1. Directional limits on persistent gravitational waves using LIGO S5 science data.
- Author
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Abadie J, Abbott BP, Abbott R, Abernathy M, Accadia T, Acernese F, Adams C, Adhikari R, Ajith P, Allen B, Allen GS, Ceron EA, Amin RS, Anderson SB, Anderson WG, Antonucci F, Arain MA, Araya MC, Aronsson M, Arun KG, Aso Y, Aston SM, Astone P, Atkinson D, Aufmuth P, Aulbert C, Babak S, Baker P, Ballardin G, Ballmer S, Barker D, Barnum S, Barone F, Barr B, Barriga P, Barsotti L, Barsuglia M, Barton MA, Bartos I, Bassiri R, Bastarrika M, Bauchrowitz J, Bauer TS, Behnke B, Beker MG, Belletoile A, Benacquista M, Bertolini A, Betzwieser J, Beveridge N, Beyersdorf PT, Bigotta S, Bilenko IA, Billingsley G, Birch J, Birindelli S, Biswas R, Bitossi M, Bizouard MA, Black E, Blackburn JK, Blackburn L, Blair D, Bland B, Blom M, Boccara C, Bock O, Bodiya TP, Bondarescu R, Bondu F, Bonelli L, Bonnand R, Bork R, Born M, Bose S, Bosi L, Bouhou B, Boyle M, Braccini S, Bradaschia C, Brady PR, Braginsky VB, Brau JE, Breyer J, Bridges DO, Brillet A, Brinkmann M, Brisson V, Britzger M, Brooks AF, Brown DA, Budzyński R, Bulik T, Bulten HJ, Buonanno A, Burguet-Castell J, Burmeister O, Buskulic D, Buy C, Byer RL, Cadonati L, Cagnoli G, Cain J, Calloni E, Camp JB, Campagna E, Campsie P, Cannizzo J, Cannon K, Canuel B, Cao J, Capano C, Carbognani F, Caride S, Caudill S, Cavaglià M, Cavalier F, Cavalieri R, Cella G, Cepeda C, Cesarini E, Chalermsongsak T, Chalkley E, Charlton P, Chassande-Mottin E, Chelkowski S, Chen Y, Chincarini A, Christensen N, Chua SS, Chung CT, Clark D, Clark J, Clayton JH, Cleva F, Coccia E, Colacino CN, Colas J, Colla A, Colombini M, Conte R, Cook D, Corbitt TR, Cornish N, Corsi A, Costa CA, Coulon JP, Coward DM, Coyne DC, Creighton JD, Creighton TD, Cruise AM, Culter RM, Cumming A, Cunningham L, Cuoco E, Dahl K, Danilishin SL, Dannenberg R, D'Antonio S, Danzmann K, Das K, Dattilo V, Daudert B, Davier M, Davies G, Davis A, Daw EJ, Day R, Dayanga T, De Rosa R, DeBra D, Degallaix J, del Prete M, Dergachev V, DeRosa R, DeSalvo R, Devanka P, Dhurandhar S, Di Fiore L, Di Lieto A, Di Palma I, Di Paolo Emilio M, Di Virgilio A, Díaz M, Dietz A, Donovan F, Dooley KL, Doomes EE, Dorsher S, Douglas ES, Drago M, Drever RW, Driggers JC, Dueck J, Dumas JC, Eberle T, Edgar M, Edwards M, Effler A, Ehrens P, Engel R, Etzel T, Evans M, Evans T, Fafone V, Fairhurst S, Fan Y, Farr BF, Fazi D, Fehrmann H, Feldbaum D, Ferrante I, Fidecaro F, Finn LS, Fiori I, Flaminio R, Flanigan M, Flasch K, Foley S, Forrest C, Forsi E, Fotopoulos N, Fournier JD, Franc J, Frasca S, Frasconi F, Frede M, Frei M, Frei Z, Freise A, Frey R, Fricke TT, Friedrich D, Fritschel P, Frolov VV, Fulda P, Fyffe M, Galimberti M, Gammaitoni L, Garofoli JA, Garufi F, Gemme G, Genin E, Gennai A, Gholami I, Ghosh S, Giaime JA, Giampanis S, Giardina KD, Giazotto A, Gill C, Goetz E, Goggin LM, González G, Gorodetsky ML, Gossler S, Gouaty R, Graef C, Granata M, Grant A, Gras S, Gray C, Greenhalgh RJ, Gretarsson AM, Greverie C, Grosso R, Grote H, Grunewald S, Guidi GM, Gustafson EK, Gustafson R, Hage B, Hall P, Hallam JM, Hammer D, Hammond G, Hanks J, Hanna C, Hanson J, Harms J, Harry GM, Harry IW, Harstad ED, Haughian K, Hayama K, Hayau JF, Hayler T, Heefner J, Heitmann H, Hello P, Heng IS, Heptonstall AW, Hewitson M, Hild S, Hirose E, Hoak D, Hodge KA, Holt K, Hosken DJ, Hough J, Howell EJ, Hoyland D, Huet D, Hughey B, Husa S, Huttner SH, Huynh-Dinh T, Ingram DR, Inta R, Isogai T, Ivanov A, Jaranowski P, Johnson WW, Jones DI, Jones G, Jones R, Ju L, Kalmus P, Kalogera V, Kandhasamy S, Kanner JB, Katsavounidis E, Kawabe K, Kawamura S, Kawazoe F, Kells W, Keppel DG, Khalaidovski A, Khalili FY, Khazanov EA, Kim H, King PJ, Kinzel DL, Kissel JS, Klimenko S, Kondrashov V, Kopparapu R, Koranda S, Kowalska I, Kozak D, Krause T, Kringel V, Krishnamurthy S, Krishnan B, Królak A, Kuehn G, Kullman J, Kumar R, Kwee P, Landry M, Lang M, Lantz B, Lastzka N, Lazzarini A, Leaci P, Leong J, Leonor I, Leroy N, Letendre N, Li J, Li TG, Liguori N, Lin H, Lindquist PE, Lockerbie NA, Lodhia D, Lorenzini M, Loriette V, Lormand M, Losurdo G, Lu P, Luan J, Lubinski M, Lucianetti A, Lück H, Lundgren AD, Machenschalk B, MacInnis M, Mageswaran M, Mailand K, Majorana E, Mak C, Maksimovic I, Man N, Mandel I, Mandic V, Mantovani M, Marchesoni F, Marion F, Márka S, Márka Z, Maros E, Marque J, Martelli F, Martin IW, Martin RM, Marx JN, Mason K, Masserot A, Matichard F, Matone L, Matzner RA, Mavalvala N, McCarthy R, McClelland DE, McGuire SC, McIntyre G, McIvor G, McKechan DJ, Meadors G, Mehmet M, Meier T, Melatos A, Melissinos AC, Mendell G, Menéndez DF, Mercer RA, Merill L, Meshkov S, Messenger C, Meyer MS, Miao H, Michel C, Milano L, Miller J, Minenkov Y, Mino Y, Mitra S, Mitrofanov VP, Mitselmakher G, Mittleman R, Moe B, Mohan M, Mohanty SD, Mohapatra SR, Moraru D, Moreau J, Moreno G, Morgado N, Morgia A, Morioka T, Mors K, Mosca S, Moscatelli V, Mossavi K, Mours B, Mow-Lowry CM, Mueller G, Mukherjee S, Mullavey A, Müller-Ebhardt H, Munch J, Murray PG, Nash T, Nawrodt R, Nelson J, Neri I, Newton G, Nishizawa A, Nocera F, Nolting D, Ochsner E, O'Dell J, Ogin GH, Oldenburg RG, O'Reilly B, O'Shaughnessy R, Osthelder C, Ottaway DJ, Ottens RS, Overmier H, Owen BJ, Page A, Pagliaroli G, Palladino L, Palomba C, Pan Y, Pankow C, Paoletti F, Papa MA, Pardi S, Pareja M, Parisi M, Pasqualetti A, Passaquieti R, Passuello D, Patel P, Pathak D, Pedraza M, Pekowsky L, Penn S, Peralta C, Perreca A, Persichetti G, Pichot M, Pickenpack M, Piergiovanni F, Pietka M, Pinard L, Pinto IM, Pitkin M, Pletsch HJ, Plissi MV, Poggiani R, Postiglione F, Prato M, Predoi V, Price LR, Prijatelj M, Principe M, Prix R, Prodi GA, Prokhorov L, Puncken O, Punturo M, Puppo P, Quetschke V, Raab FJ, Rabeling DS, Radke T, Radkins H, Raffai P, Rakhmanov M, Rankins B, Rapagnani P, Raymond V, Re V, Reed CM, Reed T, Regimbau T, Reid S, Reitze DH, Ricci F, Riesen R, Riles K, Roberts P, Robertson NA, Robinet F, Robinson C, Robinson EL, Rocchi A, Roddy S, Röver C, Rolland L, Rollins J, Romano JD, Romano R, Romie JH, Rosińska D, Rowan S, Rüdiger A, Ruggi P, Ryan K, Sakata S, Sakosky M, Salemi F, Sammut L, de la Jordana LS, Sandberg V, Sannibale V, Santamaría L, Santostasi G, Saraf S, Sassolas B, Sathyaprakash BS, Sato S, Satterthwaite M, Saulson PR, Savage R, Schilling R, Schnabel R, Schofield RM, Schulz B, Schutz BF, Schwinberg P, Scott J, Scott SM, Searle AC, Seifert F, Sellers D, Sengupta AS, Sentenac D, Sergeev A, Shaddock DA, Shapiro B, Shawhan P, Shoemaker DH, Sibley A, Siemens X, Sigg D, Singer A, Sintes AM, Skelton G, Slagmolen BJ, Slutsky J, Smith JR, Smith MR, Smith ND, Somiya K, Sorazu B, Speirits FC, Sperandio L, Stein AJ, Stein LC, Steinlechner S, Steplewski S, Stochino A, Stone R, Strain KA, Strigin S, Stroeer AS, Sturani R, Stuver AL, Summerscales TZ, Sung M, Susmithan S, Sutton PJ, Swinkels B, Szokoly GP, Talukder D, Tanner DB, Tarabrin SP, Taylor JR, Taylor R, Thomas P, Thorne KA, Thorne KS, Thrane E, Thüring A, Titsler C, Tokmakov KV, Toncelli A, Tonelli M, Torre O, Torres C, Torrie CI, Tournefier E, Travasso F, Traylor G, Trias M, Trummer J, Tseng K, Turner L, Ugolini D, Urbanek K, Vahlbruch H, Vaishnav B, Vajente G, Vallisneri M, van den Brand JF, Van Den Broeck C, van der Putten S, van der Sluys MV, van Veggel AA, Vass S, Vaulin R, Vavoulidis M, Vecchio A, Vedovato G, Veitch J, Veitch PJ, Veltkamp C, Verkindt D, Vetrano F, Viceré A, Villar AE, Vinet JY, Vocca H, Vorvick C, Vyachanin SP, Waldman SJ, Wallace L, Wanner A, Ward RL, Was M, Wei P, Weinert M, Weinstein AJ, Weiss R, Wen L, Wen S, Wessels P, West M, Westphal T, Wette K, Whelan JT, Whitcomb SE, White D, Whiting BF, Wilkinson C, Willems PA, Williams L, Willke B, Winkelmann L, Winkler W, Wipf CC, Wiseman AG, Woan G, Wooley R, Worden J, Yakushin I, Yamamoto H, Yamamoto K, Yeaton-Massey D, Yoshida S, Yu P, Yvert M, Zanolin M, Zhang L, Zhang Z, Zhao C, Zotov N, Zucker ME, and Zweizig J
- Abstract
The gravitational-wave (GW) sky may include nearby pointlike sources as well as stochastic backgrounds. We perform two directional searches for persistent GWs using data from the LIGO S5 science run: one optimized for pointlike sources and one for arbitrary extended sources. Finding no evidence to support the detection of GWs, we present 90% confidence level (C.L.) upper-limit maps of GW strain power with typical values between 2-20×10(-50) strain(2) Hz(-1) and 5-35×10(-49) strain(2) Hz(-1) sr(-1) for pointlike and extended sources, respectively. The latter result is the first of its kind. We also set 90% C.L. limits on the narrow-band root-mean-square GW strain from interesting targets including Sco X-1, SN 1987A and the Galactic center as low as ≈7×10(-25) in the most sensitive frequency range near 160 Hz.
- Published
- 2011
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