explicitly demonstrate the power of the surface density-magnification relations Sigma(z) vs. mu in the HFF clusters to constrain both distant galaxy properties and cluster lensing properties. Based on the Sigma(z) vs. mu relations, we show that the median magnification estimates from existing public models must be reliable predictors of the true magnification mu to mu, 22 pages, 13 figures, 6 tables, accepted for publication in the Astrophysical Journal, updated to be consistent with the proofs
Published: 2022

2. GWTC-2: compact binary coalescences observed by LIGO and Virgo during the first half of the third observing run

Author: Abbott R.a, Abbott T.D.b, Abraham S.c, Acernese F.d, e, Ackley K.f, Adams A.g, Adams C.h, Adhikari R.X.a, Adya V.B.i, Affeldt C.j, k, Agathos M.l, m, Agatsuma K.n, Aggarwal N.o, Aguiar O.D.p, Aiello L.q, r, Ain A.s, t, Ajith P.u, Akcay S.m, v, Allen G.w, Allocca A.s, Altin P.A.i, Amato A.x, Anand S.a, Ananyeva A.a, Anderson S.B.a, Anderson W.G.y, Angelova S.V.z, Ansoldi S.aa, Antelis J.M.ac, Antier S.ad, Appert S.a, Arai K.a, Araya M.C.a, Areeda J.S.ae, Arène M.ad, Arnaud N.af, Aronson S.M.ah, Arun K.G.ai, Asali Y.aj, Ascenzi S.q, Ashton G.f, Aston S.M.h, Astone P.al, Aubin F.am, Aufmuth P.j, Aultoneal K.ac, Austin C.b, Avendano V.an, Babak S.ad, Badaracco F.q, Bader M.K.M.ao, Bae S.ap, Baer A.M.g, Bagnasco S.aq, Baird J.ad, Ball M.ar, Ballardin G.ag, Ballmer S.W.as, Bals A.ac, Balsamo A.g, Baltus G.at, Banagiri S.au, Bankar D.c, Bankar R.S.c, Barayoga J.C.a, Barbieri C.av, Barish B.C.a, Barker D.ay, Barneo P.az, Barnum S.ba, Barone F.e, Barr B.bc, Barsotti L.ba, Barsuglia M.ad, Barta D.bd, Bartlett J.ay, Bartos I.ah, Bassiri R.be, Basti A.s, Bawaj M.bf, Bayley J.C.bc, Bazzan M.bh, Becher B.R.bj, Bécsy B.bk, Bedakihale V.M.bl, Bejger M.bm, Belahcene I.af, Beniwal D.bn, Benjamin M.G.ac, Bennett T.F.bo, Bentley J.D.n, Bergamin F.j, Berger B.K.be, Bergmann G.j, Bernuzzi S.m, Berry C.P.L.o, Bersanetti D.bp, Bertolini A.ao, Betzwieser J.h, Bhandare R.bq, Bhandari A.V.c, Bhattacharjee D.br, Bidler J.ae, Bilenko I.A.bs, Billingsley G.a, Birney R.bt, Birnholtz O.bu, Biscans S.a, Bischi M.bv, Biscoveanu S.ba, Bisht A.j, Bitossi M.s, Bizouard M.-A.bx, Blackburn J.K.a, Blackman J.by, Blair C.D.bz, Blair D.G.bz, Blair R.M.ay, Blanch O.ca, Bobba F.cb, Bode N.j, Boer M.bx, Boetzel Y.cd, Bogaert G.bx, Boldrini M.al, Bondu F.cf, Bonilla E.be, Bonnand R.am, Booker P.j, Boom B.A.ao, Bork R.a, Boschi V.s, Bose S.c, Bossilkov V.bz, Boudart V.at, Bouffanais Y.bh, Bozzi A.ag, Bradaschia C.s, Brady P.R.y, Bramley A.h, Branchesi M.q, Brau J.E.ar, Breschi M.m, Briant T.cg, Briggs J.H.bc, Brighenti F.bv, Brillet A.bx, Brinkmann M.j, Brockill P.y, Brooks A.F.a, Brooks J.ag, Brown D.D.bn, Brunett S.a, Bruno G.ch, Bruntz R.g, Buikema A.ba, Bulik T.ci, Bulten H.J.ao, Buonanno A.ck, Buscicchio R.n, Buskulic D.am, Byer R.L.be, Cabero M.j, Cadonati L.cm, Caesar M.cn, Cagnoli G.x, Cahillane C.a, Calderón Bustillo J.f, Callaghan J.D.bc, Callister T.A.co, Calloni E.e, Camp J.B.cq, Canepa M.bp, Cannon K.C.cs, Cao H.bn, Cao J.ct, Carapella G.cb, Carbognani F.ag, Carney M.F.o, Carpinelli M.cu, Carullo G.s, Carver T.L.cw, Casanueva Diaz J.ag, Casentini C.ak, Caudill S.ao, Cavaglià M.br, Cavalier F.af, Cavalieri R.ag, Cella G.s, Cerdá-Durán P.cy, Cesarini E.ak, Chaibi W.bx, Chakravarti K.c, Chan C.-L.cz, Chan C.cs, Chandra K.da, Chanial P.ag, Chao S.db, Charlton P.dc, Chase E.A.o, Chassande-Mottin E.ad, Chatterjee D.y, Chattopadhyay D.dd, Chaturvedi M.bq, Chatziioannou K.co, Chen A.cz, Chen H.Y.de, Chen X.bz, Chen Y.by, Cheng H.-P.ah, Cheong C.K.cz, Chia H.Y.ah, Chiadini F.cc, Chierici R.dg, Chincarini A.bp, Chiummo A.ag, Cho G.dh, Cho H.S.di, Cho M.cl, Choate S.cn, Christensen N.bx, Chu Q.bz, Chua S.cg, Chung K.W.dj, Chung S.bz, Ciani G.bh, Ciecielag P.bm, Cie?lar M.bm, Cifaldi M.ak, Ciobanu A.A.bn, Ciolfi R.bi, Cipriano F.bx, Cirone A.bp, Clara F.ay, Clark E.N.dl, Clark J.A.cm, Clarke L.dm, Clearwater P.dn, Clesse S.ch, Cleva F.bx, Coccia E.q, Cohadon P.-F.cg, Cohen D.E.af, Colleoni M.do, Collette C.G.dp, Collins C.n, Colpi M.av, Constancio M., Jr.p, Conti L.bi, Cooper S.J.n, Corban P.h, Corbitt T.R.b, Cordero-Carrión I.dq, Corezzi S.bf, Corley K.R.aj, Cornish N.bk, Corre D.af, Corsi A.dr, Cortese S.ag, Costa C.A.p, Cotesta R.ck, Coughlin M.W.a, Coughlin S.B.o, Coulon J.-P.bx, Countryman S.T.aj, Cousins B.ds, Couvares P.a, Covas P.B.do, Coward D.M.bz, Cowart M.J.h, Coyne D.C.a, Coyne R.dt, Creighton J.D.E.y, Creighton T.D.du, Croquette M.cg, Crowder S.G.dv, Cudell J.R.at, Cullen T.J.b, Cumming A.bc, Cummings R.bc, Cunningham L.bc, Cuoco E.ag, Cury?o M.ci, Canton T.D.af, Dálya G.dx, Dana A.be, Daneshgaranbajastani L.M.bo, D'Angelo B.bp, Danila B.dy, Danilishin S.L.dz, D'Antonio S.ak, Danzmann K.j, Darsow-Fromm C.ea, Dasgupta A.bl, Datrier L.E.H.bc, Dattilo V.ag, Dave I.bq, Davier M.af, Davies G.S.eb, Davis D.a, Daw E.J.ec, Dean R.cn, Debra D.be, Deenadayalan M.c, Degallaix J.ed, De Laurentis M.e, Deléglise S.cg, Del Favero V.ee, De Lillo F.ch, De Lillo N.bc, Del Pozzo W.s, Demarchi L.M.o, De Matteis F.ak, D'Emilio V.cw, Demos N.ba, Denker T.j, Dent T.eb, Depasse A.ch, De Pietri R.ef, De Rosa R.e, De Rossi C.ag, Desalvo R.cc, De Varona O.j, Dhurandhar S.c, Díaz M.C.du, Diaz-Ortiz M., Jr.ah, Didio N.A.as, Dietrich T.ao, Di Fiore L.e, Difronzo C.n, Di Giorgio C.cb, Di Giovanni F.cy, Di Giovanni M.ei, Di Girolamo T.e, Di Lieto A.s, Ding B.dp, Di Pace S.al, Di Palma I.al, Di Renzo F.s, Divakarla A.K.ah, Dmitriev A.n, Doctor Z.ar, D'Onofrio L.e, Donovan F.ba, Dooley K.L.cw, Doravari S.c, Dorrington I.cw, Downes T.P.y, Drago M.q, Driggers J.C.ay, Du Z.ct, Ducoin J.-G.af, Dupej P.bc, Durante O.cb, D'Urso D.cu, Duverne P.-A.af, Dwyer S.E.ay, Easter P.J.f, Eddolls G.bc, Edelman B.ar, Edo T.B.ec, Edy O.ek, Effler A.h, Eichholz J.i, Eikenberry S.S.ah, Eisenmann M.am, Eisenstein R.A.ba, Ejlli A.cw, Errico L.e, Essick R.C.de, Estellés H.do, Estevez D.am, Etienne Z.B.el, Etzel T.a, Evans M.ba, Evans T.M.h, Ewing B.E.ds, Fafone V.q, Fair H.as, Fairhurst S.cw, Fan X.ct, Farah A.M.de, Farinon S.bp, Farr B.ar, Farr W.M.co, Fauchon-Jones E.J.cw, Favata M.an, Fays M.at, Fazio M.en, Feicht J.a, Fejer M.M.be, Feng F.ad, Fenyvesi E.bd, Ferguson D.L.cm, Fernandez-Galiana A.ba, Ferrante I.s, Ferreira T.A.p, Fidecaro F.s, Figura P.ci, Fiori I.ag, Fiorucci D.q, Fishbach M.de, Fisher R.P.g, Fishner J.M.ba, Fittipaldi R.cc, Fitz-Axen M.au, Fiumara V.cc, Flaminio R.am, Floden E.au, Flynn E.ae, Fong H.cs, Font J.A.cy, Forsyth P.W.F.i, Fournier J.-D.bx, Frasca S.al, Frasconi F.s, Frei Z.dx, Freise A.n, Frey R.ar, Frey V.af, Fritschel P.ba, Frolov V.V.h, Fronzé G.G.aq, Fulda P.ah, Fyffe M.h, Gabbard H.A.bc, Gadre B.U.ck, Gaebel S.M.n, Gair J.R.ck, Gais J.cz, Galaudage S.f, Gamba R.m, Ganapathy D.ba, Ganguly A.u, Gaonkar S.G.c, Garaventa B.bp, García-Quirós C.do, Garufi F.e, Gateley B.ay, Gaudio S.ac, Gayathri V.ah, Gemme G.bp, Gennai A.s, George D.w, George J.bq, George R.N.et, Gergely L.dy, Ghonge S.cm, Ghosh A.ck, Ghosh A.ao, Ghosh S.y, Giacomazzo B.av, Giacoppo L.al, Giaime J.A.b, h, Giardina K.D.h, Gibson D.R.bt, Gier C.z, Gill K.aj, Giri P.s, Glanzer J.b, Gleckl A.E.ae, Godwin P.ds, Goetz E.ex, Goetz R.ah, Gohlke N.j, Goncharov B.f, González G.b, Gopakumar A.ey, Gossan S.E.a, Gosselin M.s, Gouaty R.am, Grace B.i, Grado A.e, Granata M.ed, Granata V.cb, Grant A.bc, Gras S.ba, Grassia P.a, Gray C.ay, Gray R.bc, Greco G.bv, Green A.C.ah, Green R.cw, Gretarsson E.M.ac, Griggs H.L.cm, Grignani G.bf, Grimaldi A.ei, Grimes E.ac, Grimm S.J.q, Grote H.cw, Grunewald S.ck, Gruning P.af, Guerrero J.G.ae, Guidi G.M.bv, Guimaraes A.R.b, Guixé G.az, Gulati H.K.bl, Guo Y.ao, Gupta A.a, Gupta A.ds, Gupta P.ao, Gustafson E.K.a, Gustafson R.fb, Guzman F.dl, Haegel L.ad, Halim O.q, Hall E.D.ba, Hamilton E.Z.cw, Hammond G.bc, Haney M.cd, Hanke M.M.j, Hanks J.ay, Hanna C.ds, Hannam M.D.cw, Hannuksela O.A.cz, Hannuksela O.ao, Hansen H.ay, Hansen T.J.ac, Hanson J.h, Harder T.bx, Hardwick T.b, Haris K.u, Harms J.q, Harry G.M.fc, Harry I.W.ek, Hartwig D.ea, Hasskew R.K.h, Haster C.-J.ba, Haughian K.bc, Hayes F.J.bc, Healy J.ee, Heidmann A.cg, Heintze M.C.h, Heinze J.j, Heinzel J.fd, Heitmann H.bx, Hellman F.fe, Hello P.af, Helmling-Cornell A.F.ar, Hemming G.ag, Hendry M.bc, Heng I.S.bc, Hennes E.ao, Hennig J.j, Hennig M.H.j, Hernandez Vivanco F.f, Heurs M.j, Hild S.dz, Hill P.z, Hines A.S.dl, Hochheim S.j, Hofgard E.be, Hofman D.ed, Hohmann J.N.ea, Holgado A.M.w, Holland N.A.i, Hollows I.J.ec, Holmes Z.J.bn, Holt K.h, Holz D.E.de, Hopkins P.cw, Horst C.y, Hough J.bc, Howell E.J.bz, Hoy C.G.cw, Hoyland D.n, Huang Y.ba, Hübner M.T.f, Huddart A.D.dm, Huerta E.A.w, Hughey B.ac, Hui V.am, Husa S.do, Huttner S.H.bc, Hutzler B.M.b, Huxford R.ds, Huynh-Dinh T.h, Idzkowski B.ci, Iess A.ak, Imperato S.o, Inchauspe H.ah, Ingram C.bn, Intini G.al, Isi M.ba, Iyer B.R.u, Jaberianhamedan V.bz, Jacqmin T.cg, Jadhav S.J.ff, Jadhav S.P.c, James A.L.cw, Jani K.cm, Janssens K.fg, Janthalur N.N.ff, Jaranowski P.fh, Jariwala D.ah, Jaume R.do, Jenkins A.C.dj, Jeunon M.au, Jiang J.ah, Johns G.R.g, Johnson-Mcdaniel N.K.l, Jones A.W.n, Jones D.I.fi, Jones J.D.ay, Jones P.n, Jones R.bc, Jonker R.J.G.ao, Ju L.bz, Junker J.j, Kalaghatgi C.V.cw, Kalogera V.o, Kamai B.a, Kandhasamy S.c, Kang G.ap, Kanner J.B.a, Kapadia S.J.u, Kapasi D.P.i, Karathanasis C.ca, Karki S.br, Kashyap R.ds, Kasprzack M.a, Kastaun W.j, Katsanevas S.ag, Katsavounidis E.ba, Katzman W.h, Kawabe K.ay, Kéfélian F.bx, Keitel D.do, Key J.S.fj, Khadka S.be, Khalili F.Y.bs, Khan I.q, Khan S.cw, Khazanov E.A.fk, Khetan N.q, Khursheed M.bq, Kijbunchoo N.i, Kim C.fl, Kim G.J.cm, Kim J.C.fm, Kim K.fn, Kim W.S.fo, Kim Y.-M.fp, Kimball C.o, King P.J.ay, Kinley-Hanlon M.bc, Kirchhoff R.j, Kissel J.S.ay, Kleybolte L.ea, Klimenko S.ah, Knowles T.D.el, Knyazev E.ba, Koch P.j, Koehlenbeck S.M.j, Koekoek G.ao, Koley S.ao, Kolstein M.ca, Komori K.ba, Kondrashov V.a, Kontos A.bj, Koper N.j, Korobko M.ea, Korth W.Z.a, Kovalam M.bz, Kozak D.B.a, Krämer C.j, Kringel V.j, Krishnendu N.V.j, Królak A.fr, Kuehn G.j, Kumar A.ff, Kumar P.ft, Kumar R.ay, Kumar R.bl, Kuns K.ba, Kwang S.y, Lackey B.D.ck, Laghi D.s, Lalande E.fu, Lam T.L.cz, Lamberts A.bx, Landry M.ay, Lane B.B.ba, Lang R.N.ba, Lange J.ee, Lantz B.be, Lanza R.K.ba, La Rosa I.am, Lartaux-Vollard A.af, Lasky P.D.f, Laxen M.h, Lazzarini A.a, Lazzaro C.bh, Leaci P.al, Leavey S.j, Lecoeuche Y.K.ay, Lee H.M.fn, Lee H.W.fm, Lee J.dh, Lee K.be, Lehmann J.j, Leon E.ae, Leroy N.af, Letendre N.am, Levin Y.f, Li A.a, Li J.ct, Li K.J.L.cz, Li T.G.F.cz, Li X.by, Linde F.ao, Linker S.D.bo, Linley J.N.bc, Littenberg T.B.fx, Liu J.j, Liu X.y, Llorens-Monteagudo M.cy, Lo R.K.L.a, Lockwood A.fy, London L.T.ba, Longo A.fz, Lorenzini M.ak, Loriette V.gb, Lormand M.h, Losurdo G.s, Lough J.D.j, Lousto C.O.ee, Lovelace G.ae, Lück H.j, Lumaca D.ak, Lundgren A.P.ek, Ma Y.by, Macas R.cw, Macinnis M.ba, Macleod D.M.cw, Macmillan I.A.O.a, Macquet A.bx, Magaña Hernandez I.y, Magaña-Sandoval F.ah, Magazzù C.s, Magee R.M.ds, Majorana E.al, Maksimovic I.gb, Maliakal S.a, Malik A.bq, Man N.bx, Mandic V.au, Mangano V.al, Mansell G.L.ay, Manske M.y, Mantovani M.ag, Mapelli M.bh, Marchesoni F.bf, Marion F.am, Márka S.aj, Márka Z.aj, Markakis C.l, Markosyan A.S.be, Markowitz A.a, Maros E.a, Marquina A.dq, Marsat S.ad, Martelli F.bv, Martin I.W.bc, Martin R.M.an, Martinez M.ca, Martinez V.x, Martynov D.V.n, Masalehdan H.ea, Mason K.ba, Massera E.ec, Masserot A.am, Massinger T.J.ba, Masso-Reid M.bc, Mastrogiovanni S.ad, Matas A.ck, Mateu-Lucena M.do, Matichard F.a, Matiushechkina M.j, Mavalvala N.ba, Maynard E.b, McCann J.J.bz, McCarthy R.ay, McClelland D.E.i, McCormick S.h, McCuller L.ba, McGuire S.C.gd, McIsaac C.ek, McIver J.ex, McManus D.J.i, McRae T.i, McWilliams S.T.el, Meacher D.y, Meadors G.D.f, Mehmet M.j, Mehta A.K.ck, Melatos A.dn, Melchor D.A.ae, Mendell G.ay, Menendez-Vazquez A.ca, Mercer R.A.y, Mereni L.ed, Merfeld K.ar, Merilh E.L.ay, Merritt J.D.ar, Merzougui M.bx, Meshkov S.a, Messenger C.bc, Messick C.et, Metzdorff R.cg, Meyers P.M.dn, Meylahn F.j, Mhaske A.c, Miani A.ei, Miao H.n, Michaloliakos I.ah, Michel C.ed, Middleton H.dn, Milano L.e, Miller A.L.ah, Millhouse M.dn, Mills J.C.cw, Milotti E.ab, Milovich-Goff M.C.bo, Minazzoli O.bx, Minenkov Y.ak, Mir L.M.ca, Mishkin A.ah, Mishra C.gg, Mistry T.ec, Mitra S.c, Mitrofanov V.P.bs, Mitselmakher G.ah, Mittleman R.ba, Mo G.ba, Mogushi K.br, Mohapatra S.R.P.ba, Mohite S.R.y, Molina I.ae, Molina-Ruiz M.fe, Mondin M.bo, Montani M.bv, Moore C.J.n, Moraru D.ay, Morawski F.bm, Moreno G.ay, Morisaki S.cs, Mours B.gh, Mow-Lowry C.M.n, Mozzon S.ek, Muciaccia F.al, Mukherjee A.bc, Mukherjee D.ds, Mukherjee S.du, Mukherjee S.bl, Mukund N.j, Mullavey A.h, Munch J.bn, Muñiz E.A.as, Murray P.G.bc, Nadji S.L.j, Nagar A.aq, Nardecchia I.ak, Naticchioni L.al, Nayak R.K.gk, Neil B.F.bz, Neilson J.cc, Nelemans G.gl, Nelson T.J.N.h, Nery M.j, Neunzert A.fj, Nitz A.H.j, Ng K.Y.ba, Ng S.bn, Nguyen C.ad, Nguyen P.ar, Nguyen T.ba, Nichols S.A.b, Nissanke S.ao, Nocera F.ag, Noh M.ex, North C.cw, Nothard D.gm, Nuttall L.K.ek, Oberling J.ay, O'Brien B.D.ah, O'Dell J.dm, Oganesyan G.q, Ogin G.H.gn, Oh J.J.fo, Oh S.H.fo, Ohme F.j, Ohta H.cs, Okada M.A.p, Olivetto C.ag, Oppermann P.j, Oram R.J.h, O'Reilly B.h, Ormiston R.G.au, Ortega L.F.ah, O'Shaughnessy R.ee, Ossokine S.ck, Osthelder C.a, Ottaway D.J.bn, Overmier H.h, Owen B.J.dr, Pace A.E.ds, Pagano G.s, Page M.A.bz, Pagliaroli G.q, Pai A.da, Pai S.A.bq, Palamos J.R.ar, Palashov O.fk, Palomba C.al, Pan H.db, Panda P.K.ff, Pang T.H.ao, Pankow C.o, Pannarale F.al, Pant B.C.bq, Paoletti F.s, Paoli A.ag, Paolone A.al, Parker W.h, Pascucci D.ao, Pasqualetti A.ag, Passaquieti R.s, Passuello D.s, Patel M.g, Patricelli B.s, Payne E.f, Pechsiri T.C.ah, Pedraza M.a, Pegoraro M.bi, Pele A.h, Penn S.gp, Perego A.ei, Perez C.J.ay, Périgois C.am, Perreca A.ei, Perriès S.dg, Petermann J.ea, Petterson D.a, Pfeiffer H.P.ck, Pham K.A.au, Phukon K.S.c, Piccinni O.J.al, Pichot M.bx, Piendibene M.s, Piergiovanni F.bv, Pierini L.al, Pierro V.cc, Pillant G.ag, Pilo F.s, Pinard L.ed, Pinto I.M.cc, Piotrzkowski K.ch, Pirello M.ay, Pitkin M.gq, Placidi E.ce, Plastino W.fz, Pluchar C.dl, Poggiani R.s, Polini E.am, Pong D.Y.T.cz, Ponrathnam S.c, Popolizio P.ag, Porter E.K.ad, Poverman A.bj, Powell J.dd, Pracchia M.am, Prajapati A.K.bl, Prasai K.be, Prasanna R.ff, Pratten G.n, Prestegard T.y, Principe M.cc, Prodi G.A.ej, Prokhorov L.n, Prosposito P.ak, Prudenzi L.ck, Puecher A.ao, Punturo M.bf, Puosi F.s, Puppo P.al, Pürrer M.ck, Qi H.cw, Quetschke V.du, Quinonez P.J.ac, Quitzow-James R.br, Raab F.J.ay, Raaijmakers G.ao, Radkins H.ay, Radulesco N.bx, Raffai P.dx, Rafferty H.gs, Rail S.X.fu, Raja S.bq, Rajan C.bq, Rajbhandari B.dr, Rakhmanov M.du, Ramirez K.E.du, Ramirez T.D.ae, Ramos-Buades A.do, Rana J.ds, Rao K.o, Rapagnani P.al, Rapol U.D.gt, Ratto B.ac, Raymond V.cw, Razzano M.s, Read J.ae, Regimbau T.am, Rei L.bp, Reid S.z, Reitze D.H.a, Rettegno P.aq, Ricci F.al, Richardson C.J.ac, Richardson J.W.a, Richardson L.dl, Ricker P.M.w, Riemenschneider G.aq, Riles K.fb, Rizzo M.o, Robertson N.A.a, Robinet F.af, Rocchi A.ak, Rocha J.A.ae, Rodriguez S.ae, Rodriguez-Soto R.D.ac, Rolland L.am, Rollins J.G.a, Roma V.J.ar, Romanelli M.cf, Romano R.d, Romel C.L.ay, Romero A.ca, Romero-Shaw I.M.f, Romie J.H.h, Ronchini S.q, Rose C.A.y, Rose D.ae, Rose K.gm, Rosell M.J.B.et, Rosi?ska D.ci, Rosofsky S.G.w, Ross M.P.fy, Rowan S.bc, Rowlinson S.J.n, Roy S.c, Roy S.gv, Ruggi P.ag, Ryan K.ay, Sachdev S.ds, Sadecki T.ay, Sadiq J.ee, Sakellariadou M.dj, Salafia O.S.av, Salconi L.ag, Saleem M.ai, Samajdar A.ao, Sanchez E.J.a, Sanchez J.H.ae, Sanchez L.E.a, Sanchis-Gual N.gw, Sanders J.R.gx, Sandles L.cw, Santiago K.A.an, Santos E.bx, Saravanan T.R.c, Sarin N.f, Sassolas B.ed, Sathyaprakash B.S.cw, Sauter O.am, Savage R.L.ay, Savant V.c, Sawant D.da, Sayah S.ed, Schaetzl D.a, Schale P.ar, Scheel M.by, Scheuer J.o, Schindler-Tyka A.ah, Schmidt P.n, Schnabel R.ea, Schofield R.M.S.ar, Schönbeck A.ea, Schreiber E.j, Schulte B.W.j, Schutz B.F.j, Schwarm O.gn, Schwartz E.cw, Scott J.bc, Scott S.M.i, Seglar-Arroyo M.am, Seidel E.w, Sellers D.h, Sengupta A.S.gv, Sennett N.ck, Sentenac D.ag, Sequino V.e, Sergeev A.fk, Setyawati Y.j, Shaffer T.ay, Shahriar M.S.o, Sharifi S.b, Sharma A.q, Sharma P.bq, Shawhan P.cl, Shen H.w, Shikauchi M.cs, Shink R.fu, Shoemaker D.H.ba, Shoemaker D.M.cm, Shukla K.fe, Shyamsundar S.bq, Sieniawska M.bm, Sigg D.ay, Singer L.P.cq, Singh D.ds, Singh N.ci, Singha A.dz, Singhal A.q, Sintes A.M.do, Sipala V.cu, Skliris V.cw, Slagmolen B.J.J.i, Slaven-Blair T.J.bz, Smetana J.n, Smith J.R.ae, Smith R.J.E.f, Somala S.N.gy, Son E.J.fo, Soni K.c, Soni S.b, Sorazu B.bc, Sordini V.dg, Sorrentino F.bp, Sorrentino N.s, Soulard R.bx, Souradeep T.c, Sowell E.dr, Spencer A.P.bc, Spera M.o, Srivastava A.K.bl, Srivastava V.as, Staats K.o, Stachie C.bx, Steer D.A.ad, Steinhoff J.ck, Steinke M.j, Steinlechner J.bc, Steinlechner S.dz, Steinmeyer D.j, Stevenson S.P.dd, Stolle-Mcallister G.gm, Stops D.J.n, Stover M.gm, Strain K.A.bc, Stratta G.bw, Strunk A.ay, Sturani R.ha, Stuver A.L.cn, Südbeck J.ea, Sudhagar S.c, Sudhir V.ba, Suh H.G.y, Summerscales T.Z.hb, Sun H.bz, Sun L.a, Sunil S.bl, Sur A.bm, Suresh J.cs, Sutton P.J.cw, Swinkels B.L.ao, Szczepa?czyk M.J.ah, Tacca M.ao, Tait S.C.bc, Talbot C.f, Tanasijczuk A.J.ch, Tanner D.B.ah, Tao D.a, Tapia A.ae, Tapia San Martin E.N.ao, Tasson J.D.fd, Taylor R.a, Tenorio R.do, Terkowski L.ea, Thirugnanasambandam M.P.c, Thomas L.M.n, Thomas M.h, Thomas P.ay, Thompson J.E.cw, Thondapu S.R.bq, Thorne K.A.h, Thrane E.f, Tiwari S.cd, Tiwari S.ey, Tiwari V.cw, Toland K.bc, Tolley A.E.ek, Tonelli M.s, Tornasi Z.bc, Torres-Forné A.ck, Torrie C.I.a, E Melo I.T.cu, Töyrä D.i, Tran A.T.dv, Trapananti A.bf, Travasso F.bf, Traylor G.h, Tringali M.C.ci, Tripathee A.fb, Trovato A.ad, Trudeau R.J.a, Tsai D.S.db, Tsang K.W.ao, Tse M.ba, Tso R.by, Tsukada L.cs, Tsuna D.cs, Tsutsui T.cs, Turconi M.bx, Ubhi A.S.n, Udall R.P.cm, Ueno K.cs, Ugolini D.gs, Unnikrishnan C.S.ey, Urban A.L.b, Usman S.A.de, Utina A.C.dz, Vahlbruch H.j, Vajente G.a, Vajpeyi A.f, Valdes G.b, Valentini M.ei, Valsan V.y, Van Bakel N.ao, Van Beuzekom M.ao, Van Den Brand J.F.J.ao, Van Den Broeck C.ao, Vander-Hyde D.C.as, Van Der Schaaf L.ao, Van Heijningen J.V.bz, Vardaro M.ao, Vargas A.F.dn, Varma V.by, Vass S.a, Vasúth M.bd, Vecchio A.n, Vedovato G.bi, Veitch J.bc, Veitch P.J.bn, Venkateswara K.fy, Venneberg J.j, Venugopalan G.a, Verkindt D.am, Verma Y.bq, Veske D.aj, Vetrano F.bv, Viceré A.bv, Viets A.D.hd, Vijaykumar A.u, Villa-Ortega V.eb, Vinet J.-Y.bx, Vitale S.ba, Vo T.as, Vocca H.bf, Vorvick C.ay, Vyatchanin S.P.bs, Wade A.R.i, Wade L.E.gm, Wade M.gm, Walet R.C.ao, Walker M.g, Wallace G.S.z, Wallace L.a, Walsh S.y, Wang J.Z.fb, Wang S.w, Wang W.H.du, Wang Y.F.cz, Ward R.L.i, Warner J.ay, Was M.am, Washington N.Y.a, Watchi J.dp, Weaver B.ay, Wei L.j, Weinert M.j, Weinstein A.J.a, Weiss R.ba, Wellmann F.j, Wen L.bz, Weßels P.j, Westhouse J.W.ac, Wette K.i, Whelan J.T.ee, White D.D.ae, White L.V.as, Whiting B.F.ah, Whittle C.ba, Wilken D.M.j, Williams D.bc, Williams M.J.bc, Williamson A.R.ek, Willis J.L.a, Willke B.j, Wilson D.J.dl, Wimmer M.H.j, Winkler W.j, Wipf C.C.a, Woan G.bc, Woehler J.j, Wofford J.K.ee, Wong I.C.F.cz, Wrangel J.j, Wright J.L.bc, Wu D.S.j, Wysocki D.M.ee, Xiao L.a, Yamamoto H.a, Yang L.en, Yang Y.ah, Yang Z.au, Yap M.J.i, Yeeles D.W.cw, Yoon A.g, Yu H.by, Yu H.ba, Yuen S.H.R.cz, Zadro?ny A.fs, Zanolin M.ac, Zelenova T.ag, Zendri J.-P.bi, Zevin M.o, Zhang J.bz, Zhang L.a, Zhang R.ah, Zhang T.n, Zhao C.bz, Zhao G.dp, Zheng Y.br, Zhou M.o, Zhou Z.o, Zhu X.J.f, Zimmerman A.B.et, Zlochower Y.ee, Zucker M.E.a, Zweizig J.a, Astrophysique Relativiste Théories Expériences Métrologie Instrumentation Signaux (ARTEMIS), Université Nice Sophia Antipolis (... - 2019) (UNS), COMUE Université Côte d'Azur (2015 - 2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015 - 2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015 - 2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Abbott, R., Abbott, T. 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L., Doravari, S., Dorrington, I., Downes, T. P., Drago, M., Driggers, J. C., Du, Z., Ducoin, J. -G., Dupej, P., Durante, O., D’Urso, D., Duverne, P. -A., Dwyer, S. E., Easter, P. J., Eddolls, G., Edelman, B., Edo, T. B., Edy, O., Effler, A., Eichholz, J., Eikenberry, S. S., Eisenmann, M., Eisenstein, R. A., Ejlli, A., Errico, L., Essick, R. C., Estellés, H., Estevez, D., Etienne, Z. B., Etzel, T., Evans, M., Evans, T. M., Ewing, B. E., Fafone, V., Fair, H., Fairhurst, S., Fan, X., Farah, A. M., Farinon, S., Farr, B., Farr, W. M., Fauchon-Jones, E. J., Favata, M., Fays, M., Fazio, M., Feicht, J., Fejer, M. M., Feng, F., Fenyvesi, E., Ferguson, D. L., Fernandez-Galiana, A., Ferrante, I., Ferreira, T. A., Fidecaro, F., Figura, P., Fiori, I., Fiorucci, D., Fishbach, M., Fisher, R. P., Fishner, J. M., Fittipaldi, R., Fitz-Axen, M., Fiumara, V., Flaminio, R., Floden, E., Flynn, E., Fong, H., Font, J. A., Forsyth, P. W. 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J., Grote, H., Grunewald, S., Gruning, P., Guerrero, J. G., Guidi, G. M., Guimaraes, A. R., Guixé, G., Gulati, H. K., Guo, Y., Gupta, Anchal, Gupta, Anuradha, Gupta, P., Gustafson, E. K., Gustafson, R., Guzman, F., Haegel, L., Halim, O., Hall, E. D., Hamilton, E. Z., Hammond, G., Haney, M., Hanke, M. M., Hanks, J., Hanna, C., Hannam, M. D., Hannuksela, O. A., Hannuksela, O., Hansen, H., Hansen, T. J., Hanson, J., Harder, T., Hardwick, T., Haris, K., Harms, J., Harry, G. M., Harry, I. W., Hartwig, D., Hasskew, R. K., Haster, C. -J., Haughian, K., Hayes, F. J., Healy, J., Heidmann, A., Heintze, M. C., Heinze, J., Heinzel, J., Heitmann, H., Hellman, F., Hello, P., Helmling-Cornell, A. F., Hemming, G., Hendry, M., Heng, I. S., Hennes, E., Hennig, J., Hennig, M. H., Hernandez Vivanco, F., Heurs, M., Hild, S., Hill, P., Hines, A. S., Hochheim, S., Hofgard, E., Hofman, D., Hohmann, J. N., Holgado, A. M., Holland, N. A., Hollows, I. J., Holmes, Z. J., Holt, K., Holz, D. 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Y., Khan, I., Khan, S., Khazanov, E. A., Khetan, N., Khursheed, M., Kijbunchoo, N., Kim, C., Kim, G. J., Kim, J. C., Kim, K., Kim, W. S., Kim, Y. -M., Kimball, C., King, P. J., Kinley-Hanlon, M., Kirchhoff, R., Kissel, J. S., Kleybolte, L., Klimenko, S., Knowles, T. D., Knyazev, E., Koch, P., Koehlenbeck, S. M., Koekoek, G., Koley, S., Kolstein, M., Komori, K., Kondrashov, V., Kontos, A., Koper, N., Korobko, M., Korth, W. Z., Kovalam, M., Kozak, D. B., Krämer, C., Kringel, V., Krishnendu, N. V., Królak, A., Kuehn, G., Kumar, A., Kumar, P., Kumar, Rahul, Kumar, Rakesh, Kuns, K., Kwang, S., Lackey, B. D., Laghi, D., Lalande, E., Lam, T. L., Lamberts, A., Landry, M., Lane, B. B., Lang, R. N., Lange, J., Lantz, B., Lanza, R. K., La Rosa, I., Lartaux-Vollard, A., Lasky, P. D., Laxen, M., Lazzarini, A., Lazzaro, C., Leaci, P., Leavey, S., Lecoeuche, Y. K., Lee, H. M., Lee, H. W., Lee, J., Lee, K., Lehmann, J., Leon, E., Leroy, N., Letendre, N., Levin, Y., Li, A., Li, J., Li, K. J. L., Li, T. G. F., Li, X., Linde, F., Linker, S. D., Linley, J. N., Littenberg, T. B., Liu, J., Liu, X., Llorens-Monteagudo, M., Lo, R. K. L., Lockwood, A., London, L. T., Longo, A., Lorenzini, M., Loriette, V., Lormand, M., Losurdo, G., Lough, J. D., Lousto, C. O., Lovelace, G., Lück, H., Lumaca, D., Lundgren, A. P., Ma, Y., Macas, R., Macinnis, M., Macleod, D. M., Macmillan, I. A. O., Macquet, A., Magaña Hernandez, I., Magaña-Sandoval, F., Magazzù, C., Magee, R. M., Majorana, E., Maksimovic, I., Maliakal, S., Malik, A., Man, N., Mandic, V., Mangano, V., Mansell, G. L., Manske, M., Mantovani, M., Mapelli, M., Marchesoni, F., Marion, F., Márka, S., Márka, Z., Markakis, C., Markosyan, A. S., Markowitz, A., Maros, E., Marquina, A., Marsat, S., Martelli, F., Martin, I. W., Martin, R. M., Martinez, M., Martinez, V., Martynov, D. V., Masalehdan, H., Mason, K., Massera, E., Masserot, A., Massinger, T. J., Masso-Reid, M., Mastrogiovanni, S., Matas, A., Mateu-Lucena, M., Matichard, F., Matiushechkina, M., Mavalvala, N., Maynard, E., Mccann, J. J., Mccarthy, R., Mcclelland, D. E., Mccormick, S., Mcculler, L., Mcguire, S. C., Mcisaac, C., Mciver, J., Mcmanus, D. J., Mcrae, T., Mcwilliams, S. T., Meacher, D., Meadors, G. D., Mehmet, M., Mehta, A. K., Melatos, A., Melchor, D. A., Mendell, G., Menendez-Vazquez, A., Mercer, R. A., Mereni, L., Merfeld, K., Merilh, E. L., Merritt, J. D., Merzougui, M., Meshkov, S., Messenger, C., Messick, C., Metzdorff, R., Meyers, P. M., Meylahn, F., Mhaske, A., Miani, A., Miao, H., Michaloliakos, I., Michel, C., Middleton, H., Milano, L., Miller, A. L., Millhouse, M., Mills, J. C., Milotti, E., Milovich-Goff, M. C., Minazzoli, O., Minenkov, Y., Mir, Ll. M., Mishkin, A., Mishra, C., Mistry, T., Mitra, S., Mitrofanov, V. P., Mitselmakher, G., Mittleman, R., Mo, G., Mogushi, K., Mohapatra, S. R. P., Mohite, S. 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A., Prokhorov, L., Prosposito, P., Prudenzi, L., Puecher, A., Punturo, M., Puosi, F., Puppo, P., Pürrer, M., Qi, H., Quetschke, V., Quinonez, P. J., Quitzow-James, R., Raab, F. J., Raaijmakers, G., Radkins, H., Radulesco, N., Raffai, P., Rafferty, H., Rail, S. X., Raja, S., Rajan, C., Rajbhandari, B., Rakhmanov, M., Ramirez, K. E., Ramirez, T. D., Ramos-Buades, A., Rana, J., Rao, K., Rapagnani, P., Rapol, U. D., Ratto, B., Raymond, V., Razzano, M., Read, J., Regimbau, T., Rei, L., Reid, S., Reitze, D. H., Rettegno, P., Ricci, F., Richardson, C. J., Richardson, J. W., Richardson, L., Ricker, P. M., Riemenschneider, G., Riles, K., Rizzo, M., Robertson, N. A., Robinet, F., Rocchi, A., Rocha, J. A., Rodriguez, S., Rodriguez-Soto, R. D., Rolland, L., Rollins, J. G., Roma, V. J., Romanelli, M., Romano, R., Romel, C. L., Romero, A., Romero-Shaw, I. M., Romie, J. H., Ronchini, S., Rose, C. A., Rose, D., Rose, K., Rosell, M. J. B., Rosińska, D., Rosofsky, S. G., Ross, M. P., Rowan, S., Rowlinson, S. J., Roy, Santosh, Roy, Soumen, Ruggi, P., Ryan, K., Sachdev, S., Sadecki, T., Sadiq, J., Sakellariadou, M., Salafia, O. S., Salconi, L., Saleem, M., Samajdar, A., Sanchez, E. J., Sanchez, J. H., Sanchez, L. E., Sanchis-Gual, N., Sanders, J. R., Sandles, L., Santiago, K. A., Santos, E., Saravanan, T. R., Sarin, N., Sassolas, B., Sathyaprakash, B. S., Sauter, O., Savage, R. L., Savant, V., Sawant, D., Sayah, S., Schaetzl, D., Schale, P., Scheel, M., Scheuer, J., Schindler-Tyka, A., Schmidt, P., Schnabel, R., Schofield, R. M. S., Schönbeck, A., Schreiber, E., Schulte, B. W., Schutz, B. F., Schwarm, O., Schwartz, E., Scott, J., Scott, S. M., Seglar-Arroyo, M., Seidel, E., Sellers, D., Sengupta, A. S., Sennett, N., Sentenac, D., Sequino, V., Sergeev, A., Setyawati, Y., Shaffer, T., Shahriar, M. S., Sharifi, S., Sharma, A., Sharma, P., Shawhan, P., Shen, H., Shikauchi, M., Shink, R., Shoemaker, D. H., Shoemaker, D. M., Shukla, K., Shyamsundar, S., Sieniawska, M., Sigg, D., Singer, L. P., Singh, D., Singh, N., Singha, A., Singhal, A., Sintes, A. M., Sipala, V., Skliris, V., Slagmolen, B. J. J., Slaven-Blair, T. J., Smetana, J., Smith, J. R., Smith, R. J. E., Somala, S. N., Son, E. J., Soni, K., Soni, S., Sorazu, B., Sordini, V., Sorrentino, F., Sorrentino, N., Soulard, R., Souradeep, T., Sowell, E., Spencer, A. P., Spera, M., Srivastava, A. K., Srivastava, V., Staats, K., Stachie, C., Steer, D. A., Steinhoff, J., Steinke, M., Steinlechner, J., Steinlechner, S., Steinmeyer, D., Stevenson, S. P., Stolle-McAllister, G., Stops, D. J., Stover, M., Strain, K. A., Stratta, G., Strunk, A., Sturani, R., Stuver, A. L., Südbeck, J., Sudhagar, S., Sudhir, V., Suh, H. G., Summerscales, T. Z., Sun, H., Sun, L., Sunil, S., Sur, A., Suresh, J., Sutton, P. J., Swinkels, B. L., Szczepańczyk, M. J., Tacca, M., Tait, S. C., Talbot, C., Tanasijczuk, A. J., Tanner, D. B., Tao, D., Tapia, A., Tapia San Martin, E. 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E., Zweizig, J., Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015 - 2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Grav. waves and fundamental physics, RS: FSE Grav. waves and fundamental physics, RS: FSE MSP, LIGO Scientific Collaboration, Virgo Collaboration, Centre National de la Recherche Scientifique (CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015 - 2019) (COMUE UCA)-Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015 - 2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Nice Sophia Antipolis (... - 2019) (UNS), COMUE Université Côte d'Azur (2015 - 2019) (COMUE UCA), Abbott, R, Abbott, T, Abraham, S, Acernese, F, Ackley, K, Adams, A, Adams, C, Adhikari, R, Adya, V, Affeldt, C, Agathos, M, Agatsuma, K, Aggarwal, N, Aguiar, O, Aiello, L, Ain, A, Ajith, P, Akcay, S, Allen, G, Allocca, A, Altin, P, Amato, A, Anand, S, 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Bischi, M, Biscoveanu, S, Bisht, A, Bitossi, M, Bizouard, M, Blackburn, J, Blackman, J, Blair, C, Blair, D, Blair, R, Blanch, O, Bobba, F, Bode, N, Boer, M, Boetzel, Y, Bogaert, G, Boldrini, M, Bondu, F, Bonilla, E, Bonnand, R, Booker, P, Boom, B, Bork, R, Boschi, V, Bose, S, Bossilkov, V, Boudart, V, Bouffanais, Y, Bozzi, A, Bradaschia, C, Brady, P, Bramley, A, Branchesi, M, Brau, J, Breschi, M, Briant, T, Briggs, J, Brighenti, F, Brillet, A, Brinkmann, M, Brockill, P, Brooks, A, Brooks, J, Brown, D, Brunett, S, Bruno, G, Bruntz, R, Buikema, A, Bulik, T, Bulten, H, Buonanno, A, Buscicchio, R, Buskulic, D, Byer, R, Cabero, M, Cadonati, L, Caesar, M, Cagnoli, G, Cahillane, C, Calderon Bustillo, J, Callaghan, J, Callister, T, Calloni, E, Camp, J, Canepa, M, Cannon, K, Cao, H, Cao, J, Carapella, G, Carbognani, F, Carney, M, Carpinelli, M, Carullo, G, Carver, T, Casanueva Diaz, J, Casentini, C, Caudill, S, Cavaglia, M, Cavalier, F, Cavalieri, R, Cella, G, Cerda-Duran, P, Cesarini, E, Chaibi, W, Chakravarti, K, Chan, C, Chandra, K, Chanial, P, Chao, S, Charlton, P, Chase, E, Chassande-Mottin, E, Chatterjee, D, Chattopadhyay, D, Chaturvedi, M, Chatziioannou, K, Chen, A, Chen, H, Chen, X, Chen, Y, Cheng, H, Cheong, C, Chia, H, Chiadini, F, Chierici, R, Chincarini, A, Chiummo, A, Cho, G, Cho, H, Cho, M, Choate, S, Christensen, N, Chu, Q, Chua, S, Chung, K, Chung, S, Ciani, G, Ciecielag, P, Cieslar, M, Cifaldi, M, Ciobanu, A, Ciolfi, R, Cipriano, F, Cirone, A, Clara, F, Clark, E, Clark, J, Clarke, L, Clearwater, P, Clesse, S, Cleva, F, Coccia, E, Cohadon, P, Cohen, D, Colleoni, M, Collette, C, Collins, C, Colpi, M, Constancio, M, Conti, L, Cooper, S, Corban, P, Corbitt, T, Cordero-Carrion, I, Corezzi, S, Corley, K, Cornish, N, Corre, D, Corsi, A, Cortese, S, Costa, C, Cotesta, R, Coughlin, M, Coughlin, S, Coulon, J, Countryman, S, Cousins, B, Couvares, P, Covas, P, Coward, D, Cowart, M, Coyne, D, Coyne, R, Creighton, J, Creighton, T, Croquette, M, Crowder, S, Cudell, J, 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Easter, P, Eddolls, G, Edelman, B, Edo, T, Edy, O, Effler, A, Eichholz, J, Eikenberry, S, Eisenmann, M, Eisenstein, R, Ejlli, A, Errico, L, Essick, R, Estelles, H, Estevez, D, Etienne, Z, Etzel, T, Evans, M, Evans, T, Ewing, B, Fafone, V, Fair, H, Fairhurst, S, Fan, X, Farah, A, Farinon, S, Farr, B, Farr, W, Fauchon-Jones, E, Favata, M, Fays, M, Fazio, M, Feicht, J, Fejer, M, Feng, F, Fenyvesi, E, Ferguson, D, Fernandez-Galiana, A, Ferrante, I, Ferreira, T, Fidecaro, F, Figura, P, Fiori, I, Fiorucci, D, Fishbach, M, Fisher, R, Fishner, J, Fittipaldi, R, Fitz-Axen, M, Fiumara, V, Flaminio, R, Floden, E, Flynn, E, Fong, H, Font, J, Forsyth, P, Fournier, J, Frasca, S, Frasconi, F, Frei, Z, Freise, A, Frey, R, Frey, V, Fritschel, P, Frolov, V, Fronze, G, Fulda, P, Fyffe, M, Gabbard, H, Gadre, B, Gaebel, S, Gair, J, Gais, J, Galaudage, S, Gamba, R, Ganapathy, D, Ganguly, A, Gaonkar, S, Garaventa, B, Garcia-Quiros, C, Garufi, F, Gateley, B, Gaudio, S, Gayathri, V, Gemme, G, Gennai, A, George, D, George, J, George, R, Gergely, L, Ghonge, S, Ghosh, A, Ghosh, S, Giacomazzo, B, Giacoppo, L, Giaime, J, Giardina, K, Gibson, D, Gier, C, Gill, K, Giri, P, Glanzer, J, Gleckl, A, Godwin, P, Goetz, E, Goetz, R, Gohlke, N, Goncharov, B, Gonzalez, G, Gopakumar, A, Gossan, S, Gosselin, M, Gouaty, R, Grace, B, Grado, A, Granata, M, Granata, V, Grant, A, Gras, S, Grassia, P, Gray, C, Gray, R, Greco, G, Green, A, Green, R, Gretarsson, E, Griggs, H, Grignani, G, Grimaldi, A, Grimes, E, Grimm, S, Grote, H, Grunewald, S, Gruning, P, Guerrero, J, Guidi, G, Guimaraes, A, Guixe, G, Gulati, H, Guo, Y, Gupta, A, Gupta, P, Gustafson, E, Gustafson, R, Guzman, F, Haegel, L, Halim, O, Hall, E, Hamilton, E, Hammond, G, Haney, M, Hanke, M, Hanks, J, Hanna, C, Hannam, M, Hannuksela, O, Hansen, H, Hansen, T, Hanson, J, Harder, T, Hardwick, T, Haris, K, Harms, J, Harry, G, Harry, I, Hartwig, D, Hasskew, R, Haster, C, Haughian, K, Hayes, F, Healy, J, Heidmann, A, Heintze, M, Heinze, J, Heinzel, J, Heitmann, H, Hellman, F, Hello, P, Helmling-Cornell, A, Hemming, G, Hendry, M, Heng, I, Hennes, E, Hennig, J, Hennig, M, Hernandez Vivanco, F, Heurs, M, Hild, S, Hill, P, Hines, A, Hochheim, S, Hofgard, E, Hofman, D, Hohmann, J, Holgado, A, Holland, N, Hollows, I, Holmes, Z, Holt, K, Holz, D, Hopkins, P, Horst, C, Hough, J, Howell, E, Hoy, C, Hoyland, D, Huang, Y, Hubner, M, Huddart, A, Huerta, E, Hughey, B, Hui, V, Husa, S, Huttner, S, Hutzler, B, Huxford, R, Huynh-Dinh, T, Idzkowski, B, Iess, A, Imperato, S, Inchauspe, H, Ingram, C, Intini, G, Isi, M, Iyer, B, Jaberianhamedan, V, Jacqmin, T, Jadhav, S, James, A, Jani, K, Janssens, K, Janthalur, N, Jaranowski, P, Jariwala, D, Jaume, R, Jenkins, A, Jeunon, M, Jiang, J, Johns, G, Johnson-Mcdaniel, N, Jones, A, Jones, D, Jones, J, Jones, P, Jones, R, Jonker, R, Ju, L, Junker, J, Kalaghatgi, C, Kalogera, V, Kamai, B, Kandhasamy, S, Kang, G, Kanner, J, Kapadia, S, Kapasi, D, Karathanasis, C, Karki, S, Kashyap, R, Kasprzack, M, Kastaun, W, Katsanevas, S, Katsavounidis, E, Katzman, W, Kawabe, K, Kefelian, F, Keitel, D, Key, J, Khadka, S, Khalili, F, Khan, I, Khan, S, Khazanov, E, Khetan, N, Khursheed, M, Kijbunchoo, N, Kim, C, Kim, G, Kim, J, Kim, K, Kim, W, Kim, Y, Kimball, C, King, P, Kinley-Hanlon, M, Kirchhoff, R, Kissel, J, Kleybolte, L, Klimenko, S, Knowles, T, Knyazev, E, Koch, P, Koehlenbeck, S, Koekoek, G, Koley, S, Kolstein, M, Komori, K, Kondrashov, V, Kontos, A, Koper, N, Korobko, M, Korth, W, Kovalam, M, Kozak, D, Kramer, C, Kringel, V, Krishnendu, N, Krolak, A, Kuehn, G, Kumar, A, Kumar, P, Kumar, R, Kuns, K, Kwang, S, Lackey, B, Laghi, D, Lalande, E, Lam, T, Lamberts, A, Landry, M, Lane, B, Lang, R, Lange, J, Lantz, B, Lanza, R, La Rosa, I, Lartaux-Vollard, A, Lasky, P, Laxen, M, Lazzarini, A, Lazzaro, C, Leaci, P, Leavey, S, Lecoeuche, Y, Lee, H, Lee, J, Lee, K, Lehmann, J, Leon, E, Leroy, N, Letendre, N, Levin, Y, Li, A, Li, J, Li, K, Li, T, Li, X, Linde, F, Linker, S, Linley, J, Littenberg, T, Liu, J, Liu, X, Llorens-Monteagudo, M, Lo, R, Lockwood, A, London, L, Longo, A, Lorenzini, M, Loriette, V, Lormand, M, Losurdo, G, Lough, J, Lousto, C, Lovelace, G, Luck, H, Lumaca, D, Lundgren, A, Ma, Y, Macas, R, Macinnis, M, Macleod, D, Macmillan, I, Macquet, A, Magana Hernandez, I, Magana-Sandoval, F, Magazzu, C, Magee, R, Majorana, E, Maksimovic, I, Maliakal, S, Malik, A, Man, N, Mandic, V, Mangano, V, Mansell, G, Manske, M, Mantovani, M, Mapelli, M, Marchesoni, F, Marion, F, Marka, S, Marka, Z, Markakis, C, Markosyan, A, Markowitz, A, Maros, E, Marquina, A, Marsat, S, Martelli, F, Martin, I, Martin, R, Martinez, M, Martinez, V, Martynov, D, Masalehdan, H, Mason, K, Massera, E, Masserot, A, Massinger, T, Masso-Reid, M, Mastrogiovanni, S, Matas, A, Mateu-Lucena, M, Matichard, F, Matiushechkina, M, Mavalvala, N, Maynard, E, Mccann, J, Mccarthy, R, Mcclelland, D, Mccormick, S, Mcculler, L, Mcguire, S, Mcisaac, C, Mciver, J, Mcmanus, D, Mcrae, T, Mcwilliams, S, Meacher, D, Meadors, G, Mehmet, M, Mehta, A, Melatos, A, Melchor, D, Mendell, G, Menendez-Vazquez, A, Mercer, R, Mereni, L, Merfeld, K, Merilh, E, Merritt, J, Merzougui, M, Meshkov, S, Messenger, C, Messick, C, Metzdorff, R, Meyers, P, Meylahn, F, Mhaske, A, Miani, A, Miao, H, Michaloliakos, I, Michel, C, Middleton, H, Milano, L, Miller, A, Millhouse, M, Mills, J, Milotti, E, Milovich-Goff, M, Minazzoli, O, Minenkov, Y, Mir, L, Mishkin, A, Mishra, C, Mistry, T, Mitra, S, Mitrofanov, V, Mitselmakher, G, Mittleman, R, Mo, G, Mogushi, K, Mohapatra, S, Mohite, S, Molina, I, Molina-Ruiz, M, Mondin, M, Montani, M, Moore, C, Moraru, D, Morawski, F, Moreno, G, Morisaki, S, Mours, B, Mow-Lowry, C, Mozzon, S, Muciaccia, F, Mukherjee, A, Mukherjee, D, Mukherjee, S, Mukund, N, Mullavey, A, Munch, J, Muniz, E, Murray, P, Nadji, S, Nagar, A, Nardecchia, I, Naticchioni, L, Nayak, R, Neil, B, Neilson, J, Nelemans, G, Nelson, T, Nery, M, Neunzert, A, Nitz, A, Ng, K, Ng, S, Nguyen, C, Nguyen, P, Nguyen, T, Nichols, S, Nissanke, S, Nocera, F, Noh, M, North, C, Nothard, D, Nuttall, L, Oberling, J, O'Brien, B, O'Dell, J, Oganesyan, G, Ogin, G, Oh, J, Oh, S, Ohme, F, Ohta, H, Okada, M, Olivetto, C, Oppermann, P, Oram, R, O'Reilly, B, Ormiston, R, Ortega, L, O'Shaughnessy, R, Ossokine, S, Osthelder, C, Ottaway, D, Overmier, H, Owen, B, Pace, A, Pagano, G, Page, M, Pagliaroli, G, Pai, A, Pai, S, Palamos, J, Palashov, O, Palomba, C, Pan, H, Panda, P, Pang, T, Pankow, C, Pannarale, F, Pant, B, Paoletti, F, Paoli, A, Paolone, A, Parker, W, Pascucci, D, Pasqualetti, A, Passaquieti, R, Passuello, D, Patel, M, Patricelli, B, Payne, E, Pechsiri, T, Pedraza, M, Pegoraro, M, Pele, A, Penn, S, Perego, A, Perez, C, Perigois, C, Perreca, A, Perries, S, Petermann, J, Petterson, D, Pfeiffer, H, Pham, K, Phukon, K, Piccinni, O, Pichot, M, Piendibene, M, Piergiovanni, F, Pierini, L, Pierro, V, Pillant, G, Pilo, F, Pinard, L, Pinto, I, Piotrzkowski, K, Pirello, M, Pitkin, M, Placidi, E, Plastino, W, Pluchar, C, Poggiani, R, Polini, E, Pong, D, Ponrathnam, S, Popolizio, P, Porter, E, Poverman, A, Powell, J, Pracchia, M, Prajapati, A, Prasai, K, Prasanna, R, Pratten, G, Prestegard, T, Principe, M, Prodi, G, Prokhorov, L, Prosposito, P, Prudenzi, L, Puecher, A, Punturo, M, Puosi, F, Puppo, P, Purrer, M, Qi, H, Quetschke, V, Quinonez, P, Quitzow-James, R, Raab, F, Raaijmakers, G, Radkins, H, Radulesco, N, Raffai, P, Rafferty, H, Rail, S, Raja, S, Rajan, C, Rajbhandari, B, Rakhmanov, M, Ramirez, K, Ramirez, T, Ramos-Buades, A, Rana, J, Rao, K, Rapagnani, P, Rapol, U, Ratto, B, Raymond, V, Razzano, M, Read, J, Regimbau, T, Rei, L, Reid, S, Reitze, D, Rettegno, P, Ricci, F, Richardson, C, Richardson, J, Richardson, L, Ricker, P, Riemenschneider, G, Riles, K, Rizzo, M, Robertson, N, Robinet, F, Rocchi, A, Rocha, J, Rodriguez, S, Rodriguez-Soto, R, Rolland, L, Rollins, J, Roma, V, Romanelli, M, Romano, R, Romel, C, Romero, A, Romero-Shaw, I, Romie, J, Ronchini, S, Rose, C, Rose, D, Rose, K, Rosell, M, Rosinska, D, Rosofsky, S, Ross, M, Rowan, S, Rowlinson, S, Roy, S, Ruggi, P, Ryan, K, Sachdev, S, Sadecki, T, Sadiq, J, Sakellariadou, M, Salafia, O, Salconi, L, Saleem, M, Samajdar, A, Sanchez, E, Sanchez, J, Sanchez, L, Sanchis-Gual, N, Sanders, J, Sandles, L, Santiago, K, Santos, E, Saravanan, T, Sarin, N, Sassolas, B, Sathyaprakash, B, Sauter, O, Savage, R, Savant, V, Sawant, D, Sayah, S, Schaetzl, D, Schale, P, Scheel, M, Scheuer, J, Schindler-Tyka, A, Schmidt, P, Schnabel, R, Schofield, R, Schonbeck, A, Schreiber, E, Schulte, B, Schutz, B, Schwarm, O, Schwartz, E, Scott, J, Scott, S, Seglar-Arroyo, M, Seidel, E, Sellers, D, Sengupta, A, Sennett, N, Sentenac, D, Sequino, V, Sergeev, A, Setyawati, Y, Shaffer, T, Shahriar, M, Sharifi, S, Sharma, A, Sharma, P, Shawhan, P, Shen, H, Shikauchi, M, Shink, R, Shoemaker, D, Shukla, K, Shyamsundar, S, Sieniawska, M, Sigg, D, Singer, L, Singh, D, Singh, N, Singha, A, Singhal, A, Sintes, A, Sipala, V, Skliris, V, Slagmolen, B, Slaven-Blair, T, Smetana, J, Smith, J, 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V., Vasuth, M., Vicere, A., Wessels, P., Yu, H., Zadrozny, A., The LIGO Scientific Collaboration, The Virgo Collaboration, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Université Nice Sophia Antipolis (1965 - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Université de Rennes (UR)-Institut National des Sciences Appliquées - Rennes (INSA Rennes), Institut National des Sciences Appliquées (INSA)-Institut National des Sciences Appliquées (INSA)-École Nationale Supérieure des Sciences Appliquées et de Technologie (ENSSAT)-Centre National de la Recherche Scientifique (CNRS), Fédération de recherche du Département de physique de l'Ecole Normale Supérieure - ENS Paris (FRDPENS), École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Collège de France (CdF (institution))-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut des Hautes Études Scientifiques (IHES), (Astro)-Particles Physics, LIGO Sci Collaboration, Faculty of Science, Gravitation and Astroparticle Physics Amsterdam, Other Research IHEF (IoP, FNWI), Astroparticle Physics (IHEF, IoP, FNWI), and IoP (FNWI)
Subjects: neutron star: binary, IMPACT, Astronomy, Binary number, General Physics and Astronomy, Astrophysics, Coalescence, Ray coordinates, binary systems, black holes, false alarm rate, mass ratio, near-real time, neutron stars, ray coordinates, total mass, 01 natural sciences, General Relativity and Quantum Cosmology, Gravitation, Cosmology & Astrophysics, GRAVITATIONAL-WAVES, 010305 fluids & plasmas, Cosmology & Astrophysics, Gravitational Waves, LIGO, Virgo, CBC, O3, EQUATION, LIGO, Gravitational wave detection, Gravitational wave sources, QC, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, BILBY, Settore FIS/03, black hole: spin, Black holes, Gravitational effects, BAYESIAN-INFERENCE, COMPACT OBJECTS, SPINMASS, False alarm rate, STATE, Binary systems, Physical Sciences, [PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], Gravitational wave source, Astrophysics - High Energy Astrophysical Phenomena, asymmetry, CBC, Gravitation, BLACK-HOLE MERGERS, PARAMETER-ESTIMATION, GW_HIGHLIGHT, data analysis method, Astrophysics::High Energy Astrophysical Phenomena, Physics, Multidisciplinary, O3, FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), Astrophysics::Cosmology and Extragalactic Astrophysics, Gravitational Wave Transient Catalog 2, Gravity waves, Physics and Astronomy(all), gravitational radiation: direct detection, 1ST, Neutron stars, binary: coalescence, Binary black hole, SEARCH, 0103 physical sciences, ddc:530, 010306 general physics, STFC, MASS-DISTRIBUTION, Gravitational Waves, Science & Technology, Gravitational wave, Virgo, Gamma rays, gravitational radiation, RCUK, black hole: mass, Mass ratio, Near-real time, binary: compact, Stars, gravitational radiation detector, Redshift, detector: sensitivity, Black hole, Neutron star, wave: model, VIRGO, black hole: binary, Physics and Astronomy, [SDU]Sciences of the Universe [physics], gravitational radiation: emission, Dewey Decimal Classification::500 | Naturwissenschaften::530 | Physik, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Total mass
Abstract: We report on gravitational wave discoveries from compact binary coalescences detected by Advanced LIGO and Advanced Virgo in the first half of the third observing run (O3a) between 1 April 2019 15:00 UTC and 1 October 2019 15:00. By imposing a false-alarm-rate threshold of two per year in each of the four search pipelines that constitute our search, we present 39 candidate gravitational wave events. At this threshold, we expect a contamination fraction of less than 10%. Of these, 26 candidate events were reported previously in near real-time through GCN Notices and Circulars; 13 are reported here for the first time. The catalog contains events whose sources are black hole binary mergers up to a redshift of ~0.8, as well as events whose components could not be unambiguously identified as black holes or neutron stars. For the latter group, we are unable to determine the nature based on estimates of the component masses and spins from gravitational wave data alone. The range of candidate events which are unambiguously identified as binary black holes (both objects $\geq 3~M_\odot$) is increased compared to GWTC-1, with total masses from $\sim 14~M_\odot$ for GW190924_021846 to $\sim 150~M_\odot$ for GW190521. For the first time, this catalog includes binary systems with significantly asymmetric mass ratios, which had not been observed in data taken before April 2019. We also find that 11 of the 39 events detected since April 2019 have positive effective inspiral spins under our default prior (at 90% credibility), while none exhibit negative effective inspiral spin. Given the increased sensitivity of Advanced LIGO and Advanced Virgo, the detection of 39 candidate events in ~26 weeks of data (~1.5 per week) is consistent with GWTC-1., Comment: This version updates with minor revisions to typographical errors. We would also like to call attention to the updated parameter estimation samples data release here: https://dcc.ligo.org/LIGO-P2000223/public
Published: 2021

3. Enhanced cluster lensing models with measured galaxy kinematics

Author: Carlo Giocoli, Eros Vanzella, G. B. Caminha, Piero Rosati, Claudio Grillo, P. Bergamini, Francesco Calura, Adriano Agnello, Giulia Rodighiero, Massimo Meneghetti, Amata Mercurio, Marco Lombardi, Andrea Biviano, and Astronomy
Subjects: DYNAMICS, DECOMPOSITION, Stellar kinematics, astro-ph.GA, Population, Dark matter, FOS: Physical sciences, DARK-MATTER HALOS, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, gravitational lensing: strong, galaxies: clusters: general, cosmology: observations, dark matter, galaxies: kinematics and dynamics, 01 natural sciences, Virial theorem, dark matter, NO, SPHERICAL GALAXIES, SLACS LENSES, 0103 physical sciences, kinematics and dynamics [galaxies], Cluster (physics), clusters: general [galaxies], DISTRIBUTIONS, education, 010303 astronomy & astrophysics, galaxies: kinematics and dynamics, Astrophysics::Galaxy Astrophysics, MASS-DISTRIBUTION, Physics, education.field_of_study, Mass distribution, 010308 nuclear & particles physics, gravitational lensing: strong, Velocity dispersion, Astronomy and Astrophysics, Astrophysics - Astrophysics of Galaxies, Galaxy, observations [cosmology], galaxies: clusters: general, Space and Planetary Science, cosmology: observations, Astrophysics of Galaxies (astro-ph.GA), strong [gravitational lensing], FRONTIER-FIELDS, 2-DIMENSIONAL KINEMATICS, ACS SURVEY
Abstract: We present an improved determination of the total mass distribution of three CLASH/HFF massive clusters, MACS J1206.2-0847 (z=0.44), MACS J0416.1-2403 (z=0.40), Abell S1063 (z=0.35). We specifically reconstruct the sub-halo mass component with robust stellar kinematics information of cluster galaxies, in combination with precise strong lensing models based on large samples of spectroscopically identified multiple images. We use VLT/MUSE integral-field spectroscopy in the cluster cores to measure the stellar velocity dispersion, $\sigma$, of 40-60 member galaxies per cluster, covering 4-5 magnitudes to $m_{F160W}\simeq 21.5$. We verify the robustness and quantify the accuracy of the velocity dispersion measurements with extensive spectral simulations. With these data, we determine the normalization and slope of the galaxy $L\mbox{-}\sigma$ Faber-Jackson relation in each cluster and use these parameters as a prior for the scaling relations of the sub-halo population in the mass distribution modeling. When compared to our previous lens models, the inclusion of member galaxies' kinematics provides a similar precision in reproducing the positions of the multiple images. However, the inherent degeneracy between the central effective velocity dispersion, $\sigma_0$, and truncation radius, $r_{cut}$, of sub-halos is strongly reduced, thus significantly alleviating possible systematics in the measurements of sub-halo masses. The three independent determinations of the $\sigma_0\mbox{-}r_{cut}$ scaling relation in each cluster are found to be fully consistent, enabling a statistical determination of sub-halo sizes as a function of $\sigma_0$, or halo masses. We derive galaxy central velocity dispersion functions of the three clusters and found them in agreement with each other. Sub-halo mass functions determined with this method can be compared with those obtained from cosmological simulations., Comment: v2: minor changes. Accepted for publication in A&A (18 pages, 11 figures)
Published: 2019

4. Systematic study of fusion-fission like events in 19F + 175Lu interactions at low energies.

Author: Bhat, Ishfaq Majeed, Shuaib, Mohd., Asnain, M. Shariq, Sharma, Vijay R., Yadav, Abhishek, Sharma, Manoj Kumar, Singh, Pushpendra P., Singh, Devendra P., Kumar, R., Singh, R.P., Muralithar, S., Singh, B.P., and Prasad, R.
Subjects: *DEEP inelastic collisions, *PARTICLES (Nuclear physics), *INDIUM, *CENTROID, *XENON, *ISOBARIC processes
Abstract: In the present work, 21 fission like residues (74 ≤ A ≤ 133) expected to be populated via fission of composite systems formed as a result of complete and incomplete fusion processes in the interaction of 19F + 175Lu have been identified at two projectile energies viz. 105 ± 1.4 and 110 ± 1.5 MeV. The production cross-sections of these residues have been measured employing the recoil-catcher activation technique followed by the off-line γ -ray spectroscopy. The mass distribution of the fission-like residues is found to be symmetric and can be fitted with a single Gaussian peak, indicating their production from the fully equilibrated composite systems. The variance and centroid for isotopic-yield and isobaric charge distributions have also been obtained for Indium ( 107 , 108 , 109 , 111 m In) and Xenon (120,121,122,123Xe) isotopes and are found to be in a reasonably good agreement with the reported literature values. In the present analysis, a self-consistent approach for determining the isobaric charge dispersion parameters has been adopted. Fission is found to be one of the competing modes of de-excitation of complete and/or incomplete fusion composites at low excitation energies where evaporation of light nuclear particle(s) is considered to be a dominant contributor. [ABSTRACT FROM AUTHOR]
Published: 2021
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5. Testing baryon-induced core formation in $\Lambda$CDM: A comparison of the DC14 and coreNFW dark matter halo models on galaxy rotation curves

Author: Maarten Baes, F. Allaert, G. Gentile, Astrophysics, Physics, and Astronomy and Astrophysics Research Group
Subjects: DWARF GALAXIES, DISC GALAXIES, Dark matter, galaxies: halos, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Disc galaxy, 01 natural sciences, dark matter, SURFACE BRIGHTNESS GALAXIES, SPHERICAL GALAXIES, kinematics and dynamics [galaxies], 0103 physical sciences, Galaxies: Evolution, 010303 astronomy & astrophysics, evolution [galaxies], Galaxy rotation curve, galaxies: kinematics and dynamics, Astrophysics::Galaxy Astrophysics, MASS-DISTRIBUTION, Dwarf galaxy, Physics, Spiral galaxy, 010308 nuclear & particles physics, GALACTIC HALOS, Astronomy and Astrophysics, PROFILES, Astrophysics - Astrophysics of Galaxies, Galaxy, halos [galaxies], Dark matter halo, Physics and Astronomy, Space and Planetary Science, Halo, STELLAR MASS, SPIRAL GALAXIES, CUSPS
Abstract: Recent cosmological hydrodynamical simulations suggest that baryonic processes, and in particular supernova feedback after bursts of star formation, can alter the structure of dark matter haloes and transform primordial cusps into shallower cores. To assess whether this mechanism offers a solution to the cusp-core controversy, simulated haloes must be compared to real dark matter haloes inferred from galaxy rotation curves. For this purpose, two new dark matter density profiles were recently derived from simulations of galaxies in complementary mass ranges: the DC14 halo ($10^{10} < M_{\text{halo}}/M_{\odot} < 8 \times 10^{11}$) and the coreNFW halo ($10^{7} < M_{\text{halo}}/M_{\odot} < 10^{9}$). Both models have individually been found to give good fits to observed rotation curves. For the DC14 model, however, the agreement of the predicted halo properties with cosmological scaling relations was confirmed by one study, but strongly refuted by another. A next question is whether the two models converge to the same solution in the mass range where both should be appropriate. To investigate this, we tested the DC14 and cNFW halo models on the rotation curves of a selection of galaxies with halo masses in the range $4 \times 10^{9}$ - $7 \times 10^{10}$ $M_{\odot}$. We further applied the DC14 model to a set of rotation curves at higher halo masses, up to $9 \times 10^{11}$ $M_{\odot}$, to verify the agreement with the cosmological scaling relations. We find that both models are generally able to reproduce the observed rotation curves, in line with earlier results, and the predicted dark matter haloes are consistent with the cosmological $c-M_{\text{halo}}$ and $M_{*}-M_{\text{halo}}$ relations. The DC14 and cNFW models are also in fairly good agreement with each other, even though DC14 tends to predict slightly less extended cores and somewhat more concentrated haloes than cNFW., Comment: 19 pages, 12 figures, accepted for publication in A&A
Published: 2017

6. Search for Gravitational Waves Associated with Gamma-Ray Bursts during the First Advanced LIGO Observing Run and Implications for the Origin of GRB 150906B

Subjects: COOLED ACCRETION DISKS, binaries: close, UNUSUAL SUPERNOVA, gravitational waves, DOUBLE NEUTRON-STARS, BAND FOLLOW-UP, gamma-ray burst: general, BLACK-HOLE, EXTENDED EMISSION, PRECURSOR ACTIVITY, RELATIVISTIC JETS, EQUATION-OF-STATE, MASS-DISTRIBUTION
Abstract: We present the results of the search for gravitational waves (GWs) associated with gamma-ray bursts detected during the first observing run of the Advanced Laser Interferometer Gravitational-Wave Observatory (LIGO). We find no evidence of a GW signal for any of the 41 gamma-ray bursts for which LIGO data are available with sufficient duration. For all gamma-ray bursts, we place lower bounds on the distance to the source using the optimistic assumption that GWs with an energy of 10(-2)M(circle dot)c(2). were emitted within the 16-500 Hz band, and we find a median 90% confidence limit of 71 Mpc at 150 Hz. For the subset of 19 short/hard gamma-ray bursts, we place lower bounds on distance with a median 90% confidence limit of 90 Mpc for binary neutron star (BNS) coalescences, and 150 and 139 Mpc for neutron star-black hole coalescences with spins aligned to the orbital angular momentum and in a generic configuration, respectively. These are the highest distance limits ever achieved by GW searches. We also discuss in detail the results of the search for GWs associated with GRB 150906B, an event that was localized by the InterPlanetary Network near the local galaxy NGC 3313, which is at a luminosity distance of 54 Mpc (z = 0.0124). Assuming the gamma-ray emission is beamed with a jet half-opening angle 99%. Further, we exclude such progenitors up to a distance of 102 Mpc and 170 Mpc, respectively.
Published: 2017

7. Search for Gravitational Waves Associated with Gamma-Ray Bursts during the First Advanced LIGO Observing Run and Implications for the Origin of GRB 150906B

Subjects: COOLED ACCRETION DISKS, binaries: close, UNUSUAL SUPERNOVA, gravitational waves, DOUBLE NEUTRON-STARS, BAND FOLLOW-UP, gamma-ray burst: general, BLACK-HOLE, EXTENDED EMISSION, PRECURSOR ACTIVITY, RELATIVISTIC JETS, EQUATION-OF-STATE, MASS-DISTRIBUTION
Abstract: We present the results of the search for gravitational waves (GWs) associated with gamma-ray bursts detected during the first observing run of the Advanced Laser Interferometer Gravitational-Wave Observatory (LIGO). We find no evidence of a GW signal for any of the 41 gamma-ray bursts for which LIGO data are available with sufficient duration. For all gamma-ray bursts, we place lower bounds on the distance to the source using the optimistic assumption that GWs with an energy of 10(-2)M(circle dot)c(2). were emitted within the 16-500 Hz band, and we find a median 90% confidence limit of 71 Mpc at 150 Hz. For the subset of 19 short/hard gamma-ray bursts, we place lower bounds on distance with a median 90% confidence limit of 90 Mpc for binary neutron star (BNS) coalescences, and 150 and 139 Mpc for neutron star-black hole coalescences with spins aligned to the orbital angular momentum and in a generic configuration, respectively. These are the highest distance limits ever achieved by GW searches. We also discuss in detail the results of the search for GWs associated with GRB 150906B, an event that was localized by the InterPlanetary Network near the local galaxy NGC 3313, which is at a luminosity distance of 54 Mpc (z = 0.0124). Assuming the gamma-ray emission is beamed with a jet half-opening angle 99%. Further, we exclude such progenitors up to a distance of 102 Mpc and 170 Mpc, respectively.
Published: 2017

8. Search for Gravitational Waves Associated with Gamma-Ray Bursts during the First Advanced LIGO Observing Run and Implications for the Origin of GRB 150906B

Author: Ligo, Scientific Collaboration, Virgo Collaboration, Ipn, Collaboration, Abbott, B. P., Abbott, R., Abbott, T. D., Abernathy, M. R., Acernese, F., Ackley, K., Adams, C., Adams, T., Addesso, P., Adhikari, R. X., Adya, V. B., Affeldt, C., Agathos, M., Agatsuma, K., Aggarwal, N., Aguiar, O. D., Aiello, L., Ain, A., Ajith, P., Allen, B., Allocca, A., Altin, P. A., Ananyeva, A., Anderson, S. B., Anderson, W. G., Appert, S., Arai, K., Araya, M. C., Areeda, J. S., Arnaud, N., Arun, K. G., Ascenzi, S., Ashton, G., Ast, M., Aston, S. M., Astone, P., Aufmuth, P., Aulbert, C., Avila-Alvarez, A., Babak, S., Bacon, P., Bader, M. K. M., Baker, P. T., Baldaccini, F., Ballardin, G., Ballmer, S. W., Barayoga, J. C., Barclay, S. E., Barish, B. C., Barker, D., Barone, F., Barr, B., Barsotti, L., Barsuglia, M., Barta, D., Bartlett, J., Bartos, I., Bassiri, R., Basti, A., Batch, J. C., Baune, C., Bavigadda, V., Bazzan, M., Beer, C., Bejger, M., Belahcene, I., Belgin, M., Bell, A. S., Berger, B. K., Bergmann, G., Berry, C. P. L., Bersanetti, D., Bertolini, A., Betzwieser, J., Bhagwat, S., Bhandare, R., Bilenko, I. A., Billingsley, G., Billman, C. R., Birch, J., Birney, R., Birnholtz, O., Biscans, S., Bisht, A., Bitossi, M., Biwer, C., Bizouard, M. A., Blackburn, J. K., Blackman, J., Blair, C. D., Blair, D. G., Blair, R. M., Bloemen, S., Bock, O., Boer, M., Bogaert, G., Bohe, A., Bondu, F., Bonnand, R., Boom, B. A., Bork, R., Boschi, V., Bose, S., Bouffanais, Y., Bozzi, A., Bradaschia, C., Brady, P. R., Braginsky, V. B., Branchesi, M., Brau, J. E., Briant, T., Brillet, A., Brinkmann, M., Brisson, V., Brockill, P., Broida, J. E., Brooks, A. F., Brown, D. A., Brown, D. D., Brown, N. M., Brunett, S., Buchanan, C. C., Buikema, A., Bulik, T., Bulten, H. J., Buonanno, A., Buskulic, D., Buy, C., Byer, R. L., Cabero, M., Cadonati, L., Cagnoli, G., Cahillane, C., Calder On Bustillo, J., Callister, T. A., Calloni, E., Camp, J. B., Canepa, M., Cannon, K. C., Cao, H., Cao, J., Capano, C. D., Capocasa, E., Carbognani, F., Caride, S., Casanueva Diaz, J., Casentini, C., Caudill, S., Cavagli A, M., Cavalier, F., Cavalieri, R., Cella, G., Cepeda, C. B., Cerboni Baiardi, L., Cerretani, G., Cesarini, E., Chamberlin, S. J., Chan, M., Chao, S., Charlton, P., Chassande-Mottin, E., Cheeseboro, B. D., Chen, H. Y., Chen, Y., Cheng, H. -P, Chincarini, A., Chiummo, A., Chmiel, T., Cho, H. S., Cho, M., Chow, J. H., Christensen, N., Chu, Q., Chua, A. J. K., Chua, S., Chung, S., Ciani, G., Clara, F., Clark, J. A., Cleva, F., Cocchieri, C., Coccia, E., Cohadon, P. -F, Colla, A., Collette, C. G., Cominsky, L., Constancio, M., Conti, L., Cooper, S. J., Corbitt, T. R., Cornish, N., Corsi, A., Cortese, S., Costa, C. A., Coughlin, M. W., Coughlin, S. B., Coulon, J. -P, Countryman, S. T., Couvares, P., Covas, P. B., Cowan, E. E., Coward, D. M., Cowart, M. J., Coyne, D. C., Coyne, R., Creighton, J. D. E., Creighton, T. D., Cripe, J., Crowder, S. G., Cullen, T. J., Cumming, A., Cunningham, L., Cuoco, E., Dal Canton, T., D Alya, G., Danilishin, S. L., D Antonio, S., Danzmann, K., Dasgupta, A., Da Silva Costa, C. F., Dattilo, V., Dave, I., Davier, M., Davies, G. S., Davis, D., Daw, E. J., Day, B., Day, R., De, S., Debra, D., Debreczeni, G., Degallaix, J., Laurentis, M., Del Eglise, S., Del Pozzo, W., Denker, T., Dent, T., Dergachev, V., Rosa, R., Derosa, R. T., Desalvo, R., Devenson, J., Devine, R. C., Dhurandhar, S., D Iaz, M. C., Di Fiore, L., Di Giovanni, M., Di Girolamo, T., Di Lieto, A., Di Pace, S., Di Palma, I., Di Virgilio, A., Doctor, Z., Dolique, V., Donovan, F., Dooley, K. L., Doravari, S., Dorrington, I., Douglas, R., Dovale Alvarez, M., Downes, T. P., Drago, M., Drever, R. W. P., Driggers, J. C., Du, Z., Ducrot, M., Dwyer, S. E., Edo, T. B., Edwards, M. C., Effler, A., Eggenstein, H. -B, Ehrens, P., Eichholz, J., Eikenberry, S. S., Eisenstein, R. A., Essick, R. C., Etienne, Z., Etzel, T., Evans, M., Evans, T. M., Everett, R., Factourovich, M., Fafone, V., Fair, H., Fairhurst, S., Fan, X., Farinon, S., Farr, B., Farr, W. M., Fauchon-Jones, E. J., Favata, M., Fays, M., Fehrmann, H., Fejer, M. M., Fern Andez Galiana, A., Ferrante, I., Ferreira, E. C., Ferrini, F., Fidecaro, F., Fiori, I., Fiorucci, D., Fisher, R. P., Flaminio, R., Fletcher, M., Fong, H., Forsyth, S. S., Fournier, J. -D, Frasca, S., Frasconi, F., Frei, Z., Freise, A., Frey, R., Frey, V., Fries, E. M., Fritschel, P., Frolov, V. V., Fulda, P., Fyffe, M., Gabbard, H., Gadre, B. U., Gaebel, S. M., Gair, J. R., Gammaitoni, L., Gaonkar, S. G., Garufi, F., Gaur, G., Gayathri, V., Gehrels, N., Gemme, G., Genin, E., Gennai, A., George, J., Gergely, L., Germain, V., Ghonge, S., Ghosh, Abhirup, Ghosh, Archisman, Ghosh, S., Giaime, J. A., Giardina, K. D., Giazotto, A., Gill, K., Glaefke, A., Goetz, E., Goetz, R., Gondan, L., Gonz Alez, G., Gonzalez Castro, J. M., Gopakumar, A., Gorodetsky, M. L., Gossan, S. E., Gosselin, M., Gouaty, R., Grado, A., Graef, C., Granata, M., Grant, A., Gras, S., Gray, C., Greco, G., Green, A. C., Paul Groot, Grote, H., Grunewald, S., Guidi, G. M., Guo, X., Gupta, A., Gupta, M. K., Gushwa, K. E., Gustafson, E. K., Gustafson, R., Hacker, J. J., Hall, B. R., Hall, E. D., Hammond, G., Haney, M., Hanke, M. M., Hanks, J., Hanna, C., Hanson, J., Hardwick, T., Harms, J., Harry, G. M., Harry, I. W., Hart, M. J., Hartman, M. T., Haster, C. -J, Haughian, K., Healy, J., Heidmann, A., Heintze, M. C., Heitmann, H., Hello, P., Hemming, G., Hendry, M., Heng, I. S., Hennig, J., Henry, J., Heptonstall, A. W., Heurs, M., Hild, S., Hoak, D., Hofman, D., Holt, K., Holz, D. E., Hopkins, P., Hough, J., Houston, E. A., Howell, E. J., Hu, Y. M., Huerta, E. A., Huet, D., Hughey, B., Husa, S., Huttner, S. H., Huynh-Dinh, T., Indik, N., Ingram, D. R., Inta, R., Isa, H. N., Isac, J. -M, Isi, M., Isogai, T., Iyer, B. R., Izumi, K., Jacqmin, T., Jani, K., Jaranowski, P., Jawahar, S., Jim Enez-Forteza, F., Johnson, W. W., Jones, D. I., Jones, R., Jonker, R. J. G., Ju, L., Junker, J., Kalaghatgi, C. V., Kalogera, V., Kandhasamy, S., Kang, G., Kanner, J. B., Karki, S., Karvinen, K. S., Kasprzack, M., Katsavounidis, E., Katzman, W., Kaufer, S., Kaur, T., Kawabe, K., K Ef Elian, F., Keitel, D., Kelley, D. B., Kennedy, R., Key, J. S., Khalili, F. Y., Khan, I., Khan, S., Khan, Z., Khazanov, E. A., Kijbunchoo, N., Kim, Chunglee, Kim, J. C., Kim, Whansun, Kim, W., Kim, Y. -M, Kimbrell, S. J., King, E. J., King, P. J., Kirchhoff, R., Kissel, J. S., Klein, B., Kleybolte, L., Klimenko, S., Koch, P., Koehlenbeck, S. M., Koley, S., Kondrashov, V., Kontos, A., Korobko, M., Korth, W. Z., Kowalska, I., Kozak, D. B., Kr&quot, Amer, C., Kringel, V., Krishnan, B., Kr Olak, A., Kuehn, G., Kumar, P., Kumar, R., Kuo, L., Kutynia, A., Lackey, B. D., Landry, M., Lang, R. N., Lange, J., Lantz, B., Lanza, R. K., Lartaux-Vollard, A., Lasky, P. D., Laxen, M., Lazzarini, A., Lazzaro, C., Leaci, P., Leavey, S., Lebigot, E. O., Lee, C. H., Lee, H. K., Lee, H. M., Lee, K., Lehmann, J., Lenon, A., Leonardi, M., Leong, J. R., Leroy, N., Letendre, N., Levin, Y., Li, T. G. F., Libson, A., Littenberg, T. B., Liu, J., Lockerbie, N. A., Lombardi, A. L., London, L. T., Lord, J. E., Lorenzini, M., Loriette, V., Lormand, M., Losurdo, G., Lough, J. D., Lovelace, G., Quot, L., Uck, H., Lundgren, A. P., Lynch, R., Ma, Y., Macfoy, S., Machenschalk, B., Macinnis, M., Macleod, D. M., Magana-Sandoval, F., Majorana, E., Maksimovic, I., Malvezzi, V., Man, N., Mandic, V., Mangano, V., Mansell, G. L., Manske, M., Mantovani, M., Marchesoni, F., Marion, F., M Arka, S., M Arka, Z., Markosyan, A. S., Maros, E., Martelli, F., Martellini, L., Martin, I. W., Martynov, D. V., Mason, K., Masserot, A., Massinger, T. 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B., Miller, J., Millhouse, M., Minenkov, Y., Ming, J., Mirshekari, S., Mishra, C., Mitra, S., Mitrofanov, V. P., Mitselmakher, G., Mittleman, R., Moggi, A., Mohan, M., Mohapatra, S. R. P., MONTANI, MATTEO, Moore, B. C., Moore, C. J., Moraru, D., Moreno, G., Morriss, S. R., Mours, B., Mow Lowry, C. M., Mueller, G., Muir, A. W., Mukherjee, Arunava, Mukherjee, D., Mukherjee, S., Mukund, N., Mullavey, A., Munch, J., Muniz, E. A. M., Murray, P. G., Mytidis, A., Napier, K., Nardecchia, I., Naticchioni, L., Nelemans, G., Nelson, T. J. N., Neri, M., Nery, M., Neunzert, A., Newport, J. M., Newton, G., Nguyen, T. T., Nielsen, A. B., Nissanke, S., Nitz, A., Noack, A., Nocera, F., Nolting, D., Normandin, M. E. N., Nuttall, L. K., Oberling, J., Ochsner, E., Oelker, E., Ogin, G. H., Oh, J. J., Oh, S. H., Ohme, F., Oliver, M., Oppermann, P., Oram, Richard J., O’Reilly, B., O’Shaughnessy, R., Ottaway, D. J., Overmier, H., Owen, B. J., Pace, A. E., Page, J., Pai, A., Pai, S. A., Palamos, J. R., Palashov, O., Palomba, C., Pal Singh, A., Pan, H., Pankow, C., Pannarale, F., Pant, B. C., Paoletti, F., Paoli, A., Papa, M. A., Paris, H. R., Parker, W., Pascucci, D., Pasqualetti, A., Passaquieti, R., Passuello, D., Patricelli, B., Pearlstone, B. L., Pedraza, M., Pedurand, R., Pekowsky, L., Pele, A., Penn, S., Perez, C. J., Perreca, A., Perri, L. M., Pfeiffer, H. P., Phelps, M., Piccinni, O. J., Pichot, M., PIERGIOVANNI, FRANCESCO, Pierro, V., Pillant, G., Pinard, L., Pinto, I. M., Pitkin, M., Poe, M., Poggiani, R., Popolizio, P., Post, A., Powell, J., Prasad, J., Pratt, J. W. W., Predoi, V., Prestegard, T., Prijatelj, M., Principe, M., Privitera, S., Prodi, G. A., Prokhorov, L. G., Puncken, O., Punturo, M., Puppo, P., Pürrer, M., Qi, H., Qin, J., Qiu, S., Quetschke, V., Quintero, E. A., Quitzow James, R., Raab, F. J., Rabeling, D. S., Radkins, H., Raffai, P., Raja, S., Rajan, C., Rakhmanov, M., Rapagnani, P., Raymond, V., Razzano, M., Re, V., Read, J., Regimbau, T., Rei, L., Reid, S., Reitze, D. H., Rew, H., Reyes, S. D., Rhoades, E., Ricci, F., Riles, K., Rizzo, M., Robertson, N. A., Robie, R., Robinet, F., Rocchi, A., Rolland, L., Rollins, J. G., Roma, V. J., Romano, R., Romie, J. H., Rosińska, D., Rowan, S., Rüdiger, A., Ruggi, P., Ryan, K., Sachdev, S., Sadecki, T., Sadeghian, L., Sakellariadou, M., Salconi, L., Saleem, M., Salemi, F., Samajdar, A., Sammut, L., Sampson, L. M., Sanchez, E. J., Sandberg, V., Sanders, J. R., Sassolas, B., Sathyaprakash, B. S., Saulson, P. R., Sauter, O., Savage, R. L., Sawadsky, A., Schale, P., Scheuer, J., Schmidt, E., Schmidt, J., Schmidt, P., Schnabel, R., Schofield, R. M. S., Schönbeck, A., Schreiber, E., Schuette, D., Schwalbe, S. G., Scott, J., Scott, S. M., Sellers, D., Sengupta, A. S., Sentenac, D., Sequino, V., Sergeev, A., Setyawati, Y., Shaddock, D. A., Shaffer, T. J., Shahriar, M. S., Shapiro, B., Shawhan, P., Sheperd, A., Shoemaker, D. H., Shoemaker, D. M., Siellez, K., Siemens, X., Sieniawska, M., Sigg, D., Silva, A. D., Singer, A., Singer, L. P., Singh, A., Singh, R., Singhal, A., Sintes, A. M., Slagmolen, B. J. J., Smith, B., Smith, J. R., Smith, R. J. E., Son, E. J., Sorazu, B., Sorrentino, F., Souradeep, T., Spencer, A. P., Srivastava, A. K., Staley, A., Steinke, M., Steinlechner, J., Steinlechner, S., Steinmeyer, D., Stephens, B. C., Stevenson, S. P., Stone, R., Strain, K. A., Straniero, N., STRATTA, MARIA GIULIANA, Strigin, S. E., Sturani, R., Stuver, A. L., Summerscales, T. Z., Sun, L., Sunil, S., Sutton, P. J., Swinkels, B. L., Szczepańczyk, M. J., Szolgyen, A., Tacca, M., Talukder, D., Tanner, D. B., Tápai, M., Taracchini, A., Taylor, R., Theeg, T., Thomas, E. G., Thomas, M., Thomas, P., Thorne, K. A., Thrane, E., Tippens, T., Tiwari, S., Tiwari, V., Tokmakov, K. V., Toland, K., Tomlinson, C., Tonelli, M., Tornasi, Z., Torrie, C. I., Töyrä, D., Travasso, F., Traylor, G., Trifirò, D., Trinastic, J., Tringali, M. C., Trozzo, L., Tse, M., Tso, R., Turconi, M., Tuyenbayev, D., Ugolini, D., Unnikrishnan, C. S., Urban, A. L., Usman, S. A., Vahlbruch, H., Vajente, G., Valdes, G., Bakel, N. van, Beuzekom, M. van, Brand, J. F. J. van den, Broeck, C. Van Den, Vander Hyde, D. C., Schaaf, L. van der, Heijningen, J. V. van, Veggel, A. A. van, Vardaro, M., Varma, V., Vass, S., Vasúth, M., Vecchio, A., Vedovato, G., Veitch, J., Veitch, P. J., Venkateswara, K., Venugopalan, G., Verkindt, D., VETRANO, FLAVIO, VICERE', ANDREA, Viets, A. D., Vinciguerra, S., Vine, D. J., Vinet, J. Y., Vitale, S., Vo, T., Vocca, H., Vorvick, C., Voss, D. V., Vousden, W. D., Vyatchanin, S. P., Wade, A. R., Wade, L. E., Wade, M., Walker, M., Wallace, L., Walsh, S., Wang, G., Wang, H., Wang, M., Wang, Y., Ward, R. L., Warner, J., Was, M., Watchi, J., Weaver, B., Wei, L. W., Weinert, M., Weinstein, A. J., Weiss, R., Wen, L., Weßels, P., Westphal, T., Wette, K., Whelan, J. T., Whiting, B. F., Whittle, C., Williams, D., Williams, R. D., Williamson, A. R., Willis, J. L., Willke, B., Wimmer, M. H., Winkler, W., Wipf, C. C., Wittel, H., Woan, G., Woehler, J., Worden, J., Wright, J. L., Wu, D. S., Wu, G., Yam, W., Yamamoto, H., Yancey, C. C., Yap, M. J., Yu, Hang, Yu, Haocun, Yvert, M., Zadrożny, A., Zangrando, L., Zanolin, M., Zendri, J. P., Zevin, M., Zhang, L., Zhang, M., Zhang, T., Zhang, Y., Zhao, C., Zhou, M., Zhou, Z., Zhu, X. J., Zucker, M. E., Zweizig, J., Aptekar, R. L., Frederiks, D. D., Golenetskii, S. V., Golovin, D. V., Hurley, K., Litvak, M. L., Mitrofanov, I. G., Rau, A., Sanin, A. B., Svinkin, D. S., Kienlin, A. von, Zhang, X., (Astro)-Particles Physics, AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Astrophysique Relativiste Théories Expériences Métrologie Instrumentation Signaux (ARTEMIS), Université Nice Sophia Antipolis (1965 - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Institut de Physique de Rennes (IPR), Université de Rennes (UR)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Kastler Brossel (LKB (Lhomond)), Fédération de recherche du Département de physique de l'Ecole Normale Supérieure - ENS Paris (FRDPENS), École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Kastler Brossel (LKB (Jussieu)), Laboratoire des matériaux avancés (LMA), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), LIGO, VIRGO, IPN, AstroParticule et Cosmologie ( APC - UMR 7164 ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ), Astrophysique Relativiste Théories Expériences Métrologie Instrumentation Signaux ( ARTEMIS ), Université Nice Sophia Antipolis ( UNS ), Université Côte d'Azur ( UCA ) -Université Côte d'Azur ( UCA ) -Institut national des sciences de l'Univers ( INSU - CNRS ) -Observatoire de la Côte d'Azur, Université Côte d'Azur ( UCA ) -Centre National de la Recherche Scientifique ( CNRS ), Institut de Physique de Rennes ( IPR ), Université de Rennes 1 ( UR1 ), Université de Rennes ( UNIV-RENNES ) -Université de Rennes ( UNIV-RENNES ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire Kastler Brossel ( LKB (Lhomond) ), Fédération de recherche du Département de physique de l'Ecole Normale Supérieure - ENS Paris ( FRDPENS ), Centre National de la Recherche Scientifique ( CNRS ) -École normale supérieure - Paris ( ENS Paris ) -Centre National de la Recherche Scientifique ( CNRS ) -École normale supérieure - Paris ( ENS Paris ) -Université Pierre et Marie Curie - Paris 6 ( UPMC ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire Kastler Brossel ( LKB (Jussieu) ), Laboratoire des matériaux avancés ( LMA ), Université Claude Bernard Lyon 1 ( UCBL ), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire de l'Accélérateur Linéaire ( LAL ), Université Paris-Sud - Paris 11 ( UP11 ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire d'Annecy de Physique des Particules ( LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules ), Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Savoie Mont Blanc ( USMB [Université de Savoie] [Université de Chambéry] ) -Centre National de la Recherche Scientifique ( CNRS ), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Centre National de la Recherche Scientifique (CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Nice Sophia Antipolis (... - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA), Université de Rennes 1 (UR1), Université de Rennes (UNIV-RENNES)-Université de Rennes (UNIV-RENNES)-Centre National de la Recherche Scientifique (CNRS), Université Pierre et Marie Curie - Paris 6 (UPMC)-Fédération de recherche du Département de physique de l'Ecole Normale Supérieure - ENS Paris (FRDPENS), Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon, Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Université Nice Sophia Antipolis (... - 2019) (UNS), Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS Paris)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS Paris)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Centre National de la Recherche Scientifique (CNRS), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy de Physique des Particules (LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules), CALTECH, Louisiana State Univ, Amer Univ, Univ Salerno, Complesso Univ Monte S Angelo, Univ Florida, LIGO Livingston Observ, Univ Savoie Mont Blanc, Univ Sannio Benevento, Ist Nazl Fis Nucl, Max Planck Inst Gravitat Phys, Nikhef, MIT, Inst Nacl Pesquisas Espaciais, Interuniv Ctr Astron & Astrophys, Tata Inst Fundamental Res, Univ Wisconsin, Leibniz Univ Hannover, Univ Pisa, Australian Natl Univ, Calif State Univ Fullerton, Univ Paris 11, Chennai Math Inst, Univ Roma Tor Vergata, Univ Hamburg, Universidade de São Paulo (USP), West Virginia Univ, Univ Perugia, EGO, Syracuse Univ, Univ Glasgow, LIGO Hanford Observ, Wigner RCP, Columbia Univ, Stanford Univ, Univ Padua, MTA Eotvos Univ, Polish Acad Sci, Georgia Inst Technol, Univ Birmingham, Univ Genoa, RRCAT, Lomonosov Moscow State Univ, Univ West Scotland, Caltech CaRT, Univ Western Australia, Radboud Univ Nijmegen, Univ Cote Azur, Univ Rennes 1, Washington State Univ, Univ Urbino Carlo Bo, Univ Oregon, UPMC Sorbonne Univ, Carleton Coll, Astron Observ Warsaw Univ, Vrije Univ Amsterdam, Univ Maryland, CNRS, Univ Claude Bernard Lyon 1, Univ Napoli Federico II, NASA, Univ Tokyo, Univ Adelaide, Tsinghua Univ, Texas Tech Univ, Univ Mississippi, Penn State Univ, Natl Tsing Hua Univ, Charles Sturt Univ, Univ Chicago, Kenyon Coll, Korea Inst Sci & Technol Informat, Univ Cambridge, Univ Roma La Sapienza, Univ Brussels, Sonoma State Univ, Montana State Univ, Northwestern Univ, Univ Illes Balears, Univ Texas Rio Grande Valley, Bellevue Coll, Inst Plasma Res, Univ Sheffield, Univ Trento, Cardiff Univ, Montclair State Univ, Natl Astron Observ Japan, Univ Toronto, Univ & Inst Adv Res, IISER TVM, Univ Szeged, Embry Riddle Aeronaut Univ, Osserv Astron Capodimonte, Univ Michigan, Rochester Inst Technol, Univ Illinois, Univ Bialystok, Univ Strathclyde, Univ Southampton, Inst Appl Phys, Seoul Natl Univ, Inje Univ Gimhae, Natl Inst Math Sci, Pusan Natl Univ, NCBJ, Monash Univ, Hanyang Univ, Chinese Univ Hong Kong, Univ Alabama, Univ Minnesota, Univ Camerino, Southern Univ & A&M Coll, Univ Melbourne, Coll William & Mary, Universidade Estadual Paulista (Unesp), Whitman Coll, Univ Lyon, Hobart & William Smith Coll, Univ Zielona Gora, Univ London, IISER Kolkata, Indian Inst Technol, Andrews Univ, Univ Siena, Trinity Univ, Univ Washington, Abilene Christian Univ, Ioffe Inst, Russian Acad Sci, Univ Calif Berkeley, Max Planck Inst Extraterr Phys, The LIGO Scientific Collaboration, The Virgo Collaboration, IPN Collaboration, Branchesi, M., Calloni, Enrico, Baiardi, L. Cerboni, DE LAURENTIS, Martina, DE ROSA, Rosario, DI GIROLAMO, Tristano, Garufi, Fabio, Greco, G., Guidi, G. M., Harms, J., Martelli, F., Milano, Leopoldo, Montani, M., Piergiovanni, F., Stratta, G., Vetrano, F., and Viceré, A.
Subjects: Gravitational Waves, LIGO, O1, GRB, [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], close [binaries], BAND FOLLOW-UP, Astrophysics::High Energy Astrophysical Phenomena, gamma-ray burst: general, FOS: Physical sciences, EXTENDED EMISSION, Gravitational Wave, General Relativity and Quantum Cosmology (gr-qc), Astrophysics::Cosmology and Extragalactic Astrophysics, general [gamma-ray burst], General Relativity and Quantum Cosmology, O1, [ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], Binaries: close, gravitational waves, LIGO, close, gamma-ray burst: general, gravitational waves [binaries], QC, MASS-DISTRIBUTION, QB, High Energy Astrophysical Phenomena (astro-ph.HE), COOLED ACCRETION DISKS, UNUSUAL SUPERNOVA, binaries: close, [ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Astronomy and Astrophysics, GRB, EQUATION-OF-STATE, Physics and Astronomy, DOUBLE NEUTRON-STARS, Space and Planetary Science, BLACK-HOLE, [PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], PRECURSOR ACTIVITY, RELATIVISTIC JETS, Astrophysics - High Energy Astrophysical Phenomena
Abstract: We present the results of the search for gravitational waves (GWs) associated with $\gamma$-ray bursts detected during the first observing run of the Advanced Laser Interferometer Gravitational-Wave Observatory (LIGO). We find no evidence of a GW signal for any of the 41 $\gamma$-ray bursts for which LIGO data are available with sufficient duration. For all $\gamma$-ray bursts, we place lower bounds on the distance to the source using the optimistic assumption that GWs with an energy of $10^{-2}M_\odot c^2$ were emitted within the $16$-$500\,$Hz band, and we find a median 90% confidence limit of 71$\,$Mpc at 150$\,$Hz. For the subset of 19 short/hard $\gamma$-ray bursts, we place lower bounds on distance with a median 90% confidence limit of 90$\,$Mpc for binary neutron star (BNS) coalescences, and 150 and 139$\,$Mpc for neutron star-black hole coalescences with spins aligned to the orbital angular momentum and in a generic configuration, respectively. These are the highest distance limits ever achieved by GW searches. We also discuss in detail the results of the search for GWs associated with GRB 150906B, an event that was localized by the InterPlanetary Network near the local galaxy NGC 3313, which is at a luminosity distance of 54$\,$Mpc ($z=0.0124$). Assuming the $\gamma$-ray emission is beamed with a jet half-opening angle $\leq 30^{\circ}$, we exclude a BNS and a neutron star-black hole in NGC 3313 as the progenitor of this event with confidence $>99$%. Further, we exclude such progenitors up to a distance of 102$\,$Mpc and 170$\,$Mpc, respectively., Comment: 18 pages, 6 figures, 3 tables
Published: 2017

9. K2-99: a subgiant hosting a transiting warm Jupiter in an eccentric orbit and a long-period companion

Author: Teriyuki Hirano, V. Wolthoff, Roi Alonso, A. P. Hatzes, Sz. Csizmadia, Norio Narita, Marshall C. Johnson, Felice Cusano, Judith Korth, Brendan P. Bowler, Juan Cabrera, Eike W. Guenther, Enric Palle, Heike Rauer, Simon Albrecht, Hans J. Deeg, Anders Erikson, Ph. Eigmüller, Michael Endl, Brandon Tingley, David Nespral, Andrew W. Mann, Alexis M. S. Smith, Martin Pätzold, Davide Gandolfi, Grzegorz Nowak, Jorge Prieto-Arranz, Sascha Grziwa, William D. Cochran, D. Hidalgo, Malcolm Fridlund, Oscar Barragán, Ignasi Ribas, ITA, USA, GBR, DEU, and ESP
Subjects: Extrasolare Planeten und Atmosphären, planets and satellites: detection, planets and satellites: individual: EPIC 212803289, 010504 meteorology & atmospheric sciences, detection [planets and satellites], KEPLER, FOS: Physical sciences, Orbital eccentricity, Astrophysics, individual: K2-99 [planets and satellites], 01 natural sciences, PLANET-PLANET INTERACTIONS, Eccentric Jupiter, Planet, 0103 physical sciences, Hot Jupiter, 010303 astronomy & astrophysics, 0105 earth and related environmental sciences, BROWN DWARF DESERT, MASS-DISTRIBUTION, Physics, LIGHT CURVES, Earth and Planetary Astrophysics (astro-ph.EP), planets and satellites: individual: K2-99, SOLAR-TYPE STARS, RADIAL-VELOCITY, planetary Systems, Subgiant, Astronomy, Astronomy and Astrophysics, HOT-JUPITERS, Planetary system, planetary system, Exoplanet, Radial velocity, GIANT PLANETS, Space and Planetary Science, EXTRASOLAR PLANETS, Astrophysics - Earth and Planetary Astrophysics
Abstract: We report the discovery from K2 of a transiting planet in an 18.25-d, eccentric (0.19$\pm$ 0.04) orbit around K2-99, an 11th magnitude subgiant in Virgo. We confirm the planetary nature of the companion with radial velocities, and determine that the star is a metal-rich ([Fe/H] = 0.20$\pm$0.05) subgiant, with mass $1.60^{+0.14}_{-0.10}~M_\odot$ and radius $3.1\pm 0.1~R_\odot$. The planet has a mass of $0.97\pm0.09~M_{\rm Jup}$ and a radius $1.29\pm0.05~R_{\rm Jup}$. A measured systemic radial acceleration of $-2.12\pm0.04~{\rm m s^{-1} d^{-1}}$ offers compelling evidence for the existence of a third body in the system, perhaps a brown dwarf orbiting with a period of several hundred days., 10 pages, 6 figures, 4 tables, accepted for publication in MNRAS
Published: 2017

10. Upper Limits On The Rates Of Binary Neutron Star And Neutron Star-Black Hole Mergers From Advanced Ligo's First Observing Run

Author: Ligo, The Scientific Collaboration, the Virgo Collaboration, Abbott, B. P., Abbott, R., Abbott, T. D., Abernathy, M. R., Acernese, F., Ackley, K., Adams, C., Adams, T., Addesso, P., Adhikari, R. X., Adya, V. B., Affeldt, C., Agathos, M., Agatsuma, K., Aggarwal, N., Aguiar, O. D., Aiello, L., Ain, A., Ajith, P., Allen, B., Allocca, A., Altin, P. A., Anderson, S. B., Anderson, W. G., Arai, K., Araya, M. C., Arceneaux, C. C., Areeda, J. S., Arnaud, N., Arun, K. G., Ascenzi, S., Ashton, G., Ast, M., Aston, S. M., Astone, P., Aufmuth, P., Aulbert, C., Babak, S., Bacon, P., Bader, M. K. M., Baker, P. T., Baldaccini, F., Ballardin, G., Ballmer, S. W., Barayoga, J. C., Barclay, S. E., Barish, B. C., Barker, D., Barone, F., Barr, B., Barsotti, L., Barsuglia, M., Barta, D., Bartlett, J., Bartos, I., Bassiri, R., Basti, A., Batch, J. C., Baune, C., Bavigadda, V., Bazzan, M., Bejger, M., Bell, A. S., Berger, B. K., Bergmann, G., Berry, C. P. L., Bersanetti, D., Bertolini, A., Betzwieser, J., Bhagwat, S., Bhandare, R., Bilenko, I. A., Billingsley, G., Birch, J., Birney, R., Biscans, S., Bisht, A., Bitossi, M., Biwer, C., Bizouard, M. A., Blackburn, J. K., Blair, C. D., Blair, D. G., Blair, R. M., Bloemen, S., Bock, O., Boer, M., Bogaert, G., Bogan, C., Bohe, A., Bond, C., Bondu, F., Bonnand, R., Boom, B. A., Bork, R., Boschi, V., Bose, S., Bouffanais, Y., Bozzi, A., Bradaschia, C., Brady, P. R., Braginsky, V. B., Branchesi, M., Brau, J. E., Briant, T., Brillet, A., Brinkmann, M., Brisson, V., Brockill, P., Broida, J. E., Brooks, A. F., Brown, D. A., Brown, D. D., Brown, N. M., Brunett, S., Buchanan, C. C., Buikema, A., Bulik, T., Bulten, H. J., Buonanno, A., Buskulic, D., Buy, C., Byer, R. L., Cabero, M., Cadonati, L., Cagnoli, G., Cahillane, C., Calder On Bustillo, J., Callister, T., Calloni, E., Camp, J. B., Cannon, K. C., Cao, J., Capano, C. D., Capocasa, E., Carbognani, F., Caride, S., Casanueva Diaz, J., Casentini, C., Caudill, S., Cavagli A, M., Cavalier, F., Cavalieri, R., Cella, G., Cepeda, C. B., Cerboni Baiardi, L., Cerretani, G., Cesarini, E., Chamberlin, S. J., Chan, M., Chao, S., Charlton, P., Chassande-Mottin, E., Cheeseboro, B. D., Chen, H. Y., Chen, Y., Cheng, C., Chincarini, A., Chiummo, A., Cho, H. S., Cho, M., Chow, J. H., Christensen, N., Chu, Q., Chua, S., Chung, S., Ciani, G., Clara, F., Clark, J. A., Cleva, F., Coccia, E., Cohadon, P. -F, Colla, A., Collette, C. G., Cominsky, L., Constancio, M., Conte, A., Conti, L., Cook, D., Corbitt, T. R., Cornish, N., Corsi, A., Cortese, S., Costa, C. A., Coughlin, M. W., Coughlin, S. B., Coulon, J. -P, Countryman, S. T., Couvares, P., Cowan, E. E., Coward, D. M., Cowart, M. J., Coyne, D. C., Coyne, R., Craig, K., Creighton, J. D. E., Cripe, J., Crowder, S. G., Cumming, A., Cunningham, L., Cuoco, E., Dal Canton, T., Danilishin, S. L., D Antonio, S., Danzmann, K., Darman, N. S., Dasgupta, A., Da Silva Costa, C. F., Dattilo, V., Dave, I., Davier, M., Davies, G. S., Daw, E. J., Day, R., De, S., Debra, D., Debreczeni, G., Degallaix, J., Laurentis, M., Del Eglise, S., Del Pozzo, W., Denker, T., Dent, T., Dergachev, V., Rosa, R., Derosa, R. T., Desalvo, R., Devine, R. C., Dhurandhar, S., D Iaz, M. C., Di Fiore, L., Di Giovanni, M., Di Girolamo, T., Di Lieto, A., Di Pace, S., Di Palma, I., Di Virgilio, A., Dolique, V., Donovan, F., Dooley, K. L., Doravari, S., Douglas, R., Downes, T. P., Drago, M., Drever, R. W. P., Driggers, J. C., Ducrot, M., Dwyer, S. E., Edo, T. B., Edwards, M. C., Effler, A., Eggenstein, H. -B, Ehrens, P., Eichholz, J., Eikenberry, S. S., Engels, W., Essick, R. C., Etzel, T., Evans, M., Evans, T. M., Everett, R., Factourovich, M., Fafone, V., Fair, H., Fairhurst, S., Fan, X., Fang, Q., Farinon, S., Farr, B., Farr, W. M., Favata, M., Fays, M., Fehrmann, H., Fejer, M. M., Fenyvesi, E., Ferrante, I., Ferreira, E. C., Ferrini, F., Fidecaro, F., Fiori, I., Fiorucci, D., Fisher, R. P., Flaminio, R., Fletcher, M., Fournier, J. -D, Frasca, S., Frasconi, F., Frei, Z., Freise, A., Frey, R., Frey, V., Fritschel, P., Frolov, V. V., Fulda, P., Fyffe, M., Gabbard, H. A. G., Gair, J. R., Gammaitoni, L., Gaonkar, S. G., Garufi, F., Gaur, G., Gehrels, N., Gemme, G., Geng, P., Genin, E., Gennai, A., George, J., Gergely, L., Germain, V., Ghosh, Abhirup, Ghosh, Archisman, Ghosh, S., Giaime, J. A., Giardina, K. D., Giazotto, A., Gill, K., Glaefke, A., Goetz, E., Goetz, R., Gondan, L., Gonz Alez, G., Gonzalez Castro, J. M., Gopakumar, A., Gordon, N. A., Gorodetsky, M. L., Gossan, S. E., Gosselin, M., Gouaty, R., Grado, A., Graef, C., Graff, P. B., Granata, M., Grant, A., Gras, S., Gray, C., Greco, G., Green, A. C., Paul Groot, Grote, H., Grunewald, S., Guidi, G. M., Guo, X., Gupta, A., Gupta, M. K., Gushwa, K. E., Gustafson, E. K., Gustafson, R., Hacker, J. J., Hall, B. R., Hall, E. D., Hammond, G., Haney, M., Hanke, M. M., Hanks, J., Hanna, C., Hannam, M. D., Hanson, J., Hardwick, T., Harms, J., Harry, G. M., Harry, I. W., Hart, M. J., Hartman, M. T., Haster, C. -J, Haughian, K., Heidmann, A., Heintze, M. C., Heitmann, H., Hello, P., Hemming, G., Hendry, M., Heng, I. S., Hennig, J., Henry, J., Heptonstall, A. W., Heurs, M., Hild, S., Hoak, D., Hofman, D., Holt, K., Holz, D. E., Hopkins, P., Hough, J., Houston, E. A., Howell, E. J., Hu, Y. M., Huang, S., Huerta, E. A., Huet, D., Hughey, B., Husa, S., Huttner, S. H., Huynh-Dinh, T., Indik, N., Ingram, D. R., Inta, R., Isa, H. N., Isac, J. -M, Isi, M., Isogai, T., Iyer, B. R., Izumi, K., Jacqmin, T., Jang, H., Jani, K., Jaranowski, P., Jawahar, S., Jian, L., Jim Enez-Forteza, F., Johnson, W. W., Jones, D. I., Jones, R., Jonker, R. J. G., Ju, L., K, Haris, Kalaghatgi, C. V., Kalogera, V., Kandhasamy, S., Kang, G., Kanner, J. B., Kapadia, S. J., Karki, S., Karvinen, K. S., Kasprzack, M., Katsavounidis, E., Katzman, W., Kaufer, S., Kaur, T., Kawabe, K., K Ef Elian, F., Kehl, M. S., Keitel, D., Kelley, D. B., Kells, W., Kennedy, R., Key, J. S., Khalili, F. Y., Khan, I., Khan, S., Khan, Z., Khazanov, E. A., Kijbunchoo, N., Kim, Chi-Woong, Kim, Chunglee, Kim, J., Kim, K., Kim, N., Kim, W., Kim, Y. -M, Kimbrell, S. J., King, E. J., King, P. J., Kissel, J. S., Klein, B., Kleybolte, L., Klimenko, S., Koehlenbeck, S. M., Koley, S., Kondrashov, V., Kontos, A., Korobko, M., Korth, W. Z., Kowalska, I., Kozak, D. B., Kringel, V., Krishnan, B., Kr Olak, A., Krueger, C., Kuehn, G., Kumar, P., Kumar, R., Kuo, L., Kutynia, A., Lackey, B. D., Landry, M., Lange, J., Lantz, B., Lasky, P. D., Laxen, M., Lazzarini, A., Lazzaro, C., Leaci, P., Leavey, S., Lebigot, E. O., Lee, C. H., Lee, H. K., Lee, H. M., Lee, K., Lenon, A., Leonardi, M., Leong, J. R., Leroy, N., Letendre, N., Levin, Y., Lewis, J. B., Li, T. G. F., Libson, A., Littenberg, T. B., Lockerbie, N. A., Lombardi, A. L., London, L. T., Lord, J. E., Lorenzini, M., Loriette, V., Lormand, M., Losurdo, G., Lough, J. D., Quot, L., Uck, H., Lundgren, A. P., Lynch, R., Ma, Y., Machenschalk, B., Macinnis, M., Macleod, D. M., Magana-Sandoval, F., Magana Zertuche, L., Magee, R. M., Majorana, E., Maksimovic, I., Malvezzi, V., Man, N., Mandic, V., Mangano, V., Mansell, G. L., Manske, M., Mantovani, M., Marchesoni, F., Marion, F., M Arka, S., M Arka, Z., Markosyan, A. S., Maros, E., Martelli, F., Martellini, L., Martin, I. W., Martynov, D. V., Marx, J. N., Mason, K., Masserot, A., Massinger, T. J., Masso-Reid, M., Mastrogiovanni, S., Matichard, F., Matone, L., Mavalvala, N., Mazumder, N., Mccarthy, R., Mcclelland, D. E., Mccormick, S., Mcguire, S. C., Mcintyre, G., Mciver, J., Mcmanus, D. J., Mcrae, T., Mcwilliams, S. T., Meacher, D., Meadors, G. D., Meidam, J., Melatos, A., Mendell, G., Mercer, R. A., Merilh, E. L., Merzougui, M., Meshkov, S., Messenger, C., Messick, C., Metzdorff, R., Meyers, P. M., Mezzani, F., Miao, H., Michel, C., Middleton, H., Mikhailov, E. E., Milano, L., Miller, A. L., Miller, A., Miller, B. B., Miller, J., Millhouse, M., Minenkov, Y., Ming, J., Mirshekari, S., Mishra, C., Mitra, S., Mitrofanov, V. P., Mitselmakher, G., Mittleman, R., Moggi, A., Mohan, M., Mohapatra, S. R. P., Montani, M., Moore, B. C., Moore, C. J., Moraru, D., Moreno, G., Morriss, S. R., Mossavi, K., Mours, B., Mow-Lowry, C. M., Mueller, G., Muir, A. W., Mukherjee, Arunava, Mukherjee, D., Mukherjee, S., Mukund, N., Mullavey, A., Munch, J., Murphy, D. J., Murray, P. G., Mytidis, A., Nardecchia, I., Naticchioni, L., Nayak, R. K., Nedkova, K., Nelemans, G., Nelson, T. J. N., Neri, M., Neunzert, A., Newton, G., Nguyen, T. T., Nielsen, A. B., Nissanke, S., Nitz, A., Nocera, F., Nolting, D., Normandin, M. E. N., Nuttall, L. K., Oberling, J., Ochsner, E., O, J., Oelker, E., Ogin, G. H., Oh, J. J., Oh, S. H., Ohme, F., Oliver, M., Oppermann, P., Oram, Richard J., O Reilly, B., O Shaughnessy, R., Ottaway, D. J., Overmier, H., Owen, B. J., Pai, A., Pai, S. A., Palamos, J. R., Palashov, O., Palomba, C., Pal-Singh, A., Pan, H., Pankow, C., Pannarale, F., Pant, B. C., Paoletti, F., Paoli, A., Papa, M. A., Paris, H. R., Parker, W., Pascucci, D., Pasqualetti, A., Passaquieti, R., Passuello, D., Patricelli, B., Patrick, Z., Pearlstone, B. L., Pedraza, M., Pedurand, R., Pekowsky, L., Pele, A., Penn, S., Perreca, A., Perri, L. M., Phelps, M., Piccinni, O. J., Pichot, M., Piergiovanni, F., Pierro, V., Pillant, G., Pinard, L., Pinto, I. M., Pitkin, M., Poe, M., Poggiani, R., Popolizio, P., Post, A., Powell, J., Prasad, J., Pratt, J., Predoi, V., Prestegard, T., Price, L. R., Prijatelj, M., Principe, M., Privitera, S., Prix, R., Prodi, G. A., Prokhorov, L., Puncken, O., Punturo, M., Puppo, P., Quot, P., Urrer, M., Qi, H., Qin, J., Qiu, S., Quetschke, V., Quintero, E. A., Quitzow-James, R., Raab, F. J., Rabeling, D. S., Radkins, H., Raffai, P., Raja, S., Rajan, C., Rakhmanov, M., Rapagnani, P., Raymond, V., Razzano, M., Re, V., Read, J., Reed, C. M., Regimbau, T., Rei, L., Reid, S., Reitze, D. H., Rew, H., Reyes, S. D., Ricci, F., Riles, K., Rizzo, M., Robertson, N. A., Robie, R., Robinet, F., Rocchi, A., Rolland, L., Rollins, J. G., Roma, V. J., Romano, R., Romanov, G., Romie, J. H., Rosi Nska, D., Rowan, S., Quot, R., Udiger, A., Ruggi, P., Ryan, K., Sachdev, S., Sadecki, T., Sadeghian, L., Sakellariadou, M., Salconi, L., Saleem, M., Salemi, F., Samajdar, A., Sammut, L., Sanchez, E. J., Sandberg, V., Sandeen, B., Sanders, J. R., Sassolas, B., Sathyaprakash, B. S., Saulson, P. R., Sauter, O. E. S., Savage, R. L., Sawadsky, A., Schale, P., Schilling, R., Schmidt, J., Schmidt, P., Schnabel, R., Schofield, R. M. S., Sch&quot, Onbeck, A., Schreiber, E., Schuette, D., Schutz, B. F., Scott, J., Scott, S. M., Sellers, D., Sengupta, A. S., Sentenac, D., Sequino, V., Sergeev, A., Setyawati, Y., Shaddock, D. A., Shaffer, T., Shahriar, M. S., Shaltev, M., Shapiro, B., Shawhan, P., Sheperd, A., Shoemaker, D. H., Shoemaker, D. M., Siellez, K., Siemens, X., Sieniawska, M., Sigg, D., Silva, A. D., Singer, A., Singer, L. P., Singh, A., Singh, R., Singhal, A., Sintes, A. M., Slagmolen, B. J. J., Smith, J. R., Smith, N. D., Smith, R. J. E., Son, E. J., Sorazu, B., Sorrentino, F., Souradeep, T., Srivastava, A. K., Staley, A., Steinke, M., Steinlechner, J., Steinlechner, S., Steinmeyer, D., Stephens, B. C., Stone, R., Strain, K. A., Straniero, N., Stratta, G., Strauss, N. A., Strigin, S., Sturani, R., Stuver, A. L., Summerscales, T. Z., Sun, L., Sunil, S., Sutton, P. J., Swinkels, B. L., Szczepa Nczyk, M. J., Tacca, M., Talukder, D., Tanner, D. B., T Apai, M., Tarabrin, S. P., Taracchini, A., Taylor, R., Theeg, T., Thirugnanasambandam, M. P., Thomas, E. G., Thomas, M., Thomas, P., Thorne, K. A., Thrane, E., Tiwari, S., Tiwari, V., Tokmakov, K. V., Toland, K., Tomlinson, C., Tonelli, M., Tornasi, Z., Torres, C. V., Torrie, C. I., Quot, T., oyr&quot, A, D., Travasso, F., Traylor, G., Trifir O, D., Tringali, M. C., Trozzo, L., Tse, M., Turconi, M., Tuyenbayev, D., Ugolini, D., Unnikrishnan, C. S., Urban, A. L., Usman, S. A., Vahlbruch, H., Vajente, G., Valdes, G., Bakel, N., Beuzekom, M., Den Brand, J. F. J., Den Broeck, C., Vander-Hyde, D. C., Schaaf, L., Heijningen, J. V., Veggel, A. A., Vardaro, M., Vass, S., Vas Uth, M., Vaulin, R., Vecchio, A., Vedovato, G., Veitch, J., Veitch, P. J., Venkateswara, K., Verkindt, D., Vetrano, F., Vicer E, A., Vinciguerra, S., Vine, D. J., Vinet, J. -Y, Vitale, S., Vo, T., Vocca, H., Vorvick, C., Voss, D. V., Vousden, W. D., Vyatchanin, S. P., Wade, A. R., Wade, L. E., Wade, M., Walker, M., Wallace, L., Walsh, S., Wang, G., Wang, H., Wang, M., Wang, X., Wang, Y., Ward, R. L., Warner, J., Was, M., Weaver, B., Wei, L. -W, Weinert, M., Weinstein, A. J., Weiss, R., Wen, L., Wessels, P., Westphal, T., Wette, K., Whelan, J. T., Whiting, B. F., Williams, R. D., Williamson, A. R., Willis, J. L., Willke, B., Wimmer, M. H., Winkler, W., Wipf, C. C., Wittel, H., Woan, G., Woehler, J., Worden, J., Wright, J. L., Wu, D. S., Wu, G., Yablon, J., Yam, W., Yamamoto, H., Yancey, C. C., Yu, H., Yvert, M., Zadro Zny, A., Zangrando, L., Zanolin, M., Zendri, J. -P, Zevin, M., Zhang, L., Zhang, M., Zhang, Y., Zhao, C., Zhou, M., Zhou, Z., Zhu, X. J., Zucker, M. E., Zuraw, S. E., Zweizig, J., Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Astrophysique Relativiste Théories Expériences Métrologie Instrumentation Signaux (ARTEMIS), Centre National de la Recherche Scientifique (CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Nice Sophia Antipolis (... - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA), Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Laboratoire des matériaux avancés (LMA), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon, VIRGO, Ligo, Abbott, B. P., Abbott, R., Abbott, T. D., Abernathy, M. R., Acernese, F., Ackley, K., Adams, C., Adams, T., Addesso, P., Adhikari, R. X., Adya, V. B., Affeldt, C., Agathos, M., Agatsuma, K., Aggarwal, N., Aguiar, O. D., Aiello, L., Ain, A., Ajith, P., Allen, B., Allocca, A., Altin, P. A., Anderson, S. B., Anderson, W. G., Arai, K., Araya, M. C., Arceneaux, C. C., Areeda, J. S., Arnaud, N., Arun, K. G., Ascenzi, S., Ashton, G., Ast, M., Aston, S. M., Astone, P., Aufmuth, P., Aulbert, C., Babak, S., Bacon, P., Bader, M. K. M., Baker, P. T., Baldaccini, F., Ballardin, G., Ballmer, S. W., Barayoga, J. C., Barclay, S. E., Barish, B. C., Barker, D., Barone, F., Barr, B., Barsotti, L., Barsuglia, M., Barta, D., Bartlett, J., Bartos, I., Bassiri, R., Basti, A., Batch, J. C., Baune, C., Bavigadda, V., Bazzan, M., Bejger, M., Bell, A. S., Berger, B. K., Bergmann, G., Berry, C. P. L., Bersanetti, D., Bertolini, A., Betzwieser, J., Bhagwat, S., Bhandare, R., Bilenko, I. A., Billingsley, G., Birch, J., Birney, R., Biscans, S., Bisht, A., Bitossi, M., Biwer, C., Bizouard, M. A., Blackburn, J. K., Blair, C. D., Blair, D. G., Blair, R. M., Bloemen, S., Bock, O., Boer, M., Bogaert, G., Bogan, C., Bohe, A., Bond, C., Bondu, F., Bonnand, R., Boom, B. A., Bork, R., Boschi, V., Bose, S., Bouffanais, Y., Bozzi, A., Bradaschia, C., Brady, P. R., Braginsky, V. B., Branchesi, M., Brau, J. E., Briant, T., Brillet, A., Brinkmann, M., Brisson, V., Brockill, P., Broida, J. E., Brooks, A. F., Brown, D. A., Brown, D. D., Brown, N. M., Brunett, S., Buchanan, C. C., Buikema, A., Bulik, T., Bulten, H. J., Buonanno, A., Buskulic, D., Buy, C., Byer, R. L., Cabero, M., Cadonati, L., Cagnoli, G., Cahillane, C., Bustillo, J. Calderón, Callister, T., Calloni, Enrico, Camp, J. B., Cannon, K. C., Cao, J., Capano, C. D., Capocasa, E., Carbognani, F., Caride, S., Diaz, J. Casanueva, Casentini, C., Caudill, S., Cavaglià, M., Cavalier, F., Cavalieri, R., Cella, G., Cepeda, C. B., Baiardi, L. Cerboni, Cerretani, G., Cesarini, E., Chamberlin, S. J., Chan, M., Chao, S., Charlton, P., Chassande Mottin, E., Cheeseboro, B. D., Chen, H. Y., Chen, Y., Cheng, C., Chincarini, A., Chiummo, A., Cho, H. S., Cho, M., Chow, J. H., Christensen, N., Chu, Q., Chua, S., Chung, S., Ciani, G., Clara, F., Clark, J. A., Cleva, F., Coccia, E., Cohadon, P. F., Colla, A., Collette, C. G., Cominsky, L., M., C. o. n. s. t. a. n. c. i. o. J. r., Conte, A., Conti, L., Cook, D., Corbitt, T. R., Cornish, N., Corsi, A., Cortese, S., Costa, C. A., Coughlin, M. W., Coughlin, S. B., Coulon, J. P., Countryman, S. T., Couvares, P., Cowan, E. E., Coward, D. M., Cowart, M. J., Coyne, D. C., Coyne, R., Craig, K., Creighton, J. D. E., Cripe, J., Crowder, S. G., Cumming, A., Cunningham, L., Cuoco, E., Canton, T. Dal, Danilishin, S. L., D’Antonio, S., Danzmann, K., Darman, N. S., Dasgupta, A., Costa, C. F. Da Silva, Dattilo, V., Dave, I., Davier, M., Davies, G. S., Daw, E. J., Day, R., De, S., Debra, D., Debreczeni, G., Degallaix, J., DE LAURENTIS, Martina, Deléglise, S., Pozzo, W. Del, Denker, T., Dent, T., Dergachev, V., Rosa, R. De, DE ROSA, Rosario, Desalvo, R., Devine, R. C., Dhurandhar, S., Díaz, M. C., Fiore, L. Di, Giovanni, M., DI GIROLAMO, Tristano, Lieto, A. Di, Pace, S. Di, Palma, I. Di, Virgilio, A. Di, Dolique, V., Donovan, F., Dooley, K. L., Doravari, S., Douglas, R., Downes, T. P., Drago, M., Drever, R. W. P., Driggers, J. C., Ducrot, M., Dwyer, S. E., Edo, T. B., Edwards, M. C., Effler, A., Eggenstein, H. B., Ehrens, P., Eichholz, J., Eikenberry, S. S., Engels, W., Essick, R. C., Etzel, T., Evans, M., Evans, T. M., Everett, R., Factourovich, M., Fafone, V., Fair, H., Fairhurst, S., Fan, X., Fang, Q., Farinon, S., Farr, B., Farr, W. M., Favata, M., Fays, M., Fehrmann, H., Fejer, M. M., Fenyvesi, E., Ferrante, I., Ferreira, E. C., Ferrini, F., Fidecaro, F., Fiori, I., Fiorucci, D., Fisher, R. P., Flaminio, R., Fletcher, M., Fournier, J. D., Frasca, S., Frasconi, F., Frei, Z., Freise, A., Frey, R., Frey, V., Fritschel, P., Frolov, V. V., Fulda, P., Fyffe, M., Gabbard, H. A. G., Gair, J. R., Gammaitoni, L., Gaonkar, S. G., Garufi, Fabio, Gaur, G., Gehrels, N., Gemme, G., Geng, P., Genin, E., Gennai, A., George, J., Gergely, L., Germain, V., Ghosh, Abhirup, Ghosh, Archisman, Ghosh, S., Giaime, J. A., Giardina, K. D., Giazotto, A., Gill, K., Glaefke, A., Goetz, E., Goetz, R., Gondan, L., González, G., Castro, J. M. Gonzalez, Gopakumar, A., Gordon, N. A., Gorodetsky, M. L., Gossan, S. E., Gosselin, M., Gouaty, R., Grado, A., Graef, C., Graff, P. B., Granata, M., Grant, A., Gras, S., Gray, C., Greco, G., Green, A. C., Groot, P., Grote, H., Grunewald, S., Guidi, G. M., Guo, X., Gupta, A., Gupta, M. K., Gushwa, K. E., Gustafson, E. K., Gustafson, R., Hacker, J. J., Hall, B. R., Hall, E. D., Hammond, G., Haney, M., Hanke, M. M., Hanks, J., Hanna, C., Hannam, M. D., Hanson, J., Hardwick, T., Harms, J., Harry, G. M., Harry, I. W., Hart, M. J., Hartman, M. T., Haster, C. J., Haughian, K., Heidmann, A., Heintze, M. C., Heitmann, H., Hello, P., Hemming, G., Hendry, M., Heng, I. S., Hennig, J., Henry, J., Heptonstall, A. W., Heurs, M., Hild, S., Hoak, D., Hofman, D., Holt, K., Holz, D. E., Hopkins, P., Hough, J., Houston, E. A., Howell, E. J., Hu, Y. M., Huang, S., Huerta, E. A., Huet, D., Hughey, B., Husa, S., Huttner, S. H., Huynh Dinh, T., Indik, N., Ingram, D. R., Inta, R., Isa, H. N., Isac, J. M., Isi, M., Isogai, T., Iyer, B. R., Izumi, K., Jacqmin, T., Jang, H., Jani, K., Jaranowski, P., Jawahar, S., Jian, L., Jiménez Forteza, F., Johnson, W. W., Jones, D. I., Jones, R., Jonker, R. J. G., Ju, L., K, Hari, Kalaghatgi, C. V., Kalogera, V., Kandhasamy, S., Kang, G., Kanner, J. B., Kapadia, S. J., Karki, S., Karvinen, K. S., Kasprzack, M., Katsavounidis, E., Katzman, W., Kaufer, S., Kaur, T., Kawabe, K., Kéfélian, F., Kehl, M. S., Keitel, D., Kelley, D. B., Kells, W., Kennedy, R., Key, J. S., Khalili, F. Y., Khan, I., Khan, S., Khan, Z., Khazanov, E. A., Kijbunchoo, N., Kim, Chi Woong, Kim, Chunglee, Kim, J., Kim, K., Kim, N., Kim, W., Kim, Y. M., Kimbrell, S. J., King, E. J., King, P. J., Kissel, J. S., Klein, B., Kleybolte, L., Klimenko, S., Koehlenbeck, S. M., Koley, S., Kondrashov, V., Kontos, A., Korobko, M., Korth, W. Z., Kowalska, I., Kozak, D. B., Kringel, V., Krishnan, B., Królak, A., Krueger, C., Kuehn, G., Kumar, P., Kumar, R., Kuo, L., Kutynia, A., Lackey, B. D., Landry, M., Lange, J., Lantz, B., Lasky, P. D., Laxen, M., Lazzarini, A., Lazzaro, C., Leaci, P., Leavey, S., Lebigot, E. O., Lee, C. H., Lee, H. K., Lee, H. M., Lee, K., Lenon, A., Leonardi, M., Leong, J. R., Leroy, N., Letendre, N., Levin, Y., Lewis, J. B., Li, T. G. F., Libson, A., Littenberg, T. B., Lockerbie, N. A., Lombardi, A. L., London, L. T., Lord, J. E., Lorenzini, M., Loriette, V., Lormand, M., Losurdo, G., Lough, J. D., Lück, H., Lundgren, A. P., Lynch, R., Ma, Y., Machenschalk, B., Macinnis, M., Macleod, D. M., Magaña Sandoval, F., Magaña Zertuche, L., Magee, R. M., Majorana, E., Maksimovic, I., Malvezzi, V., Man, N., Mandic, V., Mangano, V., Mansell, G. L., Manske, M., Mantovani, M., Marchesoni, F., Marion, F., Márka, S., Márka, Z., Markosyan, A. S., Maros, E., Martelli, F., Martellini, L., Martin, I. W., Martynov, D. V., Marx, J. N., Mason, K., Masserot, A., Massinger, T. J., Masso Reid, M., Mastrogiovanni, S., Matichard, F., Matone, L., Mavalvala, N., Mazumder, N., Mccarthy, R., Mcclelland, D. E., Mccormick, S., Mcguire, S. C., Mcintyre, G., Mciver, J., Mcmanus, D. J., Mcrae, T., Mcwilliams, S. T., Meacher, D., Meadors, G. D., Meidam, J., Melatos, A., Mendell, G., Mercer, R. A., Merilh, E. L., Merzougui, M., Meshkov, S., Messenger, C., Messick, C., Metzdorff, R., Meyers, P. M., Mezzani, F., Miao, H., Michel, C., Middleton, H., Mikhailov, E. E., Milano, Leopoldo, Miller, A. L., Miller, A., Miller, B. B., Miller, J., Millhouse, M., Minenkov, Y., Ming, J., Mirshekari, S., Mishra, C., Mitra, S., Mitrofanov, V. P., Mitselmakher, G., Mittleman, R., Moggi, A., Mohan, M., Mohapatra, S. R. P., Montani, M., Moore, B. C., Moore, C. J., Moraru, D., Moreno, G., Morriss, S. R., Mossavi, K., Mours, B., Mow Lowry, C. M., Mueller, G., Muir, A. W., Mukherjee, Arunava, Mukherjee, D., Mukherjee, S., Mukund, N., Mullavey, A., Munch, J., Murphy, D. J., Murray, P. G., Mytidis, A., Nardecchia, I., Naticchioni, L., Nayak, R. K., Nedkova, K., Nelemans, G., Nelson, T. J. N., Neri, M., Neunzert, A., Newton, G., Nguyen, T. T., Nielsen, A. B., Nissanke, S., Nitz, A., Nocera, F., Nolting, D., Normandin, M. E. N., Nuttall, L. K., Oberling, J., Ochsner, E., O’Dell, J., Oelker, E., Ogin, G. H., Oh, J. J., Oh, S. H., Ohme, F., Oliver, M., Oppermann, P., Oram, Richard J., O’Reilly, B., O’Shaughnessy, R., Ottaway, D. J., Overmier, H., Owen, B. J., Pai, A., Pai, S. A., Palamos, J. R., Palashov, O., Palomba, C., Pal Singh, A., Pan, H., Pankow, C., Pannarale, F., Pant, B. C., Paoletti, F., Paoli, A., Papa, M. A., Paris, H. R., Parker, W., Pascucci, D., Pasqualetti, A., Passaquieti, R., Passuello, D., Patricelli, B., Patrick, Z., Pearlstone, B. L., Pedraza, M., Pedurand, R., Pekowsky, L., Pele, A., Penn, S., Perreca, A., Perri, L. M., Phelps, M., Piccinni, O. J., Pichot, M., Piergiovanni, F., Pierro, V., Pillant, G., Pinard, L., Pinto, I. M., Pitkin, M., Poe, M., Poggiani, R., Popolizio, P., Post, A., Powell, J., Prasad, J., Predoi, V., Prestegard, T., Price, L. R., Prijatelj, M., Principe, M., Privitera, S., Prix, R., Prodi, G. A., Prokhorov, L., Puncken, O., Punturo, M., Puppo, P., Pürrer, M., Qi, H., Qin, J., Qiu, S., Quetschke, V., Quintero, E. A., Quitzow James, R., Raab, F. J., Rabeling, D. S., Radkins, H., Raffai, P., Raja, S., Rajan, C., Rakhmanov, M., Rapagnani, P., Raymond, V., Razzano, M., Re, V., Read, J., Reed, C. M., Regimbau, T., Rei, L., Reid, S., Reitze, D. H., Rew, H., Reyes, S. D., Ricci, F., Riles, K., Rizzo, M., Robertson, N. A., Robie, R., Robinet, F., Rocchi, A., Rolland, L., Rollins, J. G., Roma, V. J., Romano, R., Romanov, G., Romie, J. H., Rosińska, D., Rowan, S., Rüdiger, A., Ruggi, P., Ryan, K., Sachdev, S., Sadecki, T., Sadeghian, L., Sakellariadou, M., Salconi, L., Saleem, M., Salemi, F., Samajdar, A., Sammut, L., Sanchez, E. J., Sandberg, V., Sandeen, B., Sanders, J. R., Sassolas, B., Sathyaprakash, B. S., Saulson, P. R., Sauter, O. E. S., Savage, R. L., Sawadsky, A., Schale, P., Schilling, R., Schmidt, J., Schmidt, P., Schnabel, R., Schofield, R. M. S., Schönbeck, A., Schreiber, E., Schuette, D., Schutz, B. F., Scott, J., Scott, S. M., Sellers, D., Sengupta, A. S., Sentenac, D., Sequino, V., Sergeev, A., Setyawati, Y., Shaddock, D. A., Shaffer, T., Shahriar, M. S., Shaltev, M., Shapiro, B., Shawhan, P., Sheperd, A., Shoemaker, D. H., Shoemaker, D. M., Siellez, K., Siemens, X., Sieniawska, M., Sigg, D., Silva, A. D., Singer, A., Singer, L. P., Singh, A., Singh, R., Singhal, A., Sintes, A. M., Slagmolen, B. J. J., Smith, J. R., Smith, N. D., Smith, R. J. E., Son, E. J., Sorazu, B., Sorrentino, F., Souradeep, T., Srivastava, A. K., Staley, A., Steinke, M., Steinlechner, J., Steinlechner, S., Steinmeyer, D., Stephens, B. C., Stone, R., Strain, K. A., Straniero, N., Stratta, G., Strauss, N. A., Strigin, S., Sturani, R., Stuver, A. L., Summerscales, T. Z., Sun, L., Sunil, S., Sutton, P. J., Swinkels, B. L., Szczepańczyk, M. J., Tacca, M., Talukder, D., Tanner, D. B., Tápai, M., Tarabrin, S. P., Taracchini, A., Taylor, R., Theeg, T., Thirugnanasambandam, M. P., Thomas, E. G., Thomas, M., Thomas, P., Thorne, K. A., Thrane, E., Tiwari, S., Tiwari, V., Tokmakov, K. V., Toland, K., Tomlinson, C., Tonelli, M., Tornasi, Z., Torres, C. V., Torrie, C. I., Töyrä, D., Travasso, F., Traylor, G., Trifirò, D., Tringali, M. C., Trozzo, L., Tse, M., Turconi, M., Tuyenbayev, D., Ugolini, D., Unnikrishnan, C. S., Urban, A. L., Usman, S. A., Vahlbruch, H., Vajente, G., Valdes, G., Bakel, N. van, Beuzekom, M. van, van den Brand, J. F. J., Broeck, C. Van Den, Vander Hyde, D. C., Schaaf, L. van der, Heijningen, J. V. van, Veggel, A. A. van, Vardaro, M., Vass, S., Vasúth, M., Vaulin, R., Vecchio, A., Vedovato, G., Veitch, J., Veitch, P. J., Venkateswara, K., Verkindt, D., Vetrano, F., Viceré, A., Vinciguerra, S., Vine, D. J., Vinet, J. Y., Vitale, S., Vo, T., Vocca, H., Vorvick, C., Voss, D. V., Vousden, W. D., Vyatchanin, S. P., Wade, A. R., Wade, L. E., Wade, M., Walker, M., Wallace, L., Walsh, S., Wang, G., Wang, H., Wang, M., Wang, X., Wang, Y., Ward, R. L., Warner, J., Was, M., Weaver, B., Wei, L. W., Weinert, M., Weinstein, A. J., Weiss, R., Wen, L., Weßels, P., Westphal, T., Wette, K., Whelan, J. T., Whiting, B. F., Williams, R. D., Williamson, A. R., Willis, J. L., Willke, B., Wimmer, M. 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Subjects: Astronomy, gamma-ray burst: general, Astrophysics, general [gamma-ray burst], 01 natural sciences, General Relativity and Quantum Cosmology, general [binaries], Astrophysics::Solar and Stellar Astrophysics, binaries: general, gravitational waves, stars: black holes, stars: neutron, astro-ph.HE, astro-ph.CO, Astronomy and Astrophysics, Space and Planetary Science, LIGO, 010303 astronomy & astrophysics, GeneralLiterature_REFERENCE(e.g.,dictionaries,encyclopedias,glossaries), QC, POPULATION, QB, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), GAMMA-RAY BURSTS, Settore FIS/01 - Fisica Sperimentale, SPIN, ACCRETION DISK, [PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], Astrophysics::Earth and Planetary Astrophysics, Binary Neutron Star, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Cosmology and Nongalactic Astrophysics, [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Cosmology and Nongalactic Astrophysics (astro-ph.CO), Star (game theory), gr-qc, Astrophysics::High Energy Astrophysical Phenomena, Neutron Star and Black Hole, FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), Astrophysics::Cosmology and Extragalactic Astrophysics, GRAVITATIONAL-WAVE DETECTION, [ PHYS.ASTR.CO ] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], O1, [ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], MAXIMUM MASS, neutron [stars], Settore FIS/05 - Astronomia e Astrofisica, 0103 physical sciences, black holes [stars], Sensitivity (control systems), LIGO, O1, Binary Neutron Star, Neutron Star and Black Hole, STFC, Astrophysics::Galaxy Astrophysics, MASS-DISTRIBUTION, RADIO, EXPLOSION, 010308 nuclear & particles physics, Gravitational wave, RCUK, [ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Black hole, Neutron star, Physics and Astronomy, HOST GALAXY, Binaries: general, Gamma-ray burst, Dimensionless quantity
Abstract: © 2016 The American Astronomical Society. This is the publisher Version of Record Manuscript. Please refer to any applicable publisher terms of use., We report here the non-detection of gravitational waves from the merger of binary–neutron star systems and neutron star–black hole systems during the first observing run of the Advanced Laser Interferometer Gravitationalwave Observatory (LIGO). In particular, we searched for gravitational-wave signals from binary–neutron star systems with component masses Î[ ] 1, 3 M and component dimensionless spins
Published: 2016

11. Binary Black Hole Mergers in the First Advanced LIGO Observing Run

Subjects: MAXIMUM MASS, COMMON ENVELOPE, GRAVITATIONAL-WAVE TRANSIENTS, NEUTRON-STAR, GENERAL-RELATIVITY, INSPIRALLING COMPACT BINARIES, (POST)(5/2)-NEWTONIAN ORDER, PARAMETER-ESTIMATION, COALESCING BINARIES, MASS-DISTRIBUTION
Abstract: The first observational run of the Advanced LIGO detectors, from September 12, 2015 to January 19, 2016, saw the first detections of gravitational waves from binary black hole mergers. In this paper, we present full results from a search for binary black hole merger signals with total masses up to 100M. and detailed implications from our observations of these systems. Our search, based on general-relativistic models of gravitational-wave signals from binary black hole systems, unambiguously identified two signals, GW150914 and GW151226, with a significance of greater than 5 sigma over the observing period. It also identified a third possible signal, LVT151012, with substantially lower significance and with an 87% probability of being of astrophysical origin. We provide detailed estimates of the parameters of the observed systems. Both GW150914 and GW151226 provide an unprecedented opportunity to study the two-body motion of a compact-object binary in the large velocity, highly nonlinear regime. We do not observe any deviations from general relativity, and we place improved empirical bounds on several highorder post-Newtonian coefficients. From our observations, we infer stellar-mass binary black hole merger rates lying in the range 9-240 Gpc(-3) yr(-1). These observations are beginning to inform astrophysical predictions of binary black hole formation rates and indicate that future observing runs of the Advanced detector network will yield many more gravitational-wave detections.
Published: 2016

12. Binary Black Hole Mergers in the First Advanced LIGO Observing Run

Subjects: MAXIMUM MASS, COMMON ENVELOPE, GRAVITATIONAL-WAVE TRANSIENTS, NEUTRON-STAR, GENERAL-RELATIVITY, INSPIRALLING COMPACT BINARIES, (POST)(5/2)-NEWTONIAN ORDER, PARAMETER-ESTIMATION, COALESCING BINARIES, MASS-DISTRIBUTION
Abstract: The first observational run of the Advanced LIGO detectors, from September 12, 2015 to January 19, 2016, saw the first detections of gravitational waves from binary black hole mergers. In this paper, we present full results from a search for binary black hole merger signals with total masses up to 100M. and detailed implications from our observations of these systems. Our search, based on general-relativistic models of gravitational-wave signals from binary black hole systems, unambiguously identified two signals, GW150914 and GW151226, with a significance of greater than 5 sigma over the observing period. It also identified a third possible signal, LVT151012, with substantially lower significance and with an 87% probability of being of astrophysical origin. We provide detailed estimates of the parameters of the observed systems. Both GW150914 and GW151226 provide an unprecedented opportunity to study the two-body motion of a compact-object binary in the large velocity, highly nonlinear regime. We do not observe any deviations from general relativity, and we place improved empirical bounds on several highorder post-Newtonian coefficients. From our observations, we infer stellar-mass binary black hole merger rates lying in the range 9-240 Gpc(-3) yr(-1). These observations are beginning to inform astrophysical predictions of binary black hole formation rates and indicate that future observing runs of the Advanced detector network will yield many more gravitational-wave detections.
Published: 2016

13. GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence

Author: Abbott, B. P., Abbott, R., Abbott, T. D., Abernathy, M. R., Acernese, F., Ackley, K., Adams, C., Adams, T., Addesso, P., Adhikari, R. X., Adya, V. B., Affeldt, C., Agathos, M., Agatsuma, K., Aggarwal, N., Aguiar, O. D., Aiello, L., Ain, A., Ajith, P., Allen, B., Allocca, A., Altin, P. A., Anderson, S. B., Anderson, W. G., Arai, K., Araya, M. C., Arceneaux, C. C., Areeda, J. S., Arnaud, N., Arun, K. G., Ascenzi, S., Ashton, G., Ast, M., Aston, S. M., Astone, P., Aufmuth, P., Aulbert, C., Babak, S., Bacon, P., Bader, M. K. M., Baker, P. T., Baldaccini, F., Ballardin, G., Ballmer, S. W., Barayoga, J. C., Barclay, S. E., Barish, B. C., Barker, D., Barone, F., Barr, B., Barsotti, L., Barsuglia, M., Barta, D., Bartlett, J., Bartos, I., Bassiri, R., Basti, A., Batch, J. C., Baune, C., Bavigadda, V., Bazzan, M., Bejger, M., Bell, A. S., Berger, B. K., Bergmann, G., Berry, C. P. L., Bersanetti, D., Bertolini, A., Betzwieser, J., Bhagwat, S., Bhandare, R., Bilenko, I. A., Billingsley, G., Birch, J., Birney, R., Birnholtz, O., Biscans, S., Bisht, A., Bitossi, M., Biwer, C., Bizouard, M. A., Blackburn, J. K., Blair, C. D., Blair, D. G., Blair, R. M., Bloemen, S., Bock, O., Boer, M., Bogaert, G., Bogan, C., Bohe, A., Bond, C., Bondu, F., Bonnand, R., Boom, B. A., Bork, R., Boschi, V., Bose, S., Bouffanais, Y., Bozzi, A., Bradaschia, C., Brady, P. R., Braginsky, V. B., Branchesi, M., Brau, J. E., Briant, T., Brillet, A., Brinkmann, M., Brisson, V., Brockill, P., Broida, J. E., Brooks, A. F., Brown, D. A., Brown, D. D., Brown, N. M., Brunett, S., Buchanan, C. C., Buikema, A., Bulik, T., Bulten, H. J., Buonanno, A., Buskulic, D., Buy, C., Byer, R. L., Cabero, M., Cadonati, L., Cagnoli, G., Cahillane, C., Calderón Bustillo, J., Callister, T., Calloni, E., Camp, J. B., Cannon, K. C., Cao, J., Capano, C. D., Capocasa, E., Carbognani, F., Caride, S., Casanueva Diaz, J., Casentini, C., Caudill, S., Cavaglià, M., Cavalier, F., Cavalieri, R., Cella, G., Cepeda, C. B., Cerboni Baiardi, L., Cerretani, G., Cesarini, E., Chamberlin, S. J., Chan, M., Chao, S., Charlton, P., Chassande-Mottin, E., Cheeseboro, B. D., Chen, H. Y., Chen, Y., Cheng, C., Chincarini, A., Chiummo, A., Cho, H. S., Cho, M., Chow, J. H., Christensen, N., Chu, Q., Chua, S., Chung, S., Ciani, G., Clara, F., Clark, J. A., Cleva, F., Coccia, E., Cohadon, P.-F., Colla, A., Collette, C. G., Cominsky, L., Constancio, M., Conte, A., Conti, L., Cook, D., Corbitt, T. R., Cornish, N., Corsi, A., Cortese, S., Costa, C. A., Coughlin, M. W., Coughlin, S. B., Coulon, J.-P., Countryman, S. T., Couvares, P., Cowan, E. E., Coward, D. M., Cowart, M. J., Coyne, D. C., Coyne, R., Craig, K., Creighton, J. D. E., Cripe, J., Crowder, S. G., Cumming, A., Cunningham, L., Cuoco, E., Dal Canton, T., Danilishin, S. L., D’Antonio, S., Danzmann, K., Darman, N. S., Dasgupta, A., Da Silva Costa, C. F., Dattilo, V., Dave, I., Davier, M., Davies, G. S., Daw, E. J., Day, R., De, S., DeBra, D., Debreczeni, G., Degallaix, J., De Laurentis, M., Deléglise, S., Del Pozzo, W., Denker, T., Dent, T., Dergachev, V., De Rosa, R., DeRosa, R. T., DeSalvo, R., Devine, R. C., Dhurandhar, S., Díaz, M. C., Di Fiore, L., Di Giovanni, M., Di Girolamo, T., Di Lieto, A., Di Pace, S., Di Palma, I., Di Virgilio, A., Dolique, V., Donovan, F., Dooley, K. L., Doravari, S., Douglas, R., Downes, T. P., Drago, M., Drever, R. W. P., Driggers, J. C., Ducrot, M., Dwyer, S. E., Edo, T. B., Edwards, M. C., Effler, A., Eggenstein, H.-B., Ehrens, P., Eichholz, J., Eikenberry, S. S., Engels, W., Essick, R. C., Etzel, T., Evans, T. M., Everett, R., Factourovich, M., Fafone, V., Fair, H., Fairhurst, S., Fan, X., Fang, Q., Farinon, S., Farr, B., Farr, W. M., Favata, M., Fays, M., Fehrmann, H., Fejer, M. M., Fenyvesi, E., Ferrante, I., Ferreira, E. C., Ferrini, F., Fidecaro, F., Fiori, I., Fiorucci, D., Fisher, R. P., Flaminio, R., Fletcher, M., Fong, H., Fournier, J.-D., Frasca, S., Frasconi, F., Frei, Z., Freise, A., Frey, R., Frey, V., Fritschel, P., Frolov, V. V., Fulda, P., Fyffe, M., Gabbard, H. A. G., Gair, J. R., Gammaitoni, L., Gaonkar, S. G., Garufi, F., Gaur, G., Gehrels, N., Gemme, G., Geng, P., Genin, E., Gennai, A., George, J., Gergely, L., Germain, V., Ghosh, Abhirup, Ghosh, Archisman, Ghosh, S., Giaime, J. A., Giardina, K. D., Giazotto, A., Gill, K., Glaefke, A., Goetz, E., Goetz, R., Gondan, L., González, G., Gonzalez Castro, J. M., Gopakumar, A., Gordon, N. A., Gorodetsky, M. L., Gossan, S. E., Gosselin, M., Gouaty, R., Grado, A., Graef, C., Graff, P. B., Granata, M., Grant, A., Gras, S., Gray, C., Greco, G., Green, A. C., Groot, P., Grote, H., Grunewald, S., Guidi, G. M., Guo, X., Gupta, A., Gupta, M. K., Gushwa, K. E., Gustafson, E. K., Gustafson, R., Hacker, J. J., Hall, B. R., Hall, E. D., Hamilton, H., Hammond, G., Haney, M., Hanke, M. M., Hanks, J., Hanna, C., Hannam, M. D., Hanson, J., Hardwick, T., Harms, J., Harry, G. M., Harry, I. W., Hart, M. J., Hartman, M. T., Haster, C.-J., Haughian, K., Healy, J., Heidmann, A., Heintze, M. C., Heitmann, H., Hello, P., Hemming, G., Hendry, M., Heng, I. S., Hennig, J., Henry, J., Heptonstall, A. W., Heurs, M., Hild, S., Hoak, D., Hofman, D., Holt, K., Holz, D. E., Hopkins, P., Hough, J., Houston, E. A., Howell, E. J., Hu, Y. M., Huang, S., Huerta, E. A., Huet, D., Hughey, B., Husa, S., Huttner, S. H., Huynh-Dinh, T., Indik, N., Ingram, D. R., Inta, R., Isa, H. N., Isac, J.-M., Isi, M., Isogai, T., Iyer, B. R., Izumi, K., Jacqmin, T., Jang, H., Jani, K., Jaranowski, P., Jawahar, S., Jian, L., Jiménez-Forteza, F., Johnson, W. W., Johnson-McDaniel, N. K., Jones, D. I., Jones, R., Jonker, R. J. G., Ju, L., K, Haris, Kalaghatgi, C. V., Kalogera, V., Kandhasamy, S., Kang, G., Kanner, J. B., Kapadia, S. J., Karki, S., Karvinen, K. S., Kasprzack, M., Katsavounidis, E., Katzman, W., Kaufer, S., Kaur, T., Kawabe, K., Kéfélian, F., Kehl, M. S., Keitel, D., Kelley, D. B., Kells, W., Kennedy, R., Key, J. S., Khalili, F. Y., Khan, I., Khan, S., Khan, Z., Khazanov, E. A., Kijbunchoo, N., Kim, Chi-Woong, Kim, Chunglee, Kim, J., Kim, K., Kim, N., Kim, W., Kim, Y.-M., Kimbrell, S. J., King, E. J., King, P. J., Kissel, J. S., Klein, B., Kleybolte, L., Klimenko, S., Koehlenbeck, S. M., Koley, S., Kondrashov, V., Kontos, A., Korobko, M., Korth, W. Z., Kowalska, I., Kozak, D. B., Kringel, V., Krishnan, B., Królak, A., Krueger, C., Kuehn, G., Kumar, P., Kumar, R., Kuo, L., Kutynia, A., Lackey, B. D., Landry, M., Lange, J., Lantz, B., Lasky, P. D., Laxen, M., Lazzarini, A., Lazzaro, C., Leaci, P., Leavey, S., Lebigot, E. O., Lee, C. H., Lee, H. K., Lee, H. M., Lee, K., Lenon, A., Leonardi, M., Leong, J. R., Leroy, N., Letendre, N., Levin, Y., Lewis, J. B., Li, T. G. F., Libson, A., Littenberg, T. B., Lockerbie, N. A., Lombardi, A. L., London, L. T., Lord, J. E., Lorenzini, M., Loriette, V., Lormand, M., Losurdo, G., Lough, J. D., Lousto, C. O., Lück, H., Lundgren, A. P., Lynch, R., Ma, Y., Machenschalk, B., MacInnis, M., Macleod, D. M., Magaña-Sandoval, F., Magaña Zertuche, L., Magee, R. M., Majorana, E., Maksimovic, I., Malvezzi, V., Man, N., Mandel, I., Mandic, V., Mangano, V., Mansell, G. L., Manske, M., Mantovani, M., Marchesoni, F., Marion, F., Márka, S., Márka, Z., Markosyan, A. S., Maros, E., Martelli, F., Martellini, L., Martin, I. W., Martynov, D. V., Marx, J. N., Mason, K., Masserot, A., Massinger, T. J., Masso-Reid, M., Mastrogiovanni, S., Matichard, F., Matone, L., Mavalvala, N., Mazumder, N., McCarthy, R., McClelland, D. E., McCormick, S., McGuire, S. C., McIntyre, G., McIver, J., McManus, D. J., McRae, T., McWilliams, S. T., Meacher, D., Meadors, G. D., Meidam, J., Melatos, A., Mendell, G., Mercer, R. A., Merilh, E. L., Merzougui, M., Meshkov, S., Messenger, C., Messick, C., Metzdorff, R., Meyers, P. M., Mezzani, F., Miao, H., Michel, C., Middleton, H., Mikhailov, E. E., Milano, L., Miller, A. L., Miller, A., Miller, B. B., Miller, J., Millhouse, M., Minenkov, Y., Ming, J., Mirshekari, S., Mishra, C., Mitra, S., Mitrofanov, V. P., Mitselmakher, G., Mittleman, R., Moggi, A., Mohan, M., Mohapatra, S. R. P., Montani, M., Moore, B. C., Moore, C. J., Moraru, D., Moreno, G., Morriss, S. R., Mossavi, K., Mours, B., Mow-Lowry, C. M., Mueller, G., Muir, A. W., Mukherjee, Arunava, Mukherjee, D., Mukherjee, S., Mukund, N., Mullavey, A., Munch, J., Murphy, D. J., Murray, P. G., Mytidis, A., Nardecchia, I., Naticchioni, L., Nayak, R. K., Nedkova, K., Nelemans, G., Nelson, T. J. N., Neri, M., Neunzert, A., Newton, G., Nguyen, T. T., Nielsen, A. B., Nissanke, S., Nitz, A., Nocera, F., Nolting, D., Normandin, M. E. N., Nuttall, L. K., Oberling, J., Ochsner, E., O’Dell, J., Oelker, E., Ogin, G. H., Oh, J. J., Oh, S. H., Ohme, F., Oliver, M., Oppermann, P., Oram, Richard J., O’Reilly, B., O’Shaughnessy, R., Ottaway, D. J., Overmier, H., Owen, B. J., Pai, A., Pai, S. A., Palamos, J. R., Palashov, O., Palomba, C., Pal-Singh, A., Pan, H., Pankow, C., Pannarale, F., Pant, B. C., Paoletti, F., Paoli, A., Papa, M. A., Paris, H. R., Parker, W., Pascucci, D., Pasqualetti, A., Passaquieti, R., Passuello, D., Patricelli, B., Patrick, Z., Pearlstone, B. L., Pedraza, M., Pedurand, R., Pekowsky, L., Pele, A., Penn, S., Perreca, A., Perri, L. M., Pfeiffer, H. P., Phelps, M., Piccinni, O. J., Pichot, M., Piergiovanni, F., Pierro, V., Pillant, G., Pinard, L., Pinto, I. M., Pitkin, M., Poe, M., Poggiani, R., Popolizio, P., Post, A., Powell, J., Prasad, J., Predoi, V., Prestegard, T., Price, L. R., Prijatelj, M., Principe, M., Privitera, S., Prix, R., Prodi, G. A., Prokhorov, L., Puncken, O., Punturo, M., Puppo, P., Pürrer, M., Qi, H., Qin, J., Qiu, S., Quetschke, V., Quintero, E. A., Quitzow-James, R., Raab, F. J., Rabeling, D. S., Radkins, H., Raffai, P., Raja, S., Rajan, C., Rakhmanov, M., Rapagnani, P., Raymond, V., Razzano, M., Re, V., Read, J., Reed, C. M., Regimbau, T., Rei, L., Reid, S., Reitze, D. H., Rew, H., Reyes, S. D., Ricci, F., Riles, K., Rizzo, M., Robertson, N. A., Robie, R., Robinet, F., Rocchi, A., Rolland, L., Rollins, J. G., Roma, V. J., Romano, J. D., Romano, R., Romanov, G., Romie, J. H., Rosińska, D., Rowan, S., Rüdiger, A., Ruggi, P., Ryan, K., Sachdev, S., Sadecki, T., Sadeghian, L., Sakellariadou, M., Salconi, L., Saleem, M., Salemi, F., Samajdar, A., Sammut, L., Sanchez, E. J., Sandberg, V., Sandeen, B., Sanders, J. R., Sassolas, B., Sathyaprakash, B. S., Saulson, P. R., Sauter, O. E. S., Savage, R. L., Sawadsky, A., Schale, P., Schilling, R., Schmidt, J., Schmidt, P., Schnabel, R., Schofield, R. M. S., Schönbeck, A., Schreiber, E., Schuette, D., Schutz, B. F., Scott, J., Scott, S. M., Sellers, D., Sengupta, A. S., Sentenac, D., Sequino, V., Sergeev, A., Setyawati, Y., Shaddock, D. A., Shaffer, T., Shahriar, M. S., Shaltev, M., Shapiro, B., Shawhan, P., Sheperd, A., Shoemaker, D. H., Shoemaker, D. M., Siellez, K., Siemens, X., Sieniawska, M., Sigg, D., Silva, A. D., Singer, A., Singer, L. P., Singh, A., Singh, R., Singhal, A., Sintes, A. M., Slagmolen, B. J. J., Smith, J. R., Smith, N. D., Smith, R. J. E., Son, E. J., Sorazu, B., Sorrentino, F., Souradeep, T., Srivastava, A. K., Staley, A., Steinke, M., Steinlechner, J., Steinlechner, S., Steinmeyer, D., Stephens, B. C., Stevenson, S. P., Stone, R., Strain, K. A., Straniero, N., Stratta, G., Strauss, N. A., Strigin, S., Sturani, R., Stuver, A. L., Summerscales, T. Z., Sun, L., Sunil, S., Sutton, P. J., Swinkels, B. L., Szczepańczyk, M. J., Tacca, M., Talukder, D., Tanner, D. B., Tápai, M., Tarabrin, S. P., Taracchini, A., Taylor, R., Theeg, T., Thirugnanasambandam, M. P., Thomas, E. G., Thomas, M., Thomas, P., Thorne, K. A., Thrane, E., Tiwari, S., Tiwari, V., Tokmakov, K. V., Toland, K., Tomlinson, C., Tonelli, M., Tornasi, Z., Torres, C. V., Torrie, C. I., Töyrä, D., Travasso, F., Traylor, G., Trifirò, D., Tringali, M. C., Trozzo, L., Tse, M., Turconi, M., Tuyenbayev, D., Ugolini, D., Unnikrishnan, C. S., Urban, A. L., Usman, S. A., Vahlbruch, H., Vajente, G., Valdes, G., Vallisneri, M., van Bakel, N., van Beuzekom, M., van den Brand, J. F. J., Van Den Broeck, C., Vander-Hyde, D. C., van der Schaaf, L., van Heijningen, J. V., van Veggel, A. A., Vardaro, M., Vass, S., Vasúth, M., Vaulin, R., Vecchio, A., Vedovato, G., Veitch, J., Veitch, P. J., Venkateswara, K., Verkindt, D., Vetrano, F., Viceré, A., Vinciguerra, S., Vine, D. J., Vinet, J.-Y., Vitale, S., Vo, T., Vocca, H., Vorvick, C., Voss, D. V., Vousden, W. D., Vyatchanin, S. P., Wade, A. R., Wade, L. E., Wade, M., Walker, M., Wallace, L., Walsh, S., Wang, G., Wang, H., Wang, M., Wang, X., Wang, Y., Ward, R. 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E., The LIGO Scientific Collaboration, The Virgo Collaboration, Massachusetts Institute of Technology. Department of Physics, MIT Kavli Institute for Astrophysics and Space Research, Aggarwal, Nancy, Barsotti, Lisa, Biscans, Sebastien, Buikema, Aaron, Donovan, Frederick J., Essick, Reed Clasey, Fritschel, Peter K., Gras, Slawomir, Isogai, Tomoki, Katsavounidis, Erotokritos, Kontos, Antonios, Libson, Adam, Lynch, Ryan Christopher, MacInnis, Myron E., Mason, Kenneth R., Matichard, Fabrice, Mavalvala, Nergis, Miller, Jeffrey B., Mittleman, Richard K., Ray Pitambar Mohapatra, Satyanarayan, Oelker, Eric Glenn, Shoemaker, David H., Tse, Maggie, Vaulin, Ruslan, Vitale, Salvatore, Weiss, Rainer, Yam, William, Yu, Haocun, and Zucker, Michael E.
Subjects: Astronomy, Gravitational Wave, General Physics and Astronomy, Astrophysics, 01 natural sciences, General Relativity and Quantum Cosmology, gravitational waves, LIGO, binary black hole, Second Detection, GeneralLiterature_REFERENCE(e.g.,dictionaries,encyclopedias,glossaries), 010303 astronomy & astrophysics, QC, QB, LIGO Scientific Collaboration, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, Settore FIS/01 - Fisica Sperimentale, MERGER, CHOICE, [PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], Astrophysics - High Energy Astrophysical Phenomena, Sciences exactes et naturelles, [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, General Relativity and Quantum Cosmology (gr-qc), Gravitational-wave astronomy, [ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], MAXIMUM MASS, Physics and Astronomy (all), Binary black hole, 0103 physical sciences, GW151226, KAGRA, STFC, MASS-DISTRIBUTION, Gravitational Waves, 010308 nuclear & particles physics, Gravitational wave, See paper for full list of authors - 14 pages, 5 figures, RCUK, [ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Black hole, STELLAR, Physics and Astronomy, Binary Black Holes, Gravitational Waves, Second Detection, Binary Black Holes, RADIATION
Abstract: We report the observation of a gravitational-wave signal produced by the coalescence of two stellar-mass black holes. The signal, GW151226, was observed by the twin detectors of the Laser Interferometer Gravitational-Wave Observatory (LIGO) on December 26, 2015 at 03:38:53 UTC. The signal was initially identified within 70 s by an online matched-filter search targeting binary coalescences. Subsequent off-line analyses recovered GW151226 with a network signal-to-noise ratio of 13 and a significance greater than 5σ. The signal persisted in the LIGO frequency band for approximately 1 s, increasing in frequency and amplitude over about 55 cycles from 35 to 450 Hz, and reached a peak gravitational strain of 3.4-0.9+0.7×10-22. The inferred source-frame initial black hole masses are 14.2-3.7+8.3M and 7.5-2.3+2.3M, and the final black hole mass is 20.8-1.7+6.1M. We find that at least one of the component black holes has spin greater than 0.2. This source is located at a luminosity distance of 440-190+180 Mpc corresponding to a redshift of 0.09-0.04+0.03. All uncertainties define a 90% credible interval. This second gravitational-wave observation provides improved constraints on stellar populations and on deviations from general relativity., 0, info:eu-repo/semantics/published
Published: 2016

14. Search for narrow resonances in dijet final states at sqrt(s) = 8 TeV with the novel CMS technique of data scouting

Author: Khachatryan, Vardan, Sirunyan, Albert M, Flechl, Martin, Bruno, Giacomo, Mohamad Idris, Faridah, Wan Abdullah, Wan Ahmad Tajuddin, Yusli, Mohd Nizam, Zolkapli, Zukhaimira, Casimiro Linares, Edgar, Castilla-Valdez, Heriberto, De La Cruz-Burelo, Eduard, Heredia-De La Cruz, Ivan, Hernandez-Almada, Alberto, Lopez-Fernandez, Ricardo, Caudron, Adrien, Mejia Guisao, Jhovanny, Sánchez Hernández, Alberto, Carrillo Moreno, Salvador, Vazquez Valencia, Fabiola, Pedraza, Isabel, Salazar Ibarguen, Humberto Antonio, Uribe Estrada, Cecilia, Morelos Pineda, Antonio, Krofcheck, David, Butler, Philip H, Ceard, Ludivine, Ahmad, Ashfaq, Ahmad, Muhammad, Hassan, Qamar, Hoorani, Hafeez R, Khan, Wajid Ali, Qazi, Shamona, Shoaib, Muhammad, Waqas, Muhammad, Bialkowska, Helena, Bluj, Michal, De Visscher, Simon, Boimska, Bożena, Frueboes, Tomasz, Górski, Maciej, Kazana, Malgorzata, Nawrocki, Krzysztof, Romanowska-Rybinska, Katarzyna, Szleper, Michal, Zalewski, Piotr, Bunkowski, Karol, Byszuk, Adrian, Delaere, Christophe, Doroba, Krzysztof, Kalinowski, Artur, Konecki, Marcin, Krolikowski, Jan, Misiura, Maciej, Olszewski, Michal, Walczak, Marek, Bargassa, Pedrame, Beirão Da Cruz E Silva, Cristóvão, Di Francesco, Agostino, Delcourt, Martin, Faccioli, Pietro, Ferreira Parracho, Pedro Guilherme, Gallinaro, Michele, Hollar, Jonathan, Leonardo, Nuno, Lloret Iglesias, Lara, Nemallapudi, Mythra Varun, Rodrigues Antunes, Joao, Seixas, Joao, Toldaiev, Oleksii, Forthomme, Laurent, Vadruccio, Daniele, Varela, Joao, Vischia, Pietro, Bunin, Pavel, Gavrilenko, Mikhail, Golutvin, Igor, Gorbounov, Nikolai, Gorbunov, Ilya, Karjavin, Vladimir, Kozlov, Guennady, Francois, Brieuc, Lanev, Alexander, Malakhov, Alexander, Matveev, Viktor, Moisenz, Petr, Palichik, Vladimir, Perelygin, Victor, Savina, Maria, Shmatov, Sergey, Shulha, Siarhei, Skatchkov, Nikolai, Giammanco, Andrea, Smirnov, Vitaly, Zarubin, Anatoli, Chtchipounov, Leonid, Golovtsov, Victor, Ivanov, Yury, Kim, Victor, Kuznetsova, Ekaterina, Murzin, Victor, Oreshkin, Vadim, Sulimov, Valentin, Jafari, Abideh, Vorobyev, Alexey, Andreev, Yuri, Dermenev, Alexander, Gninenko, Sergei, Golubev, Nikolai, Karneyeu, Anton, Kirsanov, Mikhail, Krasnikov, Nikolai, Pashenkov, Anatoli, Tlisov, Danila, Friedl, Markus, Jez, Pavel, Toropin, Alexander, Epshteyn, Vladimir, Gavrilov, Vladimir, Lychkovskaya, Natalia, Popov, Vladimir, Pozdnyakov, Ivan, Safronov, Grigory, Spiridonov, Alexander, Toms, Maria, Vlasov, Evgueni, Komm, Matthias, Zhokin, Alexander, Chadeeva, Marina, Danilov, Mikhail, Zhemchugov, Evgenii, Andreev, Vladimir, Azarkin, Maksim, Dremin, Igor, Kirakosyan, Martin, Leonidov, Andrey, Rusakov, Sergey V, Lemaitre, Vincent, Terkulov, Adel, Baskakov, Alexey, Belyaev, Andrey, Boos, Edouard, Dubinin, Mikhail, Dudko, Lev, Ershov, Alexander, Gribushin, Andrey, Klyukhin, Vyacheslav, Kodolova, Olga, Magitteri, Alessio, Lokhtin, Igor, Miagkov, Igor, Obraztsov, Stepan, Petrushanko, Sergey, Savrin, Viktor, Snigirev, Alexander, Azhgirey, Igor, Bayshev, Igor, Bitioukov, Sergei, Elumakhov, Dmitry, Mertens, Alexandre, Kachanov, Vassili, Kalinin, Alexey, Konstantinov, Dmitri, Krychkine, Victor, Petrov, Vladimir, Ryutin, Roman, Sobol, Andrei, Troshin, Sergey, Tyurin, Nikolay, Uzunian, Andrey, Musich, Marco, Volkov, Alexey, Adzic, Petar, Cirkovic, Predrag, Devetak, Damir, Milosevic, Jovan, Rekovic, Vladimir, Alcaraz Maestre, Juan, Calvo, Enrique, Cerrada, Marcos, Chamizo Llatas, Maria, Nuttens, Claude, Colino, Nicanor, De La Cruz, Begona, Delgado Peris, Antonio, Escalante Del Valle, Alberto, Fernandez Bedoya, Cristina, Fernández Ramos, Juan Pablo, Flix, Jose, Fouz, Maria Cruz, Garcia-Abia, Pablo, Gonzalez Lopez, Oscar, Piotrzkowski, Krzysztof, Goy Lopez, Silvia, Hernandez, Jose M, Josa, Maria Isabel, Navarro De Martino, Eduardo, Pérez-Calero Yzquierdo, Antonio María, Puerta Pelayo, Jesus, Quintario Olmeda, Adrián, Redondo, Ignacio, Romero, Luciano, Senghi Soares, Mara, Quertenmont, Loic, de Trocóniz, Jorge F, Missiroli, Marino, 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Ivan, Beernaert, Kelly, Behnke, Olaf, Behrens, Ulf, Van Mechelen, Pierre, Bin Anuar, Afiq Aizuddin, Borras, Kerstin, Campbell, Alan, Connor, Patrick, Contreras-Campana, Christian, Costanza, Francesco, Diez Pardos, Carmen, Dolinska, Ganna, Eckerlin, Guenter, Eckstein, Doris, Van Remortel, Nick, Eichhorn, Thomas, Gallo, Elisabetta, Garay Garcia, Jasone, Geiser, Achim, Gizhko, Andrii, Grados Luyando, Juan Manuel, Gunnellini, Paolo, Harb, Ali, Hauk, Johannes, Hempel, Maria, Van Spilbeeck, Alex, Jung, Hannes, Kalogeropoulos, Alexis, Karacheban, Olena, Kasemann, Matthias, Keaveney, James, Kieseler, Jan, Kleinwort, Claus, Korol, Ievgen, Lange, Wolfgang, Lelek, Aleksandra, Abu Zeid, Shimaa, Leonard, Jessica, Lipka, Katerina, Lobanov, Artur, Lohmann, Wolfgang, Mankel, Rainer, Melzer-Pellmann, Isabell-Alissandra, Meyer, Andreas Bernhard, Mittag, Gregor, Mnich, Joachim, Mussgiller, Andreas, Blekman, Freya, Ntomari, Eleni, Pitzl, Daniel, Placakyte, Ringaile, Raspereza, Alexei, Roland, Benoit, 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de Physique des Particules du CNRS (IN2P3)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS), Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Centre de Calcul de l'IN2P3 (CC-IN2P3), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Institut de Physique Nucléaire de Lyon (IPNL), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), CMS, Khachatryan, V, Sirunyan, A, Tumasyan, A, Adam, W, Asilar, E, Bergauer, T, Brandstetter, J, Brondolin, E, Dragicevic, M, Erö, J, Flechl, M, Friedl, M, Frühwirth, R, Ghete, V, Hartl, C, Hörmann, N, Hrubec, J, Jeitler, M, König, A, Krätschmer, I, Liko, D, Matsushita, T, Mikulec, I, Rabady, D, 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Linacre, J, Lincoln, D, Lipton, R, Liu, T, Lopes De Sá, R, Lykken, J, Maeshima, K, Marraffino, J, Maruyama, S, Mason, D, Mcbride, P, Merkel, P, Mrenna, S, Nahn, S, Newman Holmes, C, O'Dell, V, Pedro, K, Prokofyev, O, Rakness, G, Ristori, L, Sexton Kennedy, E, Soha, A, Spalding, W, Spiegel, L, Stoynev, S, Strobbe, N, Taylor, L, Tkaczyk, S, Tran, N, Uplegger, L, Vaandering, E, Vernieri, C, Verzocchi, M, Vidal, R, Wang, M, Whitbeck, A, Acosta, D, Avery, P, Bortignon, P, Bourilkov, D, Brinkerhoff, A, Carnes, A, Carver, M, Curry, D, Das, S, Field, R, Furic, I, Konigsberg, J, Korytov, A, Ma, P, Matchev, K, Mei, H, Milenovic, P, Mitselmakher, G, Rank, D, Shchutska, L, Sperka, D, Thomas, L, Wang, J, Wang, S, Yelton, J, Linn, S, Markowitz, P, Martinez, G, Rodriguez, J, Ackert, A, Adams, J, Adams, T, Askew, A, Bein, S, Diamond, B, Hagopian, S, Hagopian, V, Johnson, K, Khatiwada, A, Prosper, H, Santra, A, Weinberg, M, Baarmand, M, Bhopatkar, V, Colafranceschi, S, Hohlmann, M, Kalakhety, H, Noonan, D, Roy, T, Yumiceva, F, Adams, M, Apanasevich, L, Berry, D, Betts, R, Bucinskaite, I, Cavanaugh, R, Evdokimov, O, Gauthier, L, Gerber, C, Hofman, D, Kurt, P, O'Brien, C, Sandoval Gonzalez, I, Turner, P, Varelas, N, Wu, Z, Zakaria, M, Zhang, J, Bilki, B, Clarida, W, Dilsiz, K, Durgut, S, Gandrajula, R, Haytmyradov, M, Khristenko, V, Merlo, J, Mermerkaya, H, Mestvirishvili, A, Moeller, A, Nachtman, J, Ogul, H, Onel, Y, Ozok, F, Penzo, A, Snyder, C, Tiras, E, Wetzel, J, Yi, K, Anderson, I, Blumenfeld, B, Cocoros, A, Eminizer, N, Fehling, D, Feng, L, Gritsan, A, Maksimovic, P, Osherson, M, Roskes, J, Sarica, U, Swartz, M, Xiao, M, Xin, Y, You, C, Al Bataineh, A, Baringer, P, Bean, A, Bowen, J, Bruner, C, Castle, J, Kenny, R, Kropivnitskaya, A, Majumder, D, Mcbrayer, W, Murray, M, Sanders, S, Stringer, R, Tapia Takaki, J, Wang, Q, Ivanov, A, Kaadze, K, Khalil, S, Makouski, M, Maravin, Y, Mohammadi, A, Saini, L, Skhirtladze, N, Toda, S, Lange, D, Rebassoo, F, Wright, D, Anelli, C, Baden, A, Baron, O, Belloni, A, Calvert, B, Eno, S, Ferraioli, C, Hadley, N, Jabeen, S, Kellogg, R, Kolberg, T, Kunkle, J, Mignerey, A, Shin, Y, Skuja, A, Tonjes, M, Tonwar, S, Apyan, A, Barbieri, R, Baty, A, Bi, R, Bierwagen, K, Brandt, S, Busza, W, Cali, I, Demiragli, Z, Di Matteo, L, Gomez Ceballos, G, Goncharov, M, Gulhan, D, Hsu, D, Iiyama, Y, Innocenti, G, Klute, M, Kovalskyi, D, Krajczar, K, Lai, Y, Lee, Y, Levin, A, Luckey, P, Marini, A, Mcginn, C, Mironov, C, Narayanan, S, Niu, X, Paus, C, Roland, C, Roland, G, Salfeld Nebgen, J, Stephans, G, Sumorok, K, Tatar, K, Varma, M, Velicanu, D, Veverka, J, Wang, T, Wyslouch, B, Yang, M, Zhukova, V, Benvenuti, A, Chatterjee, R, Dahmes, B, Evans, A, Finkel, A, Gude, A, Hansen, P, Kalafut, S, Kao, S, Klapoetke, K, Kubota, Y, Lesko, Z, Mans, J, Nourbakhsh, S, Ruckstuhl, N, Rusack, R, Tambe, N, Turkewitz, J, Acosta, J, Oliveros, S, Avdeeva, E, Bartek, R, Bloom, K, Bose, S, Claes, D, Dominguez, A, Fangmeier, C, Gonzalez Suarez, R, Kamalieddin, R, Knowlton, D, Kravchenko, I, Meier, F, Monroy, J, Siado, J, Snow, G, Stieger, B, Alyari, M, Dolen, J, George, J, Godshalk, A, Harrington, C, Iashvili, I, Kaisen, J, Kharchilava, A, Parker, A, Rappoccio, S, Roozbahani, B, Alverson, G, Barberis, E, Baumgartel, D, Chasco, M, Hortiangtham, A, Massironi, A, Morse, D, Nash, D, Orimoto, T, Teixeira De Lima, R, Trocino, D, Wang, R, Wood, D, Hahn, K, Kubik, A, Low, J, Mucia, N, Odell, N, Pollack, B, Schmitt, M, Sung, K, Trovato, M, Velasco, M, Dev, N, Hildreth, M, Hurtado Anampa, K, Jessop, C, Karmgard, D, Kellams, N, Lannon, K, Marinelli, N, Meng, F, Mueller, C, Musienko, Y, Planer, M, Reinsvold, A, Ruchti, R, Rupprecht, N, Smith, G, Taroni, S, Valls, N, Wayne, M, Wolf, M, Woodard, A, Alimena, J, Antonelli, L, Brinson, J, Bylsma, B, Durkin, L, Flowers, S, Francis, B, Hart, A, Hill, C, Hughes, R, Ji, W, Liu, B, Luo, W, Puigh, D, Rodenburg, M, Winer, B, Wulsin, H, Cooperstein, S, Driga, O, Elmer, P, Hardenbrook, J, Hebda, P, Luo, J, Marlow, D, Medvedeva, T, Mooney, M, Olsen, J, Palmer, C, Piroué, P, Stickland, D, Tully, C, Zuranski, A, Barker, A, Barnes, V, Benedetti, D, Folgueras, S, Gutay, L, Jha, M, Jones, M, Jung, A, Jung, K, Miller, D, Neumeister, N, Radburn Smith, B, Shi, X, Sun, J, Svyatkovskiy, A, Wang, F, Xie, W, Xu, L, Parashar, N, Stupak, J, Adair, A, Akgun, B, Chen, Z, Ecklund, K, Geurts, F, Guilbaud, M, Li, W, Michlin, B, Northup, M, Padley, B, Redjimi, R, Roberts, J, Rorie, J, Tu, Z, Zabel, J, Betchart, B, Bodek, A, De Barbaro, P, Demina, R, Duh, Y, Ferbel, T, Galanti, M, Garcia Bellido, A, Han, J, Hindrichs, O, Khukhunaishvili, A, Lo, K, Tan, P, Verzetti, M, Chou, J, Contreras Campana, E, Gershtein, Y, Gómez Espinosa, T, Halkiadakis, E, Heindl, M, Hidas, D, Hughes, E, Kaplan, S, Kunnawalkam Elayavalli, R, Kyriacou, S, Lath, A, Nash, K, Saka, H, Salur, S, Schnetzer, S, Sheffield, D, Somalwar, S, Stone, R, Thomas, S, Thomassen, P, Walker, M, Foerster, M, Heideman, J, Riley, G, Rose, K, Spanier, S, Thapa, K, Bouhali, O, Castaneda Hernandez, A, Celik, A, Dalchenko, M, De Mattia, M, Delgado, A, Dildick, S, Eusebi, R, Gilmore, J, Huang, T, Juska, E, Kamon, T, Krutelyov, V, Mueller, R, Pakhotin, Y, Patel, R, Perloff, A, Perniè, L, Rathjens, D, Safonov, A, Tatarinov, A, Ulmer, K, Akchurin, N, Cowden, C, Damgov, J, Dragoiu, C, Dudero, P, Faulkner, J, Kunori, S, Lamichhane, K, Libeiro, T, Undleeb, S, Volobouev, I, Delannoy, A, Greene, S, Gurrola, A, Janjam, R, Johns, W, Maguire, C, Melo, A, Ni, H, Sheldon, P, Tuo, S, Velkovska, J, Xu, Q, Arenton, M, Barria, P, Cox, B, Goodell, J, Hirosky, R, Ledovskoy, A, Li, H, Neu, C, Sinthuprasith, T, Sun, X, Wang, Y, Wolfe, E, Xia, F, Clarke, C, Harr, R, Karchin, P, Lamichhane, P, Sturdy, J, Belknap, D, Dasu, S, Dodd, L, Duric, S, Gomber, B, Grothe, M, Herndon, M, Hervé, A, Klabbers, P, Lanaro, A, Levine, A, Long, K, Loveless, R, Ojalvo, I, Perry, T, Pierro, G, Polese, G, Ruggles, T, Savin, A, Smith, N, Smith, W, Taylor, D, Verwilligen, P, Woods, N, Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Yerevan Physics Institute, Institut für Hochenergiephysik der OeAW, National Centre for Particle and High Energy Physics, Universiteit Antwerpen, Vrije Universiteit Brussel, Université Libre de Bruxelles, Ghent University, Université Catholique de Louvain, Université de Mons, Centro Brasileiro de Pesquisas Fisicas, Universidade do Estado do Rio de Janeiro (UERJ), Universidade Estadual Paulista (UNESP), Universidade Federal do ABC (UFABC), Institute for Nuclear Research and Nuclear Energy, University of Sofia, Beihang University, Institute of High Energy Physics, Peking University, Universidad de Los Andes, Mechanical Engineering and Naval Architecture, Faculty of Science, Institute Rudjer Boskovic, University of Cyprus, Charles University, Universidad San Francisco de Quito, Egyptian Network of High Energy Physics, National Institute of Chemical Physics and Biophysics, University of Helsinki, Helsinki Institute of Physics, Lappeenranta University of Technology, CEA/Saclay, IN2P3-CNRS, CNRS/IN2P3, Institut de Physique Nucléaire de Lyon, Georgian Technical University, Tbilisi State University, I. Physikalisches Institut, III. Physikalisches Institut A, III. Physikalisches Institut B, Deutsches Elektronen-Synchrotron, University of Hamburg, Institut für Experimentelle Kernphysik, NCSR Demokritos, National and Kapodistrian University of Athens, University of Ioánnina, Eötvös Loránd University, Wigner Research Centre for Physics, Institute of Nuclear Research ATOMKI, University of Debrecen, National Institute of Science Education and Research, Panjab University, University of Delhi, Saha Institute of Nuclear Physics, Indian Institute of Technology Madras, Bhabha Atomic Research Centre, Tata Institute of Fundamental Research-A, Tata Institute of Fundamental Research-B, Indian Institute of Science Education and Research (IISER), Institute for Research in Fundamental Sciences (IPM), University College Dublin, INFN Sezione di Bari, Università di Bari, Politecnico di Bari, INFN Sezione di Bologna, Università di Bologna, INFN Sezione di Catania, Università di Catania, INFN Sezione di Firenze, Università di Firenze, INFN Laboratori Nazionali di Frascati, INFN Sezione di Genova, Università di Genova, INFN Sezione di Milano-Bicocca, Università di Milano-Bicocca, INFN Sezione di Napoli, Università di Napoli Federico II, Università della Basilicata, Università G. 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Lebedev Physical Institute, Lomonosov Moscow State University, Institute for High Energy Physics, Vinca Institute of Nuclear Sciences, Centro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT), Universidad Autónoma de Madrid, Universidad de Oviedo, CSIC-Universidad de Cantabria, European Organization for Nuclear Research, Paul Scherrer Institut, ETH Zurich, Universität Zürich, National Central University, National Taiwan University (NTU), Cukurova University, Physics Department, Bogazici University, Istanbul Technical University, National Academy of Science of Ukraine, Kharkov Institute of Physics and Technology, University of Bristol, Rutherford Appleton Laboratory, Imperial College, Brunel University, Baylor University, University of Alabama, Boston University, Brown University, Davis, University of California, Riverside, San Diego, Santa Barbara, California Institute of Technology, Carnegie Mellon University, University of Colorado Boulder, Cornell University, Fairfield University, Fermi National Accelerator Laboratory, University of Florida, Florida International University, Florida State University, Florida Institute of Technology, University of Illinois at Chicago (UIC), University of Iowa, Johns Hopkins University, University of Kansas, Kansas State University, Lawrence Livermore National Laboratory, University of Maryland, Massachusetts Institute of Technology, University of Minnesota, University of Mississippi, University of Nebraska-Lincoln, State University of New York at Buffalo, Northeastern University, Northwestern University, University of Notre Dame, Ohio State University, Princeton University, University of Puerto Rico, Purdue University, Purdue University Calumet, Rice University, University of Rochester, State University of New Jersey, University of Tennessee, Texas A and M University, Texas Tech University, Vanderbilt University, University of Virginia, Wayne State University, University of Wisconsin - Madison, Vienna University of Technology, Universidade Estadual de Campinas (UNICAMP), Centre National de la Recherche Scientifique (CNRS)-IN2P3, British University in Egypt, Zewail City of Science and Technology, Fayoum University, Ain Shams University, Université de Haute Alsace, Brandenburg University of Technology, Institute of Physics, University of Visva-Bharati, University of Tehran, Islamic Azad University, Università degli Studi di Siena, International Islamic University of Malaysia, MOSTI, Consejo Nacional de Ciencia y Tecnología, Institute of Electronic Systems, St. Petersburg State Polytechnical University, University of Belgrade, National Technical University of Athens, Scuola Normale e Sezione dell'Infn, Riga Technical University, Albert Einstein Center for Fundamental Physics, Adiyaman University, Mersin University, Cag University, Piri Reis University, Gaziosmanpasa University, Ozyegin University, Izmir Institute of Technology, Marmara University, Kafkas University, Istanbul Bilgi University, Yildiz Technical University, Hacettepe University, University of Southampton, Instituto de Astrofísica de Canarias, Utah Valley University, Argonne National Laboratory, Erzincan University, Istanbul, Texas A and M University at Qatar, Khachatryan, V., Sirunyan, A. M., Tumasyan, A., Adam, W., Asilar, E., Bergauer, T., Brandstetter, J., Brondolin, E., Dragicevic, M., Erö, J., Flechl, M., Friedl, M., Frühwirth, R., Ghete, V. M., Hartl, C., Hörmann, N., Hrubec, J., Jeitler, M., König, A., Krätschmer, I., Liko, D., Matsushita, T., Mikulec, I., Rabady, D., Rad, N., Rahbaran, B., Rohringer, H., Schieck, J., Strauss, J., Treberer Treberspurg, W., Waltenberger, W., Wulz, C. E., Mossolov, V., Shumeiko, N., Suarez Gonzalez, J., Alderweireldt, S., De Wolf, E. A., Janssen, X., Knutsson, A., Lauwers, J., Van De Klundert, M., Van Haevermaet, H., Van Mechelen, P., Van Remortel, N., Van Spilbeeck, A., Abu Zeid, S., Blekman, F., D'Hondt, J., Daci, N., De Bruyn, I., Deroover, K., Heracleous, N., Lowette, S., Moortgat, S., Moreels, L., Olbrechts, A., Python, Q., Tavernier, S., Van Doninck, W., Van Mulders, P., Van Parijs, I., Brun, H., Caillol, C., Clerbaux, B., De Lentdecker, G., Delannoy, H., Fasanella, G., Favart, L., Goldouzian, R., Grebenyuk, A., Karapostoli, G., Lenzi, T., Léonard, A., Luetic, J., Maerschalk, T., Marinov, A., Randle Conde, A., Seva, T., Vander Velde, C., Vanlaer, P., Yonamine, R., Zenoni, F., Zhang, F., Cimmino, A., Cornelis, T., Dobur, D., Fagot, A., Garcia, G., Gul, M., Mccartin, J., Poyraz, D., Salva, S., Schöfbeck, R., Tytgat, M., Van Driessche, W., Yazgan, E., Zaganidis, N., Beluffi, C., Bondu, O., Brochet, S., Bruno, G., Caudron, A., Ceard, L., De Visscher, S., Delaere, C., Delcourt, M., Forthomme, L., Francois, B., Giammanco, A., Jafari, A., Jez, P., Komm, M., Lemaitre, V., Magitteri, A., Mertens, A., Musich, M., Nuttens, C., Piotrzkowski, K., Quertenmont, L., Selvaggi, M., Vidal Marono, M., Wertz, S., Beliy, N., Aldá Júnior, W. 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A., Rykaczewski, H., Finger, M., Carrera Jarrin, E., Elgammal, S., Mohamed, A., Mohammed, Y., Salama, E., Calpas, B., Kadastik, M., Murumaa, M., Perrini, L., Raidal, M., Tiko, A., Veelken, C., Eerola, P., Pekkanen, J., Voutilainen, M., Härkönen, J., Karimäki, V., Kinnunen, R., Lampén, T., Lassila Perini, K., Lehti, S., Lindén, T., Luukka, P., Peltola, T., Tuominiemi, J., Tuovinen, E., Wendland, L., Talvitie, J., Tuuva, T., Besancon, M., Couderc, F., Dejardin, M., Denegri, D., Fabbro, B., Faure, J. L., Favaro, C., Ferri, F., Ganjour, S., Ghosh, S., Givernaud, A., Gras, P., Hamel De Monchenault, G., Jarry, P., Kucher, I., Locci, E., Machet, M., Malcles, J., Rander, J., Rosowsky, A., Titov, M., Zghiche, A., Abdulsalam, A., Antropov, I., Baffioni, S., Beaudette, F., Busson, P., Cadamuro, L., Chapon, E., Charlot, C., Davignon, O., Granier De Cassagnac, R., Jo, M., Lisniak, S., Miné, P., Naranjo, I. N., Nguyen, M., Ochando, C., Ortona, G., Paganini, P., Pigard, P., Regnard, S., Salerno, R., Sirois, Y., Strebler, T., Yilmaz, Y., Zabi, A., Agram, J. L., Andrea, J., Aubin, A., Bloch, D., Brom, J. M., Buttignol, M., Chabert, E. C., Chanon, N., Collard, C., Conte, E., Coubez, X., Fontaine, J. C., Gelé, D., Goerlach, U., Le Bihan, A. C., Merlin, J. A., Skovpen, K., Van Hove, P., Gadrat, S., Beauceron, S., Bernet, C., Boudoul, G., Bouvier, E., Carrillo Montoya, C. A., Chierici, R., Contardo, D., Courbon, B., Depasse, P., El Mamouni, H., Fan, J., Fay, J., Gascon, S., Gouzevitch, M., Grenier, G., Ille, B., Lagarde, F., Laktineh, I. B., Lethuillier, M., Mirabito, L., Pequegnot, A. L., Perries, S., Popov, A., Sabes, D., Sordini, V., Vander Donckt, M., Verdier, P., Viret, S., Toriashvili, T., Lomidze, D., Autermann, C., Beranek, S., Feld, L., Heister, A., Kiesel, M. K., Klein, K., Lipinski, M., Ostapchuk, A., Preuten, M., Raupach, F., Schael, S., Schomakers, C., Schulte, J. 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Gritsan, A.V, Martin, C, Al-bataineh, A, Boren, S, Kenny, R.P, III, Khalil, S, Tapia Takaki, J.D, Saini, L.K, Eno, S.C, Gomez, J.A, Hadley, N.J, Kellogg, R.G, Mignerey, A.C, Ricci-Tam, F, Shin, Y.H, Tonjes, M.B, Tonwar, S.C, Abercrombie, D, Allen, B, Cali, I.A, D’Alfonso, M, Innocenti, G.M, Lai, Y.S, Lee, Y.-J, Luckey, P.D, Marini, A.C, Salfeld-Nebgen, J, Stephans, G.S.F, Wang, T.W, Benvenuti, A.C, Chatterjee, R.M, Kao, S.C, Acosta, J.G, Claes, D.R, Malta Rodrigues, A, Siado, J.E, Snow, G.R, Morse, D.M, Wang, R.-J, Hahn, K.A, Schmitt, M.H, Karmgard, D.J, Durkin, L.S, Winer, B.L, Wulsin, H.W, Mei, K, Barnes, V.E, Jha, M.K, Jung, A.W, Miller, D.H, Schulte, J.F, Ecklund, K.M, Geurts, F.J.M, Padley, B.P, de Barbaro, P, Duh, Y.T, Garcia-Bellido, A, Lo, K.H, Chou, J.P, Gómez Espinosa, T.A, Delannoy, A.G, Ulmer, K.A, Dudero, P.R, Arenton, M.W, Wo lfe, E, Karchin, P.E, Belknap, D.A, Buchanan, J, Pierro, G.A, Smith, W.H, and Woods
Subjects: BOSONS, General Physics, p p: scattering, data analysis method, dijet: mass spectrum, mass spectrum [dijet], P(P)OVER-BAR COLLISIONS, FOS: Physical sciences, coupling constant: upper limit, resonance: coupling, channel cross section: upper limit, High Energy Physics - Experiment, Physics and Astronomy (all), High Energy Physics - Experiment (hep-ex), lepton: coupling: low, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], ddc:550, scattering [p p], HADRON COLLIDERS, coupling [resonance], MASS-DISTRIBUTION, coupling: low [lepton], 8000 GeV-cms, SPECTRUM, 02 Physical Sciences, upper limit [channel cross section], CMS, Physics, QUARK, Settore FIS/01 - Fisica Sperimentale, dijet: final state, final state [dijet], sensitivity, mass dependence, upper limit [coupling constant], CERN LHC Coll, Physics and Astronomy, CMS Collaboration, High Energy Physics::Experiment, colliding beams [p p], narrow resonance, p p: colliding beams, Particle Physics - Experiment, experimental results
Abstract: A search for narrow resonances decaying into dijet final states is performed on data from proton-proton collisions at a center-of-mass energy of 8 TeV, corresponding to an integrated luminosity of 18.8 inverse femtobarns. The data were collected with the CMS detector using a novel technique called data scouting, in which the information associated with these selected events is much reduced, permitting collection of larger data samples. This technique enables CMS to record events containing jets at a rate of 1 kHz, by collecting the data from the high-level-trigger system. In this way, the sensitivity to low-mass resonances is increased significantly, allowing previously inaccessible couplings of new resonances to quarks and gluons to be probed. The resulting dijet mass distribution yields no evidence of narrow resonances. Upper limits are presented on the resonance cross sections as a function of mass, and compared with a variety of models predicting narrow resonances. The limits are translated into upper limits on the coupling of a leptophobic resonance Z'[B] to quarks, improving on the results obtained by previous experiments for the mass range from 500 to 800 GeV., Replaced with published version. All the figures and tables can be found at http://cms-results.web.cern.ch/cms-results/public-results/publications/EXO-14-005/index.html
Published: 2016

15. Binary Black Hole Mergers in the First Advanced LIGO Observing Run

Author: Ligo, The Scientific Collaboration, the Virgo Collaboration, Abbott, B. P., Abbott, R., Abbott, T. D., Abernathy, M. R., Acernese, F., Ackley, K., Adams, C., Adams, T., Addesso, P., Adhikari, R. X., Adya, V. B., Affeldt, C., Agathos, M., Agatsuma, K., Aggarwal, N., Aguiar, O. D., Aiello, L., Ain, A., Ajith, P., Allen, B., Allocca, A., Altin, P. A., Anderson, S. B., Anderson, W. G., Arai, K., Araya, M. C., Arceneaux, C. C., Areeda, J. S., Arnaud, N., Arun, K. G., Ascenzi, S., Ashton, G., Ast, M., Aston, S. M., Astone, P., Aufmuth, P., Aulbert, C., Babak, S., Bacon, P., Bader, M. K. M., Baker, P. T., Baldaccini, F., Ballardin, G., Ballmer, S. W., Barayoga, J. C., Barclay, S. E., Barish, B. C., Barker, D., Barone, F., Barr, B., Barsotti, L., Barsuglia, M., Barta, D., Bartlett, J., Bartos, I., Bassiri, R., Basti, A., Batch, J. C., Baune, C., Bavigadda, V., Bazzan, M., Bejger, M., Bell, A. S., Berger, B. K., Bergmann, G., Berry, C. P. L., Bersanetti, D., Bertolini, A., Betzwieser, J., Bhagwat, S., Bhandare, R., Bilenko, I. A., Billingsley, G., Birch, J., Birney, R., Birnholtz, O., Biscans, S., Bisht, A., Bitossi, M., Biwer, C., Bizouard, M. A., Blackburn, J. K., Blair, C. D., Blair, D. G., Blair, R. M., Bloemen, S., Bock, O., Boer, M., Bogaert, G., Bogan, C., Bohe, A., Bond, C., Bondu, F., Bonnand, R., Boom, B. A., Bork, R., Boschi, V., Bose, S., Bouffanais, Y., Bozzi, A., Bradaschia, C., Brady, P. R., Braginsky, V. B., Branchesi, M., Brau, J. E., Briant, T., Brillet, A., Brinkmann, M., Brisson, V., Brockill, P., Broida, J. E., Brooks, A. F., Brown, D. A., Brown, D. D., Brown, N. M., Brunett, S., Buchanan, C. C., Buikema, A., Bulik, T., Bulten, H. J., Buonanno, A., Buskulic, D., Buy, C., Byer, R. L., Cabero, M., Cadonati, L., Cagnoli, G., Cahillane, C., Calder On Bustillo, J., Callister, T., Calloni, E., Camp, J. B., Cannon, K. C., Cao, J., Capano, C. D., Capocasa, E., Carbognani, F., Caride, S., Casanueva Diaz, J., Casentini, C., Caudill, S., Cavagli A, M., Cavalier, F., Cavalieri, R., Cella, G., Cepeda, C. B., Cerboni Baiardi, L., Cerretani, G., Cesarini, E., Chamberlin, S. J., Chan, M., Chao, S., Charlton, P., Chassande-Mottin, E., Cheeseboro, B. D., Chen, H. Y., Chen, Y., Cheng, C., Chincarini, A., Chiummo, A., Cho, H. S., Cho, M., Chow, J. H., Christensen, N., Chu, Q., Chua, S., Chung, S., Ciani, G., Clara, F., Clark, J. A., Cleva, F., Coccia, E., Cohadon, P. -F, Colla, A., Collette, C. G., Cominsky, L., Constancio, M., Conte, A., Conti, L., Cook, D., Corbitt, T. R., Cornish, N., Corsi, A., Cortese, S., Costa, C. A., Coughlin, M. W., Coughlin, S. B., Coulon, J. -P, Countryman, S. T., Couvares, P., Cowan, E. E., Coward, D. M., Cowart, M. J., Coyne, D. C., Coyne, R., Craig, K., Creighton, J. D. E., Cripe, J., Crowder, S. G., Cumming, A., Cunningham, L., Cuoco, E., Dal Canton, T., Danilishin, S. L., D Antonio, S., Danzmann, K., Darman, N. S., Dasgupta, A., Da Silva Costa, C. F., Dattilo, V., Dave, I., Davier, M., Davies, G. S., Daw, E. J., Day, R., De, S., Debra, D., Debreczeni, G., Degallaix, J., Laurentis, M., Del Eglise, S., Del Pozzo, W., Denker, T., Dent, T., Dergachev, V., Rosa, R., Derosa, R. T., Desalvo, R., Devine, R. C., Dhurandhar, S., D Iaz, M. C., Di Fiore, L., Di Giovanni, M., Di Girolamo, T., Di Lieto, A., Di Pace, S., Di Palma, I., Di Virgilio, A., Dolique, V., Donovan, F., Dooley, K. L., Doravari, S., Douglas, R., Downes, T. P., Drago, M., Drever, R. W. P., Driggers, J. C., Ducrot, M., Dwyer, S. E., Edo, T. B., Edwards, M. C., Effler, A., Eggenstein, H. -B, Ehrens, P., Eichholz, J., Eikenberry, S. S., Engels, W., Essick, R. C., Etzel, T., Evans, M., Evans, T. M., Everett, R., Factourovich, M., Fafone, V., Fair, H., Fairhurst, S., Fan, X., Fang, Q., Farinon, S., Farr, B., Farr, W. M., Favata, M., Fays, M., Fehrmann, H., Fejer, M. M., Fenyvesi, E., Ferrante, I., Ferreira, E. C., Ferrini, F., Fidecaro, F., Fiori, I., Fiorucci, D., Fisher, R. P., Flaminio, R., Fletcher, M., Fong, H., Fournier, J. -D, Frasca, S., Frasconi, F., Frei, Z., Freise, A., Frey, R., Frey, V., Fritschel, P., Frolov, V. V., Fulda, P., Fyffe, M., Gabbard, H. A. G., Gaebel, S., Gair, J. R., Gammaitoni, L., Gaonkar, S. G., Garufi, F., Gaur, G., Gehrels, N., Gemme, G., Geng, P., Genin, E., Gennai, A., George, J., Gergely, L., Germain, V., Ghosh, Abhirup, Ghosh, Archisman, Ghosh, S., Giaime, J. A., Giardina, K. D., Giazotto, A., Gill, K., Glaefke, A., Goetz, E., Goetz, R., Gondan, L., Gonz Alez, G., Gonzalez Castro, J. M., Gopakumar, A., Gordon, N. A., Gorodetsky, M. L., Gossan, S. E., Gosselin, M., Gouaty, R., Grado, A., Graef, C., Graff, P. B., Granata, M., Grant, A., Gras, S., Gray, C., Greco, G., Green, A. C., Paul Groot, Grote, H., Grunewald, S., Guidi, G. M., Guo, X., Gupta, A., Gupta, M. K., Gushwa, K. E., Gustafson, E. K., Gustafson, R., Hacker, J. J., Hall, B. R., Hall, E. D., Hamilton, H., Hammond, G., Haney, M., Hanke, M. M., Hanks, J., Hanna, C., Hannam, M. D., Hanson, J., Hardwick, T., Harms, J., Harry, G. M., Harry, I. W., Hart, M. J., Hartman, M. T., Haster, C. -J, Haughian, K., Healy, J., Heidmann, A., Heintze, M. C., Heitmann, H., Hello, P., Hemming, G., Hendry, M., Heng, I. S., Hennig, J., Henry, J., Heptonstall, A. W., Heurs, M., Hild, S., Hoak, D., Hofman, D., Holt, K., Holz, D. E., Hopkins, P., Hough, J., Houston, E. A., Howell, E. J., Hu, Y. M., Huang, S., Huerta, E. A., Huet, D., Hughey, B., Husa, S., Huttner, S. H., Huynh-Dinh, T., Indik, N., Ingram, D. R., Inta, R., Isa, H. N., Isac, J. -M, Isi, M., Isogai, T., Iyer, B. R., Izumi, K., Jacqmin, T., Jang, H., Jani, K., Jaranowski, P., Jawahar, S., Jian, L., Jim Enez-Forteza, F., Johnson, W. W., Johnson-Mcdaniel, N., Jones, D. I., Jones, R., Jonker, R. J. G., Ju, L., K, Haris, Kalaghatgi, C. V., Kalogera, V., Kandhasamy, S., Kang, G., Kanner, J. B., Kapadia, S. J., Karki, S., Karvinen, K. S., Kasprzack, M., Katsavounidis, E., Katzman, W., Kaufer, S., Kaur, T., Kawabe, K., K Ef Elian, F., Kehl, M. S., Keitel, D., Kelley, D. B., Kells, W., Kennedy, R., Key, J. S., Khalili, F. Y., Khan, I., Khan, S., Khan, Z., Khazanov, E. A., Kijbunchoo, N., Kim, Chi-Woong, Kim, Chunglee, Kim, J., Kim, K., Kim, N., Kim, W., Kim, Y. -M, Kimbrell, S. J., King, E. J., King, P. J., Kissel, J. S., Klein, B., Kleybolte, L., Klimenko, S., Koehlenbeck, S. M., Koley, S., Kondrashov, V., Kontos, A., Korobko, M., Korth, W. Z., Kowalska, I., Kozak, D. B., Kringel, V., Krishnan, B., Kr Olak, A., Krueger, C., Kuehn, G., Kumar, P., Kumar, R., Kuo, L., Kutynia, A., Lackey, B. D., Landry, M., Lange, J., Lantz, B., Lasky, P. D., Laxen, M., Lazzarini, A., Lazzaro, C., Leaci, P., Leavey, S., Lebigot, E. O., Lee, C. H., Lee, H. K., Lee, H. M., Lee, K., Lenon, A., Leonardi, M., Leong, J. R., Leroy, N., Letendre, N., Levin, Y., Lewis, J. B., Li, T. G. F., Libson, A., Littenberg, T. B., Lockerbie, N. A., Lombardi, A. L., London, L. T., Lord, J. E., Lorenzini, M., Loriette, V., Lormand, M., Losurdo, G., Lough, J. D., Lousto, C., Quot, L., Uck, H., Lundgren, A. P., Lynch, R., Ma, Y., Machenschalk, B., Macinnis, M., Macleod, D. M., Magana-Sandoval, F., Magana Zertuche, L., Magee, R. M., Majorana, E., Maksimovic, I., Malvezzi, V., Man, N., Mandel, I., Mandic, V., Mangano, V., Mansell, G. L., Manske, M., Mantovani, M., Marchesoni, F., Marion, F., M Arka, S., M Arka, Z., Markosyan, A. S., Maros, E., Martelli, F., Martellini, L., Martin, I. W., Martynov, D. V., Marx, J. N., Mason, K., Masserot, A., Massinger, T. J., Masso-Reid, M., Mastrogiovanni, S., Matichard, F., Matone, L., Mavalvala, N., Mazumder, N., Mccarthy, R., Mcclelland, D. E., Mccormick, S., Mcguire, S. C., Mcintyre, G., Mciver, J., Mcmanus, D. J., Mcrae, T., Mcwilliams, S. T., Meacher, D., Meadors, G. D., Meidam, J., Melatos, A., Mendell, G., Mercer, R. A., Merilh, E. L., Merzougui, M., Meshkov, S., Messenger, C., Messick, C., Metzdorff, R., Meyers, P. M., Mezzani, F., Miao, H., Michel, C., Middleton, H., Mikhailov, E. E., Milano, L., Miller, A. L., Miller, A., Miller, B. B., Miller, J., Millhouse, M., Minenkov, Y., Ming, J., Mirshekari, S., Mishra, C., Mitra, S., Mitrofanov, V. P., Mitselmakher, G., Mittleman, R., Moggi, A., Mohan, M., Mohapatra, S. R. P., Montani, M., Moore, B. C., Moore, C. J., Moraru, D., Moreno, G., Morriss, S. R., Mossavi, K., Mours, B., Mow-Lowry, C. M., Mueller, G., Muir, A. W., Mukherjee, Arunava, Mukherjee, D., Mukherjee, S., Mukund, N., Mullavey, A., Munch, J., Murphy, D. J., Murray, P. G., Mytidis, A., Nardecchia, I., Naticchioni, L., Nayak, R. K., Nedkova, K., Nelemans, G., Nelson, T. J. N., Neri, M., Neunzert, A., Newton, G., Nguyen, T. T., Nielsen, A. B., Nissanke, S., Nitz, A., Nocera, F., Nolting, D., Normandin, M. E. N., Nuttall, L. K., Oberling, J., Ochsner, E., O, J., Oelker, E., Ogin, G. H., Oh, J. J., Oh, S. H., Ohme, F., Oliver, M., Oppermann, P., Oram, Richard J., O Reilly, B., O Shaughnessy, R., Ottaway, D. J., Overmier, H., Owen, B. J., Pai, A., Pai, S. A., Palamos, J. R., Palashov, O., Palomba, C., Pal-Singh, A., Pan, H., Pan, Y., Pankow, C., Pannarale, F., Pant, B. C., Paoletti, F., Paoli, A., Papa, M. A., Paris, H. R., Parker, W., Pascucci, D., Pasqualetti, A., Passaquieti, R., Passuello, D., Patricelli, B., Patrick, Z., Pearlstone, B. L., Pedraza, M., Pedurand, R., Pekowsky, L., Pele, A., Penn, S., Perreca, A., Perri, L. M., Pfeiffer, H., Phelps, M., Piccinni, O. J., Pichot, M., Piergiovanni, F., Pierro, V., Pillant, G., Pinard, L., Pinto, I. M., Pitkin, M., Poe, M., Poggiani, R., Popolizio, P., Porter, E., Post, A., Powell, J., Prasad, J., Predoi, V., Prestegard, T., Price, L. R., Prijatelj, M., Principe, M., Privitera, S., Prix, R., Prodi, G. A., Prokhorov, L., Puncken, O., Punturo, M., Puppo, P., Quot, P., Urrer, M., Qi, H., Qin, J., Qiu, S., Quetschke, V., Quintero, E. A., Quitzow-James, R., Raab, F. J., Rabeling, D. S., Radkins, H., Raffai, P., Raja, S., Rajan, C., Rakhmanov, M., Rapagnani, P., Raymond, V., Razzano, M., Re, V., Read, J., Reed, C. M., Regimbau, T., Rei, L., Reid, S., Reitze, D. H., Rew, H., Reyes, S. D., Ricci, F., Riles, K., Rizzo, M., Robertson, N. A., Robie, R., Robinet, F., Rocchi, A., Rolland, L., Rollins, J. G., Roma, V. J., Romano, J. D., Romano, R., Romanov, G., Romie, J. H., Rosi Nska, D., Rowan, S., Quot, R., Udiger, A., Ruggi, P., Ryan, K., Sachdev, S., Sadecki, T., Sadeghian, L., Sakellariadou, M., Salconi, L., Saleem, M., Salemi, F., Samajdar, A., Sammut, L., Sanchez, E. J., Sandberg, V., Sandeen, B., Sanders, J. R., Sassolas, B., Sathyaprakash, B. S., Saulson, P. R., Sauter, O. E. S., Savage, R. L., Sawadsky, A., Schale, P., Schilling, R., Schmidt, J., Schmidt, P., Schnabel, R., Schofield, R. M. S., Sch&quot, Onbeck, A., Schreiber, E., Schuette, D., Schutz, B. F., Scott, J., Scott, S. M., Sellers, D., Sengupta, A. S., Sentenac, D., Sequino, V., Sergeev, A., Setyawati, Y., Shaddock, D. A., Shaffer, T., Shahriar, M. S., Shaltev, M., Shapiro, B., Shawhan, P., Sheperd, A., Shoemaker, D. H., Shoemaker, D. M., Siellez, K., Siemens, X., Sieniawska, M., Sigg, D., Silva, A. D., Singer, A., Singer, L. P., Singh, A., Singh, R., Singhal, A., Sintes, A. M., Slagmolen, B. J. J., Smith, J. R., Smith, N. D., Smith, R. J. E., Son, E. J., Sorazu, B., Sorrentino, F., Souradeep, T., Srivastava, A. K., Staley, A., Steinke, M., Steinlechner, J., Steinlechner, S., Steinmeyer, D., Stephens, B. C., Stevenson, S., Stone, R., Strain, K. A., Straniero, N., Stratta, G., Strauss, N. A., Strigin, S., Sturani, R., Stuver, A. L., Summerscales, T. Z., Sun, L., Sunil, S., Sutton, P. J., Swinkels, B. L., Szczepa Nczyk, M. J., Tacca, M., Talukder, D., Tanner, D. B., T Apai, M., Tarabrin, S. P., Taracchini, A., Taylor, R., Theeg, T., Thirugnanasambandam, M. P., Thomas, E. G., Thomas, M., Thomas, P., Thorne, K. A., Thrane, E., Tiwari, S., Tiwari, V., Tokmakov, K. V., Toland, K., Tomlinson, C., Tonelli, M., Tornasi, Z., Torres, C. V., Torrie, C. I., Quot, T., oyr&quot, A, D., Travasso, F., Traylor, G., Trifir O, D., Tringali, M. C., Trozzo, L., Tse, M., Turconi, M., Tuyenbayev, D., Ugolini, D., Unnikrishnan, C. S., Urban, A. L., Usman, S. A., Vahlbruch, H., Vajente, G., Valdes, G., Vallisneri, M., Bakel, N., Beuzekom, M., Den Brand, J. F. J., Den Broeck, C., Vander-Hyde, D. C., Schaaf, L., Heijningen, J. V., Veggel, A. A., Vardaro, M., Vass, S., Vas Uth, M., Vaulin, R., Vecchio, A., Vedovato, G., Veitch, J., Veitch, P. J., Venkateswara, K., Verkindt, D., Vetrano, F., Vicer E, A., Vinciguerra, S., Vine, D. J., Vinet, J. -Y, Vitale, S., Vo, T., Vocca, H., Vorvick, C., Voss, D. V., Vousden, W. D., Vyatchanin, S. P., Wade, A. R., Wade, L. E., Wade, M., Walker, M., Wallace, L., Walsh, S., Wang, G., Wang, H., Wang, M., Wang, X., Wang, Y., Ward, R. L., Warner, J., Was, M., Weaver, B., Wei, L. -W, Weinert, M., Weinstein, A. J., Weiss, R., Wen, L., Wessels, P., Westphal, T., Wette, K., Whelan, J. T., Whitcomb, S. E., Whiting, B. F., Williams, R. D., Williamson, A. R., Willis, J. L., Willke, B., Wimmer, M. H., Winkler, W., Wipf, C. C., Wittel, H., Woan, G., Woehler, J., Worden, J., Wright, J. L., Wu, D. S., Wu, G., Yablon, J., Yam, W., Yamamoto, H., Yancey, C. C., Yu, H., Yvert, M., Zadro Zny, A., Zangrando, L., Zanolin, M., Zendri, J. -P, Zevin, M., Zhang, L., Zhang, M., Zhang, Y., Zhao, C., Zhou, M., Zhou, Z., Zhu, X. J., Zucker, M. E., Zuraw, S. E., Zweizig, J., Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Laboratoire des matériaux avancés (LMA), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Astrophysique Relativiste Théories Expériences Métrologie Instrumentation Signaux (ARTEMIS), Centre National de la Recherche Scientifique (CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Nice Sophia Antipolis (... - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA), Institut de Physique de Rennes (IPR), Université de Rennes 1 (UR1), Université de Rennes (UNIV-RENNES)-Université de Rennes (UNIV-RENNES)-Centre National de la Recherche Scientifique (CNRS), Science and Engineering Research Board, Royal Society, Canadian Institute for Advanced Research, Natural Sciences and Engineering Research Council Canada, Science and Technology Facilities Council, Ontario Ministry of Economic Development and Innovation, Ministerio de Economía y Competitividad, Scottish Funding Council, European Commission, Fundação de Amparo à Pesquisa do Estado de São Paulo, Australian Research Council, Narodowe Centrum Nauki, Országos Tudományos Kutatási Alapprogramok, Centre National de la Recherche Scientifique, Max-Planck-Gesellschaft, Research Corporation for Science Advancement, National Science Foundation, Leverhulme Trust, Ministry of Science and Technology of the People’s Republic of China, Conselleria d’Economia i Competitivitat and Conselleria d’Educació, Cultura i Universitats of the Govern de les Illes Balears, Lyon Institute of Origins, Brazilian Ministry of Science, Technology, and Innovation, Ministry of Human Resource Development, Kavli Foundation, Scottish Universities Physics Alliance, Istituto Nazionale di Fisica Nucleare, National Research Foundation of Korea, Nederlandse Organisatie voor Wetenschappelijk Onderzoek, Russian Foundation for Basic Research, VIRGO, LIGO, Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Nice Sophia Antipolis (1965 - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Université de Rennes (UR)-Centre National de la Recherche Scientifique (CNRS), California Institute of Technology, Louisiana State University, American University, Università di Salerno, Complesso Universitario di Monte S.Angelo, LIGO Livingston Observatory, CNRS/IN2P3, University of Sannio at Benevento, Max-Planck-Institut für Gravitationsphysik, Science Park, Massachusetts Institute of Technology, Instituto Nacional de Pesquisas Espaciais, Gran Sasso Science Institute, Sezione di Roma Tor Vergata, Inter-University Centre for Astronomy and Astrophysics, Tata Institute of Fundamental Research, Leibniz Universität Hannover, Università di Pisa, Sezione di Pisa, Australian National University, The University of Mississippi, California State University Fullerton, Université Paris-Saclay, Chennai Mathematical Institute, Università di Roma Tor Vergata, University of Southampton, Universität Hamburg, Sezione di Roma, Max-Planck-Institut für Gravitations-physik, Observatoire de Paris, Montana State University, Università di Perugia, Sezione di Perugia, European Gravitational Observatory (EGO), Syracuse University, University of Glasgow, LIGO Hanford Observatory, RMKI, Columbia University, Stanford University, Dipartimento di Fisica e Astronomia, Sezione di Padova, CAMK-PAN, University of Birmingham, Università degli Studi di Genova, Sezione di Genova, RRCAT, Lomonosov Moscow State University, University of the West of Scotland, University of Western Australia, Radboud University Nijmegen, CNRS, Université de Rennes 1, Washington State University, Università degli Studi di Urbino Carlo Bo, Sezione di Firenze, University of Oregon, Collège de France, Carleton College, Astronomical Observatory Warsaw University, VU University Amsterdam, University of Maryland, Georgia Institute of Technology, Université Claude Bernard Lyon 1, NASA/Goddard Space Flight Center, University of Tokyo, Tsinghua University, Texas Tech University, The Pennsylvania State University, National Tsing Hua University, Charles Sturt University, West Virginia University, University of Chicago, Caltech CaRT, Korea Institute of Science and Technology Information, Università di Roma La Sapienza, University of Brussels, Sonoma State University, Northwestern University, University of Minnesota, The University of Melbourne, Institute for Plasma Research, The University of Sheffield, The University of Texas Rio Grande Valley, Dipartimento di Fisica, Trento Institute for Fundamental Physics and Applications, Cardiff University, Montclair State University, Lendulet Astrophysics Research Group, National Astronomical Observatory of Japan, Canadian Institute for Theoretical Astrophysics,University of Toronto, University of Edinburgh, Indian Institute of Technology, University of Szeged, Embry-Riddle Aeronautical University, Osservatorio Astronomico di Capodimonte, University of Michigan, Abilene Christian University, Rochester Institute of Technology, University of Illinois at Urbana-Champaign, IAC3-IEEC, University of Bialystok, University of Strathclyde, IISER-TVM, Institute of Applied Physics, Pusan National University, Hanyang University, University of Adelaide, NCBJ, IM-PAN, Monash University, Seoul National University, The Chinese University of Hong Kong, University of Alabama in Huntsville, University of Massachusetts-Amherst, Southern University and A and M College, College of William and Mary, Universidade Estadual Paulista (UNESP), University of Cambridge, IISER-Kolkata, HSIC, Whitman College, National Institute for Mathematical Sciences, Université de Lyon, Hobart and William Smith Colleges, University of Zielona Góra, University of London, Andrews University, Università di Siena, Trinity University, University of Washington, Kenyon College, Sezione di Napoli, Laboratoire d'Annecy de Physique des Particules ( LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules ), Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Savoie Mont Blanc ( USMB [Université de Savoie] [Université de Chambéry] ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire des matériaux avancés ( LMA ), Université Claude Bernard Lyon 1 ( UCBL ), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire de l'Accélérateur Linéaire ( LAL ), Université Paris-Sud - Paris 11 ( UP11 ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ), Astrophysique Relativiste Théories Expériences Métrologie Instrumentation Signaux ( ARTEMIS ), Université Nice Sophia Antipolis ( UNS ), Université Côte d'Azur ( UCA ) -Université Côte d'Azur ( UCA ) -Institut national des sciences de l'Univers ( INSU - CNRS ) -Observatoire de la Côte d'Azur, Université Côte d'Azur ( UCA ) -Centre National de la Recherche Scientifique ( CNRS ), Institut de Physique de Rennes ( IPR ), Université de Rennes 1 ( UR1 ), Université de Rennes ( UNIV-RENNES ) -Université de Rennes ( UNIV-RENNES ) -Centre National de la Recherche Scientifique ( CNRS ), Massachusetts Institute of Technology. Department of Physics, LIGO (Observatory : Massachusetts Institute of Technology), MIT Kavli Institute for Astrophysics and Space Research, Katsavounidis, Erotokritos, Kontos, Antonios, Libson, Adam A., Lynch, Ryan Christopher, MacInnis, Myron E, Martynov, Denis, Mason, Kenneth R, Matichard, Fabrice, Mavalvala, Nergis, Miller, John, Mittleman, Richard K, Ray Pitambar Mohapatra, Satyanarayan, Oelker, Eric Glenn, Shoemaker, David H, Tse, Maggie, Vaulin, Ruslan, Vitale, Salvatore, Weiss, Rainer, Yam, William, Yu, Haocun, Zucker, Michael E, The LIGO Scientific Collaboration, The VIRGO Collaboration, (Astro)-Particles Physics, CALTECH, Louisiana State Univ, Amer Univ, Univ Salerno, Ist Nazl Fis Nucl, Univ Florida, LIGO Livingston Observ, Univ Savoie Mont Blanc, Univ Sannio Benevento, Max Planck Inst Gravitat Phys, Nikhef, MIT, Inst Nacl Pesquisas Espaciais, Interuniv Ctr Astron & Astrophys, Tata Inst Fundamental Res, Univ Wisconsin, Leibniz Univ Hannover, Univ Pisa, Australian Natl Univ, Univ Mississippi, Calif State Univ Fullerton, Univ Paris 11, Chennai Math Inst, Univ Roma Tor Vergata, Univ Southampton, Univ Hamburg, Universidade de São Paulo (USP), Montana State Univ, Univ Perugia, EGO, Syracuse Univ, Univ Glasgow, LIGO Hanford Observ, Wigner RCP, Columbia Univ, Stanford Univ, Univ Padua, CAMK PAN, Univ Birmingham, Univ Genoa, Lomonosov Moscow State Univ, Univ West Scotland, Univ Western Australia, Radboud Univ Nijmegen, Univ Cote dAzur, Univ Rennes 1, Washington State Univ, Univ Urbino Carlo Bo, Univ Oregon, UPMC Sorbonne Univ, Carleton Coll, Warsaw Univ, Vrije Univ Amsterdam, Univ Maryland, Georgia Inst Technol, CNRS IN2P3, Univ Lyon 1, Univ Naples Federico II, NASA, Univ Tokyo, Tsinghua Univ, Texas Tech Univ, Penn State Univ, Natl Tsing Hua Univ, Charles Sturt Univ, West Virginia Univ, Univ Chicago, Korea Inst Sci & Technol Informat, Univ Roma La Sapienza, Univ Brussels, Sonoma State Univ, Northwestern Univ, Univ Minnesota, Univ Melbourne, Inst Plasma Res, Univ Sheffield, Univ Texas Rio Grande Valley, Univ Trento, Cardiff Univ, Montclair State Univ, MTA Eotvos Univ, Natl Astron Observ Japan, Univ Toronto, Univ Edinburgh, Indian Inst Technol, Univ Szeged, Embry Riddle Aeronaut Univ, Osserv Astron Capodimonte, Univ Michigan, Abilene Christian Univ, Rochester Inst Technol, Univ Illinois, Univ Illes Balears, Univ Bialystok, Univ Strathclyde, IISER TVM, Inst Appl Phys, Pusan Natl Univ, Hanyang Univ, Univ Adelaide, IM PAN, Monash Univ, Seoul Natl Univ, Chinese Univ Hong Kong, Univ Alabama, Univ Massachusetts, Univ Camerino, Southern Univ & A&M Coll, Coll William & Mary, Universidade Estadual Paulista (Unesp), Univ Cambridge, IISER Kolkata, Rutherford Appleton Lab, Whitman Coll, Natl Inst Math Sci, Univ Lyon, Hobart & William Smith Coll, Univ Zielona Gora, Univ London, Andrews Univ, Univ Siena, Trinity Univ, Univ Washington, Kenyon Coll, Abbott, B. .p., Abbott, R., Abbott, T. .d., Abernathy, M. .r., Acernese, F., Ackley, K., Adams, C., Adams, T., Addesso, P., Adhikari, R. .x., Adya, V. .b., Affeldt, C., Agathos, M., Agatsuma, K., Aggarwal, N., Aguiar, O. .d., Aiello, L., Ain, A., Ajith, P., Allen, B., Allocca, A., Altin, P. .a., Anderson, S. .b., Anderson, W. .g., Arai, K., Araya, M. .c., Arceneaux, C. .c., Areeda, J. .s., Arnaud, N., Arun, K. .g., Ascenzi, S., Ashton, G., Ast, M., Aston, S. .m., Astone, P., Aufmuth, P., Aulbert, C., Babak, S., Bacon, P., Bader, M. .k. .m., Baker, P. .t., Baldaccini, F., Ballardin, G., Ballmer, S. .w., Barayoga, J. .c., Barclay, S. .e., Barish, B. .c., Barker, D., Barone, F., Barr, B., Barsotti, L., Barsuglia, M., Barta, D., Bartlett, J., Bartos, I., Bassiri, R., Basti, A., Batch, J. .c., Baune, C., Bavigadda, V., Bazzan, M., Bejger, M., Bell, A. .s., Berger, B. .k., Bergmann, G., Berry, C. .p. .l., Bersanetti, D., Bertolini, A., Betzwieser, J., Bhagwat, S., Bhandare, R., Bilenko, I. .a., Billingsley, G., Birch, J., Birney, R., Birnholtz, O., Biscans, S., Bisht, A., Bitossi, M., Biwer, C., Bizouard, M. .a., Blackburn, J. .k., Blair, C. .d., Blair, D. .g., Blair, R. .m., Bloemen, S., Bock, O., Boer, M., Bogaert, G., Bogan, C., Bohe, A., Bond, C., Bondu, F., Bonnand, R., Boom, B. .a., Bork, R., Boschi, V., Bose, S., Bouffanais, Y., Bozzi, A., Bradaschia, C., Brady, P. .r., Braginsky, V. .b., BRANCHESI, MARICA, Brau, J. .e., Briant, T., Brillet, A., Brinkmann, M., Brisson, V., Brockill, P., Broida, J. .e., Brooks, A. .f., Brown, D. .a., Brown, D. .d., Brown, N. .m., Brunett, S., Buchanan, C. .c., Buikema, A., Bulik, T., Bulten, H. .j., Buonanno, A., Buskulic, D., Buy, C., Byer, R. .l., Cabero, M., Cadonati, L., Cagnoli, G., Cahillane, C., Calderón Bustillo, J., Callister, T., Calloni, E., Camp, J. .b., Cannon, K. .c., Cao, J., Capano, C. .d., Capocasa, E., Carbognani, F., Caride, S., Casanueva Diaz, J., Casentini, C., Caudill, S., Cavaglià, M., Cavalier, F., Cavalieri, R., Cella, G., Cepeda, C. .b., CERBONI BAIARDI, LORENZO, Cerretani, G., Cesarini, E., Chamberlin, S. .j., Chan, M., Chao, S., Charlton, P., Chassande Mottin, E., Cheeseboro, B. .d., Chen, H. .y., Chen, Y., Cheng, C., Chincarini, A., Chiummo, A., Cho, H. .s., Cho, M., Chow, J. .h., Christensen, N., Chu, Q., Chua, S., Chung, S., Ciani, G., Clara, F., Clark, J. .a., Cleva, F., Coccia, E., Cohadon, P. F., Colla, A., Collette, C. .g., Cominsky, L., Constancio, M., Conte, A., Conti, L., Cook, D., Corbitt, T. .r., Cornish, N., Corsi, A., Cortese, S., Costa, C. .a., Coughlin, M. .w., Coughlin, S. .b., Coulon, J. P., Countryman, S. .t., Couvares, P., Cowan, E. .e., Coward, D. .m., Cowart, M. .j., Coyne, D. .c., Coyne, R., Craig, K., Creighton, J. .d. .e., Cripe, J., Crowder, S. .g., Cumming, A., Cunningham, L., Cuoco, E., Dal Canton, T., Danilishin, S. .l., D’Antonio, S., Danzmann, K., Darman, N. .s., Dasgupta, A., Da Silva Costa, C. .f., Dattilo, V., Dave, I., Davier, M., Davies, G. .s., Daw, E. .j., Day, R., De, S., Debra, D., Debreczeni, G., Degallaix, J., De Laurentis, M., Deléglise, S., Del Pozzo, W., Denker, T., Dent, T., Dergachev, V., De Rosa, R., Derosa, R. .t., Desalvo, R., Devine, R. .c., Dhurandhar, S., Díaz, M. .c., Di Fiore, L., Di Giovanni, M., Di Girolamo, T., Di Lieto, A., Di Pace, S., Di Palma, I., Di Virgilio, A., Dolique, V., Donovan, F., Dooley, K. .l., Doravari, S., Douglas, R., Downes, T. .p., Drago, M., Drever, R. .w. .p., Driggers, J. .c., Ducrot, M., Dwyer, S. .e., Edo, T. .b., Edwards, M. .c., Effler, A., Eggenstein, H. B., Ehrens, P., Eichholz, J., Eikenberry, S. .s., Engels, W., Essick, R. .c., Etzel, T., Evans, M., Evans, T. .m., Everett, R., Factourovich, M., Fafone, V., Fair, H., Fairhurst, S., Fan, X., Fang, Q., Farinon, S., Farr, B., Farr, W. .m., Favata, M., Fays, M., Fehrmann, H., Fejer, M. .m., Fenyvesi, E., Ferrante, I., Ferreira, E. .c., Ferrini, F., Fidecaro, F., Fiori, I., Fiorucci, D., Fisher, R. .p., Flaminio, R., Fletcher, M., Fong, H., Fournier, J. D., Frasca, S., Frasconi, F., Frei, Z., Freise, A., Frey, R., Frey, V., Fritschel, P., Frolov, V. .v., Fulda, P., Fyffe, M., Gabbard, H. .a. .g., Gaebel, S., Gair, J. .r., Gammaitoni, L., Gaonkar, S. .g., Garufi, F., Gaur, G., Gehrels, N., Gemme, G., Geng, P., Genin, E., Gennai, A., George, J., Gergely, L., Germain, V., Ghosh, Abhirup, Ghosh, Archisman, Ghosh, S., Giaime, J. .a., Giardina, K. .d., Giazotto, A., Gill, K., Glaefke, A., Goetz, E., Goetz, R., Gondan, L., González, G., Gonzalez Castro, J. .m., Gopakumar, A., Gordon, N. .a., Gorodetsky, M. .l., Gossan, S. .e., Gosselin, M., Gouaty, R., Grado, A., Graef, C., Graff, P. .b., Granata, M., Grant, A., Gras, S., Gray, C., GRECO, GIUSEPPE, Green, A. .c., Groot, P., Grote, H., Grunewald, S., GUIDI, GIANLUCA MARIA, Guo, X., Gupta, A., Gupta, M. .k., Gushwa, K. .e., Gustafson, E. .k., Gustafson, R., Hacker, J. .j., Hall, B. .r., Hall, E. .d., Hamilton, H., Hammond, G., Haney, M., Hanke, M. .m., Hanks, J., Hanna, C., Hannam, M. .d., Hanson, J., Hardwick, T., HARMS, JAN, Harry, G. .m., Harry, I. .w., Hart, M. .j., Hartman, M. .t., Haster, C. J., Haughian, K., Healy, J., Heidmann, A., Heintze, M. .c., Heitmann, H., Hello, P., Hemming, G., Hendry, M., Heng, I. .s., Hennig, J., Henry, J., Heptonstall, A. .w., Heurs, M., Hild, S., Hoak, D., Hofman, D., Holt, K., Holz, D. .e., Hopkins, P., Hough, J., Houston, E. .a., Howell, E. .j., Hu, Y. .m., Huang, S., Huerta, E. .a., Huet, D., Hughey, B., Husa, S., Huttner, S. .h., Huynh Dinh, T., Indik, N., Ingram, D. .r., Inta, R., Isa, H. .n., Isac, J. M., Isi, M., Isogai, T., Iyer, B. .r., Izumi, K., Jacqmin, T., Jang, H., Jani, K., Jaranowski, P., Jawahar, S., Jian, L., Jiménez Forteza, F., Johnson, W. .w., Johnson McDaniel, N. .k., Jones, D. .i., Jones, R., Jonker, R. .j. .g., Ju, L., K, Hari, Kalaghatgi, C. .v., Kalogera, V., Kandhasamy, S., Kang, G., Kanner, J. .b., Kapadia, S. .j., Karki, S., Karvinen, K. .s., Kasprzack, M., Katsavounidis, E., Katzman, W., Kaufer, S., Kaur, T., Kawabe, K., Kéfélian, F., Kehl, M. .s., Keitel, D., Kelley, D. .b., Kells, W., Kennedy, R., Key, J. .s., Khalili, F. .y., Khan, I., Khan, S., Khan, Z., Khazanov, E. .a., Kijbunchoo, N., Kim, Chi Woong, Kim, Chunglee, Kim, J., Kim, K., Kim, N., Kim, W., Kim, Y. M., Kimbrell, S. .j., King, E. .j., King, P. .j., Kissel, J. .s., Klein, B., Kleybolte, L., Klimenko, S., Koehlenbeck, S. .m., Koley, S., Kondrashov, V., Kontos, A., Korobko, M., Korth, W. .z., Kowalska, I., Kozak, D. .b., Kringel, V., Krishnan, B., Królak, A., Krueger, C., Kuehn, G., Kumar, P., Kumar, R., Kuo, L., Kutynia, A., Lackey, B. .d., Landry, M., Lange, J., Lantz, B., Lasky, P. .d., Laxen, M., Lazzarini, A., Lazzaro, C., Leaci, P., Leavey, S., Lebigot, E. .o., Lee, C. .h., Lee, H. .k., Lee, H. .m., Lee, K., Lenon, A., Leonardi, M., Leong, J. .r., Leroy, N., Letendre, N., Levin, Y., Lewis, J. .b., Li, T. .g. .f., Libson, A., Littenberg, T. .b., Lockerbie, N. .a., Lombardi, A. .l., London, L. .t., Lord, J. .e., Lorenzini, M., Loriette, V., Lormand, M., Losurdo, G., Lough, J. .d., Lousto, C., Lück, H., Lundgren, A. .p., Lynch, R., Ma, Y., Machenschalk, B., Macinnis, M., Macleod, D. .m., Magaña Sandoval, F., Magaña Zertuche, L., Magee, R. .m., Majorana, E., Maksimovic, I., Malvezzi, V., Man, N., Mandel, I., Mandic, V., Mangano, V., Mansell, G. .l., Manske, M., Mantovani, M., Marchesoni, F., Marion, F., Márka, S., Márka, Z., Markosyan, A. .s., Maros, E., MARTELLI, FILIPPO, Martellini, L., Martin, I. .w., Martynov, D. .v., Marx, J. .n., Mason, K., Masserot, A., Massinger, T. .j., Masso Reid, M., Mastrogiovanni, S., Matichard, F., Matone, L., Mavalvala, N., Mazumder, N., Mccarthy, R., Mcclelland, D. .e., Mccormick, S., Mcguire, S. .c., Mcintyre, G., Mciver, J., Mcmanus, D. .j., Mcrae, T., Mcwilliams, S. .t., Meacher, D., Meadors, G. .d., Meidam, J., Melatos, A., Mendell, G., Mercer, R. .a., Merilh, E. .l., Merzougui, M., Meshkov, S., Messenger, C., Messick, C., Metzdorff, R., Meyers, P. .m., Mezzani, F., Miao, H., Michel, C., Middleton, H., Mikhailov, E. .e., Milano, L., Miller, A. .l., Miller, A., Miller, B. .b., Miller, J., Millhouse, M., Minenkov, Y., Ming, J., Mirshekari, S., Mishra, C., Mitra, S., Mitrofanov, V. .p., Mitselmakher, G., Mittleman, R., Moggi, A., Mohan, M., Mohapatra, S. .r. .p., MONTANI, MATTEO, Moore, B. .c., Moore, C. .j., Moraru, D., Moreno, G., Morriss, S. .r., Mossavi, K., Mours, B., Mow Lowry, C. .m., Mueller, G., Muir, A. .w., Mukherjee, Arunava, Mukherjee, D., Mukherjee, S., Mukund, N., Mullavey, A., Munch, J., Murphy, D. .j., Murray, P. .g., Mytidis, A., Nardecchia, I., Naticchioni, L., Nayak, R. .k., Nedkova, K., Nelemans, G., Nelson, T. .j. .n., Neri, M., Neunzert, A., Newton, G., Nguyen, T. .t., Nielsen, A. .b., Nissanke, S., Nitz, A., Nocera, F., Nolting, D., Normandin, M. .e. .n., Nuttall, L. .k., Oberling, J., Ochsner, E., O’Dell, J., Oelker, E., Ogin, G. .h., Oh, J. .j., Oh, S. .h., Ohme, F., Oliver, M., Oppermann, P., Oram, Richard J., O’Reilly, B., O’Shaughnessy, R., Ottaway, D. .j., Overmier, H., Owen, B. .j., Pai, A., Pai, S. .a., Palamos, J. .r., Palashov, O., Palomba, C., Pal Singh, A., Pan, H., Pan, Y., Pankow, C., Pannarale, F., Pant, B. .c., Paoletti, F., Paoli, A., Papa, M. .a., Paris, H. .r., Parker, W., Pascucci, D., Pasqualetti, A., Passaquieti, R., Passuello, D., Patricelli, B., Patrick, Z., Pearlstone, B. .l., Pedraza, M., Pedurand, R., Pekowsky, L., Pele, A., Penn, S., Perreca, A., Perri, L. .m., Pfeiffer, H. .p., Phelps, M., Piccinni, O. .j., Pichot, M., PIERGIOVANNI, FRANCESCO, Pierro, V., Pillant, G., Pinard, L., Pinto, I. .m., Pitkin, M., Poe, M., Poggiani, R., Popolizio, P., Porter, E., Post, A., Powell, J., Prasad, J., Predoi, V., Prestegard, T., Price, L. .r., Prijatelj, M., Principe, M., Privitera, S., Prix, R., Prodi, G. .a., Prokhorov, L., Puncken, O., Punturo, M., Puppo, P., Pürrer, M., Qi, H., Qin, J., Qiu, S., Quetschke, V., Quintero, E. .a., Quitzow James, R., Raab, F. .j., Rabeling, D. .s., Radkins, H., Raffai, P., Raja, S., Rajan, C., Rakhmanov, M., Rapagnani, P., Raymond, V., Razzano, M., Re, V., Read, J., Reed, C. .m., Regimbau, T., Rei, L., Reid, S., Reitze, D. .h., Rew, H., Reyes, S. .d., Ricci, F., Riles, K., Rizzo, M., Robertson, N. .a., Robie, R., Robinet, F., Rocchi, A., Rolland, L., Rollins, J. .g., Roma, V. .j., Romano, J. .d., Romano, R., Romanov, G., Romie, J. .h., Rosińska, D., Rowan, S., Rüdiger, A., Ruggi, P., Ryan, K., Sachdev, S., Sadecki, T., Sadeghian, L., Sakellariadou, M., Salconi, L., Saleem, M., Salemi, F., Samajdar, A., Sammut, L., Sanchez, E. .j., Sandberg, V., Sandeen, B., Sanders, J. .r., Sassolas, B., Sathyaprakash, B. .s., Saulson, P. .r., Sauter, O. .e. .s., Savage, R. .l., Sawadsky, A., Schale, P., Schilling, R., Schmidt, J., Schmidt, P., Schnabel, R., Schofield, R. .m. .s., Schönbeck, A., Schreiber, E., Schuette, D., Schutz, B. .f., Scott, J., Scott, S. .m., Sellers, D., Sengupta, A. .s., Sentenac, D., Sequino, V., Sergeev, A., Setyawati, Y., Shaddock, D. .a., Shaffer, T., Shahriar, M. .s., Shaltev, M., Shapiro, B., Shawhan, P., Sheperd, A., Shoemaker, D. .h., Shoemaker, D. .m., Siellez, K., Siemens, X., Sieniawska, M., Sigg, D., Silva, A. .d., Singer, A., Singer, L. .p., Singh, A., Singh, R., Singhal, A., Sintes, A. .m., Slagmolen, B. .j. .j., Smith, J. .r., Smith, N. .d., Smith, R. .j. .e., Son, E. .j., Sorazu, B., Sorrentino, F., Souradeep, T., Srivastava, A. .k., Staley, A., Steinke, M., Steinlechner, J., Steinlechner, S., Steinmeyer, D., Stephens, B. .c., Stevenson, S., Stone, R., Strain, K. .a., Straniero, N., STRATTA, MARIA GIULIANA, Strauss, N. .a., Strigin, S., Sturani, R., Stuver, A. .l., Summerscales, T. .z., Sun, L., Sunil, S., Sutton, P. .j., Swinkels, B. .l., Szczepańczyk, M. .j., Tacca, M., Talukder, D., Tanner, D. .b., Tápai, M., Tarabrin, S. .p., Taracchini, A., Taylor, R., Theeg, T., Thirugnanasambandam, M. .p., Thomas, E. .g., Thomas, M., Thomas, P., Thorne, K. .a., Thrane, E., Tiwari, S., Tiwari, V., Tokmakov, K. .v., Toland, K., Tomlinson, C., Tonelli, M., Tornasi, Z., Torres, C. .v., Torrie, C. .i., Töyrä, D., Travasso, F., Traylor, G., Trifirò, D., Tringali, M. .c., Trozzo, L., Tse, M., Turconi, M., Tuyenbayev, D., Ugolini, D., Unnikrishnan, C. .s., 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Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO), QC1-999, Astrophysics::High Energy Astrophysical Phenomena, Gravitational Wave, FOS: Physical sciences, General Physics and Astronomy, General Relativity and Quantum Cosmology (gr-qc), [ PHYS.ASTR.CO ] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], General Relativity and Quantum Cosmology, [ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], MAXIMUM MASS, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Physics and Astronomy (all), See paper for full list of authors - 15 pages + 4 appendices, 12 figures, Settore FIS/05 - Astronomia e Astrofisica, COMMON ENVELOPE, NEUTRON-STAR, LIGO, GENERAL-RELATIVITY, O1 run, QC, (POST)(5/2)-NEWTONIAN ORDER, QB, MASS-DISTRIBUTION, Gravitational Waves, GRAVITATIONAL-WAVE TRANSIENTS, Physics, Settore FIS/01 - Fisica Sperimentale, Binary Black Hole Merger, gravitational wave, black holes, Physics and Astronomy, Binary Black Hole Mergers, [PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], Gravitational Waves, Binary Black Hole Mergers, O1 run, LIGO, INSPIRALLING COMPACT BINARIES, Astrophysics - Cosmology and Nongalactic Astrophysics, PARAMETER-ESTIMATION, COALESCING BINARIES
Abstract: The first observational run of the Advanced LIGO detectors, from September 12, 2015 to January 19, 2016, saw the first detections of gravitational waves from binary black hole mergers. In this paper we present full results from a search for binary black hole merger signals with total masses up to $100 M_\odot$ and detailed implications from our observations of these systems. Our search, based on general-relativistic models of gravitational wave signals from binary black hole systems, unambiguously identified two signals, GW150914 and GW151226, with a significance of greater than $5\sigma$ over the observing period. It also identified a third possible signal, LVT151012, with substantially lower significance, and with an 87% probability of being of astrophysical origin. We provide detailed estimates of the parameters of the observed systems. Both GW150914 and GW151226 provide an unprecedented opportunity to study the two-body motion of a compact-object binary in the large velocity, highly nonlinear regime. We do not observe any deviations from general relativity, and place improved empirical bounds on several high-order post-Newtonian coefficients. From our observations we infer stellar-mass binary black hole merger rates lying in the range $9-240 \mathrm{Gpc}^{-3} \mathrm{yr}^{-1}$. These observations are beginning to inform astrophysical predictions of binary black hole formation rates, and indicate that future observing runs of the Advanced detector network will yield many more gravitational wave detections., Comment: 36 pages + 4 appendices, 14 figures; updated author list and references, final journal version, with appended Erratum for figures 7 and 8
Published: 2016

16. Search for Narrow Resonances in Dijet Final States at root s=8 TeV with the Novel CMS Technique of Data Scouting

Author: Khachatryan, V., Sirunyan, A. M., Tumasyan, A., Adam, W., Asilar, E., Bergauer, T., Brandstetter, J., Brondolin, E., Dragicevic, M., Eroe, J., Flechl, M., Friedl, M., Fruehwirth, R., Ghete, V. M., Hartl, C., Hoermann, N., Hrubec, J., Jeitler, M., Koenig, A., Kraetschmer, I., Liko, D., Matsushita, T., Mikulec, I., Rabady, D., Rad, N., Rahbaran, B., Rohringer, H., Schieck, J., Strauss, J., Treberer Treberspurg, W., Waltenberger, W., Wulz, C. E., Mossolov, V., Shumeiko, N., Gonzalez, J. Suarez, Alderweireldt, S., De Wolf, E. A., Janssen, X., Knutsson, A., Lauwers, J., Van De Klundert, M., Van Haevermaet, H., Van Mechelen, P., Van Remortel, N., Van Spilbeeck, A., Abu Zeid, S., Blekman, F., D'Hondt, J., Daci, N., De Bruyn, I., Deroover, K., Heracleous, N., Lowette, S., Moortgat, S., Moreels, L., Olbrechts, A., Python, Q., Tavernier, S., Van Doninck, W., Van Mulders, P., Van Parijs, I., Brun, H., Caillol, C., Clerbaux, B., De Lentdecker, G., Delannoy, H., Fasanella, G., Favart, L., Goldouzian, R., Grebenyuk, A., Karapostoli, G., Lenzi, T., Leonard, A., Luetic, J., Maerschalk, T., Marinov, A., Randle conde, A., Seva, T., Vander Velde, C., Vanlaer, P., Yonamine, R., Zenoni, F., Zhang, F., Cimmino, A., Cornelis, T., Dobur, D., Fagot, A., Garcia, G., Gul, M., Mccartin, J., Poyraz, D., Salva, S., Schofbeck, R., Tytgat, M., Van Driessche, W., Yazgan, E., Zaganidis, N., Beluffi, C., Bondu, O., Brochet, S., Bruno, G., Caudron, A., Ceard, L., De Visscher, S., Delaere, C., Delcourt, M., Forthomme, L., Francois, B., Giammanco, A., Jafari, A., Jez, P., Komm, M., Lemaitre, V., Magitteri, A., Mertens, A., Musich, M., Nuttens, C., Piotrzkowski, K., Quertenmont, L., Selvaggi, M., Marono, M. 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P., Redjimi, R., Roberts, J., Rorie, J., Tu, Z., Zabel, J., Betchart, B., Bodek, A., de Barbaro, P., Demina, R., Duh, Y. T., Ferbel, T., Galanti, M., Garcia Bellido, A., Han, J., Hindrichs, O., Khukhunaishvili, A., K. H., Lo, Tan, P., Verzetti, M., Chou, J. P., Contreras Campana, E., Gershtein, Y., Espinosa, T. A. Gomez, Halkiadakis, E., Heindl, M., Hidas, D., Hughes, E., Kaplan, S., Elayavalli, R. Kunnawalkam, Kyriacou, S., Lath, A., Nash, K., Saka, H., Salur, S., Schnetzer, S., Sheffield, D., Somalwar, S., Stone, R., Thomas, S., Thomassen, P., Walker, M., Foerster, M., Heideman, J., Riley, G., Rose, K., Spanier, S., Thapa, K., Bouhali, O., Hernandez, A. Castaneda, Celik, A., Dalchenko, M., De Mattia, M., Delgado, A., Dildick, S., Eusebi, R., Gilmore, J., Huang, T., Juska, E., Kamon, T., Krutelyov, V., Mueller, R., Pakhotin, Y., Patel, R., Perloff, A., Pernie, L., Rathjens, D., Safonov, A., Tatarinov, A., Ulmer, K. A., Akchurin, N., Cowden, C., Damgov, J., Dragoiu, C., Dudero, P. R., Faulkner, J., Kunori, S., Lamichhane, K., Libeiro, T., Undleeb, S., Volobouev, I., Delannoy, A. G., Greene, S., Gurrola, A., Janjam, R., Johns, W., Maguire, C., Melo, A., Ni, H., Sheldon, P., Tuo, S., Velkovska, J., Xu, Q., Arenton, M. W., Barria, P., Cox, B., Goodell, J., Hirosky, R., Ledovskoy, A., Li, H., Neu, C., Sinthuprasith, T., Sun, X., Wang, Y., Wolfe, E., Xia, F., Clarke, C., Harr, R., Karchin, P. E., Lamichhane, P., Sturdy, J., Belknap, D. A., Dasu, S., Dodd, L., Duric, S., Gomber, B., Grothe, M., Herndon, M., Herve, A., Klabbers, P., Lanaro, A., Levine, A., Long, K., Loveless, R., Ojalvo, I., Perry, T., Pierro, G. A., Polese, G., Ruggles, T., Savin, A., Smith, N., Smith, W. H., Taylor, D., Verwilligen, P., Woods, N., Yerevan Phys Inst, Inst Hochenergiephys OeAW, Natl Ctr Particle & High Energy Phys, Univ Antwerp, Vrije Univ Brussel, Univ Libre Bruxelles, Univ Ghent, Catholic Univ Louvain, Univ Mons, Ctr Brasileiro Pesquisas Fis, Universidade do Estado do Rio de Janeiro (UERJ), Universidade Estadual Paulista (Unesp), Universidade Federal do ABC (UFABC), Inst Nucl Energy Res, Univ Sofia, Beihang Univ, Inst High Energy Phys, Peking Univ, Univ Los Andes, Univ Split, Rudjer Boskovic Inst, Univ Cyprus, Charles Univ Prague, Univ San Francisco Quito, Acad Sci Res & Technol Arab Republ Egypt, NICPB, Univ Helsinki, Helsinki Inst Phys, Lappeenranta Univ Technol, CEA Saclay, Ecole Polytech, Univ Haute Alsace Mulhouse, CNRS, Univ Lyon 1, Georgian Tech Univ, Tbilisi State Univ, Rhein Westfal TH Aachen, Deutsches Elektronen Synchrotron, Univ Hamburg, Inst Expt Kernphys, NCSR Demokritos, Univ Athens, Univ Ioannina, Eotvos Lorand Univ, Wigner Res Ctr Phys, Inst Nucl Res ATOMKI, Univ Debrecen, Natl Inst Sci Educ & Res, Panjab Univ, Univ Delhi, Saha Inst Nucl Phys, Indian Inst Technol, Bhabha Atom Res Ctr, Tata Inst Fundamental Res A, Tata Inst Fundamental Res B, IISER, Inst Res Fundamental Sci IPM, Univ Coll Dublin, Ist Nazl Fis Nucl, Univ Bari, Politecn Bari, Univ Bologna, Univ Catania, Univ Florence, Univ Genoa, Univ Milano Bicocca, Univ Napoli Federico II, Univ Basilicata, Univ G Marconi, Univ Padua, Univ Trento, Univ Pavia, Univ Perugia, Univ Pisa, Scuola Normale Super Pisa, Univ Roma, Univ Turin, Univ Piemonte Orientale, Univ Trieste, Kyungpook Natl Univ, Chonbuk Natl Univ, Hanyang Univ, Korea Univ, Seoul Natl Univ, Univ Seoul, Sungkyunkwan Univ, Vilnius Univ, Univ Malaya, Ctr Invest & Estudios Avanzados IPN, Univ Iberoamer, Benemerita Univ Autonoma Puebla, Univ Autonoma San Luis Potosi, Univ Auckland, Univ Canterbury, Quaid I Azam Univ, Natl Ctr Nucl Res, Univ Warsaw, Lab Instrumentacao & Fis Expt Particulas, Joint Inst Nucl Res, Petersburg Nucl Phys Inst, Inst Nucl Res, Inst Theoret & Expt Phys, Natl Res Nucl Univ, PN Lebedev Phys Inst, Lomonosov Moscow State Univ, Univ Belgrade, Vinca Inst Nucl Sci, Ctr Invest Energet Medioambient & Tecnol CIEMAT, Univ Autonoma Madrid, Univ Oviedo, Univ Cantabria, European Org Nucl Res, Paul Scherrer Inst, Swiss Fed Inst Technol, Univ Zurich, Natl Cent Univ, NTU, Chulalongkorn Univ, Cukurova Univ, Middle East Tech Univ, Bogazici Univ, Istanbul Tech Univ, Natl Acad Sci Ukraine, Kharkov Inst Phys & Technol, Univ Bristol, Rutherford Appleton Lab, Imperial Coll, Brunel Univ, Baylor Univ, Univ Alabama, Boston Univ, Brown Univ, Univ Calif Davis, Univ Calif Los Angeles, Univ Calif Riverside, Univ Calif San Diego, Univ Calif Santa Barbara, CALTECH, Carnegie Mellon Univ, Univ Colorado, Cornell Univ, Fairfield Univ, Fermilab Natl Accelerator Lab, Univ Florida, Florida Int Univ, Florida State Univ, Florida Inst Technol, UIC, Univ Iowa, Johns Hopkins Univ, Univ Kansas, Kansas State Univ, Lawrence Livermore Natl Lab, Univ Maryland, MIT, Univ Minnesota, Univ Mississippi, Univ Nebraska, SUNY Buffalo, Northeastern Univ, Northwestern Univ, Univ Notre Dame, Ohio State Univ, Princeton Univ, Univ Puerto Rico, Purdue Univ, Purdue Univ Calumet, Rice Univ, Univ Rochester, Rutgers State Univ, Univ Tennessee, Texas A&M Univ, Texas Tech Univ, Vanderbilt Univ, Univ Virginia, Wayne State Univ, Univ Wisconsin, Vienna Univ Technol, Universidade Estadual de Campinas (UNICAMP), British Univ Egypt, Zewail City Sci & Technol, Fayoum Univ, Ain Shams Univ, Univ Haute Alsace, Brandenburg Tech Univ Cottbus, Indian Inst Sci Educ & Res, Inst Phys, Visva Bharati Univ, Univ Ruhuna, Isfahan Univ Technol, Univ Tehran, Islamic Azad Univ, Univ Siena, Int Islamic Univ Malaysia, Agensi Nuklear Malaysia, Consejo Nacl Ciencia & Technol, Warsaw Univ Technol, St Petersburg State Polytech Univ, Natl Tech Univ Athens, Riga Tech Univ, Albert Einstein Ctr Fundamental Phys, Adiyaman Univ, Mersin Univ, Cag Univ, Piri Reis Univ, Gaziosmanpasa Univ, Ozyegin Univ, Izmir Inst Technol, Marmara Univ, Kafkas Univ, Istanbul Bilgi Univ, Yildiz Tech Univ, Hacettepe Univ, Univ Southampton, Inst Astrofis Canarias, Utah Valley Univ, Argonne Natl Lab, Erzincan Univ, and Mimar Sinan Univ
Subjects: BOSONS, SPECTRUM, Science & Technology, FISICA DELLE PARTICELLE, Physics, Physics, Multidisciplinary, P(P)OVER-BAR COLLISIONS, QUARK, HADRON COLLIDERS, Physics and Astronomy (all), MASS-DISTRIBUTION, Physical Sciences, High Energy Physics::Experiment
Abstract: Made available in DSpace on 2018-11-27T17:35:16Z (GMT). No. of bitstreams: 0 Previous issue date: 2016-07-14 BMWFW (Austria) FWF (Austria) FNRS (Belgium) FWO (Belgium) Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq) Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES) Fundação de Amparo à Pesquisa do Estado do Rio de Janeiro (FAPERJ) Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP) MES (Bulgaria) CERN CAS (China) MoST (China) NSFC (China) COLCIENCIAS (Colombia) MSES (Croatia) CSF (Croatia) RPF (Cyprus) MoER (Estonia) ERC IUT (Estonia) ERDF (Estonia) Academy of Finland (Finland) MEC (Finland) HIP (Finland) CEA (France) CNRS/IN2P3 (France) BMBF (Germany) DFG (Germany) HGF (Germany) GSRT (Greece) OTKA (Hungary) NIH (Hungary) DAE (India) DST (India) IPM (Iran) SFI (Ireland) INFN (Italy) MSIP (Republic of Korea) NRF (Republic of Korea) LAS (Lithuania) MOE (Malaysia) UM (Malaysia) BUAP (Mexico) CINVESTAV (Mexico) CONACYT (Mexico) LNS (Mexico) SEP (Mexico) UASLP-FAI (Mexico) MBIE (New Zealand) PAEC (Pakistan) MSHE (Poland) NSC (Poland) FCT (Portugal) JINR (Dubna) MON (Russia) RosAtom (Russia) RAS (Russia) RFBR (Russia) MESTD (Serbia) SEIDI (Spain) CPAN (Spain) Swiss Funding Agencies (Switzerland) MST (Taipei) ThEPCenter (Thailand) IPST (Thailand) STAR (Thailand) NSTDA (Thailand) TUBITAK (Turkey) TAEK (Turkey) NASU (Ukraine) SFFR (Ukraine) STFC (United Kingdom) DOE (USA) NSF (USA) A search for narrow resonances decaying into dijet final states is performed on data from proton-proton collisions at a center-of-mass energy of 8 TeV, corresponding to an integrated luminosity of 18.8 fb(-1). The data were collected with the CMS detector using a novel technique called data scouting, in which the information associated with these selected events is much reduced, permitting collection of larger data samples. This technique enables CMS to record events containing jets at a rate of 1 kHz, by collecting the data from the high-level-trigger system. In this way, the sensitivity to low-mass resonances is increased significantly, allowing previously inaccessible couplings of new resonances to quarks and gluons to be probed. The resulting dijet mass distribution yields no evidence of narrow resonances. Upper limits are presented on the resonance cross sections as a function of mass, and compared with a variety of models predicting narrow resonances. The limits are translated into upper limits on the coupling of a leptophobic resonance Z'(B) to quarks, improving on the results obtained by previous experiments for the mass range from 500 to 800 GeV. Yerevan Phys Inst, Yerevan, Armenia Inst Hochenergiephys OeAW, Vienna, Austria Natl Ctr Particle & High Energy Phys, Minsk, Byelarus Univ Antwerp, Antwerp, Belgium Vrije Univ Brussel, Brussels, Belgium Univ Libre Bruxelles, Brussels, Belgium Univ Ghent, Ghent, Belgium Catholic Univ Louvain, Louvain La Neuve, Belgium Univ Mons, Mons, Belgium Ctr Brasileiro Pesquisas Fis, Rio De Janeiro, Brazil Univ Estado Rio de Janeiro, Rio De Janeiro, Brazil Univ Estadual Paulista, Sao Paulo, Brazil Univ Fed ABC, Sao Paulo, Brazil Inst Nucl Energy Res, Sofia, Bulgaria Univ Sofia, Sofia, Bulgaria Beihang Univ, Beijing, Peoples R China Inst High Energy Phys, Beijing, Peoples R China Peking Univ, State Key Lab Nucl Phys & Technol, Beijing, Peoples R China Univ Los Andes, Bogota, Colombia Univ Split, Fac Elect Engn Mech Engn & Naval Architecture, Split, Croatia Univ Split, Fac Sci, Split, Croatia Rudjer Boskovic Inst, Zagreb, Croatia Univ Cyprus, Nicosia, Cyprus Charles Univ Prague, Prague, Czech Republic Univ San Francisco Quito, Quito, Ecuador Acad Sci Res & Technol Arab Republ Egypt, Egyptian Network High Energy Phys, Cairo, Egypt NICPB, Tallinn, Estonia Univ Helsinki, Dept Phys, Helsinki, Finland Helsinki Inst Phys, Helsinki, Finland Lappeenranta Univ Technol, Lappeenranta, Finland CEA Saclay, DSM IRFU, Gif Sur Yvette, France Ecole Polytech, CNRS, IN2P3, Lab Leprince Ringuet, Palaiseau, France Univ Haute Alsace Mulhouse, Univ Strasbourg, Inst Pluridisciplinaire Hubert Curien, CNRS,IN2P3, Strasbourg, France CNRS, Inst Natl Phys Nucl & Phys Particules, Ctr Calcul, IN2P3, Villeurbanne, France Univ Lyon 1, CNRS, IN2P3, Inst Phys Nucl Lyon, Villeurbanne, France Georgian Tech Univ, Tbilisi, Rep of Georgia Tbilisi State Univ, Tbilisi, Rep of Georgia Rhein Westfal TH Aachen, Inst Phys 1, Aachen, Germany Rhein Westfal TH Aachen, Phys Inst A 3, Aachen, Germany Rhein Westfal TH Aachen, Phys Inst B 3, Aachen, Germany Deutsches Elektronen Synchrotron, Hamburg, Germany Univ Hamburg, Hamburg, Germany Inst Expt Kernphys, Karlsruhe, Germany NCSR Demokritos, INPP, Aghia Paraskevi, Greece Univ Athens, Athens, Greece Univ Ioannina, Ioannina, Greece Eotvos Lorand Univ, MTA ELTE Lendulet CMS Particle & Nucl Phys Grp, Budapest, Hungary Wigner Res Ctr Phys, Budapest, Hungary Inst Nucl Res ATOMKI, Debrecen, Hungary Univ Debrecen, Debrecen, Hungary Natl Inst Sci Educ & Res, Bhubaneswar, Orissa, India Panjab Univ, Chandigarh, India Univ Delhi, Delhi, India Saha Inst Nucl Phys, Kolkata, India Indian Inst Technol, Madras, Tamil Nadu, India Bhabha Atom Res Ctr, Bombay, Maharashtra, India Tata Inst Fundamental Res A, Bombay, Maharashtra, India Tata Inst Fundamental Res B, Bombay, Maharashtra, India IISER, Pune, Maharashtra, India Inst Res Fundamental Sci IPM, Tehran, Iran Univ Coll Dublin, Dublin, Ireland Ist Nazl Fis Nucl, Sez Bari, Bari, Italy Univ Bari, Bari, Italy Politecn Bari, Bari, Italy Ist Nazl Fis Nucl, Sez Bologna, Bologna, Italy Univ Bologna, Bologna, Italy Ist Nazl Fis Nucl, Sez Catania, Catania, Italy Univ Catania, Catania, Italy Ist Nazl Fis Nucl, Sez Firenze, Florence, Italy Univ Florence, Florence, Italy Ist Nazl Fis Nucl, Lab Nazl Frascati, Frascati, Italy Ist Nazl Fis Nucl, Sez Genova, Genoa, Italy Univ Genoa, Genoa, Italy Ist Nazl Fis Nucl, Sez Milano Bicocca, Milan, Italy Univ Milano Bicocca, Milan, Italy Ist Nazl Fis Nucl, Sez Napoli, Rome, Italy Univ Napoli Federico II, Rome, Italy Univ Basilicata, Rome, Italy Univ G Marconi, Rome, Italy Ist Nazl Fis Nucl, Sez Padova, Trento, Italy Univ Padua, Trento, Italy Univ Trento, Trento, Italy Ist Nazl Fis Nucl, Sez Pavia, Pavia, Italy Univ Pavia, Pavia, Italy Ist Nazl Fis Nucl, Sez Perugia, Perugia, Italy Univ Perugia, Perugia, Italy Ist Nazl Fis Nucl, Sez Pisa, Pisa, Italy Univ Pisa, Pisa, Italy Scuola Normale Super Pisa, Pisa, Italy Ist Nazl Fis Nucl, Sez Roma, Rome, Italy Univ Roma, Rome, Italy Ist Nazl Fis Nucl, Sez Torino, Novara, Italy Univ Turin, Novara, Italy Univ Piemonte Orientale, Novara, Italy Ist Nazl Fis Nucl, Sez Trieste, Trieste, Italy Univ Trieste, Trieste, Italy Kyungpook Natl Univ, Daegu, South Korea Chonbuk Natl Univ, Jeonju, South Korea Hanyang Univ, Seoul, South Korea Korea Univ, Seoul, South Korea Seoul Natl Univ, Seoul, South Korea Univ Seoul, Seoul, South Korea Sungkyunkwan Univ, Suwon, South Korea Vilnius Univ, Vilnius, Lithuania Univ Malaya, Natl Ctr Particle Phys, Kuala Lumpur, Malaysia Ctr Invest & Estudios Avanzados IPN, Mexico City, DF, Mexico Univ Iberoamer, Mexico City, DF, Mexico Benemerita Univ Autonoma Puebla, Puebla, Mexico Univ Autonoma San Luis Potosi, San Luis Potosi, Mexico Univ Auckland, Auckland, New Zealand Univ Canterbury, Christchurch, New Zealand Quaid I Azam Univ, Natl Ctr Phys, Islamabad, Pakistan Natl Ctr Nucl Res, Otwock, Poland Univ Warsaw, Fac Phys, Inst Expt Phys, Warsaw, Poland Lab Instrumentacao & Fis Expt Particulas, Lisbon, Portugal Joint Inst Nucl Res, Dubna, Russia Petersburg Nucl Phys Inst, St Petersburg, Russia Inst Nucl Res, Moscow, Russia Inst Theoret & Expt Phys, Moscow, Russia Natl Res Nucl Univ, MEPhI, Moscow, Russia PN Lebedev Phys Inst, Moscow, Russia Lomonosov Moscow State Univ, Skobeltsyn Inst Nucl Phys, Moscow, Russia Inst High Energy Phys, State Res Ctr Russian Federat, Protvino, Russia Univ Belgrade, Fac Phys, Belgrade, Serbia Vinca Inst Nucl Sci, Belgrade, Serbia Ctr Invest Energet Medioambient & Tecnol CIEMAT, Madrid, Spain Univ Autonoma Madrid, Madrid, Spain Univ Oviedo, Oviedo, Spain Univ Cantabria, CSIC, Inst Fis Cantabria IFCA, Santander, Spain European Org Nucl Res, CERN, Geneva, Switzerland Paul Scherrer Inst, Villigen, Switzerland Swiss Fed Inst Technol, Inst Particle Phys, Zurich, Switzerland Univ Zurich, Zurich, Switzerland Natl Cent Univ, Chungli, Taiwan NTU, Taipei, Taiwan Chulalongkorn Univ, Fac Sci, Dept Phys, Bangkok, Thailand Cukurova Univ, Adana, Turkey Middle East Tech Univ, Dept Phys, Ankara, Turkey Bogazici Univ, Istanbul, Turkey Istanbul Tech Univ, Istanbul, Turkey Natl Acad Sci Ukraine, Inst Scintillat Mat, Kharkov, Ukraine Kharkov Inst Phys & Technol, Natl Sci Ctr, Kharkov, Ukraine Univ Bristol, Bristol, Avon, England Rutherford Appleton Lab, Didcot, Oxon, England Imperial Coll, London, England Brunel Univ, Uxbridge, Middx, England Baylor Univ, Waco, TX 76798 USA Univ Alabama, Tuscaloosa, AL USA Boston Univ, Boston, MA 02215 USA Brown Univ, Providence, RI 02912 USA Univ Calif Davis, Davis, CA 95616 USA Univ Calif Los Angeles, Los Angeles, CA USA Univ Calif Riverside, Riverside, CA 92521 USA Univ Calif San Diego, La Jolla, CA 92093 USA Univ Calif Santa Barbara, Santa Barbara, CA 93106 USA CALTECH, Pasadena, CA 91125 USA Carnegie Mellon Univ, Pittsburgh, PA 15213 USA Univ Colorado, Boulder, CO 80309 USA Cornell Univ, Ithaca, NY USA Fairfield Univ, Fairfield, CT 06430 USA Fermilab Natl Accelerator Lab, POB 500, Batavia, IL 60510 USA Univ Florida, Gainesville, FL USA Florida Int Univ, Miami, FL 33199 USA Florida State Univ, Tallahassee, FL 32306 USA Florida Inst Technol, Melbourne, FL 32901 USA UIC, Chicago, IL USA Univ Iowa, Iowa City, IA USA Johns Hopkins Univ, Baltimore, MD USA Univ Kansas, Lawrence, KS 66045 USA Kansas State Univ, Manhattan, KS 66506 USA Lawrence Livermore Natl Lab, Livermore, CA USA Univ Maryland, College Pk, MD 20742 USA MIT, Cambridge, MA 02139 USA Univ Minnesota, Minneapolis, MN USA Univ Mississippi, Oxford, MS USA Univ Nebraska, Lincoln, NE USA SUNY Buffalo, Buffalo, NY USA Northeastern Univ, Boston, MA 02115 USA Northwestern Univ, Evanston, IL USA Univ Notre Dame, Notre Dame, IN 46556 USA Ohio State Univ, Columbus, OH 43210 USA Princeton Univ, Princeton, NJ 08544 USA Univ Puerto Rico, Mayaguez, PR USA Purdue Univ, W Lafayette, IN 47907 USA Purdue Univ Calumet, Hammond, LA USA Rice Univ, Houston, TX USA Univ Rochester, Rochester, NY 14627 USA Rutgers State Univ, Piscataway, NJ USA Univ Tennessee, Knoxville, TN USA Texas A&M Univ, College Stn, TX USA Texas Tech Univ, Lubbock, TX 79409 USA Vanderbilt Univ, 221 Kirkland Hall, Nashville, TN 37235 USA Univ Virginia, Charlottesville, VA USA Wayne State Univ, Detroit, MI USA Univ Wisconsin, Madison, WI USA Vienna Univ Technol, Vienna, Austria Univ Estadual Campinas, Campinas, Brazil CNRS, IN2P3, Paris, France British Univ Egypt, Cairo, Egypt Zewail City Sci & Technol, Zewail, Egypt Fayoum Univ, Al Fayyum, Egypt Ain Shams Univ, Cairo, Egypt Univ Haute Alsace, Mulhouse, France Brandenburg Tech Univ Cottbus, Cottbus, Germany Indian Inst Sci Educ & Res, Bhopal, India Inst Phys, Bhubaneswar, Orissa, India Visva Bharati Univ, Santini Ketan, W Bengal, India Univ Ruhuna, Matara, Sri Lanka Isfahan Univ Technol, Esfahan, Iran Univ Tehran, Dept Engn Sci, Tehran, Iran Islamic Azad Univ, Sci & Res Branch, Plasma Phys Res Ctr, Tehran, Iran Univ Siena, Siena, Italy Int Islamic Univ Malaysia, Kuala Lumpur, Malaysia Agensi Nuklear Malaysia, MOSTI, Kajang, Malaysia Consejo Nacl Ciencia & Technol, Mexico City, DF, Mexico Warsaw Univ Technol, Inst Elect Syst, Warsaw, Poland St Petersburg State Polytech Univ, St Petersburg, Russia Univ Roma, Ist Nazl Fis Nucl, Sez Roma, Rome, Italy Natl Tech Univ Athens, Athens, Greece Ist Nazl Fis Nucl, Scuola Normale & Sez, Pisa, Italy Riga Tech Univ, Riga, Latvia Albert Einstein Ctr Fundamental Phys, Bern, Switzerland Adiyaman Univ, Adiyaman, Turkey Mersin Univ, Mersin, Turkey Cag Univ, Mersin, Turkey Piri Reis Univ, Istanbul, Turkey Gaziosmanpasa Univ, Tokat, Turkey Ozyegin Univ, Istanbul, Turkey Izmir Inst Technol, Izmir, Turkey Marmara Univ, Istanbul, Turkey Kafkas Univ, Kars, Turkey Istanbul Bilgi Univ, Istanbul, Turkey Yildiz Tech Univ, Istanbul, Turkey Hacettepe Univ, Ankara, Turkey Univ Southampton, Sch Phys & Astron, Southampton, Hants, England Inst Astrofis Canarias, San Cristobal la Laguna, Spain Utah Valley Univ, Orem, UT USA Univ Roma, Fac Ingn, Rome, Italy Argonne Natl Lab, 9700 S Cass Ave, Argonne, IL 60439 USA Erzincan Univ, Erzincan, Turkey Mimar Sinan Univ, Istanbul, Turkey Texas A&M Univ, Doha, Qatar Univ Estadual Paulista, Sao Paulo, Brazil
Published: 2016

17. CLASH-VLT: A highly precise strong lensing model of the galaxy cluster RXC J2248.7 - 4431 (Abell S1063) and prospects for cosmography

Author: Eros Vanzella, G. B. Caminha, Andrea Biviano, Brenda Frye, Bodo L. Ziegler, Keiichi Umetsu, Marc Postman, Christian Maier, Dan Coe, Italo Balestra, Marco Lombardi, M. Annunziatella, Anton M. Koekemoer, Stella Seitz, Piero Rosati, Amata Mercurio, Stefano Ettori, Sherry H. Suyu, Alexander Fritz, Tom Broadhurst, Stefano Borgani, Claudio Grillo, Peter Melchior, Paolo Tozzi, Karina Caputi, Mario Nonino, Marisa Girardi, A. Monna, Adi Zitrin, Raphael Gobat, C. Delgado-Correal, W. Karman, Massimo Meneghetti, Barbara Sartoris, E. Munari, Caminha, G. B, Grillo, C., Rosati, P., Balestra, I., Karman, W., Lombardi, M., Mercurio, A., Nonino, M., Tozzi, P., Zitrin, A., Biviano, A., Girardi, Marisa, Koekemoer, A. M., Melchior, P., Meneghetti, M., Munari, Emiliano, Suyu, S. H., Umetsu, K., Annunziatella, Marianna, Borgani, Stefano, Broadhurst, T., Caputi, K. I., Coe, D., Delgado Correal, C., Ettori, S., Fritz, A., Frye, B., Gobat, R., Maier, C., Monna, A., Postman, M., Sartoris, Barbara, Seitz, S., Vanzella, E., Ziegler, B., Università degli Studi di Ferrara (UniFE), Dark Cosmology Centre (DARK), Niels Bohr Institute [Copenhagen] (NBI), Faculty of Science [Copenhagen], University of Copenhagen = Københavns Universitet (KU)-University of Copenhagen = Københavns Universitet (KU)-Faculty of Science [Copenhagen], University of Copenhagen = Københavns Universitet (KU)-University of Copenhagen = Københavns Universitet (KU), INAF - Osservatorio Astronomico di Trieste (OAT), Istituto Nazionale di Astrofisica (INAF), Astrophysique Interprétation Modélisation (AIM (UMR_7158 / UMR_E_9005 / UM_112)), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7), Max-Planck-Institut für Extraterrestrische Physik (MPE), Università degli Studi di Ferrara = University of Ferrara (UniFE), University of Copenhagen = Københavns Universitet (UCPH)-University of Copenhagen = Københavns Universitet (UCPH)-Faculty of Science [Copenhagen], University of Copenhagen = Københavns Universitet (UCPH)-University of Copenhagen = Københavns Universitet (UCPH), Astrophysique Interprétation Modélisation (AIM (UMR7158 / UMR_E_9005 / UM_112)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Astronomy, and University of Ferrara [Ferrara]
Subjects: Observational cosmology, galaxy cluster, Cosmological parameters, Dark matter, Galaxies: clusters: individual: RXC J2248.7-4431, Gravitational lensing: strong, Astronomy and Astrophysics, Space and Planetary Science, COSMOLOGICAL CONSTRAINTS, Cosmology and Nongalactic Astrophysics (astro-ph.CO), MAGNIFICATION MAPS, media_common.quotation_subject, gravitational lensing, FOS: Physical sciences, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Lambda, 01 natural sciences, Omega, Cosmology, dark matter, NO, SPACE-TELESCOPE OBSERVATIONS, galaxy clusters, 0103 physical sciences, DARK-MATTER, LY-ALPHA NEBULA, cosmological parameters, 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics, MASS-DISTRIBUTION, media_common, Physics, Line-of-sight, Mass distribution, 010308 nuclear & particles physics, FRONTIER FIELDS CLUSTERS, gravitational lensing: strong, Astrophysics - Astrophysics of Galaxies, Galaxy, Redshift, Universe, GRAVITATIONAL LENSES, LYMAN-BREAK GALAXIES, galaxies: clusters: individual: RXC J2248.7-4431, Astrophysics of Galaxies (astro-ph.GA), HIGH-REDSHIFT, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We perform a comprehensive study of the total mass distribution of the galaxy cluster RXCJ2248 ($z=0.348$) with a set of high-precision strong lensing models, which take advantage of extensive spectroscopic information on many multiply lensed systems. In the effort to understand and quantify inherent systematics in parametric strong lensing modelling, we explore a collection of 22 models where we use different samples of multiple image families, parametrizations of the mass distribution and cosmological parameters. As input information for the strong lensing models, we use the CLASH HST imaging data and spectroscopic follow-up observations, carried out with the VIMOS and MUSE spectrographs, to identify bona-fide multiple images. A total of 16 background sources, over the redshift range $1.0-6.1$, are multiply lensed into 47 images, 24 of which are spectroscopically confirmed and belong to 10 individual sources. The cluster total mass distribution and underlying cosmology in the models are optimized by matching the observed positions of the multiple images on the lens plane. We show that with a careful selection of a sample of spectroscopically confirmed multiple images, the best-fit model reproduces their observed positions with a rms of $0.3$ in a fixed flat $\Lambda$CDM cosmology, whereas the lack of spectroscopic information lead to biases in the values of the model parameters. Allowing cosmological parameters to vary together with the cluster parameters, we find (at $68\%$ confidence level) $\Omega_m=0.25^{+0.13}_{-0.16}$ and $w=-1.07^{+0.16}_{-0.42}$ for a flat $\Lambda$CDM model, and $\Omega_m=0.31^{+0.12}_{-0.13}$ and $\Omega_\Lambda=0.38^{+0.38}_{-0.27}$ for a universe with $w=-1$ and free curvature. Using toy models mimicking the overall configuration of RXCJ2248, we estimate the impact of the line of sight mass structure on the positional rms to be $0.3\pm 0.1$.(ABRIDGED), Comment: 23 pages, 13 figures, accepted for publication in A&A
Published: 2016

18. The rotation curves shapes of late-type dwarf galaxies

Author: Renzo Sancisi, J. M. van der Hulst, Rob A. Swaters, T. S. van Albada, Kapteyn Astronomical Institute, and Astronomy
Subjects: VISIBLE MATTER, Cosmology and Nongalactic Astrophysics (astro-ph.CO), FOS: Physical sciences, DARK-MATTER HALOS, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Luminosity, Gravitational potential, SURFACE BRIGHTNESS GALAXIES, IRREGULAR GALAXIES, surveys, UNIVERSAL DENSITY PROFILE, Surface brightness, galaxies: irregular, Galaxy rotation curve, Astrophysics::Galaxy Astrophysics, galaxies: kinematics and dynamics, Dwarf galaxy, MASS-DISTRIBUTION, Physics, Spiral galaxy, Astronomy and Astrophysics, galaxies: dwarf, WESTERBORK HI SURVEY, Galaxy, NEUTRAL HYDROGEN, Space and Planetary Science, Irregular galaxy, SPIRAL GALAXIES, Astrophysics - Cosmology and Nongalactic Astrophysics, VELOCITY-FIELDS
Abstract: We present rotation curves derived for a sample of 62 late-type dwarf galaxies that have been observed as part of the Westerbork HI Survey of Spiral and Irregular Galaxies (WHISP) project. The rotation curves were derived by interactively fitting model data cubes to the observed cubes, taking rotation curve shape, HI distribution, inclination, and the size of the beam into account. This makes it possible to correct for the effects of beam smearing. The dwarf galaxies in our sample have rotation-curve shapes that are similar to those of late-type spiral galaxies, in the sense that their rotation curves, when expressed in units of disk scale lengths, rise as steeply in the inner parts and start to flatten at two disk scale lengths. None of the galaxies in our sample have solid-body rotation curves that extend beyond three scale lengths. The logarithmic outer rotation curve slopes are similar between late-type dwarf and spiral galaxies. Thus, whether the flat part of the rotation curve is reached seems to depend more on the extent of the rotation curve than on its amplitude. We also find that the outer rotation curve shape does not strongly depend on luminosity, at least for galaxies fainter than M_R~-19. We find that in spiral galaxies and in the central regions of late-type dwarf galaxies, the shape of the central distribution of light and the inner rise of the rotation curve are related. This implies that galaxies with stronger central concentrations of light also have higher central mass densities, and it suggests that the luminous mass dominates the gravitational potential in the central regions, even in low surface brightness dwarf galaxies., Comment: 22 pages, 2009 A&A 493, 871
Published: 2009

19. Modified gravity models and the central cusp of dark matter halos in galaxies

Author: Paulo L. de Oliveira, Júlio C. Fabris, Davi C. Rodrigues, Gianfranco Gentile, Physics, Astrophysics, and Astronomy and Astrophysics Research Group
Subjects: DWARF GALAXIES, Dark matter, RESOLUTION ROTATION CURVES, FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, dark matter, General Relativity and Quantum Cosmology, SCALING BEHAVIOR, Gravitation, SURFACE BRIGHTNESS GALAXIES, FINE-STRUCTURE CONSTANT, kinematics and dynamics [galaxies], DENSITY PROFILE, COSMOLOGICAL CONSTANT, Galaxy rotation curve, Astrophysics::Galaxy Astrophysics, MASS-DISTRIBUTION, Physics, astrophysics, Astronomy and Astrophysics, Astrophysics - Astrophysics of Galaxies, Galaxy, Modified Newtonian dynamics, Dark matter halo, spiral [galaxies], MODIFIED NEWTONIAN DYNAMICS, Physics and Astronomy, gravitation, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), Cuspy halo problem, Halo, SPIRAL GALAXIES
Abstract: The N-body dark matter (DM) simulations point that DM density profiles, e.g. the NFW halo, should be cuspy in its center, but observations disfavour this kind of DM profile. Here we consider whether the observed rotation curves "close" to the galactic centre can favour modified gravity models in comparison to the NFW halo, and how to quantify such difference. Two explicit modified gravity models are considered, MOND and a more recent approach called RGGR (in reference to Renormalization Group effects in General Relativity). It is also the purpose of this work to significantly extend the sample on which RGGR has been tested in comparison to other approaches. By analysing 62 galaxies from five samples, we find that: i) there is a radius, given by half the disk scale length, below which RGGR and MOND can match the data about as well or better than NFW, albeit the formers have fewer free parameters; ii) considering the complete rotation curve data, RGGR could achieve fits with better agreement than MOND, and almost as good as a NFW halo with two free parameters (NFW and RGGR have respectively two and one more free parameters than MOND)., 24 pages, 7 figures, 7 tables. Accepted in MNRAS
Published: 2014

20. Investigating potential planetary nebula/cluster pairs

Author: Dante Minniti, Andres-Nicolas Chene, Francesco Mauro, Jura Borissova, Wolfgang Gieren, Giovanni Carraro, Radostin Kurtev, David G. Turner, Alex C. Gormaz-Matamala, Daniel J. Majaess, Christian Moni Bidin, Charles Jose Bonatto, and Doug Geisler
Subjects: PARCOS-PARALLAXES, Vista Variables in the Via Lactea, planetary nebulae, open clusters and associations, HORIZONTAL-BRANCH STARS, STATISTICAL DISTANCE SCALE, MEAN RADIAL-VELOCITIES, GALACTIC OPEN CLUSTERS, MAIN-SEQUENCE STARS, NEBULA NGC 2438, PROPER MOTIONSHIP, PARCOS-PARALLAXES, MASS-DISTRIBUTION, CLOSE BINARIES, open clusters and associations, Population, FOS: Physical sciences, STATISTICAL DISTANCE SCALE, PROPER MOTIONSHIP, Espectros astronômicos, Astrophysics, Dinamica estelar, Photometry (optics), HORIZONTAL-BRANCH STARS, Astronomia infravermelha, Bulge, Aglomerados estelares, education, Solar and Stellar Astrophysics (astro-ph.SR), GALACTIC OPEN CLUSTERS, MASS-DISTRIBUTION, Physics, Nebulosas planetarias, education.field_of_study, general [Open clusters and associations], NEBULA NGC 2438, Astronomy and Astrophysics, planetary nebulae, Astrophysics - Astrophysics of Galaxies, Planetary nebula, CLOSE BINARIES, MEAN RADIAL-VELOCITIES, Radial velocity, Stars, Fotometria astronômica, Astrophysics - Solar and Stellar Astrophysics, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), general [Planetary nebulae], MAIN-SEQUENCE STARS, Open cluster
Abstract: Fundamental parameters characterizing the end-state of intermediate-mass stars may be constrained by discovering planetary nebulae (PNe) in open clusters (OCs). Cluster membership may be exploited to establish the distance, luminosity, age, and physical size for PNe, and the intrinsic luminosity and mass of its central star. Four potential PN-OC associations were investigated, to assess the cluster membership for the PNe. Radial velocities were measured from intermediate-resolution optical spectra, complemented with previous estimates in the literature. When the radial velocity study supported the PN/OC association, we analyzed if other parameters (e.g., age, distance, reddening, central star brightness) were consistent with this conclusion. Our measurements imply that the PNe VBe3 and HeFa1 are not members of the OCs NGC5999 and NGC6067, respectively, and likely belong to the background bulge population. Conversely, consistent radial velocities indicate that NGC2452/NGC2453 could be associated, but our results are not conclusive and additional observations are warranted. Finally, we demonstrate that all the available information point to He2-86 being a young, highly internally obscured PN member of NGC4463. New near-infrared photometry acquired via the Vista Variables in the Via Lactea ESO public survey was used in tandem with existing UBV photometry to measure the distance, reddening, and age of NGC4463, finding d=1.55+-0.10 kpc, E(B-V)=0.41+-0.02, and tau=65+-10 Myr, respectively. The same values should be adopted for the PN if the proposed cluster membership will be confirmed., Accepted for publication in A&A
Published: 2014

21. On the apparent coupling of neutral hydrogen and dark matter in spiral galaxies

Author: T. S. van Albada, Renzo Sancisi, Henk Hoekstra, Kapteyn Astronomical Institute, and Astronomy
Subjects: Dark matter, FOS: Physical sciences, chemistry.chemical_element, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, galaxies : kinematics and dynamics, NGC-247, SURFACE PHOTOMETRY, dark matter, GALACTIC DISKS, Cluster (physics), HI ROTATION CURVES, KINEMATICS, galaxies : haloes, Scaling, Helium, Galaxy rotation curve, Astrophysics::Galaxy Astrophysics, MASS-DISTRIBUTION, Physics, Coupling, Spiral galaxy, Astrophysics (astro-ph), NGC-5585, Astronomy and Astrophysics, SCULPTOR GROUP GALAXIES, Galaxy, cosmology : theory, LIGHT, chemistry, Space and Planetary Science, methods : analytical, galaxies : spiral, NGC-3109
Abstract: We have studied a mass model for spiral galaxies in which the dark matter surface density is a scaled version of the observed HI surface density. Applying this mass model to a sample of 24 spiral galaxies with reliable rotation curves one obtains good fits for most galaxies. The scaling factors cluster around 7, after correction for the presence of primordial helium. But for several cases different, often larger, values are found. For galaxies that can not be fitted well the discrepancy occurs at large radii and results from a fairly rapid decline of the HI surface density in the outermost regions. Because of such imperfections and in view of possible selection effects it is not possible to conclude here that there is a real coupling between HI and dark matter in spiral galaxies., Comment: Accepted for publication in MNRAS; 8 pages, 3 figures
Published: 2001

22. Photoionization modelling of planetary nebulae - II. Galactic bulge nebulae, a comparison with literature results

Subjects: methods : data analysis, MAGNITUDES, ISM : abundances, EVOLUTION, CHEMICAL-COMPOSITIONS, ABUNDANCES, TEMPERATURES, planetary nebulae : general, Astrophysics::Solar and Stellar Astrophysics, SPECTROPHOTOMETRY, Astrophysics::Earth and Planetary Astrophysics, CENTRAL STARS, ATMOSPHERES, EMISSION, Astrophysics::Galaxy Astrophysics, MASS-DISTRIBUTION
Abstract: We have constructed photoionization models of five galactic bulge planetary nebulae using our automatic method, which enables a fully self-consistent determination of the physical parameters of a planetary nebula. The models are constrained using the spectrum, the IRAS and radio fluxes and the angular diameter of the nebula. We also conducted a literature search for physical parameters determined with classical methods for these nebulae. Comparison of the distance-independent physical parameters with published data shows that the stellar temperatures generally are in good agreement and can be considered reliable. The literature data for the electron temperature, electron density and also for the abundances show a large spread, indicating that the use of line diagnostics is not reliable and that the accuracy of these methods needs to be improved. Comparison of the various abundance determinations indicates that the uncertainty in the electron temperature is the main source of uncertainty in the abundance determination. The stellar magnitudes predicted by the photoionization models are in good agreement with observed values.
Published: 1999

23. Lensed galaxies in Abell 370 - I. Modeling the number counts and redshift distribution of background sources

Subjects: galaxies : evolution, galaxies : clusters : individual : A 370, RICH CLUSTER AC-114, GIANT ARCS, EVOLUTION, ARC STATISTICS, GRAVITATIONAL ARCLETS, cosmology : observations, SPACE-TELESCOPE OBSERVATIONS, cosmology : gravitational lensing, RECONSTRUCTION, FIELD, DISTANT CLUSTER, MASS-DISTRIBUTION
Abstract: We present new observations of the cluster-lens Abell 370: a deep HST/WFPC2 F675W image and ESO 3.6m spectroscopy of faint galaxies. These observations shed new light on the statistical properties of faint lensed galaxies. In particular, we spectroscopically confirm the multiple image nature of the B2-B3 gravitational pair (Kneib et al. 1993), and determine a redshift of z = 0.806 +/- 0.002 which is in very good agreement with earlier predictions. A refined mass model of the cluster core (that includes cluster galaxy halos) is presented, based on a number of newly identified multiple images. Following Bezecourt et al. (1998a), we combine the new cluster mass model with a spectrophotometric prescription for galaxy evolution to predict the arclets number counts and redshift distribution in the I-IST image. In particular, the ellipticity distribution of background sources is taken into account, in order to properly estimate the statistical number and redshift distribution of arclets. We show that the redshift distribution of arclets, and particularly its high redshift tail can be used as a strong constraint to disentangle different galaxy evolution scenarios. A hierarchical model which includes number density evolution is favored by our analysis. Finally, we compute the depletion curves :For the faint galaxy number counts and discuss their wavelength dependence.
Published: 1999

24. Parameter estimation for compact binary coalescence signals with the first generation gravitational-wave detector network

Author: R. De Rosa, Laura Cadonati, Rana X. Adhikari, Carlos Cepeda, Robert J. McCarthy, Linqing Wen, B. Machenschalk, F. Donovan, V. Lhuillier, Susan M. Scott, Teviet Creighton, G. McIntyre, D. Lodhia, Maik Frede, Chad Hanna, M. Branchesi, J. C. Batch, K. A. Hodge, A. K. Zadrożny, V. Boschi, V. Malvezzi, M. Bebronne, Carl-Johan Haster, N. Morgado, L. Rolland, Fabrizio Barone, M. Mohan, N. Man, K. Haughian, Ludovico Carbone, P. Couvares, Benno Willke, E. Goetz, T. Dent, Kazuhiro Hayama, D. Talukder, C. V. Torres, I. W. Harry, R. Gouaty, M. Factourovich, J. Betzwieser, Antoine Heidmann, Leo Singer, L. Naticchioni, M. A. Barton, Carl L. Rodriguez, Sascha Husa, Meng Wang, C. Wilkinson, D. Amariutei, Janyce Franc, David H. Shoemaker, Holger J. Pletsch, D. Verkindt, R. L. Ward, P. J. Sutton, J. H. Romie, R. Kurdyumov, A. F. Brooks, Lutz Winkelmann, Kasem Mossavi, M. T. Hartman, V. Kringel, M. Pihlaja, Tomasz Bulik, François Bondu, Fausto Acernese, V. Kondrashov, H. Overmier, S. Kandhasamy, N. A. Robertson, C. N. Colacino, Jordan Camp, R. G. Oldenberg, D.B. DeBra, S. Braccini, V. Litvine, T. Bhadbade, J. Breyer, C. Gray, G. Kuehn, L. Cunningham, Alessandra Buonanno, M. Mantovani, Kentaro Somiya, M. Brinkmann, F. J. Raab, F. Garufi, G. Santostasi, F. Nocera, D. J. White, C. Zhao, Fiona C. Speirits, John Veitch, D. Sellers, C. Affeldt, D. Hammer, Y. Minenkov, D. Feldbaum, T. Meier, A. Morgia, Fabio Postiglione, S. Chung, C. Poux, R. Gustafson, M. E. Normandin, Eric Howell, I. Yakushin, L. Sammut, Zoltán Keresztes, F. Cleva, C. Titsler, Sunil Susmithan, R. Taylor, W. Chen, W. Z. Korth, P. Wessels, L. Pinard, J. Garcia, Jong H. Chow, A. Pasqualetti, S. E. Whitcomb, P. Kwee, K. A. Thorne, S. Giampanis, A. Gennai, H. Wittel, Federico Ferrini, S. Penn, D. Barker, T. P. Bodiya, G. Vajente, Kazuhiro Agatsuma, M. A. Bizouard, V. Loriette, L. K. Nuttall, M. MacInnis, S. Gil-Casanova, M. R. Abernathy, F. Frasconi, A. S. Stroeer, Peter Kalmus, P. Rapagnani, F. Seifert, Peter Fritschel, T. Accadia, David Jones, S. E. Strigin, C. Buy, B. Behnke, Riccardo Sturani, G. M. Harry, Nico Lastzka, K. Venkateswara, V. Predoi, I. W. Martin, J. C. Driggers, Virginio Sannibale, David E. McClelland, J. Macarthur, Y. Bao, G. Billingsley, S. Roddy, Tristan Briant, Marco Cavaglia, Badri Krishnan, V. Dattilo, M. Tse, D. M. Macleod, L. Bosi, S. Foley, H. Kaufer, D. Hoak, D. Sentenac, S. Mosca, Patrick Brady, R. Schilling, Matthew Evans, P. J. Veitch, G. Kang, M. Vavoulidis, C. R. Ramet, R. Flaminio, B. L. Swinkels, Huan Yang, Kip S. Thorne, T. Chalermsongsak, Alessandro Bertolini, J. Zweizig, Saranya Ghosh, Ryan DeRosa, Koji Arai, Sanichiro Yoshida, Jeffery Kline, Xuan Wang, J. D. Lough, A. R. Wade, C. M. Mow-Lowry, Jessica McIver, Stefan Hild, S. D'Antonio, Graham Woan, M. Rodruck, Jonah Kanner, Sergey P. Vyatchanin, B. Schulz, M. Pichot, R. Kasturi, A. M. Sintes, J. O'Dell, T. Dayanga, R. Inta, S. Klimenko, A. W. Heptonstall, Peter R. Saulson, Zhi Liu, M. Born, K. Mailand, Peter Aufmuth, Sebastian Steinlechner, M. Damjanic, T. Reed, C. Graef, Tania Regimbau, A. Khalaidovski, R. Engel, Robert L. Byer, Stuart Reid, F. Salemi, A. Brillet, A. Conte, K. Kaufman, A. Singer, Lee Samuel Finn, J. C. Dumas, D. Ugolini, B. F. Whiting, T. Huynh-Dinh, Timothy A Welborn, Enrico Calloni, G. Traylor, R. L. Savage, A. S. Bell, Thomas Corbitt, V. Herrera, C. A. Costa, J.-F. Hayau, M. Yvert, T. D. Abbott, Y. J. Jang, Seiji Kawamura, Elizabeth Harstad, Hyun-Chul Kim, R. Mittleman, M. Lormand, Robert Stone, Nelson Christensen, D. Keitel, L. G. Prokhorov, J. S. Kissel, C. J. Bell, A. Stochino, S. B. Anderson, B. Moe, Ruslan Vaulin, P. Leaci, A. Colla, J. Aasi, V. P. Mitrofanov, S. Dorsher, T. Etzel, H. P. Daveloza, A. Di Lieto, C. Van Den Broeck, Chris Pankow, B. Mours, J. N. Marx, László Á. Gergely, Albert Lazzarini, R. Passaquieti, L. Wallace, A. Królak, R. Frey, Marc Favata, K. Yamamoto, L. E. Wade, L. Palladino, Bernard F. Schutz, Masa-Katsu Fujimoto, J. Heefner, Li Ju, M. Shaltev, N. Letendre, A. Langley, E. Jesse, Mirko Prato, W. Del Pozzo, P. F. Cohadon, David B. Tanner, Roger Jones, N. Zotov, K. Mason, T. Isogai, D. Nolting, M. Sung, A. Nitz, F. Y. Khalili, G. Mazzolo, M. Vasúth, L. Bonelli, G. A. Prodi, Alexander Wanner, C. T. Y. Chung, Rahul Biswas, Michael E Zucker, Daniel A. Shaddock, J. Hanson, Trevor Sidery, H. Heitmann, A. Di Virgilio, Karoline Wiesner, P. J. King, T. Eberle, A. Chiummo, B. Shapiro, A. Allocca, M. Stefszky, John A. Clark, Sanjeev Dhurandhar, R. Cavalieri, Jordi Burguet-Castell, V. Re, B. Bland, N. Beveridge, C. I. Torrie, B. Rankins, Joshua Yablon, M. Blom, Elena Cesarini, M. Pedraza, Stefaan Franco, J. P. Zendri, Y. Wan, Ben Farr, F. Martelli, E. Amador Ceron, F. Piergiovanni, Chang-Hwan Lee, Ho-Gyu Lee, Luca Gammaitoni, Guido Mueller, A. G. Wiseman, Kipp Cannon, Walter Winkler, Kevin M. Ryan, D. R. Ingram, Phil Willems, K. Kawabe, Xin Chen, R. M. Martin, J. Slutsky, Imre Bartos, J. H. Clayton, M. Di Paolo Emilio, A. S. Markosyan, Namjun Kim, Grant David Meadors, Takao Mori, V. Quetschke, Bangalore Suryanarayana Sathyaprakash, S. M. Aston, Harald Lück, J. Logue, Michael W. Coughlin, Paul Fulda, Maria Alessandra Papa, F. Cavalier, M. Prijatelj, E. Tournefier, A. Basti, David Murphy, M. Holtrop, D. C. Coyne, K. Grover, K. Izumi, Katrin Dahl, F. Travasso, M. Davier, R. S. Ottens, Michał Bejger, A. Effler, C. Palomba, Collin Capano, A. Giazotto, P. Shawhan, M. H. Wimmer, I. Ferrante, J. Abadie, M. Mageswaran, Xavier Siemens, J.-P. Coulon, B. J. J. Slagmolen, Hee-Suk Cho, M. Britzger, S. C. McGuire, E. Black, Satya Mohapatra, J. R. Smith, R. Bork, S. Privitera, T. Nash, Z. Frei, Ilya Mandel, E. Macdonald, I. Leonor, M. Was, B. Lantz, Andreas Freise, Vincenzo Pierro, Philip Graff, G. H. Ogin, A. Perreca, M. C. Araya, G. Gemme, M. Drago, Guenakh Mitselmakher, John Miller, T. Prestegard, V. Brisson, S. Ast, C. M. Reed, K. Kokeyama, Eric Thrane, Eric W. James, C. Michel, Sarah Caudill, P. Puppo, Chiara M. F. Mingarelli, P. Charlton, H. Vocca, J.-D. Fournier, Alessandra Corsi, Matthew Pitkin, D. Rosińska, I. Maksimovic, O. Puncken, D. Friedrich, J. Marque, B. K. Kim, G. Hemming, R. Wooley, R. J. S. Greenhalgh, D. Passuello, A. Viceré, Hyun Lee, Anton B. Ivanov, A. L. Stuver, A. M. Sergeev, Yi Chen, M. S. Meyer, S. Sankar, C. Griffo, M. Wade, R. Quitzow-James, B. Daudert, P. G. Murray, N. D. Smith-Lefebvre, P. Baker, J. Birch, S. Frasca, R. M. S. Schofield, Matthew Benacquista, E. J. Daw, I. Fiori, Riccardo Bassiri, J. H. Hough, Jolien D. E. Creighton, S. Caride, Rainer Weiss, Benjamin J. Owen, M. Granata, E. Coccia, E. Maros, S. Doravari, Igor Neri, F. Ricci, R. W. P. Drever, Paolo Addesso, K. D. Giardina, Christian D. Ott, C. Gill, Samuel J. Waldman, Marco Aurelio Diaz, C. Bradaschia, M. Tonelli, V. Necula, W. W. Johnson, A. P. M. ter Braack, I. Santiago-Prieto, Innocenzo M. Pinto, Larry R. Price, J. G. Rollins, C. Bogan, I. A. Bilenko, Ik Siong Heng, A. Rüdiger, David J. Ottaway, J. F. J. van den Brand, M. Tacca, V. V. Frolov, Martin Hendry, Christopher Wipf, K. V. Tokmakov, Richard A. Matzner, Lindy Blackburn, B. Bouhou, C. Robinson, Douglas R. Cook, K. Holt, Chunglee Kim, Piotr Jaranowski, Florent Robinet, Matthew West, C. Messenger, Riccardo Paoletti, Thanh Vinh Nguyen, David Blair, M. Parisi, M. G. Beker, S. Steplewski, Emma L. Robinson, Fan Zhang, Michele Zanolin, Martin Hewitson, Junwei Cao, Benjamin William Allen, G. Szeifert, Karsten Danzmann, M. Colombini, V. Kalogera, Stephen Fairhurst, Joseph Gleason, M. Galimberti, V. Sandberg, D. H. Reitze, F. Marion, G. Gelencser, S. Grunewald, N. Leroy, M. Kasprzack, V. Fafone, Charlotte Bond, M. Punturo, Leopoldo Milano, C. Lawrie, G. D. Hammond, Stanislav Babak, John Nelson, Amanda J. Page, Ping Koy Lam, G. Debreczeni, F. Paoletti, Duncan A. Brown, M. Heurs, M. Bastarrika, M. E. Gáspár, G. Vedovato, D. B. Kozak, P. Ruggi, C. Vorvick, M. Jacobson, M. J. Cowart, B. Sorazu, S. Márka, H. Yamamoto, Mallory S. E. Roberts, A. Thüring, Kenneth A. Strain, M. C. Heintze, P. Schwinberg, C. C. Yancey, Ruxandra Bondarescu, G. Mendell, Fabio Marchesoni, P. Hello, Moritz Mehmet, Richard O'Shaughnessy, B. Barr, J. Steinlechner, A. C. Melissinos, Andrea Chincarini, P. Astone, B. Sassolas, G. R. Skelton, W. G. Anderson, C. Osthelder, Andrew Lundgren, G. Cella, C. L. Mueller, V. Raymond, T. Z. Summerscales, Giacomo Ciani, A. Mullavey, B. P. Abbott, E. K. Gustafson, W. Katzman, R. J.E. Smith, D. E. Clark, Jonathan R. Gair, L. A. Forte, D. O. Bridges, Rebecca Fisher, J. Li, B. E. Aylott, F. Carbognani, Malik Rakhmanov, J. Worden, L. Williams, A. Le Roux, Prayush Kumar, S. Vass, N. A. Lockerbie, Roy Williams, Kyungmin Kim, A. M. Cruise, Fabrice Matichard, G. P. Newton, Ettore Majorana, S. Vitale, M. Fyffe, Yueh-Feng Liu, B. O'Reilly, P. Ehrens, Gabriela Gonzalez, J. M. Hallam, W. Kells, Lucía Santamaría, Vladimir Dergachev, James Whelan, M. Bitossi, E. Forsi, P. Ajith, R. Riesen, M. Cordier, K. Wette, Vuk Mandic, John J. Oh, Th. S. Bauer, D. B. Kelley, Timothy Evans, Zhihui Du, C. Adams, D. Sigg, Eric Oelker, S. W. Ballmer, Yi Pan, J. A. Giaime, Y. M. Kim, Tenglin Li, R. M. Cutler, Rosa Poggiani, P. Campsie, G. Moreno, S. P. Tarabrin, Shaun Hooper, D. F. Menéndez, P. Raffai, Stefan Goßler, I. Kowalska, J. Hanks, S. Van Der Putten, Ranjan Gupta, H. Radkins, E. Saracco, J. C. Barayoga, C. Tomlinson, Richard J. Abbott, Soma Mukherjee, Michael L. Gorodetsky, Drew Keppel, J. M. Berliner, T. Westphal, A. E. Villar, H. Müller-Ebhardt, M. V. Plissi, Nergis Mavalvala, David Coward, Jerome Degallaix, Sheon Chua, C. J. Guido, Christian Röver, R. Bonnand, L. Sperandio, D. S. Rabeling, Rocco Romano, I. Di Palma, Hartmut Grote, Farhan Feroz, G. Losurdo, John D. Scott, D. L. Kinzel, R. A. Mercer, Neil J. Cornish, Matthew P. Edgar, Jesper Munch, P. E. Lindquist, M. A. Frei, D. Fazi, S. H. Huttner, D. Atkinson, Andrew Melatos, M. Lorenzini, A. Masserot, L. Taffarello, Ilya Belopolski, A. Mytidis, Atsushi J. Nishizawa, H. J. Bulten, T. T. Fricke, Roberto Conte, C. Aulbert, D. Simakov, Scott Koranda, L. Matone, J. R. Leong, Evan Ochsner, A. J. Weinstein, P. T. Beyersdorf, M. Landry, L. Di Fiore, M. Barsuglia, A. Grant, L. Zhang, Roman Schnabel, J. E. Brau, B. Canuel, A. A. van Veggel, Efim A. Khazanov, G. Ballardin, M. Phelps, F. Clara, P. Thomas, Erik Katsavounidis, Douglas H Beck, M. J. Lubinski, K. Evans, Rajesh Kumar, Vladimir B. Braginsky, H. Vahlbruch, K. Riles, J. Y. Vinet, N. Fotopoulos, M. Weinert, F. Fidecaro, G. M. Guidi, A. Cumming, E. Genin, A. M. Gretarsson, J. Bauchrowitz, J. K. Blackburn, E. Chassande-Mottin, Sheila Rowan, Todd Adams, Gianluca Persichetti, G. Endroczi, Haixing Miao, S. L. Danilishin, O. Bock, István Rácz, K. L. Dooley, Lisa Barsotti, Alessandra Toncelli, R. J. G. Jonker, Jan Harms, D. Buskulic, F. Kawazoe, O. Torre, E. Cuoco, S. Meshkov, Seog Oh, H. Fehrmann, D. Moraru, Gianpietro Cagnoli, D. Yeaton-Massey, F. Vetrano, S. E. Dwyer, J. Pöld, Suvadeep Bose, Z. Márka, Alberto Vecchio, Will M. Farr, A. Dietz, B. Hughey, E. Steinert, M. R. Smith, M. Edwards, M. Pickenpack, A. Rocchi, T. Hong, Maria Ilaria Del Principe, M. Agathos, S. R. Morriss, Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), APC - Cosmologie, AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut de Physique de Rennes (IPR), Université de Rennes (UR)-Centre National de la Recherche Scientifique (CNRS), Laboratoire des matériaux avancés (LMA), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Astrophysique Relativiste Théories Expériences Métrologie Instrumentation Signaux (ARTEMIS), Université Nice Sophia Antipolis (1965 - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), APC - Gravitation (APC-Gravitation), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Max-Planck-Gesellschaft-Max-Planck-Gesellschaft, Ecole Superieure de Physique et de Chimie Industrielles de la Ville de Paris (ESPCI Paris), Université Paris sciences et lettres (PSL), The LIGO Scientific Collaboration, The Virgo Collaboration, Aasi, J., Abadie, J., Abbott, B. P., Abbott, R., Abbott, T. D., Abernathy, M., Accadia, T., Acernese, F., Adams, C., Adams, T., Addesso, P., Adhikari, R., Affeldt, C., Agathos, M., Agatsuma, K., Ajith, P., Allen, B., Allocca, A., Amador Ceron, E., Amariutei, D., Anderson, S. B., Anderson, W. G., Arai, K., Araya, M. C., Ast, S., Aston, S. M., Astone, P., Atkinson, D., Aufmuth, P., Aulbert, C., Aylott, B. E., Babak, S., Baker, P., Ballardin, G., Ballmer, S., Bao, Y., Barayoga, J. C. B., Barker, D., Barone, F., Barr, B., Barsotti, L., Barsuglia, M., Barton, M. A., Bartos, I., Bassiri, R., Bastarrika, M., Basti, A., Batch, J., Bauchrowitz, J., Bauer, T. h. S., Bebronne, M., Beck, D., Behnke, B., Bejger, M., Beker, M. G., Bell, A. S., Bell, C., Belopolski, I., Benacquista, M., Berliner, J. M., Bertolini, A., Betzwieser, J., Beveridge, N., Beyersdorf, P. T., Bhadbade, T., Bilenko, I. A., Billingsley, G., Birch, J., Biswas, R., Bitossi, M., Bizouard, M. A., Black, E., Blackburn, J. K., Blackburn, L., Blair, D., Bland, B., Blom, M., Bock, O., Bodiya, T. P., Bogan, C., Bond, C., Bondarescu, R., Bondu, F., Bonelli, L., Bonnand, R., Bork, R., Born, M., Boschi, V., Bose, S., Bosi, L., Bouhou, B., Braccini, S., Bradaschia, C., Brady, P. R., Braginsky, V. B., Branchesi, M., Brau, J. E., Breyer, J., Briant, T., Bridges, D. O., Brillet, A., Brinkmann, M., Brisson, V., Britzger, M., Brooks, A. F., Brown, D. A., Bulik, T., Bulten, H. J., Buonanno, A., Burguet?castell, J., Buskulic, D., Buy, C., Byer, R. L., Cadonati, L., Cagnoli, G., Calloni, Enrico, Camp, J. B., Campsie, P., Cannon, K., Canuel, B., Cao, J., Capano, C. D., Carbognani, F., Carbone, L., Caride, S., Caudill, S., Cavagli?, M., Cavalier, F., Cavalieri, R., Cella, G., Cepeda, C., Cesarini, E., Chalermsongsak, T., Charlton, P., Chassande Mottin, E., Chen, W., Chen, X., Chen, Y., Chincarini, A., Chiummo, A., Cho, H. S., Chow, J., Christensen, N., Chua, S. S. Y., Chung, C. T. Y., Chung, S., Ciani, G., Clara, F., Clark, D. E., Clark, J. A., Clayton, J. H., Cleva, F., Coccia, E., Cohadon, P. F., Colacino, C. N., Colla, A., Colombini, M., Conte, A., Conte, R., Cook, D., Corbitt, T. R., Cordier, M., Cornish, N., Corsi, A., Costa, C. A., Coughlin, M., Coulon, J. P., Couvares, P., Coward, D. M., Cowart, M., Coyne, D. C., Creighton, J. D. E., Creighton, T. D., Cruise, A. M., Cumming, A., Cunningham, L., Cuoco, E., Cutler, R. M., Dahl, K., Damjanic, M., Danilishin, S. L., D?antonio, S., Danzmann, K., Dattilo, V., Daudert, B., Daveloza, H., Davier, M., Daw, E. J., Dayanga, T., DE ROSA, Rosario, Debra, D., Debreczeni, G., Degallaix, J., Del Pozzo, W., Dent, T., Dergachev, V., Derosa, R., Dhurandhar, S., Di Fiore, L., Di Lieto, A., Di Palma, I., Di Paolo Emilio, M., Di Virgilio, A., D?az, M., Dietz, A., Donovan, F., Dooley, K. L., Doravari, S., Dorsher, S., Drago, M., Drever, R. W. P., Driggers, J. C., Du, Z., Dumas, J. C., Dwyer, S., Eberle, T., Edgar, M., Edwards, M., Effler, A., Ehrens, P., Endr?czi, G., Engel, R., Etzel, T., Evans, K., Evans, M., Evans, T., Factourovich, M., Fafone, V., Fairhurst, S., Farr, B. F., Farr, W. M., Favata, M., Fazi, D., Fehrmann, H., Feldbaum, D., Feroz, F., Ferrante, I., Ferrini, F., Fidecaro, F., Finn, L. S., Fiori, I., Fisher, R. P., Flaminio, R., Foley, S., Forsi, E., Forte, L. A., Fotopoulos, N., Fournier, J. D., Franc, J., Franco, S., Frasca, S., Frasconi, F., Frede, M., Frei, M. A., Frei, Z., Freise, A., Frey, R., Fricke, T. T., Friedrich, D., Fritschel, P., Frolov, V. V., Fujimoto, M. K., Fulda, P. J., Fyffe, M., Gair, J., Galimberti, M., Gammaitoni, L., Garcia, J., Garufi, Fabio, G?sp?r, M. E., Gelencser, G., Gemme, G., Genin, E., Gennai, A., Gergely, L. ?., Ghosh, S., Giaime, J. A., Giampanis, S., Giardina, K. D., Giazotto, A., Gil Casanova, S., Gill, C., Gleason, J., Goetz, E., Gonz?lez, G., Gorodetsky, M. L., Go?ler, S., Gouaty, R., Graef, C., Graff, P. B., Granata, M., Grant, A., Gray, C., Greenhalgh, R. J. S., Gretarsson, A. M., Griffo, C., Grote, H., Grover, K., Grunewald, S., Guidi, G. M., Guido, C., Gupta, R., Gustafson, E. K., Gustafson, R., Hallam, J. M., Hammer, D., Hammond, G., Hanks, J., Hanna, C., Hanson, J., Harms, J., Harry, G. M., Harry, I. W., Harstad, E. D., Hartman, M. T., Haster, C. J., Haughian, K., Hayama, K., Hayau, J. F., Heefner, J., Heidmann, A., Heintze, M. C., Heitmann, H., Hello, P., Hemming, G., Hendry, M. A., Heng, I. S., Heptonstall, A. W., Herrera, V., Heurs, M., Hewitson, M., Hild, S., Hoak, D., Hodge, K. A., Holt, K., Holtrop, M., Hong, T., Hooper, S., Hough, J., Howell, E. J., Hughey, B., Husa, S., Huttner, S. H., Huynh Dinh, T., Ingram, D. R., Inta, R., Isogai, T., Ivanov, A., Izumi, K., Jacobson, M., James, E., Jang, Y. J., Jaranowski, P., Jesse, E., Johnson, W. W., Jones, D. I., Jones, R., Jonker, R. J. G., Ju, L., Kalmus, P., Kalogera, V., Kandhasamy, S., Kang, G., Kanner, J. B., Kasprzack, M., Kasturi, R., Katsavounidis, E., Katzman, W., Kaufer, H., Kaufman, K., Kawabe, K., Kawamura, S., Kawazoe, F., Keitel, D., Kelley, D., Kells, W., Keppel, D. G., Keresztes, Z., Khalaidovski, A., Khalili, F. Y., Khazanov, E. A., Kim, B. K., Kim, C., Kim, H., Kim, K., Kim, N., Kim, Y. M., King, P. J., Kinzel, D. L., Kissel, J. S., Klimenko, S., Kline, J., Kokeyama, K., Kondrashov, V., Koranda, S., Korth, W. Z., Kowalska, I., Kozak, D., Kringel, V., Krishnan, B., Kr?lak, A., Kuehn, G., Kumar, P., Kumar, R., Kurdyumov, R., Kwee, P., Lam, P. K., Landry, M., Langley, A., Lantz, B., Lastzka, N., Lawrie, C., Lazzarini, A., Le Roux, A., Leaci, P., Lee, C. H., Lee, H. K., Lee, H. M., Leong, J. R., Leonor, I., Leroy, N., Letendre, N., Lhuillier, V., Li, J., T. G. F., Li, Lindquist, P. E., Litvine, V., Liu, Y., Liu, Z., Lockerbie, N. A., Lodhia, D., Logue, J., Lorenzini, M., Loriette, V., Lormand, M., Losurdo, G., Lough, J., Lubinski, M., L?ck, H., Lundgren, A. P., Macarthur, J., Macdonald, E., Machenschalk, B., Macinnis, M., Macleod, D. M., Mageswaran, M., Mailand, K., Majorana, E., Maksimovic, I., Malvezzi, V., Man, N., Mandel, I., Mandic, V., Mantovani, M., Marchesoni, F., Marion, F., M?rka, S., M?rka, Z., Markosyan, A., Maros, E., Marque, J., Martelli, F., Martin, I. W., Martin, R. M., Marx, J. N., Mason, K., Masserot, A., Matichard, F., Matone, L., Matzner, R. A., Mavalvala, N., Mazzolo, G., Mccarthy, R., Mcclelland, D. E., Mcguire, S. C., Mcintyre, G., Mciver, J., Meadors, G. D., Mehmet, M., Meier, T., Melatos, A., Melissinos, A. C., Mendell, G., Men?ndez, D. F., Mercer, R. A., Meshkov, S., Messenger, C., Meyer, M. S., Miao, H., Michel, C., Milano, L., Miller, J., Minenkov, Y., Mingarelli, C. M. F., Mitrofanov, V. P., Mitselmakher, G., Mittleman, R., Moe, B., Mohan, M., Mohapatra, S. R. P., Moraru, D., Moreno, G., Morgado, N., Morgia, A., Mori, T., Morriss, S. R., Mosca, S., Mossavi, K., Mours, B., Mow?lowry, C. M., Mueller, C. L., Mueller, G., Mukherjee, S., Mullavey, A., M?ller Ebhardt, H., Munch, J., Murphy, D., Murray, P. G., Mytidis, A., Nash, T., Naticchioni, L., Necula, V., Nelson, J., Neri, I., Newton, G., Nguyen, T., Nishizawa, A., Nitz, A., Nocera, F., Nolting, D., Normandin, M. E., Nuttall, L., Ochsner, E., O?dell, J., Oelker, E., Ogin, G. H., J. J., Oh, S. H., Oh, Oldenberg, R. G., O?reilly, B., O?shaughnessy, R., Osthelder, C., Ott, C. D., Ottaway, D. J., Ottens, R. S., Overmier, H., Owen, B. J., Page, A., Palladino, L., Palomba, C., Pan, Y., Pankow, C., Paoletti, F., Paoletti, R., Papa, M. A., Parisi, M., Pasqualetti, A., Passaquieti, R., Passuello, D., Pedraza, M., Penn, S., Perreca, A., Persichetti, G., Phelps, M., Pichot, M., Pickenpack, M., Piergiovanni, F., Pierro, V., Pihlaja, M., Pinard, L., Pinto, I. M., Pitkin, M., Pletsch, H. J., Plissi, M. V., Poggiani, R., P?ld, J., Postiglione, F., Poux, C., Prato, M., Predoi, V., Prestegard, T., Price, L. R., Prijatelj, M., Principe, M., Privitera, S., Prodi, G. A., Prokhorov, L. G., Puncken, O., Punturo, M., Puppo, P., Quetschke, V., Quitzow James, R., Raab, F. J., Rabeling, D. S., R?cz, I., Radkins, H., Raffai, P., Rakhmanov, M., Ramet, C., Rankins, B., Rapagnani, P., Raymond, V., Re, V., Reed, C. M., Reed, T., Regimbau, T., Reid, S., Reitze, D. H., Ricci, F., Riesen, R., Riles, K., Roberts, M., Robertson, N. A., Robinet, F., Robinson, C., Robinson, E. L., Rocchi, A., Roddy, S., Rodriguez, C., Rodruck, M., Rolland, L., Rollins, J. G., Romano, R., Romie, J. H., Rosi?ska, D., R?ver, C., Rowan, S., R?diger, A., Ruggi, P., Ryan, K., Salemi, F., Sammut, L., Sandberg, V., Sankar, S., Sannibale, V., Santamar?a, L., Santiago Prieto, I., Santostasi, G., Saracco, E., Sassolas, B., Sathyaprakash, B. S., Saulson, P. R., Savage, R. L., Schilling, R., Schnabel, R., Schofield, R. M. S., Schulz, B., Schutz, B. F., Schwinberg, P., Scott, J., Scott, S. M., Seifert, F., Sellers, D., Sentenac, D., Sergeev, A., Shaddock, D. A., Shaltev, M., Shapiro, B., Shawhan, P., Shoemaker, D. H., Sidery, T. L., Siemens, X., Sigg, D., Simakov, D., Singer, A., Singer, L., Sintes, A. M., Skelton, G. R., Slagmolen, B. J. J., Slutsky, J., Smith, J. R., Smith, M. R., Smith, R. J. E., Smith Lefebvre, N. D., Somiya, K., Sorazu, B., Speirits, F. C., Sperandio, L., Stefszky, M., Steinert, E., Steinlechner, J., Steinlechner, S., Steplewski, S., Stochino, A., Stone, R., Strain, K. A., Strigin, S. E., Stroeer, A. S., Sturani, R., Stuver, A. L., Summerscales, T. Z., Sung, M., Susmithan, S., Sutton, P. J., Swinkels, B., Szeifert, G., Tacca, M., Taffarello, L., Talukder, D., Tanner, D. B., Tarabrin, S. P., Taylor, R., ter Braack, A. P. M., Thomas, P., Thorne, K. A., Thorne, K. S., Thrane, E., Th?ring, A., Titsler, C., Tokmakov, K. V., Tomlinson, C., Toncelli, A., Tonelli, M., Torre, O., Torres, C. V., Torrie, C. I., Tournefier, E., Travasso, F., Traylor, G., Tse, M., Ugolini, D., Vahlbruch, H., Vajente, G., van den Brand, J. F. J., Van Den Broeck, C., van der Putten, S., van Veggel, A. A., Vass, S., Vasuth, M., Vaulin, R., Vavoulidis, M., Vecchio, A., Vedovato, G., Veitch, J., Veitch, P. J., Venkateswara, K., Verkindt, D., Vetrano, F., Vicer?, A., Villar, A. E., Vinet, J. Y., Vitale, S., Vocca, H., Vorvick, C., Vyatchanin, S. P., Wade, A., Wade, L., Wade, M., Waldman, S. J., Wallace, L., Wan, Y., Wang, M., Wang, X., Wanner, A., Ward, R. L., Was, M., Weinert, M., Weinstein, A. J., Weiss, R., Welborn, T., Wen, L., Wessels, P., West, M., Westphal, T., Wette, K., Whelan, J. T., Whitcomb, S. E., White, D. J., Whiting, B. F., Wiesner, K., Wilkinson, C., Willems, P. A., Williams, L., Williams, R., Willke, B., Wimmer, M., Winkelmann, L., Winkler, W., Wipf, C. C., Wiseman, A. G., Wittel, H., Woan, G., Wooley, R., Worden, J., Yablon, J., Yakushin, I., Yamamoto, H., Yamamoto, K., Yancey, C. C., Yang, H., Yeaton Massey, D., Yoshida, S., Yvert, M., Zadro?ny, A., Zanolin, M., Zendri, J. P., Zhang, F., Zhang, L., Zhao, C., Zotov, N., Zucker, M. E., Zweizig, J., Pinto, Innocenzo, Laboratoire d'Annecy de Physique des Particules (LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules), Physique Corpusculaire et Cosmologie - Collège de France (PCC), Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-AstroParticule et Cosmologie (APC (UMR_7164)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Université de Rennes 1 (UR1), Université de Rennes (UNIV-RENNES)-Université de Rennes (UNIV-RENNES)-Centre National de la Recherche Scientifique (CNRS), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Centre National de la Recherche Scientifique (CNRS), Université Nice Sophia Antipolis (... - 2019) (UNS), Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), ESPCI ParisTech, Laboratoire d'Annecy de Physique des Particules ( LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules ), Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Savoie Mont Blanc ( USMB [Université de Savoie] [Université de Chambéry] ) -Centre National de la Recherche Scientifique ( CNRS ), Physique Corpusculaire et Cosmologie - Collège de France ( PCC ), Collège de France ( CdF ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Paris Diderot - Paris 7 ( UPD7 ) -Centre National de la Recherche Scientifique ( CNRS ) -Collège de France ( CdF ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Paris Diderot - Paris 7 ( UPD7 ) -Centre National de la Recherche Scientifique ( CNRS ) -AstroParticule et Cosmologie ( APC - UMR 7164 ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ) -Centre National de la Recherche Scientifique ( CNRS ) -Observatoire de Paris-Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ), Laboratoire de l'Accélérateur Linéaire ( LAL ), Université Paris-Sud - Paris 11 ( UP11 ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ), Institut de Physique de Rennes ( IPR ), Université de Rennes 1 ( UR1 ), Université de Rennes ( UNIV-RENNES ) -Université de Rennes ( UNIV-RENNES ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire des matériaux avancés ( LMA ), Université Claude Bernard Lyon 1 ( UCBL ), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ) -Centre National de la Recherche Scientifique ( CNRS ), AstroParticule et Cosmologie ( APC - UMR 7164 ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ), Astrophysique Relativiste Théories Expériences Métrologie Instrumentation Signaux ( ARTEMIS ), Université Nice Sophia Antipolis ( UNS ), Université Côte d'Azur ( UCA ) -Université Côte d'Azur ( UCA ) -Institut national des sciences de l'Univers ( INSU - CNRS ) -Observatoire de la Côte d'Azur, Université Côte d'Azur ( UCA ) -Centre National de la Recherche Scientifique ( CNRS ), APC - Gravitation ( APC-Gravitation ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ) -Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ) -Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut), Max-Planck-Institut-Max-Planck-Institut, Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon, Centre National de la Recherche Scientifique (CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Nice Sophia Antipolis (... - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), and (Astro)-Particles Physics
Subjects: Gravitational-wave observatory, Physics and Astronomy (miscellaneous), ELECTROMAGNETIC COUNTERPARTS, MASS-DISTRIBUTION, BLACK-HOLES, TRANSIENTS, INSPIRALS, COSMOLOGY, PHYSICS, SEARCH, Astrophysics, Parameter space, 01 natural sciences, neutron stars, General Relativity and Quantum Cosmology, Detection of gravitational wave, 010303 astronomy & astrophysics, QC, LIGO Scientific Collaboration, QB, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, Estimation theory, [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Detector, Settore FIS/01 - Fisica Sperimentale, Nuclear and High Energy Physics, Justice and Strong Institutions, gravitational waves, [PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], Astrophysics - High Energy Astrophysical Phenomena, Algorithm, Gravitation, [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], SDG 16 - Peace, FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), [ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], Settore FIS/05 - Astronomia e Astrofisica, 0103 physical sciences, 010308 nuclear & particles physics, Gravitational wave, Model selection, SDG 16 - Peace, Justice and Strong Institutions, [ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], black holes, LIGO, cosmology: observations, [ SDU.ASTR.HE ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]
Abstract: Compact binary systems with neutron stars or black holes are one of the most promising sources for ground-based gravitational wave detectors. Gravitational radiation encodes rich information about source physics; thus parameter estimation and model selection are crucial analysis steps for any detection candidate events. Detailed models of the anticipated waveforms enable inference on several parameters, such as component masses, spins, sky location and distance that are essential for new astrophysical studies of these sources. However, accurate measurements of these parameters and discrimination of models describing the underlying physics are complicated by artifacts in the data, uncertainties in the waveform models and in the calibration of the detectors. Here we report such measurements on a selection of simulated signals added either in hardware or software to the data collected by the two LIGO instruments and the Virgo detector during their most recent joint science run, including a "blind injection" where the signal was not initially revealed to the collaboration. We exemplify the ability to extract information about the source physics on signals that cover the neutron star and black hole parameter space over the individual mass range 1 Msun - 25 Msun and the full range of spin parameters. The cases reported in this study provide a snap-shot of the status of parameter estimation in preparation for the operation of advanced detectors., Comment: 23 pages, 18 figures. LIGO Document P1200021. See the announcement for this paper on ligo.org at: http://www.ligo.org/science/Publication-S6PE/index.php. For a repository of data used in the publication, go to: https://dcc.ligo.org/LIGO-P1200021/public; Modifications thanks to referee reports
Published: 2013

25. Local space density and formation rate of planetary nebulae

Subjects: stars, HOT, STANDARD CANDLES, Astrophysics::High Energy Astrophysical Phenomena, distances, PROPER MOTIONS, Astrophysics::Cosmology and Extragalactic Astrophysics, planetary nebulae, NLTE-ANALYSIS, BINARY CENTRAL STAR, general, X-rays, Astrophysics::Solar and Stellar Astrophysics, NON-LTE ANALYSIS, Astrophysics::Earth and Planetary Astrophysics, WHITE-DWARFS, Astrophysics::Galaxy Astrophysics, HIGH-RESOLUTION SPECTROSCOPY, white dwarfs, fundamental parameters, MASS-DISTRIBUTION, GALACTIC-CENTER
Abstract: Individual distances of 50 nearby planetary nebulae are determined using a variety of methods, but excluding statistical methods or distance scales. These distances, together with a discussion of the sample completeness, are used to determine local PN formation rate. Together with the brightness of the nebula, its ionized mass is derived. The evolution of the ionized mass is discussed. As a by-product, the Zanstra temperature of the central stars of the optically thick nebulae is found. Interestingly this temperature indicates that the DA white dwarfs in the sample are considerably hotter than previously thought. Finally, with the help of the galactic bulge PN, a luminosity function for PN in the galaxy is derived.
Published: 1996

26. Analytical properties of Einasto dark matter haloes

Author: Maarten Baes, Francisco Frutos-Alfaro, E. Retana-Montenegro, Gianfranco Gentile, and E. Van Hese
Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO), Dark matter, FOS: Physical sciences, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, SCALING RELATIONS, dark matter, STRUCTURAL PARAMETERS, analytical [methods], weak [gravitational lensing], UNIVERSAL DENSITY PROFILE, ELLIPTIC GALAXIES, clusters: general [galaxies], EARLY-TYPE GALAXIES, ANALYTICAL EXPRESSIONS, Einasto profile, MASS-DISTRIBUTION, Physics, Spiral galaxy, Mass distribution, DEPROJECTED SERSIC MODEL, Astronomy and Astrophysics, LOW SURFACE BRIGHTNESS, Integral transform, halos [galaxies], Dark matter halo, Physics and Astronomy, Space and Planetary Science, strong [gravitational lensing], Series expansion, Surface mass, SPIRAL GALAXIES, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: Recent high-resolution N-body CDM simulations indicate that nonsingular three-parameter models such as the Einasto profile perform better than the singular two-parameter models, e.g. the Navarro, Frenk and White, in fitting a wide range of dark matter haloes. While many of the basic properties of the Einasto profile have been discussed in previous studies, a number of analytical properties are still not investigated. In particular, a general analytical formula for the surface density, an important quantity that defines the lensing properties of a dark matter halo, is still lacking to date. To this aim, we used a Mellin integral transform formalism to derive a closed expression for the Einasto surface density and related properties in terms of the Fox H and Meijer G functions, which can be written as series expansions. This enables arbitrary-precision calculations of the surface density and the lensing properties of realistic dark matter halo models. Furthermore, we compared the S\'ersic and Einasto surface mass densities and found differences between them, which implies that the lensing properties for both profiles differ., Comment: 10 pages, 2 figures. Accepted for publication in Astronomy and Astrophysics
Published: 2012

27. SPIRAL STRUCTURE OF M-83 - DISTRIBUTION AND KINEMATICS OF THE ATOMIC AND IONIZED HYDROGEN

Subjects: INTERSTELLAR MEDIUM, GALAXY NGC-6946, NEUTRAL-HYDROGEN, KINEMATICS AND DYNAMICS, GENERAL, SURFACE PHOTOMETRY, RADIO-CONTINUUM EMISSION, GALAXIES, H-II REGIONS, STRUCTURE OF, SPIRAL, STAR FORMATION, DENSITY WAVE, CARBON-MONOXIDE, GIANT MOLECULAR ASSOCIATIONS, INDIVIDUAL (M-83), MASS-DISTRIBUTION
Abstract: We present high-resolution observations of the atomic hydrogen (H I) and Hbeta emission lines in the southern grand-design spiral galaxy M 83. Contrary to the case of M51, we have not detected streaming motions of a magnitude of 60-90 km s-1 (in the plane of the disk) across the spiral arms of M 83 either in H I or in Hbeta. The Hbeta observations hint at streaming motions at a level of 35 km s-1, comparable to the motions seen in M81. Significant deviations from circular rotation are observed in the regions where the bar connects with the spiral arms, both in H I and Hbeta. The gas is moving tangentially faster in these regions compared to a simple model for the rotation in the disk of M 83. These motions are similar to the streaming motions observed in CO (Kenney & Lord 1991). The H I observations have revealed a large-scale displacement (700 pc) of the atomic gas from the dust lane along a 7 kpc stretch of the inner eastern spiral arm of M 83. This separation can not be explained by beam smoothing. The atomic gas in that part of the arm is coincident with the ridge of H II complexes along the outer edge of the spiral arm. The observations, as well as recent CO observations of the eastern arm of M 83, are discussed in the context of two scenarios that attempt to explain the observed morphology of the interstellar medium (ISM) in the eastern spiral arm. The dissociation scenario assumes the ISM to be predominantly molecular at the position of the dust lanes and to (partly) dissociate into the observed H I ridge downstream. The diffuse-shock scenario assumes that the massive clouds shock at the observed location of the CO, H I, and H II regions, whereas a shock in a more diffuse medium results in the dust lane upstream. We argue in this paper that the effect of heating of the CO in the spiral arm may have been underestimated in the interpretation of the CO observations. Heating may have increased the CO brightness downstream from the shock substantially in which case the observed CO distribution across the spiral arm does not accurately reflect the underlying distribution of the molecular gas. The dissociation scenario appears to apply in M51, and the diffuse-shock scenario in M81; these are two galaxies which may be at opposite extremes with regard to the strength of the density-wave shock and the fraction of ISM in molecular hydrogen. M 83 may be an intermediate case lacking the strong density-wave shock, a suggestion which is observationally supported by our failure to detect streaming motions like those in M51.
Published: 1993

28. The dark matter halo shape of edge-on disk galaxies III. Modelling the HI observations

Author: Kenneth C. Freeman, P. C. van der Kruit, J. O'Brien, and Astronomy
Subjects: galaxies: halos, FOS: Physical sciences, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Flattening, Gravitational potential, GALACTIC DISKS, Differential rotation, Galaxy rotation curve, Astrophysics::Galaxy Astrophysics, galaxies: kinematics and dynamics, MASS-DISTRIBUTION, Physics, Velocity dispersion, Astronomy and Astrophysics, Astrophysics - Astrophysics of Galaxies, Galaxy, NGC 891, Dark matter halo, NEUTRAL HYDROGEN, Space and Planetary Science, GAS, Astrophysics of Galaxies (astro-ph.GA), ROTATION CURVES, galaxies: structure, MILKY-WAY, Halo, VELOCITY DISPERSION, SPIRAL GALAXIES, galaxies: ISM, HIGH-RESOLUTION
Abstract: This is the third paper in a series in which we attempt to put constraints on the flattening of dark halos in disk galaxies. For this purpose we need to analyse the observed XV diagrams in edge-on galaxies to accurately measure the radial HI surface density, the rotation curve and the HI velocity dispersion. We present the results of the modelling of HI observations of 8 HI-rich, late-type, edge-on galaxies. In all of these we find differential rotation. Most systems display HI velocity dispersions of 6.5 to 7.5 km s$^{-1}$ and all except one show radial structure. There is an increase in the mean HI velocity dispersion with maximum rotation velocity, at least up to 120 km s$^{-1}$. Next we analyse the observations to derive the radial variation of the thickness (flaring) of the HI layer. We find that with the exception of the asymmetric IC5052, all of the galaxies in our sample are good candidates for 3D mass modelling to measure the dark halo shape. The flaring profiles are symmetric and have a common shape, increasing linearly inside the stellar disks and exponential outside where the gravitational potential is dominated by the dark halo. In the best example, UGC7321, we find in the inner regions small deviations from the midplane and accompanying increases in thickness of the HI layer that are possibly a result of perturbations by a relatively strong bar., Accepted for publication by Astronomy & Astrophysics. Higher resolution version available at http://www.astro.rug.nl/~vdkruit/jea3/homepage/12567.pdf
Published: 2010

29. A DARK-HALO-DOMINATED GALAXY - NGC-5585

Subjects: NEUTRAL HYDROGEN, ROTATION CURVES, NGC-3198, SPIRAL GALAXIES, MATTER, PARAMETERS, H-I, MASS-DISTRIBUTION
Abstract: Studies of the light distribution, the H I kinematics, and the mass distribution of NGC 5585, a late-type spiral galaxy in the M101 group, are presented. From the photometry, an extrapolated central surface brightness B(0)c = 21.94 mag arcsec-2 and a scale length alpha-1 = 1.4 kpc are derived for the stellar disk. The H I distribution reaches a diameter of 12 arcmin, more than two times the optical diameter. The velocity field reveals a strong warp. The position angle is shown to vary from 45-degrees to 55-degrees in the outer parts, while the inclination is fairly constant at 52-degrees. The rotation curve, derived from this velocity field, reaches a maximum velocity of approximately 90 km s-1, extending out to 7 optical scale lengths. Combining the optical and kinematical data, mass models for NGC 5585 were built using both the "best-fit" and the "maximum-disk" approaches. For both models, the dark-halo component is by far the main contributor to the rotation curve and its basic parameters are fairly well constrained with a core radius r(c) = 3.0 +/- 0.2 kpc and a central density rho-0 = 0.054 +/- 0.006 M . pc-3. At the last observed point (r = 9.65 kpc), approximately 90% of the total mass is dark. Even the gaseous component is dynamically more important than the stellar disk component. In fact, despite being a fairly bright system with M(T)0(B) = -17.5, NGC 5585 is similar to many fainter dwarf systems where the stellar disk is clearly not self-gravitating even in the inner parts.
Published: 1991

30. Declining Rotation Curves: The End of a Conspiracy?

Author: J. H. van Gorkom and Stefano Casertano
Subjects: Dark matter, Angular velocity, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Rotation, Hubble sequence, symbols.namesake, Circular motion, DISK, Galaxy rotation curve, Astrophysics::Galaxy Astrophysics, TIDAL TORQUES, MASS-DISTRIBUTION, Physics, NEUTRAL HYDROGEN OBSERVATIONS, CCD SURFACE PHOTOMETRY, DARK MATTER, GALACTIC HALOS, Astronomy, Astronomy and Astrophysics, 21-CM LINE, Galaxy, Space and Planetary Science, symbols, Hydrogen line, SPIRAL GALAXIES, FIELD GALAXIES
Abstract: New observations of H I rotation curves at the Very Large Array have uncovered two galaxies with rotation curves declining between 1 and 3 optical radii. The velocity decrease is large, more than 50 km s-1 (approximately 25% of the maximum rotation velocity), and is present on both sides of the galaxies; projection effects can be ruled out. We interpret the decrease in rotation velocity as an indication of a large ratio of luminous to dark mass in the luminous regions of these systems. An analysis of the current observations combined with rotation curves from the literature shows a clear correlation between peak circular velocity of a galaxy, its central surface brightness and the slope of the rotation curve in the outer parts. This correlation indicates a weakening of the well-known conspiracy between luminous and dark matter, and may provide evidence in favor of the idea that dark matter is baryonic. Although we do not sample the full morphological Hubble sequence, a strong correlation between slope of the rotation curve and morphological type is found. This result seems to support earlier suggestions that the ratio between the mass in dark and luminous matter might be the critical parameter that controls the Hubble sequence.
Published: 1991

31. Spatially Resolved Stellar Kinematics of Field Early-Type Galaxies at z=1: Evolution of the Rotation Rate

Author: Arjen van der Wel and Roeland P. van der Marel
Subjects: Stellar kinematics, FOS: Physical sciences, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Virial theorem, Luminosity, STAR-FORMATION, cD, ELLIPTIC GALAXIES, Z=0.5 CLUSTERS, kinematics and dynamics [galaxies], TO-LIGHT RATIO, fundamental parameters [galaxies], Surface brightness, evolution [galaxies], Astrophysics::Galaxy Astrophysics, LENTICULAR GALAXIES, MASS-DISTRIBUTION, Physics, Astrophysics (astro-ph), Velocity dispersion, Astronomy and Astrophysics, SAURON PROJECT, Galaxy, Redshift, Physics and Astronomy, Space and Planetary Science, FUNDAMENTAL PLANE, Elliptical galaxy, Astrophysics::Earth and Planetary Astrophysics, DYNAMICAL MODELS, MORPHOLOGY-DENSITY RELATION, elliptical and lenticular [galaxies]
Abstract: We use the spatial information of our previously published VLT/FORS2 absorption line spectroscopy to measure mean stellar velocity and velocity dispersion profiles of 25 field early-type galaxies at a median redshift z=0.97 (full range 0.6, Comment: To appear in ApJ 683 (9 pages, 7 figures). Minor changes included to match published version
Published: 2008

32. The survival of dark matter halos in the cluster Cl0024+16

Author: Ian Smail, Marceau Limousin, Sean M. Moran, Tommaso Treu, Richard S. Ellis, Priyamvada Natarajan, Oliver Czoske, Jean-Paul Kneib, Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Astronomy, and Beaussier, Catherine
Subjects: Cold dark matter, Structure formation, media_common.quotation_subject, Dark matter, galaxies: halos, FOS: Physical sciences, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, dark matter, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], 0103 physical sciences, HIGH-VELOCITY CLOUDS, 010306 general physics, 010303 astronomy & astrophysics, Galaxy cluster, Weak gravitational lensing, Astrophysics::Galaxy Astrophysics, MASS-DISTRIBUTION, media_common, Physics, Mass distribution, Astrophysics (astro-ph), RICH CLUSTERS, Astronomy and Astrophysics, HUBBLE-SPACE-TELESCOPE, FIELD SPECTROSCOPIC SURVEY, ADIABATIC CONTRACTION, LENSING ANALYSIS, Galaxy, Universe, [PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], galaxies: clusters: general, Space and Planetary Science, DIGITAL SKY SURVEY, GALAXY CLUSTERS, SPIRAL GALAXIES
Abstract: Theories of structure formation in a cold dark matter dominated Universe predict that massive clusters of galaxies assemble from the hierarchical merging of lower mass subhalos. Exploiting strong and weak gravitational lensing signals inferred from panoramic HST imaging data, we present a high resolution reconstruction of the mass distribution in the massive, lensing cluster Cl0024+16. Applying galaxy-galaxy lensing techniques we track the fate of dark matter subhalos as a function of projected cluster-centric radius out to 5 Mpc, well beyond the virial radius. We report the first detection of the statistical lensing signal of dark matter subhalos associated with late-type galaxies in clusters. The mass of a typical dark matter subhalo that hosts an L* galaxy increases with projected cluster-centric radius in line with expectations from the tidal stripping hypothesis. Early-type galaxies appear to be hosted on average in more massive dark matter subhalos compared to late-type galaxies. We interpret our findings as evidence for the active assembly of mass via tidal stripping in galaxy clusters. The mass function of dark matter subhalos as a function of projected cluster-centric radius, is compared with an equivalent mass function derived from clusters in the Millenium Run simulation populated with galaxies using semi-analytic models. The shape of the lensing determined mass functions are in very good agreement with the subhalo mass functions derived from the Millenium Run simulation. However, simulated subhalos appear to be more efficiently stripped than lensing observations suggest. (Abridged), 35 pages, 7 figures, revised version, accepted by ApJ
Published: 2007

33. Structure and dynamics of disks in galaxies

Author: van der Kruit, PC, DaCosta, GS, Jerjen, H, and Kapteyn Astronomical Institute
Subjects: ON SPIRAL GALAXIES, GALACTIC DISKS, 3-DIMENSIONAL DISTRIBUTION, STABILITY, STELLAR KINEMATICS, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics::Earth and Planetary Astrophysics, BAND SURFACE PHOTOMETRY, IC-5249, DOMINATED GALAXIES, Astrophysics::Galaxy Astrophysics, PARAMETERS, MASS-DISTRIBUTION
Abstract: One the most cited papers in astronomy is Ken Freeman's 1970 paper on exponential disks in galaxies. In this contribution I review what has been done in this area since then and what we can infer about systematic properties of disks in galaxies from surface photometry, HI synthesis observations and measurements of stellar kinematics. Most disks have radial truncations at 3.6 +/- 0.6 radial scalelengths h(R). Galaxy disk thicknesses h(R)/h(z) = 7.3 +/- 2.2 imply that these disk cannot be "maximum disks". I briefly discuss a recent study of the "superthin" edge-on galaxy IC 5249.
Published: 2002

34. Structure and dynamics of disks in galaxies

Subjects: ON SPIRAL GALAXIES, GALACTIC DISKS, 3-DIMENSIONAL DISTRIBUTION, STABILITY, STELLAR KINEMATICS, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics::Earth and Planetary Astrophysics, BAND SURFACE PHOTOMETRY, IC-5249, DOMINATED GALAXIES, Astrophysics::Galaxy Astrophysics, PARAMETERS, MASS-DISTRIBUTION
Abstract: One the most cited papers in astronomy is Ken Freeman's 1970 paper on exponential disks in galaxies. In this contribution I review what has been done in this area since then and what we can infer about systematic properties of disks in galaxies from surface photometry, HI synthesis observations and measurements of stellar kinematics. Most disks have radial truncations at 3.6 +/- 0.6 radial scalelengths h(R). Galaxy disk thicknesses h(R)/h(z) = 7.3 +/- 2.2 imply that these disk cannot be "maximum disks". I briefly discuss a recent study of the "superthin" edge-on galaxy IC 5249.
Published: 2002

35. Gravitational lensing in modified Newtonian dynamics

Author: Edwin L. Turner and Daniel J. Mortlock
Subjects: relativity, General relativity, media_common.quotation_subject, Cosmic microwave background, Dark matter, gravitational lensing, UNIVERSE, FOS: Physical sciences, Cosmological constant, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Astronomy & Astrophysics, Gravitational microlensing, dark matter, astro-ph, 0201 Astronomical and Space Sciences, RECONSTRUCTION, Astrophysics::Galaxy Astrophysics, COSMOLOGICAL CONSTANT, media_common, acceleration of particles, MASS-DISTRIBUTION, Physics, Science & Technology, Astrophysics (astro-ph), Astronomy and Astrophysics, Universe, Modified Newtonian dynamics, COLD DARK-MATTER, GALAXIES, Gravitational lens, DEFLECTION, Space and Planetary Science, gravitation, Physics::Space Physics, Physical Sciences, DIGITAL SKY SURVEY, CLUSTERS, LOCAL GROUP
Abstract: Modified Newtonian dynamics (MOND) is an alternative theory of gravity that aims to explain large-scale dynamics without recourse to any form of dark matter. However the theory is incomplete, lacking a relativistic counterpart, and so makes no definite predictions about gravitational lensing. The most obvious form that MONDian lensing might take is that photons experience twice the deflection of massive particles moving at the speed of light, as in general relativity (GR). In such a theory there is no general thin-lens approximation (although one can be made for spherically-symmetric deflectors), but the three-dimensional acceleration of photons is in the same direction as the relativistic acceleration would be. In regimes where the deflector can reasonably be approximated as a single point-mass (specifically low-optical depth microlensing and weak galaxy-galaxy lensing), this naive formulation is consistent with observations. Forthcoming galaxy-galaxy lensing data and the possibility of cosmological microlensing have the potential to distinguish unambiguously between GR and MOND. Some tests can also be performed with extended deflectors, for example by using surface brightness measurements of lens galaxies to model quasar lenses, although the breakdown of the thin-lens approximation allows an extra degree of freedom. Nonetheless, it seems unlikely that simple ellipsoidal galaxies can explain both constraints. Further, the low-density universe implied by MOND must be completely dominated by the cosmological constant (to fit microwave background observations), and such models are at odds with the low frequency of quasar lenses. These conflicts might be resolved by a fully consistent relativistic extension to MOND; the alternative is that MOND is not an accurate description of the universe., Comment: MNRAS, in press; 11 pages, 10 figures
Published: 2001

36. Photoionization modelling of planetary nebulae - II. Galactic bulge nebulae, a comparison with literature results

Author: van Hoof, PAM, Van de Steene, GC, and Kapteyn Astronomical Institute
Subjects: methods : data analysis, MAGNITUDES, ISM : abundances, EVOLUTION, CHEMICAL-COMPOSITIONS, ABUNDANCES, TEMPERATURES, planetary nebulae : general, Astrophysics::Solar and Stellar Astrophysics, SPECTROPHOTOMETRY, Astrophysics::Earth and Planetary Astrophysics, CENTRAL STARS, ATMOSPHERES, EMISSION, Astrophysics::Galaxy Astrophysics, MASS-DISTRIBUTION
Abstract: We have constructed photoionization models of five galactic bulge planetary nebulae using our automatic method, which enables a fully self-consistent determination of the physical parameters of a planetary nebula. The models are constrained using the spectrum, the IRAS and radio fluxes and the angular diameter of the nebula. We also conducted a literature search for physical parameters determined with classical methods for these nebulae. Comparison of the distance-independent physical parameters with published data shows that the stellar temperatures generally are in good agreement and can be considered reliable. The literature data for the electron temperature, electron density and also for the abundances show a large spread, indicating that the use of line diagnostics is not reliable and that the accuracy of these methods needs to be improved. Comparison of the various abundance determinations indicates that the uncertainty in the electron temperature is the main source of uncertainty in the abundance determination. The stellar magnitudes predicted by the photoionization models are in good agreement with observed values.
Published: 1999

37. Lensed galaxies in Abell 370 I. Modeling the number counts and redshift distribution of background sources

Author: Bézecourt, J., Jean-Paul Kneib, Soucail, G., Ebbels, T. M. D., and Kapteyn Astronomical Institute
Subjects: galaxies : evolution, galaxies : clusters : individual : A 370, RICH CLUSTER AC-114, Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, GIANT ARCS, EVOLUTION, ARC STATISTICS, GRAVITATIONAL ARCLETS, cosmology : observations, SPACE-TELESCOPE OBSERVATIONS, cosmology : gravitational lensing, RECONSTRUCTION, FIELD, DISTANT CLUSTER, Astrophysics::Galaxy Astrophysics, MASS-DISTRIBUTION
Abstract: We present new observations of the cluster-lens Abell 370: a deep HST/WFPC2 F675W image and ESO 3.6m spectroscopy of faint galaxies. These observations shade new lights on the statistical properties of faint lensed galaxies. In particular, we spectroscopically confirm the multiple image nature of the B2--B3 gravitational pair (Kneib et al. 1993), and determine a redshift of z=0.806 which is in very good agreement with earlier predictions. A refined mass model of the cluster core (that includes cluster galaxy halos) is presented, based on a number of newly identified multiple images. Following Bezecourt et al. (1998a), we combine the new cluster mass model with a spectrophotometric prescription for galaxy evolution to predict the arclets number counts and redshift distribution in the HST image. In particular, the ellipticity distribution of background sources is taken into account, in order to properly estimate the statistical number and redshift distribution of arclets. We show that the redshift distribution of arclets, and particularly its high redshift tail can be used as a strong constraint to disentangle different galaxy evolution scenario. A hierarchical model which includes a number density evolution is favored by our analysis. Finally, we compute the depletion curves in the faint galaxies number counts and discuss its wavelength dependence., 10 pages, Astronomy and Astrophysics in press
Published: 1998

38. SPIRAL STRUCTURE OF M-83 - DISTRIBUTION AND KINEMATICS OF THE ATOMIC AND IONIZED HYDROGEN

Author: TILANUS, RPJ, ALLEN, RJ, and Kapteyn Astronomical Institute
Subjects: INTERSTELLAR MEDIUM, GENERAL, GALAXY NGC-6946, NEUTRAL-HYDROGEN, GALAXIES, STRUCTURE OF, INTERSTELLAR MEDIUM, KINEMATICS AND DYNAMICS, SURFACE PHOTOMETRY, RADIO-CONTINUUM EMISSION, H-II REGIONS, STAR FORMATION, DENSITY WAVE, GALAXIES, SPIRAL, GALAXIES, INDIVIDUAL (M-83), CARBON-MONOXIDE, GIANT MOLECULAR ASSOCIATIONS, MASS-DISTRIBUTION
Abstract: We present high-resolution observations of the atomic hydrogen (H I) and Hbeta emission lines in the southern grand-design spiral galaxy M 83. Contrary to the case of M51, we have not detected streaming motions of a magnitude of 60-90 km s-1 (in the plane of the disk) across the spiral arms of M 83 either in H I or in Hbeta. The Hbeta observations hint at streaming motions at a level of 35 km s-1, comparable to the motions seen in M81. Significant deviations from circular rotation are observed in the regions where the bar connects with the spiral arms, both in H I and Hbeta. The gas is moving tangentially faster in these regions compared to a simple model for the rotation in the disk of M 83. These motions are similar to the streaming motions observed in CO (Kenney & Lord 1991). The H I observations have revealed a large-scale displacement (700 pc) of the atomic gas from the dust lane along a 7 kpc stretch of the inner eastern spiral arm of M 83. This separation can not be explained by beam smoothing. The atomic gas in that part of the arm is coincident with the ridge of H II complexes along the outer edge of the spiral arm. The observations, as well as recent CO observations of the eastern arm of M 83, are discussed in the context of two scenarios that attempt to explain the observed morphology of the interstellar medium (ISM) in the eastern spiral arm. The dissociation scenario assumes the ISM to be predominantly molecular at the position of the dust lanes and to (partly) dissociate into the observed H I ridge downstream. The diffuse-shock scenario assumes that the massive clouds shock at the observed location of the CO, H I, and H II regions, whereas a shock in a more diffuse medium results in the dust lane upstream. We argue in this paper that the effect of heating of the CO in the spiral arm may have been underestimated in the interpretation of the CO observations. Heating may have increased the CO brightness downstream from the shock substantially in which case the observed CO distribution across the spiral arm does not accurately reflect the underlying distribution of the molecular gas. The dissociation scenario appears to apply in M51, and the diffuse-shock scenario in M81; these are two galaxies which may be at opposite extremes with regard to the strength of the density-wave shock and the fraction of ISM in molecular hydrogen. M 83 may be an intermediate case lacking the strong density-wave shock, a suggestion which is observationally supported by our failure to detect streaming motions like those in M51.
Published: 1993

39. A DARK-HALO-DOMINATED GALAXY - NGC-5585

Author: COTE, S, CARIGNAN, C, and SANCISI, R
Subjects: NEUTRAL HYDROGEN, ROTATION CURVES, NGC-3198, Astrophysics::Earth and Planetary Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, SPIRAL GALAXIES, MATTER, Astrophysics::Galaxy Astrophysics, PARAMETERS, H-I, MASS-DISTRIBUTION
Abstract: Studies of the light distribution, the H I kinematics, and the mass distribution of NGC 5585, a late-type spiral galaxy in the M101 group, are presented. From the photometry, an extrapolated central surface brightness B(0)c = 21.94 mag arcsec-2 and a scale length alpha-1 = 1.4 kpc are derived for the stellar disk. The H I distribution reaches a diameter of 12 arcmin, more than two times the optical diameter. The velocity field reveals a strong warp. The position angle is shown to vary from 45-degrees to 55-degrees in the outer parts, while the inclination is fairly constant at 52-degrees. The rotation curve, derived from this velocity field, reaches a maximum velocity of approximately 90 km s-1, extending out to 7 optical scale lengths. Combining the optical and kinematical data, mass models for NGC 5585 were built using both the "best-fit" and the "maximum-disk" approaches. For both models, the dark-halo component is by far the main contributor to the rotation curve and its basic parameters are fairly well constrained with a core radius r(c) = 3.0 +/- 0.2 kpc and a central density rho-0 = 0.054 +/- 0.006 M . pc-3. At the last observed point (r = 9.65 kpc), approximately 90% of the total mass is dark. Even the gaseous component is dynamically more important than the stellar disk component. In fact, despite being a fairly bright system with M(T)0(B) = -17.5, NGC 5585 is similar to many fainter dwarf systems where the stellar disk is clearly not self-gravitating even in the inner parts.
Published: 1991

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