Author: "Sault, R. J." / Publication Year Range: Last 10 years - Searchworks@Jio Institute Digital Library Search Results

Your search keyword '"Sault, R. J."' showing total 39 results

Start Over Author "Sault, R. J." Publication Year Range Last 10 years

39 results on '"Sault, R. J."'

1. First ALMA Millimeter Wavelength Maps of Jupiter, with a Multi-Wavelength Study of Convection

Author: de Pater, Imke, Sault, R. J., Moeckel, Chris, Moullet, Arielle, Wong, Michael H., Goullaud, Charles, DeBoer, David, Butler, Bryan, Bjoraker, Gordon, Adamkovics, Mate, Cosentino, Richard, Donnelly, Padraig T., Fletcher, Leigh N., Kasaba, Yasumasa, Orton, Glenn, Rogers, John, Sinclair, James, and Villard, Eric
Subjects: Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: We obtained the first maps of Jupiter at 1-3 mm wavelength with the Atacama Large Millimeter/Submillimeter Array (ALMA) on 3-5 January 2017, just days after an energetic eruption at 16.5S jovigraphic latitude had been reported by the amateur community, and about 2-3 months after the detection of similarly energetic eruptions in the northern hemisphere, at 22.2-23.0N. Our observations, probing below the ammonia cloud deck, show that the erupting plumes in the SEB bring up ammonia gas from the deep atmosphere. While models of plume eruptions that are triggered at the water condensation level explain data taken at uv-visible and mid-infrared wavelengths, our ALMA observations provide a crucial, hitherto missing, link in the moist convection theory by showing that ammonia gas from the deep atmosphere is indeed brought up in these plumes. Contemporaneous HST data show that the plumes reach altitudes as high as the tropopause. We suggest that the plumes at 22.2-23.0N also rise up well above the ammonia cloud deck, and that descending air may dry the neighboring belts even more than in quiescent times, which would explain our observations in the north., Comment: 28 pages, 12 figures, 4 tables
Published: 2019
Full Text: View/download PDF

2. Jupiter's Ammonia Distribution Derived from VLA Maps at 3--37 GHz

Author: de Pater, I., Sault, R. J., Wong, M. H., Fletcher, L. N., DeBoer, D., and Butler, B.
Subjects: Astrophysics - Earth and Planetary Astrophysics
Abstract: We observed Jupiter four times over a full rotation (10 hrs) with the upgraded Karl G. Jansky Very Large Array (VLA) between December 2013 and December 2014. Preliminary results at 4-17 GHz were presented in de Pater et al. (2016); in the present paper we present the full data set at frequencies between 3 and 37 GHz. Major findings are: (i) the radio-hot belt at 8.5--11$^\circ$N latitude, near the interface between the North Equatorial Belt (NEB) and the Equatorial Zone (EZ) is prominent at all frequencies (3--37 GHz). Its location coincides with the southern latitudes of the NEB (7--17$^{\circ}$ N). (ii) Longitude-smeared maps reveal belts and zones at all frequencies at latitudes $\lesssim |20^\circ|$. The lowest brightness temperature is in the EZ near a latitude of 4$^\circ$N, and the NEB has the highest brightness temperature near 11$^\circ$N. The bright part of the NEB increases in latitudinal extent (spreads towards the north) with deceasing frequency, i.e., with depth into the atmosphere. In longitude-resolved maps, several belts, in particular in the southern hemisphere, are not continuous along the latitude line, but broken into small segments as if caused by an underlying wave. (iii) Model fits to longitude-smeared spectra are obtained at each latitude. These show a high NH$_3$ abundance (volume mixing ratio $\sim 4 \times 10^{-4}$) in the deep ($P>8-10$ bar) atmosphere, decreasing at higher altitudes due to cloud formation (e.g., in zones), or dynamics in combination with cloud condensation (belts). In the NEB ammonia gas is depleted down to at least the 20 bar level with an abundance of $1.75 \times 10^{-4}$. (iv) Using the entire VLA dataset, we confirm that the planet is extremely dynamic in the upper layers of the atmosphere, at $P<$2--3 bar, i.e., at the altitudes where clouds form. [Abridged], Comment: 35 pages, 17 figures, published in Icarus
Published: 2019
Full Text: View/download PDF

3. Potential for Solar System Science with the ngVLA

Author: de Pater, Imke, Butler, Bryan, Sault, R. J., Moullet, Arielle, Moeckel, Chris, Tollefson, Joshua, de Kleer, Katherine, Gurwell, Mark, and Milam, Stefanie
Subjects: Astrophysics - Earth and Planetary Astrophysics
Abstract: Radio wavelength observations of solar system bodies are a powerful method of probing many characteristics of those bodies. From surface and subsurface, to atmospheres (including deep atmospheres of the giant planets), to rings, to the magnetosphere of Jupiter, these observations provide unique information on current state, and sometimes history, of the bodies. The ngVLA will enable the highest sensitivity and resolution observations of this kind, with the potential to revolutionize our understanding of some of these bodies. In this article, we present a review of state-of-the-art radio wavelength observations of a variety of bodies in our solar system, varying in size from ring particles and small near-Earth asteroids to the giant planets. Throughout the review we mention improvements for each body (or class of bodies) to be expected with the ngVLA. A simulation of a Neptune-sized object is presented in Section 6. Section 7 provides a brief summary for each type of object, together with the type of measurements needed for all objects throughout the Solar System.
Published: 2018

4. Illuminating the past 8 billion years of cold gas towards two gravitationally lensed quasars

Author: Allison, J. R., Moss, V. A., Macquart, J. -P., Curran, S. J., Duchesne, S. W., Mahony, E. K., Sadler, E. M., Whiting, M. T., Bannister, K. W., Chippendale, A. P., Edwards, P. G., Harvey-Smith, L., Heywood, I., Indermuehle, B. T., Lenc, E., Marvil, J., McConnell, D., and Sault, R. J.
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: Using the Boolardy Engineering Test Array of the Australian Square Kilometre Array Pathfinder (ASKAP BETA), we have carried out the first $z = 0 - 1$ survey for HI and OH absorption towards the gravitationally lensed quasars PKSB1830$-$211 and MGJ0414$+$0534. Although we detected all previously reported intervening systems towards PKSB1830$-$211, in the case of MGJ0414+0534 three systems were not found, indicating that the original identifications may have been confused with radio frequency interference. Given the sensitivity of our data, we find that our detection yield is consistent with the expected frequency of intervening HI systems estimated from previous surveys for 21-cm emission in nearby galaxies and $z \sim 3$ damped Lyman $\alpha$ absorbers. We find spectral variability in the $z = 0.886$ face-on spiral galaxy towards PKSB1830$-$211, from observations undertaken with the Westerbork Synthesis Radio Telescope in 1997/1998 and ASKAP BETA in 2014/2015. The HI equivalent width varies by a few per cent over approximately yearly time-scales. This long-term spectral variability is correlated between the north-east and south-west images of the core, and with the total flux density of the source, implying that it is observationally coupled to intrinsic changes in the quasar. The absence of any detectable variability in the ratio of HI associated with the two core images is in stark contrast to the behaviour previously seen in the molecular lines. We therefore infer that coherent opaque HI structures in this galaxy are larger than the parsec-scale molecular clouds found at mm-wavelengths., Comment: 19 pages, 11 figures, published in MNRAS
Published: 2016
Full Text: View/download PDF

5. The Australian Square Kilometre Array Pathfinder: Performance of the Boolardy Engineering Test Array

Author: McConnell, D., Allison, J. R., Bannister, K., Bell, M. E., Bignall, H. E., Chippendale, A. P., Edwards, P. G., Harvey-Smith, L., Hegarty, S., Heywood, I., Hotan, A. W., Indermuehle, B. T., Lenc, E., Marvil, J., Popping, A., Raja, W., Reynolds, J. E., Sault, R. J., Serra, P., Voronkov, M. A., Whiting, M., Amy, S. W., Axtens, P., Ball, L., Bateman, T. J., Bock, D. C. -J., Bolton, R., Brodrick, D., Brothers, M., Brown, A. J., Bunton, J. D., Cheng, W., Cornwell, T., DeBoer, D., Feain, I., Gough, R., Gupta, N., Guzman, J. C., Hampson, G. A., Hay, S., Hayman, D. B., Hoyle, S., Humphreys, B., Jacka, C., Jackson, C. A., Jackson, S., Jeganathan, K., Joseph, J., Koribalski, B. S., Leach, M., Lensson, E. S., MacLeod, A., Mackay, S., Marquarding, M., McClure-Griffiths, N. M., Mirtschin, P., Mitchell, D., Neuhold, S., Ng, A., Norris, R., Pearce, S., Qiao, R. Y., Schinckel, A. E. T., Shields, M., Shimwell, T. W., Storey, M., Troup, E., Turner, B., Tuthill, J., Tzioumis, A., Wark, R. M., Westmeier, T., Wilson, C., and Wilson, T.
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: We describe the performance of the Boolardy Engineering Test Array (BETA), the prototype for the Australian Square Kilometre Array Pathfinder telescope ASKAP. BETA is the first aperture synthesis radio telescope to use phased array feed technology, giving it the ability to electronically form up to nine dual-polarization beams. We report the methods developed for forming and measuring the beams, and the adaptations that have been made to the traditional calibration and imaging procedures in order to allow BETA to function as a multi-beam aperture synthesis telescope. We describe the commissioning of the instrument and present details of BETA's performance: sensitivity, beam characteristics, polarimetric properties and image quality. We summarise the astronomical science that it has produced and draw lessons from operating BETA that will be relevant to the commissioning and operation of the final ASKAP telescope., Comment: Accepted for publication in PASA
Published: 2016
Full Text: View/download PDF

6. The radio spectral energy distribution of infrared-faint radio sources

Author: Herzog, A., Norris, R. P., Middelberg, E., Seymour, N., Spitler, L. R., Emonts, B. H. C., Franzen, T. M. O., Hunstead, R., Intema, H. T., Marvil, J., Parker, Q. A., Sirothia, S. K., Hurley-Walker, N., Bell, M., Bernardi, G., Bowman, J. D., Briggs, F., Cappallo, R. J., Callingham, J. R., Deshpande, A. A., Dwarakanath, K. S., For, B. -Q., Greenhill, L. J., Hancock, P., Hazelton, B. J., Hindson, L., Johnston-Hollitt, M., Kapinska, A. D., Kaplan, D. L., Lenc, E., Lonsdale, C. J., McKinley, B., McWhirter, S. R., Mitchell, D. A., Morales, M. F., Morgan, E., Morgan, J., Oberoi, D., Offringa, A., Ord, S. M., Prabu, T., Procopio, P., Shankar, N. Udaya, Srivani, K. S., Staveley-Smith, L., Subrahmanyan, R., Tingay, S. J., Wayth, R. B., Webster, R. L., Williams, A., Williams, C. L., Wu, C., Zheng, Q., Chippendale, A. P., Harvey-Smith, L., Heywood, I., Indermuehle, B., Popping, A., Sault, R. J., and Whiting, M. T.
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: Infrared-faint radio sources (IFRS) are a class of radio-loud (RL) active galactic nuclei (AGN) at high redshifts (z > 1.7) that are characterised by their relative infrared faintness, resulting in enormous radio-to-infrared flux density ratios of up to several thousand. We aim to test the hypothesis that IFRS are young AGN, particularly GHz peaked-spectrum (GPS) and compact steep-spectrum (CSS) sources that have a low frequency turnover. We use the rich radio data set available for the Australia Telescope Large Area Survey fields, covering the frequency range between 150 MHz and 34 GHz with up to 19 wavebands from different telescopes, and build radio spectral energy distributions (SEDs) for 34 IFRS. We then study the radio properties of this class of object with respect to turnover, spectral index, and behaviour towards higher frequencies. We also present the highest-frequency radio observations of an IFRS, observed with the Plateau de Bure Interferometer at 105 GHz, and model the multi-wavelength and radio-far-infrared SED of this source. We find IFRS usually follow single power laws down to observed frequencies of around 150 MHz. Mostly, the radio SEDs are steep, but we also find ultra-steep SEDs. In particular, IFRS show statistically significantly steeper radio SEDs than the broader RL AGN population. Our analysis reveals that the fractions of GPS and CSS sources in the population of IFRS are consistent with the fractions in the broader RL AGN population. We find that at least 18% of IFRS contain young AGN, although the fraction might be significantly higher as suggested by the steep SEDs and the compact morphology of IFRS. The detailed multi-wavelength SED modelling of one IFRS shows that it is different from ordinary AGN, although it is consistent with a composite starburst-AGN model with a star formation rate of 170 solar masses per year., Comment: 25 pages, 7 figures, 5 tables, accepted for publication in A&A
Published: 2016
Full Text: View/download PDF

7. Supplement: Localization and broadband follow-up of the gravitational-wave transient GW150914

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., Barthelmy, S., Bartlett, J., Bartos, I., Bassiri, R., Basti, A., Batch, J. C., Baune, C., Bavigadda, V., Bazzan, M., Behnke, B., Bejger, M., Bell, A. S., Bell, C. J., Berger, B. K., Bergman, J., 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., Bodiya, T. P., Boer, M., Bogaert, G., Bogan, C., Bohe, A., Bojtos, P., 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., Brooks, A. F., Brown, D. A., Brown, D. D., Brown, N. M., Buchanan, C. C., Buikema, A., Bulik, T., Bulten, H. J., Buonanno, A., Buskulic, D., Buy, C., Byer, R. L., Cadonati, L., Cagnoli, G., Cahillane, C., Bustillo, J. C., Callister, T., Calloni, E., Camp, J. B., Cannon, K. C., Cao, J., Capano, C. D., Capocasa, E., Carbognani, F., Caride, S., Diaz, J. C., Casentini, C., Caudill, S., Cavaglià, M., Cavalier, F., Cavalieri, R., Cella, G., Cepeda, C. B., Baiardi, L. C., Cerretani, G., Cesarini, E., Chakraborty, R., Chalermsongsak, T., Chamberlin, S. J., Chan, M., Chao, S., Charlton, P., Chassande-Mottin, E., 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 Jr., 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., Canton, T. Dal, Danilishin, S. L., D'Antonio, S., Danzmann, K., Darman, N. S., Dattilo, V., Dave, I., Daveloza, H. P., Davier, M., Davies, G. S., Daw, E. J., Day, R., DeBra, D., Debreczeni, G., Degallaix, J., De Laurentis, M., Deléglise, S., Del Pozzo, W., Denker, T., Dent, T., Dereli, H., Dergachev, V., DeRosa, R. T., De Rosa, R., DeSalvo, R., Dhurandhar, S., Díaz, M. C., Di Fiore, L., Di Giovanni, M., Di Lieto, A., Di Pace, S., Di Palma, I., Di Virgilio, A., Dojcinoski, G., Dolique, V., Donovan, F., Dooley, K. L., Doravari, S., Douglas, R., 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., 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., Ferrante, I., Ferreira, E. C., Ferrini, F., Fidecaro, F., Fiori, I., Fiorucci, D., Fisher, R. P., Flaminio, R., Fletcher, M., Fournier, J. -D., Franco, S., Frasca, S., Frasconi, F., Frei, Z., Freise, A., Frey, R., Frey, V., Fricke, T. T., Fritschel, P., Frolov, V. V., Fulda, P., Fyffe, M., Gabbard, H. A. G., Gair, J. R., Gammaitoni, L., Gaonkar, S. G., Garufi, F., Gatto, A., Gaur, G., Gehrels, N., Gemme, G., Gendre, B., Genin, E., Gennai, A., George, J., Gergely, L., Germain, V., Ghosh, A., 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. G., Gopakumar, A., Gordon, N. A., Gorodetsky, M. L., Gossan, S. E., Gosselin, M., Gouaty, R., 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., Haris, K., 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., Heptonstall, A. W., Heurs, M., Hild, S., Hoak, D., Hodge, K. A., Hofman, D., Hollitt, S. E., Holt, K., Holz, D. E., Hopkins, P., Hosken, D. J., 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., Idrisy, A., Indik, N., Ingram, D. R., Inta, R., Isa, H. N., Isac, J. -M., Isi, M., Islas, G., Isogai, T., Iyer, B. R., Izumi, K., Jacqmin, T., Jang, H., Jani, K., Jaranowski, P., Jawahar, S., Jiménez-Forteza, F., Johnson, W. W., Jones, D. I., Jones, R., Jonker, R. J. G., Ju, L., Kalaghatgi, C. V., Kalogera, V., Kandhasamy, S., Kang, G., Kanner, J. B., Karki, S., Kasprzack, M., Katsavounidis, E., Katzman, W., Kaufer, S., Kaur, T., Kawabe, K., Kawazoe, F., Kéfélian, F., Kehl, M. S., Keitel, D., Kelley, D. B., Kells, W., Kennedy, R., Key, J. S., Khalaidovski, A., Khalili, F. Y., Khan, I., Khan, S., Khan, Z., Khazanov, E. A., Kijbunchoo, N., Kim, C., Kim, J., Kim, K., Kim, N., Kim, Y. -M., King, E. J., King, P. J., Kinzel, D. L., Kissel, J. S., Kleybolte, L., Klimenko, S., Koehlenbeck, S. M., Kokeyama, K., Koley, S., Kondrashov, V., Kontos, A., Korobko, M., Korth, W. Z., Kowalska, I., Kozak, D. B., Kringel, V., Królak, A., Krueger, C., Kuehn, G., Kumar, P., Kuo, L., Kutynia, A., Lackey, B. D., Landry, M., Lange, J., Lantz, B., Lasky, P. D., 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., Levine, B. M., Li, T. G. F., Libson, A., Littenberg, T. B., Lockerbie, N. A., Logue, J., Lombardi, A. L., Lord, J. E., Lorenzini, M., Loriette, V., Lormand, M., Losurdo, G., Lough, J. D., Lück, H., Lundgren, A. P., Luo, J., Lynch, R., Ma, Y., MacDonald, T., Machenschalk, B., MacInnis, M., Macleod, D. M., Magaña-Sandoval, F., Magee, R. M., Mageswaran, 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., Martin, R. M., Martynov, D. V., Marx, J. N., Mason, K., Masserot, A., Massinger, T. J., Masso-Reid, M., Matichard, F., Matone, L., Mavalvala, N., Mazumder, N., Mazzolo, G., McCarthy, R., McClelland, D. E., McCormick, S., McGuire, S. C., McIntyre, G., McIver, J., McManus, D. J., McWilliams, S. T., Meacher, D., Meadors, G. D., Meidam, J., Melatos, A., Mendell, G., Mendoza-Gandara, D., Mercer, R. A., Merilh, E., Merzougui, M., Meshkov, S., Messenger, C., Messick, C., Meyers, P. M., Mezzani, F., Miao, H., Michel, C., Middleton, H., Mikhailov, E. E., Milano, L., 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, C. L., Mueller, G., Muir, A. W., Mukherjee, A., 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., Necula, V., Nedkova, K., Nelemans, G., 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, R. J., O'Reilly, B., O'Shaughnessy, R., Ottaway, D. J., Ottens, R. S., Overmier, H., Owen, B. J., Pai, A., Pai, S. A., Palamos, J. R., Palashov, O., Palliyaguru, N., 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., Phelps, M., Piccinni, O., Pichot, M., Piergiovanni, F., Pierro, V., Pillant, G., Pinard, L., Pinto, I. M., Pitkin, M., Poggiani, R., Popolizio, P., Post, A., Powell, J., Prasad, J., Predoi, V., Premachandra, S. S., Prestegard, T., Price, L. R., Prijatelj, M., Principe, M., Privitera, S., Prodi, G. A., Prokhorov, L., Puncken, O., Punturo, M., Puppo, P., Pürrer, M., Qi, H., Qin, J., Quetschke, V., Quintero, E. A., Quitzow-James, R., Raab, F. J., Rabeling, D. S., Radkins, H., Raffai, P., Raja, S., 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., 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., 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., 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., Sentenac, D., Sequino, V., Sergeev, A., Serna, G., Setyawati, Y., Sevigny, A., Shaddock, D. A., Shah, S., Shahriar, M. S., Shaltev, M., Shao, Z., Shapiro, B., Shawhan, P., Sheperd, A., Shoemaker, D. H., Shoemaker, D. M., Siellez, K., Siemens, X., Sigg, D., Silva, A. D., Simakov, D., Singer, A., 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., 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., Thorne, K. S., Thrane, E., Tiwari, S., Tiwari, V., Tokmakov, K. V., Tomlinson, C., Tonelli, M., 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., van Bakel, N., van Beuzekom, M., Brand, J. F. J. van den, Broeck, C. Van Den, 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., 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., Welborn, T., Wen, L., Weßels, P., Westphal, T., Wette, K., Whelan, J. T., White, D. J., 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., Worden, J., Wright, J. L., Wu, G., Yablon, J., Yam, W., Yamamoto, H., Yancey, C. C., Yap, M. J., Yu, H., Yvert, M., Zadrożny, A., Zangrando, L., Zanolin, M., Zendri, J. -P., Zevin, M., Zhang, F., Zhang, L., Zhang, M., Zhang, Y., Zhao, C., Zhou, M., Zhou, Z., Zhu, X. J., Zucker, M. E., Zuraw, S. E., Zweizig, J., Allison, J., Bannister, K., Bell, M. E., Chatterjee, S., Chippendale, A. P., Edwards, P. G., Harvey-Smith, L., Heywood, Ian, Hotan, A., Indermuehle, B., Marvil, J., McConnell, D., Murphy, T., Popping, A., Reynolds, J., Sault, R. J., Voronkov, M. A., Whiting, M. T., Castro-Tirado, A. J., Cunniffe, R., Jelínek, M., Tello, J. C., Oates, S. R., Hu, Y. -D., Kubánek, P., Guziy, S., Castellón, A., García-Cerezo, A., Muñoz, V. F., del Pulgar, C. Pérez, Castillo-Carrión, S., Cerón, J. M. Castro, Hudec, R., Caballero-García, M. D., Páta, P., Vitek, S., Adame, J. A., Konig, S., Rendón, F., Sanguino, T. de J. Mateo, Fernández-Muñoz, R., Yock, P. C., Rattenbury, N., Allen, W. H., Querel, R., Jeong, S., Park, I. H., Bai, J., Cui, Ch., Fan, Y., Wang, Ch., Hiriart, D., Lee, W. H., Claret, A., Sánchez-Ramírez, R., Pandey, S. B., Mediavilla, T., Sabau-Graziati, L., Abbott, T. M. C., Abdalla, F. B., Allam, S., Annis, J., Armstrong, R., Benoit-Lévy, A., Berger, E., Bernstein, R. A., Bertin, E., Brout, D., Buckley-Geer, E., Burke, D. L., Capozzi, D., Carretero, J., Castander, F. J., Chornock, R., Cowperthwaite, P. S., Crocce, M., Cunha, C. E., D'Andrea, C. B., da Costa, L. N., Desai, S., Diehl, H. T., Dietrich, J. P., Doctor, Z., Drlica-Wagner, A., Drout, M. R., Eifler, T. F., Estrada, J., Evrard, A. E., Fernandez, E., Finley, D. A., Flaugher, B., Foley, R. J., Fong, W. -F., Fosalba, P., Fox, D. B., Frieman, J., Fryer, C. L., Gaztanaga, E., Gerdes, D. W., Goldstein, D. A., Gruen, D., Gruendl, R. A., Gutierrez, G., Herner, K., Honscheid, K., James, D. J., Johnson, M. D., Johnson, M. W. G., Karliner, I., Kasen, D., Kent, S., Kessler, R., Kim, A. G., Kind, M. C., Kuehn, K., Kuropatkin, N., Lahav, O., Li, T. S., Lima, M., Lin, H., Maia, M. A. G., Margutti, R., Marriner, J., Martini, P., Matheson, T., Melchior, P., Metzger, B. D., Miller, C. J., Miquel, R., Neilsen, E., Nichol, R. C., Nord, B., Nugent, P., Ogando, R., Petravick, D., Plazas, A. A., Quataert, E., Roe, N., Romer, A. K., Roodman, A., Rosell, A. C., Rykoff, E. S., Sako, M., Sanchez, E., Scarpine, V., Schindler, R., Schubnell, M., Scolnic, D., Sevilla-Noarbe, I., Sheldon, E., Smith, N., Smith, R. C., Soares-Santos, M., Sobreira, F., Stebbins, A., Suchyta, E., Swanson, M. E. C., Tarle, G., Thaler, J., Thomas, D., Thomas, R. C., Tucker, D. L., Vikram, V., Walker, A. R., Wechsler, R. H., Wester, W., Yanny, B., Zuntz, J., Connaughton, V., Burns, E., Goldstein, A., Briggs, M. S., Zhang, B. -B., Hui, C. M., Jenke, P., Wilson-Hodge, C. A., Bhat, P. N., Bissaldi, E., Cleveland, W., Fitzpatrick, G., Giles, M. M., Gibby, M. H., Greiner, J., von Kienlin, A., Kippen, R. M., McBreen, S., Mailyan, B., Meegan, C. A., Paciesas, W. S., Preece, R. D., Roberts, O., Sparke, L., Stanbro, M., Toelge, K., Veres, P., Yu, H. -F., Blackburn, L., Ackermann, M., Ajello, M., Albert, A., Anderson, B., Atwood, W. B., Axelsson, M., Baldini, L., Barbiellini, G., Bastieri, D., Bellazzini, R., Blandford, R. D., Bloom, E. D., Bonino, R., Bottacini, E., Brandt, T. J., Bruel, P., Buson, S., Caliandro, G. A., Cameron, R. A., Caragiulo, M., Caraveo, P. A., Cavazzuti, E., Charles, E., Chekhtman, A., Chiang, J., Chiaro, G., Ciprini, S., Cohen-Tanugi, J., Cominsky, L. R., Costanza, F., Cuoco, A., D'Ammando, F., de Palma, F., Desiante, R., Digel, S. W., Di Lalla, N., Di Mauro, M., Di Venere, L., Domínguez, A., Drell, P. S., Dubois, R., Favuzzi, C., Ferrara, E. C., Franckowiak, A., Fukazawa, Y., Funk, S., Fusco, P., Gargano, F., Gasparrini, D., Giglietto, N., Giommi, P., Giordano, F., Giroletti, M., Glanzman, T., Godfrey, G., Gomez-Vargas, G. A., Green, D., Grenier, I. A., Grove, J. E., Guiriec, S., Hadasch, D., Harding, A. K., Hays, E., Hewitt, J. W., Hill, A. B., Horan, D., Jogler, T., Jóhannesson, G., Johnson, A. S., Kensei, S., Kocevski, D., Kuss, M., La Mura, G., Larsson, S., Latronico, L., Li, J., Li, L., Longo, F., Loparco, F., Lovellette, M. N., Lubrano, P., Magill, J., Maldera, S., Manfreda, A., Marelli, M., Mayer, M., Mazziotta, M. N., McEnery, J. E., Meyer, M., Michelson, P. F., Mirabal, N., Mizuno, T., Moiseev, A. A., Monzani, M. E., Moretti, E., Morselli, A., Moskalenko, I. V., Negro, M., Nuss, E., Ohsugi, T., Omodei, N., Orienti, M., Orlando, E., Ormes, J. F., Paneque, D., Perkins, J. S., Pesce-Rollins, M., Piron, F., Pivato, G., Porter, T. A., Racusin, J. L., Rainò, S., Rando, R., Razzaque, S., Reimer, A., Reimer, O., Salvetti, D., Parkinson, P. M. Saz, Sgrò, C., Simone, D., Siskind, E. J., Spada, F., Spandre, G., Spinelli, P., Suson, D. J., Tajima, H., Thayer, J. B., Thompson, D. J., Tibaldo, L., Torres, D. F., Troja, E., Uchiyama, Y., Venters, T. M., Vianello, G., Wood, K. S., Wood, M., Zhu, S., Zimmer, S., Brocato, E., Cappellaro, E., Covino, S., Grado, A., Nicastro, L., Palazzi, E., Pian, E., Amati, L., Antonelli, L. A., Capaccioli, M., D'Avanzo, P., D'Elia, V., Getman, F., Giuffrida, G., Iannicola, G., Limatola, L., Lisi, M., Marinoni, S., Marrese, P., Melandri, A., Piranomonte, S., Possenti, A., Pulone, L., Rossi, A., Stamerra, A., Stella, L., Testa, V., Tomasella, L., Yang, S., Bazzano, A., Bozzo, E., Brandt, S., Courvoisier, T. J. -L., Ferrigno, C., Hanlon, L., Kuulkers, E., Laurent, P., Mereghetti, S., Roques, J. P., Savchenko, V., Ubertini, P., Kasliwal, M. M., Singer, L. P., Cao, Y., Duggan, G., Kulkarni, S. R., Bhalerao, V., Miller, A. A., Barlow, T., Bellm, E., Manulis, I., Rana, J., Laher, R., Masci, F., Surace, J., Rebbapragada, U., Van Sistine, A., Sesar, B., Perley, D., Ferreti, R., Prince, T., Kendrick, R., Horesh, A., Hurley, K., Golenetskii, S. V., Aptekar, R. L., Frederiks, D. D., Svinkin, D. S., Rau, A., Zhang, X., Smith, D. M., Cline, T., Krimm, H., Abe, F., Doi, M., Fujisawa, K., Kawabata, K. S., Morokuma, T., Motohara, K., Tanaka, M., Ohta, K., Yanagisawa, K., Yoshida, M., Baltay, C., Rabinowitz, D., Ellman, N., Rostami, S., Bersier, D. F., Bode, M. F., Collins, C. A., Copperwheat, C. M., Darnley, M. J., Galloway, D. K., Gomboc, A., Kobayashi, S., Mazzali, P., Mundell, C. G., Piascik, A. S., Pollacco, Don, Steele, I. A., Ulaczyk, K., Broderick, J. W., Fender, R. P., Jonker, P. G., Rowlinson, A., Stappers, B. W., Wijers, R. A. M. J., Lipunov, V., Gorbovskoy, E., Tyurina, N., Kornilov, V., Balanutsa, P., Kuznetsov, A., Buckley, D., Rebolo, R., Serra-Ricart, M., Israelian, G., Budnev, N. M., Gress, O., Ivanov, K., Poleshuk, V., Tlatov, A., Yurkov, V., Kawai, N., Serino, M., Negoro, H., Nakahira, S., Mihara, T., Tomida, H., Ueno, S., Tsunemi, H., Matsuoka, M., Croft, S., Feng, L., Franzen, T. M. O., Gaensler, B. M., Johnston-Hollitt, M., Kaplan, D. L., Morales, M. F., Tingay, S. J., Wayth, R. B., Williams, A., Smartt, S. J., Chambers, K. C., Smith, K. W., Huber, M. E., Young, D. R., Wright, D. E., Schultz, A., Denneau, L., Flewelling, H., Magnier, E. A., Primak, N., Rest, A., Sherstyuk, A., Stalder, B., Stubbs, C. W., Tonry, J., Waters, C., Willman, M., E., F. Olivares, Campbell, H., Kotak, R., Sollerman, J., Smith, M., Dennefeld, M., Anderson, J. P., Botticella, M. T., Chen, T. -W., Valle, M. D., Elias-Rosa, N., Fraser, M., Inserra, C., Kankare, E., Kupfer, T., Harmanen, J., Galbany, L., Guillou, L. Le, Lyman, J. D., Maguire, K., Mitra, A., Nicholl, M., Razza, A., Terreran, G., Valenti, S., Gal-Yam, A., Ćwiek, A., Ćwiok, M., Mankiewicz, L., Opiela, R., Zaremba, M., Żarnecki, A. F., Onken, C. A., Scalzo, R. A., Schmidt, B. P., Wolf, C., Yuan, F., Evans, P. A., Kennea, J. A., Burrows, D. N., Campana, S., Cenko, S. B., Marshall, F. E., Nousek, J., O'Brien, P., Osborne, J. P., Palmer, D., Perri, M., Siegel, M., Tagliaferri, G., Klotz, A., Turpin, D., Laugier, R., Beroiz, M., Peñuela, T., Macri, L. M., Oelkers, R. J., Lambas, D. G., Vrech, R., Cabral, J., Colazo, C., Dominguez, M., Sanchez, B., Gurovich, S., Lares, M., Marshall, J. L., DePoy, D. L., Padilla, N., Pereyra, N. A., Benacquista, M., Tanvir, N. R., Wiersema, K., Levan, A. J., Steeghs, D., Hjorth, J., Fynbo, J. P. U., Malesani, D., Milvang-Jensen, B., Watson, D., Irwin, M., Fernandez, C. G., McMahon, R. G., Banerji, M., Gonzalez-Solares, E., Schulze, S., Postigo, A. de U., Thoene, C. C., Cano, Z., and Rosswog, S.
Subjects: Astrophysics - High Energy Astrophysical Phenomena, General Relativity and Quantum Cosmology
Abstract: This Supplement provides supporting material for arXiv:1602.08492 . We briefly summarize past electromagnetic (EM) follow-up efforts as well as the organization and policy of the current EM follow-up program. We compare the four probability sky maps produced for the gravitational-wave transient GW150914, and provide additional details of the EM follow-up observations that were performed in the different bands., Comment: For the main Letter, see arXiv:1602.08492
Published: 2016
Full Text: View/download PDF

8. High-velocity OH megamasers in IRAS 20100-4156: Evidence for a Supermassive Black Hole

Author: Harvey-Smith, L., Allison, J. R., Green, J. A., Bannister, K. W., Chippendale, A., Edwards, P. G., Heywood, I., Hotan, A. W., Lenc, E., Marvil, J., McConnell, D., Phillips, C. P., Sault, R. J., Serra, P., Stevens, J., Voronkov, M., and Whiting, M.
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: We report the discovery of new, high-velocity narrow-line components of the OH megamaser in IRAS 20100-4156. Results from the Australian Square Kilometre Array Pathfinder (ASKAP)'s Boolardy Engineering Test Array (BETA) and the Australia Telescope Compact Array (ATCA) provide two independent measurements of the OH megamaser spectrum. We found evidence for OH megamaser clumps at $-$409 and $-$562 km/s (blue-shifted) from the systemic velocity of the galaxy, in addition to the lines previously known. The presence of such high velocities in the molecular emission from IRAS 20100$-$4156 could be explained by a ~50 pc molecular ring enclosing an approximately 3.8 billion solar mass black hole. We also discuss two alternatives, i.e. that the narrow-line masers are dynamically coupled to the wind driven by the active galactic nucleus or they are associated with two separate galactic nuclei. The comparison between the BETA and ATCA spectra provides another scientific verification of ASKAP's BETA. Our data, combined with previous measurements of the source enabled us to study the variability of the source over a twenty-six year period. The flux density of the brightest OH maser components has reduced by more than a factor of two between 1988 and 2015, whereas a secondary narrow-line component has more than doubled in the same time. Plans for high-resolution VLBI follow-up of this source are discussed, as are prospects for discovering new OH megamasers during the ASKAP early science program., Comment: Accepted to MNRAS. Seven pages, three figures
Published: 2016
Full Text: View/download PDF

9. Localization and broadband follow-up of the gravitational-wave transient GW150914

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., Barthelmy, S., Bartlett, J., Bartos, I., Bassiri, R., Basti, A., Batch, J. C., Baune, C., Bavigadda, V., Bazzan, M., Behnke, B., Bejger, M., Bell, A. S., Bell, C. J., Berger, B. K., Bergman, J., 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., Bodiya, T. P., Boer, M., Bogaert, G., Bogan, C., Bohe, A., Bojtos, P., 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., Brooks, A. F., Brown, D. A., Brown, D. D., Brown, N. M., Buchanan, C. C., Buikema, A., Bulik, T., Bulten, H. J., Buonanno, A., Buskulic, D., Buy, C., Byer, R. L., Cadonati, L., Cagnoli, G., Cahillane, C., Bustillo, J. C., Callister, T., Calloni, E., Camp, J. B., Cannon, K. C., Cao, J., Capano, C. D., Capocasa, E., Carbognani, F., Caride, S., Diaz, J. C., Casentini, C., Caudill, S., Cavaglià, M., Cavalier, F., Cavalieri, R., Cella, G., Cepeda, C. B., Baiardi, L. C., Cerretani, G., Cesarini, E., Chakraborty, R., Chalermsongsak, T., Chamberlin, S. J., Chan, M., Chao, S., Charlton, P., Chassande-Mottin, E., 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 Jr., 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., Canton, T. Dal, Danilishin, S. L., D'Antonio, S., Danzmann, K., Darman, N. S., Dattilo, V., Dave, I., Daveloza, H. P., Davier, M., Davies, G. S., Daw, E. J., Day, R., DeBra, D., Debreczeni, G., Degallaix, J., De Laurentis, M., Deléglise, S., Del Pozzo, W., Denker, T., Dent, T., Dereli, H., Dergachev, V., DeRosa, R. T., De Rosa, R., DeSalvo, R., Dhurandhar, S., Díaz, M. C., Di Fiore, L., Di Giovanni, M., Di Lieto, A., Di Pace, S., Di Palma, I., Di Virgilio, A., Dojcinoski, G., Dolique, V., Donovan, F., Dooley, K. L., Doravari, S., Douglas, R., 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., 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., Ferrante, I., Ferreira, E. C., Ferrini, F., Fidecaro, F., Fiori, I., Fiorucci, D., Fisher, R. P., Flaminio, R., Fletcher, M., Fournier, J. -D., Franco, S., Frasca, S., Frasconi, F., Frei, Z., Freise, A., Frey, R., Frey, V., Fricke, T. T., Fritschel, P., Frolov, V. V., Fulda, P., Fyffe, M., Gabbard, H. A. G., Gair, J. R., Gammaitoni, L., Gaonkar, S. G., Garufi, F., Gatto, A., Gaur, G., Gehrels, N., Gemme, G., Gendre, B., Genin, E., Gennai, A., George, J., Gergely, L., Germain, V., Ghosh, A., 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. G., Gopakumar, A., Gordon, N. A., Gorodetsky, M. L., Gossan, S. E., Gosselin, M., Gouaty, R., 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., Haris, K., 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., Heptonstall, A. W., Heurs, M., Hild, S., Hoak, D., Hodge, K. A., Hofman, D., Hollitt, S. E., Holt, K., Holz, D. E., Hopkins, P., Hosken, D. J., 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., Idrisy, A., Indik, N., Ingram, D. R., Inta, R., Isa, H. N., Isac, J. -M., Isi, M., Islas, G., Isogai, T., Iyer, B. R., Izumi, K., Jacqmin, T., Jang, H., Jani, K., Jaranowski, P., Jawahar, S., Jiménez-Forteza, F., Johnson, W. W., Jones, D. I., Jones, R., Jonker, R. J. G., Ju, L., Kalaghatgi, C. V., Kalogera, V., Kandhasamy, S., Kang, G., Kanner, J. B., Karki, S., Kasprzack, M., Katsavounidis, E., Katzman, W., Kaufer, S., Kaur, T., Kawabe, K., Kawazoe, F., Kéfélian, F., Kehl, M. S., Keitel, D., Kelley, D. B., Kells, W., Kennedy, R., Key, J. S., Khalaidovski, A., Khalili, F. Y., Khan, I., Khan, S., Khan, Z., Khazanov, E. A., Kijbunchoo, N., Kim, C., Kim, J., Kim, K., Kim, N., Kim, Y. -M., King, E. J., King, P. J., Kinzel, D. L., Kissel, J. S., Kleybolte, L., Klimenko, S., Koehlenbeck, S. M., Kokeyama, K., Koley, S., Kondrashov, V., Kontos, A., Korobko, M., Korth, W. Z., Kowalska, I., Kozak, D. B., Kringel, V., Królak, A., Krueger, C., Kuehn, G., Kumar, P., Kuo, L., Kutynia, A., Lackey, B. D., Landry, M., Lange, J., Lantz, B., Lasky, P. D., 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., Levine, B. M., Li, T. G. F., Libson, A., Littenberg, T. B., Lockerbie, N. A., Logue, J., Lombardi, A. L., Lord, J. E., Lorenzini, M., Loriette, V., Lormand, M., Losurdo, G., Lough, J. D., Lück, H., Lundgren, A. P., Luo, J., Lynch, R., Ma, Y., MacDonald, T., Machenschalk, B., MacInnis, M., Macleod, D. M., Magaña-Sandoval, F., Magee, R. M., Mageswaran, 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., Martin, R. M., Martynov, D. V., Marx, J. N., Mason, K., Masserot, A., Massinger, T. J., Masso-Reid, M., Matichard, F., Matone, L., Mavalvala, N., Mazumder, N., Mazzolo, G., McCarthy, R., McClelland, D. E., McCormick, S., McGuire, S. C., McIntyre, G., McIver, J., McManus, D. J., McWilliams, S. T., Meacher, D., Meadors, G. D., Meidam, J., Melatos, A., Mendell, G., Mendoza-Gandara, D., Mercer, R. A., Merilh, E., Merzougui, M., Meshkov, S., Messenger, C., Messick, C., Meyers, P. M., Mezzani, F., Miao, H., Michel, C., Middleton, H., Mikhailov, E. E., Milano, L., 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, C. L., Mueller, G., Muir, A. W., Mukherjee, A., 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., Necula, V., Nedkova, K., Nelemans, G., 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, R. J., O'Reilly, B., O'Shaughnessy, R., Ottaway, D. J., Ottens, R. S., Overmier, H., Owen, B. J., Pai, A., Pai, S. A., Palamos, J. R., Palashov, O., Palliyaguru, N., 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., Phelps, M., Piccinni, O., Pichot, M., Piergiovanni, F., Pierro, V., Pillant, G., Pinard, L., Pinto, I. M., Pitkin, M., Poggiani, R., Popolizio, P., Post, A., Powell, J., Prasad, J., Predoi, V., Premachandra, S. S., Prestegard, T., Price, L. R., Prijatelj, M., Principe, M., Privitera, S., Prodi, G. A., Prokhorov, L., Puncken, O., Punturo, M., Puppo, P., Pürrer, M., Qi, H., Qin, J., Quetschke, V., Quintero, E. A., Quitzow-James, R., Raab, F. J., Rabeling, D. S., Radkins, H., Raffai, P., Raja, S., 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., 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., 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., 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., Sentenac, D., Sequino, V., Sergeev, A., Serna, G., Setyawati, Y., Sevigny, A., Shaddock, D. A., Shah, S., Shahriar, M. S., Shaltev, M., Shao, Z., Shapiro, B., Shawhan, P., Sheperd, A., Shoemaker, D. H., Shoemaker, D. M., Siellez, K., Siemens, X., Sigg, D., Silva, A. D., Simakov, D., Singer, A., 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., 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., Thorne, K. S., Thrane, E., Tiwari, S., Tiwari, V., Tokmakov, K. V., Tomlinson, C., Tonelli, M., 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., van Bakel, N., van Beuzekom, M., Brand, J. F. J. van den, Broeck, C. Van Den, 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., 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., Welborn, T., Wen, L., Weßels, P., Westphal, T., Wette, K., Whelan, J. T., White, D. J., 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., Worden, J., Wright, J. L., Wu, G., Yablon, J., Yam, W., Yamamoto, H., Yancey, C. C., Yap, M. J., Yu, H., Yvert, M., Zadrożny, A., Zangrando, L., Zanolin, M., Zendri, J. -P., Zevin, M., Zhang, F., Zhang, L., Zhang, M., Zhang, Y., Zhao, C., Zhou, M., Zhou, Z., Zhu, X. J., Zucker, M. E., Zuraw, S. E., Zweizig, J., Allison, J., Bannister, K., Bell, M. E., Chatterjee, S., Chippendale, A. P., Edwards, P. G., Harvey-Smith, L., Heywood, Ian, Hotan, A., Indermuehle, B., Marvil, J., McConnell, D., Murphy, T., Popping, A., Reynolds, J., Sault, R. J., Voronkov, M. A., Whiting, M. T., Castro-Tirado, A. J., Cunniffe, R., Jelínek, M., Tello, J. C., Oates, S. R., Hu, Y. -D., Kubánek, P., Guziy, S., Castellón, A., García-Cerezo, A., Muñoz, V. F., del Pulgar, C. Pérez, Castillo-Carrión, S., Cerón, J. M. Castro, Hudec, R., Caballero-García, M. D., Páta, P., Vitek, S., Adame, J. A., Konig, S., Rendón, F., Sanguino, T. de J. Mateo, Fernández-Muñoz, R., Yock, P. C., Rattenbury, N., Allen, W. H., Querel, R., Jeong, S., Park, I. H., Bai, J., Cui, Ch., Fan, Y., Wang, Ch., Hiriart, D., Lee, W. H., Claret, A., Sánchez-Ramírez, R., Pandey, S. B., Mediavilla, T., Sabau-Graziati, L., Abbott, T. M. C., Abdalla, F. B., Allam, S., Annis, J., Armstrong, R., Benoit-Lévy, A., Berger, E., Bernstein, R. A., Bertin, E., Brout, D., Buckley-Geer, E., Burke, D. L., Capozzi, D., Carretero, J., Castander, F. J., Chornock, R., Cowperthwaite, P. S., Crocce, M., Cunha, C. E., D'Andrea, C. B., da Costa, L. N., Desai, S., Diehl, H. T., Dietrich, J. P., Doctor, Z., Drlica-Wagner, A., Drout, M. R., Eifler, T. F., Estrada, J., Evrard, A. E., Fernandez, E., Finley, D. A., Flaugher, B., Foley, R. J., Fong, W. -F., Fosalba, P., Fox, D. B., Frieman, J., Fryer, C. L., Gaztanaga, E., Gerdes, D. W., Goldstein, D. A., Gruen, D., Gruendl, R. A., Gutierrez, G., Herner, K., Honscheid, K., James, D. J., Johnson, M. D., Johnson, M. W. G., Karliner, I., Kasen, D., Kent, S., Kessler, R., Kim, A. G., Kind, M. C., Kuehn, K., Kuropatkin, N., Lahav, O., Li, T. S., Lima, M., Lin, H., Maia, M. A. G., Margutti, R., Marriner, J., Martini, P., Matheson, T., Melchior, P., Metzger, B. D., Miller, C. J., Miquel, R., Neilsen, E., Nichol, R. C., Nord, B., Nugent, P., Ogando, R., Petravick, D., Plazas, A. A., Quataert, E., Roe, N., Romer, A. K., Roodman, A., Rosell, A. C., Rykoff, E. S., Sako, M., Sanchez, E., Scarpine, V., Schindler, R., Schubnell, M., Scolnic, D., Sevilla-Noarbe, I., Sheldon, E., Smith, N., Smith, R. C., Soares-Santos, M., Sobreira, F., Stebbins, A., Suchyta, E., Swanson, M. E. C., Tarle, G., Thaler, J., Thomas, D., Thomas, R. C., Tucker, D. L., Vikram, V., Walker, A. R., Wechsler, R. H., Wester, W., Yanny, B., Zuntz, J., Connaughton, V., Burns, E., Goldstein, A., Briggs, M. S., Zhang, B. -B., Hui, C. M., Jenke, P., Wilson-Hodge, C. A., Bhat, P. N., Bissaldi, E., Cleveland, W., Fitzpatrick, G., Giles, M. M., Gibby, M. H., Greiner, J., von Kienlin, A., Kippen, R. M., McBreen, S., Mailyan, B., Meegan, C. A., Paciesas, W. S., Preece, R. D., Roberts, O., Sparke, L., Stanbro, M., Toelge, K., Veres, P., Yu, H. -F., Blackburn, L., Ackermann, M., Ajello, M., Albert, A., Anderson, B., Atwood, W. B., Axelsson, M., Baldini, L., Barbiellini, G., Bastieri, D., Bellazzini, R., Blandford, R. D., Bloom, E. D., Bonino, R., Bottacini, E., Brandt, T. J., Bruel, P., Buson, S., Caliandro, G. A., Cameron, R. A., Caragiulo, M., Caraveo, P. A., Cavazzuti, E., Charles, E., Chekhtman, A., Chiang, J., Chiaro, G., Ciprini, S., Cohen-Tanugi, J., Cominsky, L. R., Costanza, F., Cuoco, A., D'Ammando, F., de Palma, F., Desiante, R., Digel, S. W., Di Lalla, N., Di Mauro, M., Di Venere, L., Domínguez, A., Drell, P. S., Dubois, R., Favuzzi, C., Ferrara, E. C., Franckowiak, A., Fukazawa, Y., Funk, S., Fusco, P., Gargano, F., Gasparrini, D., Giglietto, N., Giommi, P., Giordano, F., Giroletti, M., Glanzman, T., Godfrey, G., Gomez-Vargas, G. A., Green, D., Grenier, I. A., Grove, J. E., Guiriec, S., Hadasch, D., Harding, A. K., Hays, E., Hewitt, J. W., Hill, A. B., Horan, D., Jogler, T., Jóhannesson, G., Johnson, A. S., Kensei, S., Kocevski, D., Kuss, M., La Mura, G., Larsson, S., Latronico, L., Li, J., Li, L., Longo, F., Loparco, F., Lovellette, M. N., Lubrano, P., Magill, J., Maldera, S., Manfreda, A., Marelli, M., Mayer, M., Mazziotta, M. N., McEnery, J. E., Meyer, M., Michelson, P. F., Mirabal, N., Mizuno, T., Moiseev, A. A., Monzani, M. E., Moretti, E., Morselli, A., Moskalenko, I. V., Negro, M., Nuss, E., Ohsugi, T., Omodei, N., Orienti, M., Orlando, E., Ormes, J. F., Paneque, D., Perkins, J. S., Pesce-Rollins, M., Piron, F., Pivato, G., Porter, T. A., Racusin, J. L., Rainò, S., Rando, R., Razzaque, S., Reimer, A., Reimer, O., Salvetti, D., Parkinson, P. M. Saz, Sgrò, C., Simone, D., Siskind, E. J., Spada, F., Spandre, G., Spinelli, P., Suson, D. J., Tajima, H., Thayer, J. B., Thompson, D. J., Tibaldo, L., Torres, D. F., Troja, E., Uchiyama, Y., Venters, T. M., Vianello, G., Wood, K. S., Wood, M., Zhu, S., Zimmer, S., Brocato, E., Cappellaro, E., Covino, S., Grado, A., Nicastro, L., Palazzi, E., Pian, E., Amati, L., Antonelli, L. A., Capaccioli, M., D'Avanzo, P., D'Elia, V., Getman, F., Giuffrida, G., Iannicola, G., Limatola, L., Lisi, M., Marinoni, S., Marrese, P., Melandri, A., Piranomonte, S., Possenti, A., Pulone, L., Rossi, A., Stamerra, A., Stella, L., Testa, V., Tomasella, L., Yang, S., Bazzano, A., Bozzo, E., Brandt, S., Courvoisier, T. J. -L., Ferrigno, C., Hanlon, L., Kuulkers, E., Laurent, P., Mereghetti, S., Roques, J. P., Savchenko, V., Ubertini, P., Kasliwal, M. M., Singer, L. P., Cao, Y., Duggan, G., Kulkarni, S. R., Bhalerao, V., Miller, A. A., Barlow, T., Bellm, E., Manulis, I., Rana, J., Laher, R., Masci, F., Surace, J., Rebbapragada, U., Van Sistine, A., Sesar, B., Perley, D., Ferreti, R., Prince, T., Kendrick, R., Horesh, A., Hurley, K., Golenetskii, S. V., Aptekar, R. L., Frederiks, D. D., Svinkin, D. S., Rau, A., Zhang, X., Smith, D. M., Cline, T., Krimm, H., Abe, F., Doi, M., Fujisawa, K., Kawabata, K. S., Morokuma, T., Motohara, K., Tanaka, M., Ohta, K., Yanagisawa, K., Yoshida, M., Baltay, C., Rabinowitz, D., Ellman, N., Rostami, S., Bersier, D. F., Bode, M. F., Collins, C. A., Copperwheat, C. M., Darnley, M. J., Galloway, D. K., Gomboc, A., Kobayashi, S., Mazzali, P., Mundell, C. G., Piascik, A. S., Pollacco, Don, Steele, I. A., Ulaczyk, K., Broderick, J. W., Fender, R. P., Jonker, P. G., Rowlinson, A., Stappers, B. W., Wijers, R. A. M. J., Lipunov, V., Gorbovskoy, E., Tyurina, N., Kornilov, V., Balanutsa, P., Kuznetsov, A., Buckley, D., Rebolo, R., Serra-Ricart, M., Israelian, G., Budnev, N. M., Gress, O., Ivanov, K., Poleshuk, V., Tlatov, A., Yurkov, V., Kawai, N., Serino, M., Negoro, H., Nakahira, S., Mihara, T., Tomida, H., Ueno, S., Tsunemi, H., Matsuoka, M., Croft, S., Feng, L., Franzen, T. M. O., Gaensler, B. M., Johnston-Hollitt, M., Kaplan, D. L., Morales, M. F., Tingay, S. J., Wayth, R. B., Williams, A., Smartt, S. J., Chambers, K. C., Smith, K. W., Huber, M. E., Young, D. R., Wright, D. E., Schultz, A., Denneau, L., Flewelling, H., Magnier, E. A., Primak, N., Rest, A., Sherstyuk, A., Stalder, B., Stubbs, C. W., Tonry, J., Waters, C., Willman, M., E., F. Olivares, Campbell, H., Kotak, R., Sollerman, J., Smith, M., Dennefeld, M., Anderson, J. P., Botticella, M. T., Chen, T. -W., Valle, M. D., Elias-Rosa, N., Fraser, M., Inserra, C., Kankare, E., Kupfer, T., Harmanen, J., Galbany, L., Guillou, L. Le, Lyman, J. D., Maguire, K., Mitra, A., Nicholl, M., Razza, A., Terreran, G., Valenti, S., Gal-Yam, A., Ćwiek, A., Ćwiok, M., Mankiewicz, L., Opiela, R., Zaremba, M., Żarnecki, A. F., Onken, C. A., Scalzo, R. A., Schmidt, B. P., Wolf, C., Yuan, F., Evans, P. A., Kennea, J. A., Burrows, D. N., Campana, S., Cenko, S. B., Marshall, F. E., Nousek, J., O'Brien, P., Osborne, J. P., Palmer, D., Perri, M., Siegel, M., Tagliaferri, G., Klotz, A., Turpin, D., Laugier, R., Beroiz, M., Peñuela, T., Macri, L. M., Oelkers, R. J., Lambas, D. G., Vrech, R., Cabral, J., Colazo, C., Dominguez, M., Sanchez, B., Gurovich, S., Lares, M., Marshall, J. L., DePoy, D. L., Padilla, N., Pereyra, N. A., Benacquista, M., Tanvir, N. R., Wiersema, K., Levan, A. J., Steeghs, D., Hjorth, J., Fynbo, J. P. U., Malesani, D., Milvang-Jensen, B., Watson, D., Irwin, M., Fernandez, C. G., McMahon, R. G., Banerji, M., Gonzalez-Solares, E., Schulze, S., Postigo, A. de U., Thoene, C. C., Cano, Z., and Rosswog, S.
Subjects: Astrophysics - High Energy Astrophysical Phenomena, General Relativity and Quantum Cosmology
Abstract: A gravitational-wave (GW) transient was identified in data recorded by the Advanced Laser Interferometer Gravitational-wave Observatory (LIGO) detectors on 2015 September 14. The event, initially designated G184098 and later given the name GW150914, is described in detail elsewhere. By prior arrangement, preliminary estimates of the time, significance, and sky location of the event were shared with 63 teams of observers covering radio, optical, near-infrared, X-ray, and gamma-ray wavelengths with ground- and space-based facilities. In this Letter we describe the low-latency analysis of the GW data and present the sky localization of the first observed compact binary merger. We summarize the follow-up observations reported by 25 teams via private Gamma-ray Coordinates Network circulars, giving an overview of the participating facilities, the GW sky localization coverage, the timeline and depth of the observations. As this event turned out to be a binary black hole merger, there is little expectation of a detectable electromagnetic (EM) signature. Nevertheless, this first broadband campaign to search for a counterpart of an Advanced LIGO source represents a milestone and highlights the broad capabilities of the transient astronomy community and the observing strategies that have been developed to pursue neutron star binary merger events. Detailed investigations of the EM data and results of the EM follow-up campaign are being disseminated in papers by the individual teams., Comment: For Supplement, see https://arxiv.org/abs/1604.07864
Published: 2016
Full Text: View/download PDF

10. Wide-field broadband radio imaging with phased array feeds: a pilot multi-epoch continuum survey with ASKAP-BETA

Author: Heywood, I., Bannister, K. W., Marvil, J., Allison, J. R., Ball, L., Bell, M. E., Bock, D. C. -J., Brothers, M., Bunton, J. D., Chippendale, A. P., Cooray, F., Cornwell, T. J., DeBoer, D., Edwards, P., Gough, R., Gupta, N., Harvey-Smith, L., Hay, S., Hotan, A. W., Indermuehle, B., Jacka, C., Jackson, C. A., Johnston, S., Kimball, A. E., Koribalski, B. S., Lenc, E., Macleod, A., McClure-Griffiths, N., McConnell, D., Mirtschin, P., Murphy, T., Neuhold, S., Norris, R. P., Pearce, S., Popping, A., Qiao, R. Y., Reynolds, J. E., Sadler, E. M., Sault, R. J., Schinckel, A. E. T., Serra, P., Shimwell, T. W., Stevens, J., Tuthill, J., Tzioumis, A., Voronkov, M. A., Westmeier, T., and Whiting, M. T.
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: The Boolardy Engineering Test Array is a 6 x 12 m dish interferometer and the prototype of the Australian Square Kilometre Array Pathfinder (ASKAP), equipped with the first generation of ASKAP's phased array feed (PAF) receivers. These facilitate rapid wide-area imaging via the deployment of simultaneous multiple beams within a 30 square degree field of view. By cycling the array through 12 interleaved pointing positions and using 9 digitally formed beams we effectively mimic a traditional 1 hour x 108 pointing survey, covering 150 square degrees over 711 - 1015 MHz in 12 hours of observing time. Three such observations were executed over the course of a week. We verify the full bandwidth continuum imaging performance and stability of the system via self-consistency checks and comparisons to existing radio data. The combined three epoch image has arcminute resolution and a 1-sigma thermal noise level of 375 micro-Jy per beam, although the effective noise is a factor 3 higher due to residual sidelobe confusion. From this we derive a catalogue of 3,722 discrete radio components, using the 35 percent fractional bandwidth to measure in-band spectral indices for 1,037 of them. A search for transient events reveals one significantly variable source within the survey area. The survey covers approximately two-thirds of the Spitzer South Pole Telescope Deep Field. This pilot project demonstrates the viability and potential of using PAFs to rapidly and accurately survey the sky at radio wavelengths., Comment: 20 pages, 13 figures, 4 tables. Accepted for publication in MNRAS
Published: 2016
Full Text: View/download PDF

11. A pilot ASKAP survey of radio transient events in the region around the intermittent pulsar PSR J1107-5907

Author: Hobbs, G., Heywood, I., Bell, M. E., Kerr, M., Rowlinson, A., Johnston, S., Shannon, R. M., Voronkov, M. A., Ward, C., Banyer, J., Hancock, P. J., Murphy, Tara, Allison, J. R., Amy, S. W., Ball, L., Bannister, K., Bock, D. C. -J., Brodrick, D., Brothers, M., Brown, A. J., Bunton, J. D., Chapman, J., Chippendale, A. P., Chung, Y., DeBoer, D., Diamond, P., Edwards, P. G., Ekers, R., Ferris, R. H., Forsyth, R., Gough, R., Grancea, A., Gupta, N., Harvey-Smith, L., Hay, S., Hayman, D. B., Hotan, A. W., Hoyle, S., Humphreys, B., Indermuehle, B., Jacka, C. E., Jackson, C. A., Jackson, S., Jeganathan, K., Joseph, J, Kendall, R., Kiraly, D., Koribalski, B., Leach, M., Lenc, E., MacLeod, A., Mader, S., Marquarding, M., Marvil, J., McClure-Griffiths, N., McConnell, D., Mirtschin, P., Neuhold, S., Ng, A., Norris, R. P., O'Sullivan, J., Pearce, S., Phillips, C. J., Popping, A., Qiao, R. Y., Reynolds, J. E., Roberts, P., Sault, R. J., Schinckel, A. E. T., Serra, P., Shaw, R., Shimwell, T. W., Storey, M., Sweetnam, A. W., Tzioumis, A., Westmeier, T., Whiting, M., and Wilson, C. D.
Subjects: Astrophysics - Solar and Stellar Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: We use observations from the Boolardy Engineering Test Array (BETA) of the Australian Square Kilometre Array Pathfinder (ASKAP) telescope to search for transient radio sources in the field around the intermittent pulsar PSR J1107-5907. The pulsar is thought to switch between an "off" state in which no emission is detectable, a weak state and a strong state. We ran three independent transient detection pipelines on two-minute snapshot images from a 13 hour BETA observation in order to 1) study the emission from the pulsar, 2) search for other transient emission from elsewhere in the image and 3) to compare the results from the different transient detection pipelines. The pulsar was easily detected as a transient source and, over the course of the observations, it switched into the strong state three times giving a typical timescale between the strong emission states of 3.7 hours. After the first switch it remained in the strong state for almost 40 minutes. The other strong states lasted less than 4 minutes. The second state change was confirmed using observations with the Parkes radio telescope. No other transient events were found and we place constraints on the surface density of such events on these timescales. The high sensitivity Parkes observations enabled us to detect individual bright pulses during the weak state and to study the strong state over a wide observing band. We conclude by showing that future transient surveys with ASKAP will have the potential to probe the intermittent pulsar population., Comment: Accepted by MNRAS
Published: 2015
Full Text: View/download PDF

12. Tracing the neutral gas environments of young radio AGN with ASKAP

Author: Allison, J. R., Sadler, E. M., Moss, V. A., Harvey-Smith, L., Heywood, I., Indermuehle, B. T., McConnell, D., Sault, R. J., and Whiting, M. T.
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: At present neutral atomic hydrogen (HI) gas in galaxies at redshifts above $z \sim 0.3$ (the extent of 21-cm emission surveys in individual galaxies) and below $z \sim 1.7$ (where the Lyman-$\alpha$ line is not observable with ground-based telescopes) has remained largely unexplored. The advent of precursor telescopes to the Square Kilometre Array will allow us to conduct the first systematic radio-selected 21-cm absorption surveys for HI over these redshifts. While HI absorption is a tracer of the reservoir of cold neutral gas in galaxies available for star formation, it can also be used to reveal the extreme kinematics associated with jet-driven neutral outflows in radio-loud active galactic nuclei. Using the six-antenna Boolardy Engineering Test Array of the Australian Square Kilometre Array Pathfinder, we have demonstrated that in a single frequency tuning we can detect HI absorption over a broad range of redshifts between $z = 0.4$ and $1.0$. As part of our early science and commissioning program, we are now carrying out a search for absorption towards a sample of the brightest GPS and CSS sources in the southern sky. These intrinsically compact sources present us with an opportunity to study the circumunuclear region of recently re-started radio galaxies, in some cases showing direct evidence of mechanical feedback through jet-driven outflows. With the sensitivity of the full ASKAP array we will be able to study the kinematics of atomic gas in a few thousand radio galaxies, testing models of radio jet feedback well beyond the nearby Universe, Comment: 5 pages, 3 figures. Accepted for publication in Astronomische Nachrichten. In proceedings of the "5th Workshop on CSS and GPS radio sources", held in Rimini (Italy) in May 2015
Published: 2015
Full Text: View/download PDF

13. ASKAP HI imaging of the galaxy group IC 1459

Author: Serra, P., Koribalski, B., Kilborn, V., Allison, J. R., Amy, S. W., Ball, L., Bannister, K., Bell, M. E., Bock, D. C. -J., Bolton, R., Bowen, M., Boyle, B., Broadhurst, S., Brodrick, D., Brothers, M., Bunton, J. D., Chapman, J., Cheng, W., Chippendale, A. P., Chung, Y., Cooray, F., Cornwell, T., DeBoer, D., Diamond, P., Forsyth, R., Gough, R., Gupta, N., Hampson, G. A., Harvey-Smith, L., Hay, S., Hayman, D. B., Heywood, I., Hotan, A. W., Hoyle, S., Humphreys, B., Indermuehle, B., Jacka, C., Jackson, C. A., Jackson, S., Jeganathan, K., Johnston, S., Joseph, J, Kamphuis, P., Leach, M., Lenc, E., Lensson, E., Mackay, S., Marquarding, M., Marvil, J., McClure-Griffiths, N., McConnell, D., Meyer, M., Mirtschin, P., Neuhold, S., Ng, A., Norris, R. P., O'Sullivan, J., Pathikulangara, J., Pearce, S., Phillips, C., Popping, A., Qiao, R. Y., Reynolds, J. E., Roberts, P., Sault, R. J., Schinckel, A. E. T., Shaw, R., Shimwell, T. W., Staveley-Smith, L., Storey, M., Sweetnam, A. W., Troup, E., Tzioumis, A., Voronkov, M. A., Westmeier, T., Whiting, M., Wilson, C., Wong, O. I., and Wu, X.
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: We present HI imaging of the galaxy group IC 1459 carried out with six antennas of the Australian SKA Pathfinder equipped with phased-array feeds. We detect and resolve HI in eleven galaxies down to a column density of $\sim10^{20}$ cm$^{-2}$ inside a ~6 deg$^2$ field and with a resolution of ~1 arcmin on the sky and ~8 km/s in velocity. We present HI images, velocity fields and integrated spectra of all detections, and highlight the discovery of three HI clouds -- two in the proximity of the galaxy IC 5270 and one close to NGC 7418. Each cloud has an HI mass of $10^9$ M$_\odot$ and accounts for ~15% of the HI associated with its host galaxy. Available images at ultraviolet, optical and infrared wavelengths do not reveal any clear stellar counterpart of any of the clouds, suggesting that they are not gas-rich dwarf neighbours of IC 5270 and NGC 7418. Using Parkes data we find evidence of additional extended, low-column-density HI emission around IC 5270, indicating that the clouds are the tip of the iceberg of a larger system of gas surrounding this galaxy. This result adds to the body of evidence on the presence of intra-group gas within the IC 1459 group. Altogether, the HI found outside galaxies in this group amounts to several times $10^9$ M$_\odot$, at least 10% of the HI contained inside galaxies. This suggests a substantial flow of gas in and out of galaxies during the several billion years of the group's evolution., Comment: MNRAS accepted
Published: 2015
Full Text: View/download PDF

14. Discovery of HI gas in a young radio galaxy at $z = 0.44$ using the Australian Square Kilometre Array Pathfinder

Author: Allison, J. R., Sadler, E. M., Moss, V. A., Whiting, M. T., Hunstead, R. W., Pracy, M. B., Curran, S. J., Croom, S. M., Glowacki, M., Morganti, R., Shabala, S. S., Zwaan, M. A., Allen, G., Amy, S. W., Axtens, P., Ball, L., Bannister, K. W., Barker, S., Bell, M. E., Bock, D. C. -J., Bolton, R., Bowen, M., Boyle, B., Braun, R., Broadhurst, S., Brodrick, D., Brothers, M., Brown, A., Bunton, J. D., Cantrall, C., Chapman, J., Cheng, W., Chippendale, A. P., Chung, Y., Cooray, F., Cornwell, T., DeBoer, D., Diamond, P., Edwards, P. G., Ekers, R., Feain, I., Ferris, R. H., Forsyth, R., Gough, R., Grancea, A., Gupta, N., Guzman, J. C., Hampson, G., Harvey-Smith, L., Haskins, C., Hay, S., Hayman, D. B., Heywood, I., Hotan, A. W., Hoyle, S., Humphreys, B., Indermuehle, B. T., Jacka, C., Jackson, C., Jackson, S., Jeganathan, K., Johnston, S., Joseph, J., Kendall, R., Kesteven, M., Kiraly, D., Koribalski, B. S., Leach, M., Lenc, E., Lensson, E., Mackay, S., Macleod, A., Marquarding, M., Marvil, J., McClure-Griffiths, N., McConnell, D., Mirtschin, P., Norris, R. P., Neuhold, S., Ng, A., O'Sullivan, J., Pathikulangara, J., Pearce, S., Phillips, C., Popping, A., Qiao, R. Y., Reynolds, J. E., Roberts, P., Sault, R. J., Schinckel, A., Serra, P., Shaw, R., Shields, M., Shimwell, T., Storey, M., Sweetnam, T., Troup, E., Turner, B., Tuthill, J., Tzioumis, A., Voronkov, M. A., Westmeier, T., and Wilson, C. D.
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: We report the discovery of a new 21-cm HI absorption system using commissioning data from the Boolardy Engineering Test Array of the Australian Square Kilometre Array Pathfinder (ASKAP). Using the 711.5 - 1015.5 MHz band of ASKAP we were able to conduct a blind search for the 21-cm line in a continuous redshift range between $z = 0.4$ and 1.0, which has, until now, remained largely unexplored. The absorption line is detected at $z = 0.44$ towards the GHz-peaked spectrum radio source PKS B1740$-$517 and demonstrates ASKAP's excellent capability for performing a future wide-field survey for HI absorption at these redshifts. Optical spectroscopy and imaging using the Gemini-South telescope indicates that the HI gas is intrinsic to the host galaxy of the radio source. The narrow OIII emission lines show clear double-peaked structure, indicating either large-scale outflow or rotation of the ionized gas. Archival data from the \emph{XMM-Newton} satellite exhibit an absorbed X-ray spectrum that is consistent with a high column density obscuring medium around the active galactic nucleus. The HI absorption profile is complex, with four distinct components ranging in width from 5 to 300 km s$^{-1}$ and fractional depths from 0.2 to 20 per cent. In addition to systemic HI gas, in a circumnuclear disc or ring structure aligned with the radio jet, we find evidence for a possible broad outflow of neutral gas moving at a radial velocity of $v \sim 300$ km s$^{-1}$. We infer that the expanding young radio source ($t_{\rm age} \approx 2500$ yr) is cocooned within a dense medium and may be driving circumnuclear neutral gas in an outflow of $\sim$ 1 $\mathrm{M}_{\odot}$ yr$^{-1}$., Comment: 18 pages, 11 figures, accepted for publication in MNRAS
Published: 2015
Full Text: View/download PDF

15. The Murchison Widefield Array Correlator

Author: Ord, S. M., Crosse, B., Emrich, D., Pallot, D., Wayth, R. B., Clark, M. A., Tremblay, S. E., Arcus, W., Barnes, D., Bell, M., Bernardi, G., Bhat, N. D. R., Bowman, J. D., Briggs, F., Bunton, J. D., Cappallo, R. J., Corey, B. E., Deshpande, A. A., deSouza, L., Ewell-Wice, A., Feng, L., Goeke, R., Greenhill, L. J., Hazelton, B. J., Herne, D., Hewitt, J. N., Hindson, L., Hurley-Walker, H., Jacobs, D., Johnston-Hollitt, M., Kaplan, D. L., Kasper, J. C., Kincaid, B. B., Koenig, R., Kratzenberg, E., Kudryavtseva, N., Lenc, E., Lonsdale, C. J., Lynch, M. J., McKinley, B., McWhirter, S. R., Mitchell, D. A., Morales, M. F., Morgan, E., Oberoi, D., Offringa, A., Pathikulangara, J., Pindor, B., Prabu, T., Procopio, P., Remillard, R. A., Riding, J., Rogers, A. E. E., Roshi, A., Salah, J. E., Sault, R. J., Shankar, N. Udaya, Srivani, K. S., Stevens, J., Subrahmanyan, R., Tingay, S. J., Waterson, M., Webster, R. L., Whitney, A. R., Williams, A., Williams, C. L., and Wyithe, J. S. B.
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics, Computer Science - Computational Engineering, Finance, and Science
Abstract: The Murchison Widefield Array (MWA) is a Square Kilometre Array (SKA) Precursor. The telescope is located at the Murchison Radio--astronomy Observatory (MRO) in Western Australia (WA). The MWA consists of 4096 dipoles arranged into 128 dual polarisation aperture arrays forming a connected element interferometer that cross-correlates signals from all 256 inputs. A hybrid approach to the correlation task is employed, with some processing stages being performed by bespoke hardware, based on Field Programmable Gate Arrays (FPGAs), and others by Graphics Processing Units (GPUs) housed in general purpose rack mounted servers. The correlation capability required is approximately 8 TFLOPS (Tera FLoating point Operations Per Second). The MWA has commenced operations and the correlator is generating 8.3 TB/day of correlation products, that are subsequently transferred 700 km from the MRO to Perth (WA) in real-time for storage and offline processing. In this paper we outline the correlator design, signal path, and processing elements and present the data format for the internal and external interfaces., Comment: 17 pages, 9 figures. Accepted for publication in PASA. Some figures altered to meet astro-ph submission requirements
Published: 2015
Full Text: View/download PDF

16. Long-lasting, deep effect of Saturn’s giant storms

Author: Li, Cheng, primary, de Pater, Imke, additional, Moeckel, Chris, additional, Sault, R. J., additional, Butler, Bryan, additional, deBoer, David, additional, and Zhang, Zhimeng, additional
Published: 2023
Full Text: View/download PDF

17. Peering through Jupiter's clouds with radio spectral imaging

Author: de Pater, Imke, Sault, R. J., Butler, Bryan, DeBoer, David, and Wong, Michael H.
Published: 2016

18. Prospects to study the Ice Giants with the ngVLA

Author: Pater, Imke de, primary, Moeckel, Chris, additional, Tollefson, Joshua, additional, Butler, Bryan, additional, Kleer, Katherine de, additional, Fletcher, Leigh, additional, Gurwell, Mark A., additional, Luszcz-Cook, Statia, additional, Milam, Stefanie, additional, Molter, Edward, additional, Moullet, Arielle, additional, Sault, R. J., additional, and Spilker, Thomas R., additional
Published: 2021
Full Text: View/download PDF

19. Mapping satellite surfaces and atmospheres with ground-based radio interferometry

Author: de Kleer, Katherine, Butler, Bryan, Cordiner, Martin, de Pater, Imke, Gurwell, Mark, Lazio, Joseph, Milam, Stefanie, Moeckel, Chris, Moullet, Arielle, Murphy, Eric, Sault, R. J., Tollefson, Joshua, Trumbo, Samantha, de Kleer, Katherine, Butler, Bryan, Cordiner, Martin, de Pater, Imke, Gurwell, Mark, Lazio, Joseph, Milam, Stefanie, Moeckel, Chris, Moullet, Arielle, Murphy, Eric, Sault, R. J., Tollefson, Joshua, and Trumbo, Samantha
Abstract: Ground-based interferometry at mm-cm wavelengths provides a powerful tool for characterizing satellite surfaces and atmospheres. We present the science enabled by the ALMA (current) and ngVLA (proposed) arrays, including recent results as well as future work in the context of planned and proposed spacecraft missions.
Published: 2020

20. A new layout optimization technique for interferometric arrays and the final MWA antenna layout

Author: Haystack Observatory, MIT Kavli Institute for Astrophysics and Space Research, Beardsley, A. P., Hazelton, B. J., Morales, M. F., Capallo, R.J., Goeke, Robert F, Emrich, D., Lonsdale, Colin John, Arcus, W., Barnes, D., Bernardi, G., Bowman, J. D., Bunton, J. D., Corey, Brian E, Deshpande, A., deSouza, L., Gaensler, B. M., Greenhill, L. J., Herne, D., Hewitt, Jacqueline N, Kaplan, D. L., Kasper, J. C., Kincaid, Barton B., Koenig, R., Kratzenberg, Eric W, Lynch, M. J., McWhirter, S. R., Mitchell, D. A., Morgan, Edward H, Oberoi, Divya, Ord, S. M., Pathikulangara, J., Prabu, T., Rogers, Alan E E, Roshi, A., Salah, Joseph E., Sault, R. J., Shankar, N. Udaya, Srivani, K. S., Stevens, J., Subrahmanyan, R., Tingay, S. J., Wayth, R. B., Waterson, M., Webster, R. L., Whitney, Alan R, Williams, A., Williams, C. L., Wyithe, J. S. B., Remillard, Ronald A, Haystack Observatory, MIT Kavli Institute for Astrophysics and Space Research, Beardsley, A. P., Hazelton, B. J., Morales, M. F., Capallo, R.J., Goeke, Robert F, Emrich, D., Lonsdale, Colin John, Arcus, W., Barnes, D., Bernardi, G., Bowman, J. D., Bunton, J. D., Corey, Brian E, Deshpande, A., deSouza, L., Gaensler, B. M., Greenhill, L. J., Herne, D., Hewitt, Jacqueline N, Kaplan, D. L., Kasper, J. C., Kincaid, Barton B., Koenig, R., Kratzenberg, Eric W, Lynch, M. J., McWhirter, S. R., Mitchell, D. A., Morgan, Edward H, Oberoi, Divya, Ord, S. M., Pathikulangara, J., Prabu, T., Rogers, Alan E E, Roshi, A., Salah, Joseph E., Sault, R. J., Shankar, N. Udaya, Srivani, K. S., Stevens, J., Subrahmanyan, R., Tingay, S. J., Wayth, R. B., Waterson, M., Webster, R. L., Whitney, Alan R, Williams, A., Williams, C. L., Wyithe, J. S. B., and Remillard, Ronald A
Abstract: Antenna layout is an important design consideration for radio interferometers because it determines the quality of the snapshot point spread function (PSF, or array beam). This is particularly true for experiments targeting the 21-cm Epoch of Reionization signal as the quality of the foreground subtraction depends directly on the spatial dynamic range and thus the smoothness of the baseline distribution. Nearly all sites have constraints on where antennas can be placed - even at the remote Australian location of the Murchison Widefield Array (MWA) there are rock outcrops, flood zones, heritages areas, emergency runways and trees. These exclusion areas can introduce spatial structure into the baseline distribution that enhances the PSF sidelobes and reduces the angular dynamic range. In this paper we present a new method of constrained antenna placement that reduces the spatial structure in the baseline distribution. This method not only outperforms random placement algorithms that avoid exclusion zones, but surprisingly outperforms random placement algorithms without constraints to provide what we believe are the smoothest constrained baseline distributions developed to date. We use our new algorithm to determine antenna placements for the originally planned MWA, and present the antenna locations, baseline distribution and snapshot PSF for this array choice., U.S. National Science Foundation (grants AST CAREER-0847753, AST-0457585, AST-0908884 and PHY-0835713), Australian Research Council (grants LE0775621 and LE0882938), U.S. Air Force Office of Scientific Research (grant FA9550-0510247)
Published: 2020

21. First ALMA Millimeter-wavelength Maps of Jupiter, with a Multiwavelength Study of Convection

Author: de Pater, I. (author), Sault, R. J. (author), Moeckel, Chris (author), Moullet, Arielle (author), Wong, Michael H. (author), Goullaud, Charles (author), Deboer, David (author), Butler, Bryan J. (author), Bjoraker, Gordon (author), de Pater, I. (author), Sault, R. J. (author), Moeckel, Chris (author), Moullet, Arielle (author), Wong, Michael H. (author), Goullaud, Charles (author), Deboer, David (author), Butler, Bryan J. (author), and Bjoraker, Gordon (author)
Abstract: We obtained the first maps of Jupiter at 1-3 mm wavelength with the Atacama Large Millimeter/Submillimeter Array (ALMA) on 2017 January 3-5, just days after an energetic eruption at 16.5S jovigraphic latitude had been reported by the amateur community, and about two to three months after the detection of similarly energetic eruptions in the northern hemisphere, at 22.2-23.0N. Our observations, probing below the ammonia cloud deck, show that the erupting plumes in the South Equatorial Belt bring up ammonia gas from the deep atmosphere. While models of plume eruptions that are triggered at the water condensation level explain data taken at uv-visible and mid-infrared wavelengths, our ALMA observations provide a crucial, hitherto missing, link in the moist convection theory by showing that ammonia gas from the deep atmosphere is indeed brought up in these plumes. Contemporaneous Hubble Space Telescope data show that the plumes reach altitudes as high as the tropopause. We suggest that the plumes at 22.2-23.0N also rise up well above the ammonia cloud deck and that descending air may dry the neighboring belts even more than in quiescent times, which would explain our observations in the north., Astrodynamics & Space Missions
Published: 2019
Full Text: View/download PDF

22. Jupiter's ammonia distribution derived from VLA maps at 3–37 GHz

Author: de Pater, I. (author), Sault, R. J. (author), Wong, Michael H. (author), Fletcher, Leigh N. (author), DeBoer, David (author), Butler, Bryan (author), de Pater, I. (author), Sault, R. J. (author), Wong, Michael H. (author), Fletcher, Leigh N. (author), DeBoer, David (author), and Butler, Bryan (author)
Abstract: We observed Jupiter four times over a full rotation (10 h) with the upgraded Karl G. Jansky Very Large Array (VLA) between December 2013 and December 2014. Preliminary results at 4–17 GHz were presented in de Pater et al. (2016); in the present paper we present the full data set at frequencies between 3 and 37 GHz. Major findings are: i) The radio-hot belt at 8.5–11° N latitude, near the interface between the North Equatorial Belt (NEB) and the Equatorial Zone (EZ) is prominent at all frequencies (3–37 GHz). Its location coincides with the southern latitudes of the NEB (7–17° N). ii) Longitude-smeared maps reveal belts and zones at all frequencies at latitudes ≲ |20°|. At higher latitudes numerous fainter bands are visible at frequencies ≳ 7 GHz. The lowest brightness temperature is in the EZ near a latitude of 4° N, and the NEB has the highest brightness temperature near 11° N. The bright part of the NEB increases in latitudinal extent (spreads towards the north) with deceasing frequency, i.e., with depth into the atmosphere. In longitude-resolved maps, several belts, in particular in the southern hemisphere, are not continuous along the latitude line, but broken into small segments as if caused by an underlying wave. iii) Model fits to longitude-smeared spectra are obtained at each latitude. These show a high NH3 abundance (volume mixing ratio ∼4×10−4) in the deep (P > 8–10 bar) atmosphere, decreasing at higher altitudes due to cloud formation (e.g., in zones), or dynamics in combination with cloud condensation (belts). In the NEB ammonia gas is depleted down to at least the 20 bar level with an abundance of 1.75×10−4. The NH3 abundance at latitudes > |50|° is characterized by a relatively low value (∼1.75×10−4) between ∼ 1 and 10 bar. iv) Using the entire VLA dataset, we confirm that the planet is extremely dynamic in the upper layers of the atmosphere, at P < 2–3 bar, i.e., at the altitudes where clouds form. At most latitudes the relative humidity with, Astrodynamics & Space Missions
Published: 2019
Full Text: View/download PDF

23. First ALMA Millimeter-wavelength Maps of Jupiter, with a Multiwavelength Study of Convection

Author: de Pater, Imke, primary, Sault, R. J., additional, Moeckel, Chris, additional, Moullet, Arielle, additional, Wong, Michael H., additional, Goullaud, Charles, additional, DeBoer, David, additional, Butler, Bryan J., additional, Bjoraker, Gordon, additional, Ádámkovics, Máté, additional, Cosentino, Richard, additional, Donnelly, Padraig T., additional, Fletcher, Leigh N., additional, Kasaba, Yasumasa, additional, Orton, Glenn S., additional, Rogers, John H., additional, Sinclair, James A., additional, and Villard, Eric, additional
Published: 2019
Full Text: View/download PDF

24. Potential for Solar System Science with the ngVLA

Author: Murphy, Eric J., de Pater, Imke, Butler, Bryan, Sault, R. J., Moullet, Arielle, Moeckel, Chris, Tollefson, Joshua, de Kleer, Katherine, Gurwell, Mark, Milam, Stefanie, Murphy, Eric J., de Pater, Imke, Butler, Bryan, Sault, R. J., Moullet, Arielle, Moeckel, Chris, Tollefson, Joshua, de Kleer, Katherine, Gurwell, Mark, and Milam, Stefanie
Abstract: Radio wavelength observations of solar system bodies are a powerful method of probing many characteristics of those bodies. From surface and subsurface, to atmospheres (including deep atmospheres of the giant planets), to rings, to the magnetosphere of Jupiter, these observations provide unique information on the current state, and sometimes history, of the bodies. The ngVLA will enable the highest sensitivity and resolution observations of this kind, with the potential to revolutionize our understanding of some of these bodies. In this article, we present a review of state-of-the-art radio wavelength observations of a variety of bodies in our solar system, varying in size from ring particles and small near-Earth asteroids to the giant planets. Throughout the review we mention improvements for each body (or class of bodies) to be expected with the ngVLA. A simulation of a Neptune-sized object is presented in Section 6. Section 7 provides a brief summary for each type of object, together with the type of measurements needed for all objects throughout the Solar System.
Published: 2018

25. Supplement: 'Localization and Broadband Follow-up of the Gravitational-wave Transient GW150914' (2016, ApJS, 225, 8)

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., Bodiya, T. P., Goetz, R., Mihara, T., Gondan, L., González, G., Castro, J. M. G., Gopakumar, A., Gordon, N. A., Gorodetsky, M. L., Miao, H., Gossan, S. E., Walsh, S., Johnson, M. D., Aston, S. M., Tomida, H., Gosselin, M., Gouaty, R., Graef, C., Graff, P. B., Granata, M., Grant, A., Gras, S., Wang, G., Michel, C., Gray, C., Greco, G., Ueno, S., Johnson, M. W. G., Green, A. C., Astone, P., Groot, P., Grote, H., Grunewald, S., Vikram, V., Guidi, G. M., Guo, X., Nichol, R. C., Gupta, A., Tsunemi, H., Gupta, M. K., Gushwa, K. E., Karliner, I., Gustafson, E. K., Gustafson, R., Wang, H., Aufmuth, P., Hacker, J. J., Hall, B. R., Hall, E. D., Middleton, H., Cavalier, F., Hammond, G., Haney, M., Hanke, M. M., Hanks, J., Wang, M., Braginsky, V. B., Hanna, C., Hannam, M. D., Hanson, J., Aulbert, C., Hardwick, T., Cowperthwaite, P. S., Mikhailov, E. E., Haris, K., Harms, J., Wang, X., Harry, G. M., Harry, I. W., Hart, M. J., Kasen, D., Hartman, M. T., Haster, C. -J., Haughian, K., Matsuoka, M., Heidmann, A., Milano, L., Wang, Y., Babak, S., Heintze, M. C., Heitmann, H., Hello, P., Hemming, G., Hendry, M., Kent, S., Heng, I. S., MAXI Collaboration, Hennig, J., Ward, R. L., Heptonstall, A. W., Miller, J., Heurs, M., Hild, S., Bacon, P., Hoak, D., Hodge, K. A., Hofman, D., Hollitt, S. E., Mason, K., Warner, J., Kessler, R., Holt, K., Holz, D. E., Millhouse, M., Hopkins, P., Hosken, D. J., Hough, J., Houston, E. A., Bader, M. K. M., Howell, E. J., Smith, M., Fraser, M., Croft, S., Hu, Y. M., Huang, S., Kim, A. G., Huerta, E. A., Królak, A., Batch, J. C., Huet, D., Hughey, B., Husa, S., Martini, P., Huttner, S. H., Feng, L., Huynh-Dinh, T., Idrisy, A., Baker, P. T., Indik, N., Ingram, D. R., Carrasco Kind, M., Minenkov, Y., Inta, R., Was, M., Isa, H. N., Isac, J. -M., Franzen, T. M. O., Isi, M., Islas, G., Isogai, T., Iyer, B. R., Izumi, K., Baldaccini, F., Jacqmin, T., Weaver, B., Ming, J., Kuehn, K., Jang, H., Gaensler, B. M., Jani, K., Jaranowski, P., Jawahar, S., Jiménez-Forteza, F., Johnson, W. W., Jones, D. I., Boer, M., Jones, R., Jonker, R. J. G., Mirshekari, S., Ballardin, G., Johnston-Hollitt, M., Kuropatkin, N., Ju, L., Kalaghatgi, C. V., Kalogera, V., Kandhasamy, S., Wei, L. -W., Kang, G., Kanner, J. B., Karki, S., Kasprzack, M., Mishra, C., Kaplan, D. L., Katsavounidis, E., Katzman, W., Lahav, O., Ballmer, S. W., Walker, A. R., Kaufer, S., Kaur, T., Kawabe, K., Kawazoe, F., Kéfélian, F., Kehl, M. S., Morales, M. F., Nord, B., Keitel, D., Kelley, D. B., Weinert, M., Kells, W., Li, T. S., Kennedy, R., Barayoga, J. C., Key, J. S., Khalaidovski, A., Khalili, F. Y., Tingay, S. J., Khan, I., Mitra, S., Weinstein, A. J., Khan, S., Khan, Z., Khazanov, E. A., Kijbunchoo, N., Lima, M., Kim, C., Kim, J., Barclay, S. E., Crocce, M., Kim, K., Weiss, R., Kim, N., Mitrofanov, V. P., Kim, Y. -M., King, E. J., King, P. J., Kinzel, D. L., Kissel, J. S., Branchesi, M., Kleybolte, L., Cavalieri, R., Blackburn, J. K., Welborn, T., Klimenko, S., Koehlenbeck, S. M., Barish, B. C., Mitselmakher, G., Kokeyama, K., Koley, S., Kondrashov, V., Kontos, A., Korobko, M., Korth, W. Z., Martin, R. M., Masserot, A., Mittleman, R., Barker, D., Moggi, A., Mohan, M., Baune, C., Mohapatra, S. R. P., Montani, M., Moore, B. C., Nugent, P., Matone, L., Moore, C. J., Wayth, R. B., Moraru, D., Moreno, G., Krueger, C., Morriss, S. R., Mossavi, K., Mours, B., Mow-Lowry, C. M., Bavigadda, V., Wen, L., Mueller, C. L., Mueller, G., Williams, A., Ogando, R., Muir, A. W., Mukherjee, A., Kuehn, G., Mukherjee, D., Mukherjee, S., Mukund, N., Lord, J. E., Mullavey, A., Munch, J., Murphy, D. J., Murchison Wide-field Array (MWA Collaboration), Bazzan, M., Murray, P. G., Petravick, D., Mytidis, A., Kumar, P., Nardecchia, I., Wessels, P., Naticchioni, L., Nayak, R. K., Necula, V., Nedkova, K., Smartt, S. J., Nelemans, G., Neri, M., Neunzert, A., Behnke, B., Plazas, A. A., Westphal, T., Kuo, L., Newton, G., Nguyen, T. T., Nielsen, A. B., Nissanke, S., Chambers, K. C., Nitz, A., Nocera, F., Nolting, D., Normandin, M. E. N., Wette, K., Nuttall, L. K., Oberling, J., Kutynia, A., Quataert, E., Bejger, M., Ochsner, E., Smith, K. W., O'Dell, J., Oelker, E., Ogin, G. H., Whelan, J. T., Oh, J. J., Oh, S. H., Ohme, F., Oliver, M., Maia, M. A. G., Oppermann, P., Roe, N., Huber, M. E., Oram, R. J., Bell, A. S., Bogaert, G., O'Reilly, B., O'Shaughnessy, R., Ottaway, D. J., Ottens, R. S., Overmier, H., Owen, B. J., Lackey, B. D., Pai, A., Young, D. R., Pai, S. A., Thorne, K. S., Allen, W. H., Fernández-Muñoz, R., Romer, A. K., Palamos, J. R., Palashov, O., Bell, C. J., Palliyaguru, N., Palomba, C., Pal-Singh, A., Landry, M., Wright, D. E., Wechsler, R. H., Pan, H., Pankow, C., Pannarale, F., Pant, B. C., Affeldt, C., Paoletti, F., Paoli, A., Papa, M. A., Berger, B. K., Paris, H. R., White, D. J., Cunha, C. E., Lange, J., Parker, W., Pascucci, D., Pasqualetti, A., Passaquieti, R., Passuello, D., Briant, T., Patricelli, B., Patrick, Z., Inserra, C., Pearlstone, B. L., Massinger, T. J., Pedraza, M., Lantz, B., Bergman, J., Pedurand, R., Pekowsky, L., Pele, A., Penn, S., Perreca, A., Whiting, B. F., Roodman, A., Phelps, M., Schultz, A., Piccinni, O., Pichot, M., Lasky, P. D., Piergiovanni, F., Pierro, V., Bergmann, G., Pillant, G., Williams, R. D., Pinard, L., Pinto, I. M., Pitkin, M., Cella, G., Rosell, A. C., Poggiani, R., Popolizio, P., Barone, F., Post, A., Powell, J., Lorenzini, M., Prasad, J., Predoi, V., Berry, C. P. L., Premachandra, S. S., Denneau, L., Prestegard, T., Price, L. R., Rykoff, E. S., Prijatelj, M., Lazzarini, A., Williamson, A. R., Principe, M., Privitera, S., Prodi, G. A., Prokhorov, L., Puncken, O., Flewelling, H., Punturo, M., Bersanetti, D., Puppo, P., Pürrer, M., Willis, J. L., Sako, M., Lazzaro, C., Qi, H., Qin, J., Quetschke, V., Quintero, E. A., Magnier, E. A., Quitzow-James, R., Raab, F. J., Rabeling, D. S., Willke, B., Radkins, H., Bertolini, A., Raffai, P., Leaci, P., Sanchez, E., Raja, S., Rakhmanov, M., Primak, N., Rapagnani, P., Raymond, V., Levine, B. M., Wimmer, M. H., Razzano, M., Re, V., Read, J., Reed, C. M., Regimbau, T., Leavey, S., Betzwieser, J., Scarpine, V., Rest, A., Rei, L., Winkler, W., Reid, S., Reitze, D. H., Rew, H., Reyes, S. D., Ricci, F., Riles, K., Robertson, N. A., Margutti, R., Robie, R., Sherstyuk, A., Wipf, C. C., Robinet, F., Schindler, R., Bhagwat, S., Rocchi, A., Rolland, L., Rollins, J. G., Roma, V. J., Romano, R., Romanov, G., Lebigot, E. O., Wittel, H., Stalder, B., Romie, J. H., Rosińska, D., Rowan, S., Yock, P. C., Schubnell, M., Rüdiger, A., Bhandare, R., Ruggi, P., Ryan, K., Kankare, E., Sachdev, S., Stubbs, C. W., Lee, C. H., Sadecki, T., Sadeghian, L., Salconi, L., Saleem, M., Salemi, F., Scolnic, D., Samajdar, A., Wester, W., Sammut, L., Bilenko, I. A., Masso-Reid, M., Sanchez, E. J., Lee, H. K., Sandberg, V., Sandeen, B., Sanders, J. R., Sassolas, B., Sathyaprakash, B. S., Bogan, C., Saulson, P. R., Sevilla-Noarbe, I., Sauter, O., D'Andrea, C. B., Savage, R. L., Sawadsky, A., Lee, H. M., Billingsley, G., Schale, P., Schilling, R., Woan, G., Schmidt, J., Schmidt, P., Schnabel, R., Schofield, R. M. S., Tonry, J., Brillet, A., Schönbeck, A., Schreiber, E., Lee, K., Schuette, D., Loriette, V., Schutz, B. F., Birch, J., Scott, J., Scott, S. M., Sellers, D., Waters, C., Sentenac, D., Sequino, V., Sheldon, E., Sergeev, A., Worden, J., Lenon, A., Serna, G., Setyawati, Y., Sevigny, A., Shaddock, D. A., Birney, R., Cepeda, C. B., Shah, S., Shahriar, M. S., Shaltev, M., Thrane, E., Wright, J. L., Shao, Z., Smith, N., Barr, B., Shapiro, B., Shawhan, P., Sheperd, A., Shoemaker, D. H., Willman, M., Shoemaker, D. M., Siellez, K., Wu, G., Biscans, S., Siemens, X., Sigg, D., Silva, A. D., Leonardi, M., Smith, R. C., Simakov, D., Singer, A., Pan-STARRS Collaboration, Singh, A., Yablon, J., Singh, R., Singhal, A., Sintes, A. M., Slagmolen, B. J. J., Bisht, A., Smith, J. R., Leong, J. R., Smith, N. D., Soares-Santos, M., Olivares E., F., Yam, W., Smith, R. J. E., Son, E. J., Sorazu, B., Sorrentino, F., Souradeep, T., Srivastava, A. K., Staley, A., Steinke, M., Leroy, N., Bitossi, M., Yamamoto, H., Campbell, H., Steinlechner, J., Sobreira, F., Steinlechner, S., Steinmeyer, D., Stephens, B. C., Stone, R., Strain, K. A., Straniero, N., STRATTA, MARIA GIULIANA, Bozzi, A., Marriner, J., Kotak, R., Strauss, N. A., Strigin, S., Biwer, C., Stebbins, A., Sturani, R., Stuver, A. L., Summerscales, T. Z., Sun, L., Yancey, C. C., Sutton, P. J., Swinkels, B. L., Sollerman, J., Letendre, N., Szczepańczyk, M. J., Tacca, M., Talukder, D., Tanner, D. B., Rattenbury, N., Suchyta, E., Yap, M. J., Bizouard, M. A., Tápai, M., Tarabrin, S. P., Matichard, F., Taracchini, A., Levin, Y., Taylor, R., Theeg, T., Thirugnanasambandam, M. P., Thomas, E. G., Yanny, B., Thomas, M., Thomas, P., Swanson, M. E. C., Thorne, K. A., Yu, H., Tiwari, S., Lormand, M., Bohe, A., Yvert, M., Zadrożny, A., Zangrando, L., Zanolin, M., Kupfer, T., Zendri, J. -P., Zevin, M., Zhang, F., Tiwari, V., Zhang, L., Zuntz, J., Losurdo, G., Zhang, M., Zhang, Y., Bojtos, P., Zhao, C., Harmanen, J., Zhou, M., Zhou, Z., Tokmakov, K. V., Zhu, X. J., Zucker, M. E., Zuraw, S. E., Zweizig, J., Lough, J. D., Dark Energy Survey Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, Galbany, L., Allison, J., Tomlinson, C., Bond, C., Bannister, K., Bell, M. E., Chatterjee, S., Chippendale, A. P., Edwards, P. G., Lück, H., Harvey-Smith, L., Brisson, V., Le Guillou, L., Tonelli, M., Heywood, Ian, Hotan, A., Indermuehle, B., Marvil, J., Bondu, F., McConnell, D., Murphy, T., Popping, A., Lundgren, A. P., Reynolds, J., Torres, C. V., Cerretani, G., Sault, R. J., Dark Energy Camera GW-EM Collaboration, Voronkov, M. A., Whiting, M. T., Australian Square Kilometer Array Pathfinder (ASKAP Collaboration), Castro-Tirado, A. J., Cunniffe, R., Bonnand, R., Jelínek, M., da Costa, L. N., Barsuglia, M., Lyman, J. D., Tello, J. C., Oates, S. R., Hu, Y. -D., Connaughton, V., Kubánek, P., Guziy, S., Castellón, A., García-Cerezo, A., Tarle, G., Muñoz, V. F., Pérez del Pulgar, C., CASENTINI, CLAUDIO, Maguire, K., Luo, J., Boom, B. A., Castillo-Carrión, S., Castro Cerón, J. M., Hudec, R., Burns, E., Torrie, C. I., Caballero-García, M. D., Páta, P., Vitek, S., Adame, J. A., Lin, H., Konig, S., Matheson, T., Rendón, F., Mateo Sanguino, T. de J., Goldstein, A., Töyrä, D., Querel, R., Briggs, M. S., Zhang, B. -B., Hui, C. M., Jenke, P., Miquel, R., Wilson-Hodge, C. A., Bhat, P. N., Lynch, R., Brockill, P., Li, T. G. F., Bissaldi, E., Cleveland, W., Fitzpatrick, G., Jeong, S., Giles, M. M., Gibby, M. H., Mitra, A., Greiner, J., von Kienlin, A., Kippen, R. M., Blair, C. D., Ma, Y., McBreen, S., Mailyan, B., Brooks, A. F., Meegan, C. A., Paciesas, W. S., Park, I. H., Nicholl, M., Preece, R. D., Roberts, O., Travasso, F., Sparke, L., Stanbro, M., MacDonald, T., Toelge, K., Veres, P., Yu, H. -F., Blackburn, L., Brown, D. A., Razza, A., Fermi GBM Collaboration, Traylor, G., Bai, J., Ackermann, M., Ajello, M., Albert, A., Machenschalk, B., Anderson, B., Atwood, W. B., Axelsson, M., Baldini, L., Desai, S., Trifirò, D., Barbiellini, G., Bastieri, D., Brown, D. D., Cui, Ch., Bellazzini, R., Blandford, R. D., MacInnis, M., Bloom, E. D., Bonino, R., Bottacini, E., Tringali, M. C., Terreran, G., Brandt, T. J., Bruel, P., Buson, S., Caliandro, G. A., Cameron, R. A., Fan, Y., Brown, N. M., Macleod, D. M., Caragiulo, M., Trozzo, L., CARAVEO, PATRIZIA, Valenti, S., Cavazzuti, E., Charles, E., Chekhtman, A., Chiang, J., Chiaro, G., Ciprini, S., Cohen-Tanugi, J., Boschi, V., Dennefeld, M., Magaña-Sandoval, F., Cominsky, L. R., Gal-Yam, A., Buchanan, C. C., Costanza, F., Cuoco, A., D'AMMANDO, FILIPPO, de Palma, F., Desiante, R., Digel, S. W., Tse, M., Di Lalla, N., Di Mauro, M., Magee, R. M., Jonker, P. G., PESSTO Collaboration, Wang, Ch., Di Venere, L., Domínguez, A., Agathos, M., Buikema, A., Turconi, M., Drell, P. S., Dubois, R., Favuzzi, C., Ferrara, E. C., Franckowiak, A., Ćwiek, A., Mageswaran, M., Fukazawa, Y., Hiriart, D., Funk, S., Thaler, J., Fusco, P., Gargano, F., Gasparrini, D., Bulik, T., Giglietto, N., Giommi, P., Aguiar, O. D., Giordano, F., Barta, D., Giroletti, M., Tuyenbayev, D., Glanzman, T., Lee, W. H., Godfrey, G., Gomez-Vargas, G. A., Green, D., Grenier, I. A., Grove, J. E., Mavalvala, N., Bulten, H. J., Guiriec, S., Libson, A., Melchior, P., Hadasch, D., Harding, A. K., Hays, E., Claret, A., Hewitt, J. W., Hill, A. B., Horan, D., Cesarini, E., Jogler, T., Ugolini, D., Jóhannesson, G., Johnson, A. S., Majorana, E., Buonanno, A., Kensei, S., Kocevski, D., Kuss, M., Sánchez-Ramírez, R., La Mura, G., Ćwiok, M., Unnikrishnan, C. S., Larsson, S., Latronico, L., Li, J., Li, L., Maksimovic, I., Longo, F., Loparco, F., Buskulic, D., Lovellette, M. N., Lubrano, P., Blair, D. G., Mankiewicz, L., Pandey, S. B., Magill, J., Maldera, S., Manfreda, A., MARELLI, MARTINO, Malvezzi, V., Mayer, M., Mazziotta, M. N., McEnery, J. E., Urban, A. L., Meyer, M., Opiela, R., Buy, C., Michelson, P. F., Mediavilla, T., Mirabal, N., Mizuno, T., Moiseev, A. A., Man, N., Monzani, M. E., Usman, S. A., Moretti, E., Morselli, A., Diehl, H. T., Moskalenko, I. V., Negro, M., Nuss, E., Byer, R. L., Sabau-Graziati, L., Ohsugi, T., Omodei, N., Anderson, J. P., Mandel, I., Orienti, M., Orlando, E., Zaremba, M., Ormes, J. F., Paneque, D., Perkins, J. S., Pesce-Rollins, M., Piron, F., Pivato, G., Vahlbruch, H., BOOTES Collaboration, Cadonati, L., Mandic, V., Porter, T. A., Rowlinson, A., Żarnecki, A. F., Racusin, J. L., Rainò, S., Rando, R., Razzaque, S., Vajente, G., Reimer, A., Reimer, O., Salvetti, D., Saz Parkinson, P. M., Abbott, T. M. C., Mangano, V., Pi of Sky Collaboration, Sgrò, C., Cagnoli, G., Simone, D., Valdes, G., Siskind, E. J., Spada, F., Spandre, G., Spinelli, P., Suson, D. J., Tajima, H., Thayer, J. B., Onken, C. A., Mansell, G. L., Bose, S., van Bakel, N., Thompson, D. J., Tibaldo, L., Cahillane, C., Torres, D. F., Troja, E., Uchiyama, Y., Venters, T. M., Vianello, G., Scalzo, R. A., Wood, K. S., Brinkmann, M., Manske, M., Wood, M., Abdalla, F. B., Zhu, S., Zimmer, S., Fermi LAT Collaboration, Agatsuma, K., Bustillo, J. C., BROCATO, Enzo, Mazumder, N., Littenberg, T. B., CAPPELLARO, Enrico, COVINO, Stefano, Mantovani, M., GRADO, ANIELLO, NICASTRO, LUCIANO, Allam, S., PALAZZI, ELIANA, PIAN, Elena, AMATI, LORENZO, ANTONELLI, Lucio Angelo, van Beuzekom, M., Schmidt, B. P., Capaccioli, M., Callister, T., D'AVANZO, Paolo, Metzger, B. D., D'Elia, V., GETMAN, FEDOR, Giuffrida, G., Annis, J., Iannicola, G., van den Brand, J. F. J., Limatola, L., Wolf, C., LISI, Massimiliano, MARINONI, SILVIA, MARRESE, Paola Maria, MELANDRI, Andrea, Barthelmy, S., Calloni, E., PIRANOMONTE, Silvia, POSSENTI, ANDREA, Van Den Broeck, C., PULONE, Luigi, Armstrong, R., Chakraborty, R., ROSSI, Andrea, STAMERRA, Antonio, Stella, L., Testa, V., TOMASELLA, Lina, Marchesoni, F., Yang, S., Vander-Hyde, D. C., GRAvitational Wave Inaf TeAm (GRAWITA), Camp, J. B., Bazzano, A., Yuan, F., Bozzo, E., Benoit-Lévy, A., Brandt, S., Courvoisier, T. J. -L., Ferrigno, C., Hanlon, L., BOTTICELLA, MARIA TERESA, Marion, F., Kuulkers, E., Laurent, P., MEREGHETTI, Sandro, SkyMapper Collaboration, Roques, J. P., Cannon, K. C., Savchenko, V., Berger, E., Ubertini, P., Blair, R. M., INTEGRAL Collaboration, Kasliwal, M. M., Márka, S., Singer, L. P., Cao, Y., Stappers, B. W., Dietrich, J. P., Duggan, G., Kulkarni, S. R., Bhalerao, V., van der Schaaf, L., Miller, A. A., Cao, J., Bernstein, R. A., Barlow, T., Bellm, E., Márka, Z., Manulis, I., Evans, P. A., Rana, J., Laher, R., van Heijningen, J. V., Masci, F., Surace, J., Rebbapragada, U., Van Sistine, A., Sesar, B., Bertin, E., Capano, C. D., Markosyan, A. S., Kennea, J. A., Perley, D., van Veggel, A. A., Ferreti, R., Prince, T., Kendrick, R., Horesh, A., Intermediate Palomar Transient Factory (iPTF Collaboration), Hurley, K., Golenetskii, S. V., Aptekar, R. L., Brout, D., Burrows, D. N., Vardaro, M., Maros, E., Frederiks, D. D., Capocasa, E., Svinkin, D. S., Rau, A., Zhang, X., Smith, D. M., Cline, T., Krimm, H., InterPlanetary Network, Vass, S., CAMPANA, Sergio, Abe, F., Martelli, F., Buckley-Geer, E., Doi, M., Fujisawa, K., Carbognani, F., Kawabata, K. S., Morokuma, T., Motohara, K., Lockerbie, N. A., Tanaka, M., Bartos, I., Ohta, K., Yanagisawa, K., Martellini, L., Yoshida, M., Bouffanais, Y., J-GEM Collaboration, Baltay, C., Rabinowitz, D., Thomas, D., Caride, S., Ellman, N., Cenko, S. B., Rostami, S., La Silla-QUEST Survey, Bersier, D. F., Martin, I. W., Bode, M. F., Collins, C. A., Burke, D. L., Vasúth, M., Copperwheat, C. M., Darnley, M. J., Galloway, D. K., Marshall, F. E., Gomboc, A., Aggarwal, N., Diaz, J. C., Kobayashi, S., Miller, C. J., Mazzali, P., Vaulin, R., Mundell, C. G., Piascik, A. S., Capozzi, D., Pollacco, Don, Nousek, J., Steele, I. A., Ulaczyk, K., Liverpool Telescope Collaboration, Broderick, J. W., Fender, R. P., Baiardi, L. C., O'Brien, P., Carretero, J., Chalermsongsak, T., Osborne, J. P., Doctor, Z., Palmer, D., PERRI, Matteo, Siegel, M., Mazzolo, G., TAGLIAFERRI, Gianpiero, Vecchio, A., Swift Collaboration, Klotz, A., Wijers, R. A. M. J., Turpin, D., Laugier, R., TAROT Collaboration, Chamberlin, S. J., Drlica-Wagner, A., Zadko Collaboration, Algerian National Observatory, Algerian Collaboration, Vedovato, G., McCarthy, R., C2PU Collaboration, Beroiz, M., Low Frequency Array (LOFAR Collaboration), Peñuela, T., Macri, L. M., Oelkers, R. J., Lambas, D. G., Vrech, R., Cabral, J., Veitch, J., Drout, M. R., Chan, M., McClelland, D. E., Colazo, C., Lipunov, V., Dominguez, M., Sanchez, B., Gurovich, S., Lares, M., Marshall, J. L., Bloemen, S., DePoy, D. L., Padilla, N., Pereyra, N. A., Eifler, T. F., McCormick, S., Gorbovskoy, E., Benacquista, M., Chao, S., TOROS Collaboration, Tanvir, N. R., Veitch, P. J., Wiersema, K., Levan, A. J., Steeghs, D., Hjorth, J., Fynbo, J. P. U., Malesani, D., Tyurina, N., McGuire, S. C., Estrada, J., Milvang-Jensen, B., Venkateswara, K., Watson, D., Charlton, P., Irwin, M., Fernandez, C. G., McMahon, R. G., Banerji, M., Gonzalez-Solares, E., Bartlett, J., Schulze, S., McIntyre, G., Verkindt, D., de Ugarte Postigo, A., Evrard, A. E., Thoene, C. C., Cano, Z., Rosswog, S., Chassande-Mottin, E., VISTA Collaboration, ASCENZI, STEFANO, Kornilov, V., Barsotti, L., MANGANO, VALERIA, Kowalska, I., McIver, J., MUKHERJEE, DIPANJAN, SALEMI, Filippo, Fernandez, E., SANCHEZ RAMIREZ, RUBEN, DI MAURO, Maria Giuseppina, GIROLETTI, MARCELLO, Balanutsa, P., Vetrano, F., Chen, H. Y., ORIENTI, Monica, Bork, R., STELLA, Luigi, Bradaschia, C., TESTA, Vincenzo, BAZZANO, ANGELA, Chen, Y., Caudill, S., Thomas, R. C., Aiello, L., Cheng, C., Chincarini, A., Chiummo, A., Brau, J. E., Cho, H. S., Cho, M., Chow, J. H., Finley, D. A., Christensen, N., Chen, T. -W., Kuznetsov, A., Chu, Q., Chua, S., Chung, S., Ain, A., Ciani, G., McManus, D. J., Clara, F., Clark, J. A., Cleva, F., Viceré, A., Coccia, E., Buckley, D., Flaugher, B., Cohadon, P. -F., Colla, A., Collette, C. G., Cominsky, L., Constancio, M., Jr., McWilliams, S. T., Ajith, P., Vinciguerra, S., Conte, A., Conti, L., Castander, F. J., Cook, D., Corbitt, T. R., Foley, R. J., Cornish, N., Corsi, A., Cortese, S., Costa, C. A., Vine, D. J., Meacher, D., Coughlin, M. W., Coughlin, S. B., Rebolo, R., Allen, B., Coulon, J. -P., Countryman, S. T., Couvares, P., Fong, W. -F., Cowan, E. E., Vinet, J. -Y., Coward, D. M., Cowart, M. J., Bassiri, R., Coyne, D. C., Serra-Ricart, M., Coyne, R., Craig, K., Creighton, J. D. E., Allocca, A., Cripe, J., Vitale, S., Crowder, S. G., Fosalba, P., Cumming, A., Cunningham, L., Meadors, G. D., Israelian, G., Cuoco, E., Dal Canton, T., Danilishin, S. L., D'Antonio, S., Vo, T., Danzmann, K., Darman, N. S., Altin, P. A., Dattilo, V., Fox, D. B., Dave, I., Budnev, N. M., Meidam, J., Daveloza, H. P., Davier, M., Bock, O., Davies, G. S., Daw, E. J., Day, R., DeBra, D., Debreczeni, G., Degallaix, J., Anderson, S. B., Martynov, D. V., Frieman, J., Melatos, A., Vocca, H., De Laurentis, M., Deléglise, S., Del Pozzo, W., Denker, T., Dent, T., Dereli, H., Dergachev, V., DeRosa, R. T., Gress, O., De Rosa, R., Logue, J., DeSalvo, R., Kozak, D. B., Mendell, G., Fryer, C. L., Anderson, W. G., Dhurandhar, S., Díaz, M. C., Di Fiore, L., Di Giovanni, M., Ivanov, K., Vorvick, C., Di Lieto, A., Di Pace, S., Di Palma, I., Di Virgilio, A., Mendoza-Gandara, D., Dojcinoski, G., Gaztanaga, E., Dolique, V., Arai, K., Donovan, F., DELLA VALLE, Massimo, Poleshuk, V., Dooley, K. L., Doravari, S., Douglas, R., Downes, T. P., Drago, M., Mercer, R. A., Drever, R. W. P., Driggers, J. C., Gerdes, D. W., Voss, D., Du, Z., Tlatov, A., Ducrot, M., Araya, M. C., Dwyer, S. E., Edo, T. B., Edwards, M. C., Effler, A., Neilsen, E., Eggenstein, H. -B., Tucker, D. L., Ehrens, P., Eichholz, J., Cavagliá, M., Brady, P. R., Eikenberry, S. S., Engels, W., Essick, R. C., Arceneaux, C. C., Etzel, T., Evans, M., Vousden, W. D., Merilh, E., Evans, T. M., Everett, R., Yurkov, V., Factourovich, M., Fafone, V., Goldstein, D. A., Fair, H., Fairhurst, S., Fan, X., Vyatchanin, S. P., Fang, Q., Areeda, J. S., Merzougui, M., Farinon, S., Chornock, R., Farr, B., Farr, W. M., Favata, M., Fays, M., Gruen, D., Wade, A. R., Fehrmann, H., Fejer, M. M., Ferrante, I., Ferreira, E. C., Meshkov, S., MASTER Collaboration, Ferrini, F., Arnaud, N., Fidecaro, F., Fiori, I., Wade, L. E., Fiorucci, D., Fisher, R. P., Gruendl, R. A., Flaminio, R., Fletcher, M., Fournier, J. -D., Kawai, N., Messenger, C., Franco, S., Frasca, S., Wade, M., Frasconi, F., Arun, K. G., Frei, Z., Freise, A., Frey, R., Gutierrez, G., Frey, V., Serino, M., Fricke, T. T., Basti, A., Walker, M., Fritschel, P., Frolov, V. V., Fulda, P., Fyffe, M., Gabbard, H. A. G., Ascenzi, S., Gair, J. R., Gammaitoni, L., Marx, J. N., Herner, K., Wallace, L., Gaonkar, S. G., Messick, C., Garufi, F., Gatto, A., Gaur, G., Gehrels, N., Gemme, G., Gendre, B., Genin, E., Negoro, H., Lombardi, A. L., Ashton, G., Gennai, A., Honscheid, K., Kringel, V., Meyers, P. M., George, J., Gergely, L., Germain, V., Ghosh, A., Ghosh, S., ELIAS DE LA ROSA, NANCY DEL CARMEN, Nakahira, S., Giaime, J. A., Giardina, K. D., Giazotto, A., Gill, K., Ast, M., Mezzani, F., James, D. J., Glaefke, A., and Goetz, E.
Abstract: This Supplement provides supporting material for Abbott et al. (2016a). We briefly summarize past electromagnetic (EM) follow-up efforts as well as the organization and policy of the current EM follow-up program. We compare the four probability sky maps produced for the gravitational-wave transient GW150914, and provide additional details of the EM follow-up observations that were performed in the different bands.
Published: 2016

26. Illuminating the past 8 billion years of cold gas towards two gravitationally lensed quasars

Author: Allison, J. R., primary, Moss, V. A., additional, Macquart, J.-P., additional, Curran, S. J., additional, Duchesne, S. W., additional, Mahony, E. K., additional, Sadler, E. M., additional, Whiting, M. T., additional, Bannister, K. W., additional, Chippendale, A. P., additional, Edwards, P. G., additional, Harvey-Smith, L., additional, Heywood, I., additional, Indermuehle, B. T., additional, Lenc, E., additional, Marvil, J., additional, McConnell, D., additional, and Sault, R. J., additional
Published: 2016
Full Text: View/download PDF

27. The radio spectral energy distribution of infrared-faint radio sources

Author: Herzog, A., primary, Norris, R. P., additional, Middelberg, E., additional, Seymour, N., additional, Spitler, L. R., additional, Emonts, B. H. C., additional, Franzen, T. M. O., additional, Hunstead, R., additional, Intema, H. T., additional, Marvil, J., additional, Parker, Q. A., additional, Sirothia, S. K., additional, Hurley-Walker, N., additional, Bell, M., additional, Bernardi, G., additional, Bowman, J. D., additional, Briggs, F., additional, Cappallo, R. J., additional, Callingham, J. R., additional, Deshpande, A. A., additional, Dwarakanath, K. S., additional, For, B.-Q., additional, Greenhill, L. J., additional, Hancock, P., additional, Hazelton, B. J., additional, Hindson, L., additional, Johnston-Hollitt, M., additional, Kapińska, A. D., additional, Kaplan, D. L., additional, Lenc, E., additional, Lonsdale, C. J., additional, McKinley, B., additional, McWhirter, S. R., additional, Mitchell, D. A., additional, Morales, M. F., additional, Morgan, E., additional, Morgan, J., additional, Oberoi, D., additional, Offringa, A., additional, Ord, S. M., additional, Prabu, T., additional, Procopio, P., additional, Udaya Shankar, N., additional, Srivani, K. S., additional, Staveley-Smith, L., additional, Subrahmanyan, R., additional, Tingay, S. J., additional, Wayth, R. B., additional, Webster, R. L., additional, Williams, A., additional, Williams, C. L., additional, Wu, C., additional, Zheng, Q., additional, Bannister, K. W., additional, Chippendale, A. P., additional, Harvey-Smith, L., additional, Heywood, I., additional, Indermuehle, B., additional, Popping, A., additional, Sault, R. J., additional, and Whiting, M. T., additional
Published: 2016
Full Text: View/download PDF

28. High-velocity OH megamasers in IRAS 20100−4156: evidence for a supermassive black hole

Author: Harvey-Smith, L., primary, Allison, J. R., additional, Green, J. A., additional, Bannister, K. W., additional, Chippendale, A., additional, Edwards, P. G., additional, Heywood, I., additional, Hotan, A. W., additional, Lenc, E., additional, Marvil, J., additional, McConnell, D., additional, Phillips, C. J., additional, Sault, R. J., additional, Serra, P., additional, Stevens, J., additional, Voronkov, M., additional, and Whiting, M., additional
Published: 2016
Full Text: View/download PDF

29. Wide-field broad-band radio imaging with phased array feeds: a pilot multi-epoch continuum survey with ASKAP-BETA

Author: Heywood, I., primary, Bannister, K. W., additional, Marvil, J., additional, Allison, J. R., additional, Ball, L., additional, Bell, M. E., additional, Bock, D. C.-J., additional, Brothers, M., additional, Bunton, J. D., additional, Chippendale, A. P., additional, Cooray, F., additional, Cornwell, T. J., additional, De Boer, D., additional, Edwards, P., additional, Gough, R., additional, Gupta, N., additional, Harvey-Smith, L., additional, Hay, S., additional, Hotan, A. W., additional, Indermuehle, B., additional, Jacka, C., additional, Jackson, C. A., additional, Johnston, S., additional, Kimball, A. E., additional, Koribalski, B. S., additional, Lenc, E., additional, Macleod, A., additional, McClure-Griffiths, N., additional, McConnell, D., additional, Mirtschin, P., additional, Murphy, T., additional, Neuhold, S., additional, Norris, R. P., additional, Pearce, S., additional, Popping, A., additional, Qiao, R. Y., additional, Reynolds, J. E., additional, Sadler, E. M., additional, Sault, R. J., additional, Schinckel, A. E. T., additional, Serra, P., additional, Shimwell, T. W., additional, Stevens, J., additional, Tuthill, J., additional, Tzioumis, A., additional, Voronkov, M. A., additional, Westmeier, T., additional, and Whiting, M. T., additional
Published: 2016
Full Text: View/download PDF

30. Tracing the neutral gas environments of young radio AGN with ASKAP

Author: Allison, J.R., primary, Sadler, E.M., additional, Moss, V.A., additional, Harvey‐Smith, L., additional, Heywood, I., additional, Indermuehle, B.T., additional, McConnell, D., additional, Sault, R. J., additional, and Whiting, M. T., additional
Published: 2016
Full Text: View/download PDF

31. A pilot ASKAP survey of radio transient events in the region around the intermittent pulsar PSR J1107−5907

Author: Hobbs, G., primary, Heywood, I., additional, Bell, M. E., additional, Kerr, M., additional, Rowlinson, A., additional, Johnston, S., additional, Shannon, R. M., additional, Voronkov, M. A., additional, Ward, C., additional, Banyer, J., additional, Hancock, P. J., additional, Murphy, Tara, additional, Allison, J. R., additional, Amy, S. W., additional, Ball, L., additional, Bannister, K., additional, Bock, D. C.-J., additional, Brodrick, D., additional, Brothers, M., additional, Brown, A. J., additional, Bunton, J. D., additional, Chapman, J., additional, Chippendale, A. P., additional, Chung, Y., additional, DeBoer, D., additional, Diamond, P., additional, Edwards, P. G., additional, Ekers, R., additional, Ferris, R. H., additional, Forsyth, R., additional, Gough, R., additional, Grancea, A., additional, Gupta, N., additional, Harvey-Smith, L., additional, Hay, S., additional, Hayman, D. B., additional, Hotan, A. W., additional, Hoyle, S., additional, Humphreys, B., additional, Indermuehle, B., additional, Jacka, C. E., additional, Jackson, C. A., additional, Jackson, S., additional, Jeganathan, K., additional, Joseph, J, additional, Kendall, R., additional, Kiraly, D., additional, Koribalski, B., additional, Leach, M., additional, Lenc, E., additional, MacLeod, A., additional, Mader, S., additional, Marquarding, M., additional, Marvil, J., additional, McClure-Griffiths, N., additional, McConnell, D., additional, Mirtschin, P., additional, Neuhold, S., additional, Ng, A., additional, Norris, R. P., additional, O'Sullivan, J., additional, Pearce, S., additional, Phillips, C. J., additional, Popping, A., additional, Qiao, R. Y., additional, Reynolds, J. E., additional, Roberts, P., additional, Sault, R. J., additional, Schinckel, A. E. T., additional, Serra, P., additional, Shaw, R., additional, Shimwell, T. W., additional, Storey, M., additional, Sweetnam, A. W., additional, Tzioumis, A., additional, Westmeier, T., additional, Whiting, M., additional, and Wilson, C. D., additional
Published: 2016
Full Text: View/download PDF

32. The Australian Square Kilometre Array Pathfinder: Performance of the Boolardy Engineering Test Array

Author: McConnell, D., primary, Allison, J. R., additional, Bannister, K., additional, Bell, M. E., additional, Bignall, H. E., additional, Chippendale, A. P., additional, Edwards, P. G., additional, Harvey-Smith, L., additional, Hegarty, S., additional, Heywood, I., additional, Hotan, A. W., additional, Indermuehle, B. T., additional, Lenc, E., additional, Marvil, J., additional, Popping, A., additional, Raja, W., additional, Reynolds, J. E., additional, Sault, R. J., additional, Serra, P., additional, Voronkov, M. A., additional, Whiting, M., additional, Amy, S. W., additional, Axtens, P., additional, Ball, L., additional, Bateman, T. J., additional, Bock, D. C.-J., additional, Bolton, R., additional, Brodrick, D., additional, Brothers, M., additional, Brown, A. J., additional, Bunton, J. D., additional, Cheng, W., additional, Cornwell, T., additional, DeBoer, D., additional, Feain, I., additional, Gough, R., additional, Gupta, N., additional, Guzman, J. C., additional, Hampson, G. A., additional, Hay, S., additional, Hayman, D. B., additional, Hoyle, S., additional, Humphreys, B., additional, Jacka, C., additional, Jackson, C. A., additional, Jackson, S., additional, Jeganathan, K., additional, Joseph, J., additional, Koribalski, B. S., additional, Leach, M., additional, Lensson, E. S., additional, MacLeod, A., additional, Mackay, S., additional, Marquarding, M., additional, McClure-Griffiths, N. M., additional, Mirtschin, P., additional, Mitchell, D., additional, Neuhold, S., additional, Ng, A., additional, Norris, R., additional, Pearce, S., additional, Qiao, R. Y., additional, Schinckel, A. E. T., additional, Shields, M., additional, Shimwell, T. W., additional, Storey, M., additional, Troup, E., additional, Turner, B., additional, Tuthill, J., additional, Tzioumis, A., additional, Wark, R. M., additional, Westmeier, T., additional, Wilson, C., additional, and Wilson, T., additional
Published: 2016
Full Text: View/download PDF

33. Erratum: Discovery of H i gas in a young radio galaxy at $\boldsymbol {z = 0.44}$ using the Australian Square Kilometre Array Pathfinder

Author: Allison, J. R., primary, Sadler, E. M., additional, Moss, V. A., additional, Whiting, M. T., additional, Hunstead, R. W., additional, Pracy, M. B., additional, Curran, S. J., additional, Croom, S. M., additional, Glowacki, M., additional, Morganti, R., additional, Shabala, S. S., additional, Zwaan, M. A., additional, Allen, G., additional, Amy, S. W., additional, Axtens, P., additional, Ball, L., additional, Bannister, K. W., additional, Barker, S., additional, Bell, M. E., additional, Bock, D. C.-J., additional, Bolton, R., additional, Bowen, M., additional, Boyle, B., additional, Braun, R., additional, Broadhurst, S., additional, Brodrick, D., additional, Brothers, M., additional, Brown, A., additional, Bunton, J. D., additional, Cantrall, C., additional, Chapman, J., additional, Cheng, W., additional, Chippendale, A. P., additional, Chung, Y., additional, Cooray, F., additional, Cornwell, T., additional, DeBoer, D., additional, Diamond, P., additional, Edwards, P. G., additional, Ekers, R., additional, Feain, I., additional, Ferris, R. H., additional, Forsyth, R., additional, Gough, R., additional, Grancea, A., additional, Gupta, N., additional, Guzman, J. C., additional, Hampson, G., additional, Harvey-Smith, L., additional, Haskins, C., additional, Hay, S., additional, Hayman, D. B., additional, Heywood, I., additional, Hotan, A. W., additional, Hoyle, S., additional, Humphreys, B., additional, Indermuehle, B. T., additional, Jacka, C., additional, Jackson, C., additional, Jackson, S., additional, Jeganathan, K., additional, Johnston, S., additional, Joseph, J., additional, Kendall, R., additional, Kesteven, M., additional, Kiraly, D., additional, Koribalski, B. S., additional, Leach, M., additional, Lenc, E., additional, Lensson, E., additional, Mackay, S., additional, Macleod, A., additional, Marquarding, M., additional, Marvil, J., additional, McClure-Griffiths, N., additional, McConnell, D., additional, Mirtschin, P., additional, Norris, R. P., additional, Neuhold, S., additional, Ng, A., additional, O'Sullivan, J., additional, Pathikulangara, J., additional, Pearce, S., additional, Phillips, C., additional, Popping, A., additional, Qiao, R. Y., additional, Reynolds, J. E., additional, Roberts, P., additional, Sault, R. J., additional, Schinckel, A., additional, Serra, P., additional, Shaw, R., additional, Shields, M., additional, Shimwell, T., additional, Storey, M., additional, Sweetnam, T., additional, Troup, E., additional, Turner, B., additional, Tuthill, J., additional, Tzioumis, A., additional, Voronkov, M. A., additional, Westmeier, T., additional, and Wilson, C. D., additional
Published: 2015
Full Text: View/download PDF

34. Discovery of H i gas in a young radio galaxy at z = 0.44 using the Australian Square Kilometre Array Pathfinder

Author: Allison, J. R., primary, Sadler, E. M., additional, Moss, V. A., additional, Whiting, M. T., additional, Hunstead, R. W., additional, Pracy, M. B., additional, Curran, S. J., additional, Croom, S. M., additional, Glowacki, M., additional, Morganti, R., additional, Shabala, S. S., additional, Zwaan, M. A., additional, Allen, G., additional, Amy, S. W., additional, Axtens, P., additional, Ball, L., additional, Bannister, K. W., additional, Barker, S., additional, Bell, M. E., additional, Bock, D. C.-J., additional, Bolton, R., additional, Bowen, M., additional, Boyle, B., additional, Braun, R., additional, Broadhurst, S., additional, Brodrick, D., additional, Brothers, M., additional, Brown, A., additional, Bunton, J. D., additional, Cantrall, C., additional, Chapman, J., additional, Cheng, W., additional, Chippendale, A. P., additional, Chung, Y., additional, Cooray, F., additional, Cornwell, T., additional, DeBoer, D., additional, Diamond, P., additional, Edwards, P. G., additional, Ekers, R., additional, Feain, I., additional, Ferris, R. H., additional, Forsyth, R., additional, Gough, R., additional, Grancea, A., additional, Gupta, N., additional, Guzman, J. C., additional, Hampson, G., additional, Harvey-Smith, L., additional, Haskins, C., additional, Hay, S., additional, Hayman, D. B., additional, Heywood, I., additional, Hotan, A. W., additional, Hoyle, S., additional, Humphreys, B., additional, Indermuehle, B. T., additional, Jacka, C., additional, Jackson, C., additional, Jackson, S., additional, Jeganathan, K., additional, Johnston, S., additional, Joseph, J., additional, Kendall, R., additional, Kesteven, M., additional, Kiraly, D., additional, Koribalski, B. S., additional, Leach, M., additional, Lenc, E., additional, Lensson, E., additional, Mackay, S., additional, Macleod, A., additional, Marquarding, M., additional, Marvil, J., additional, McClure-Griffiths, N., additional, McConnell, D., additional, Mirtschin, P., additional, Norris, R. P., additional, Neuhold, S., additional, Ng, A., additional, O'Sullivan, J., additional, Pathikulangara, J., additional, Pearce, S., additional, Phillips, C., additional, Popping, A., additional, Qiao, R. Y., additional, Reynolds, J. E., additional, Roberts, P., additional, Sault, R. J., additional, Schinckel, A., additional, Serra, P., additional, Shaw, R., additional, Shields, M., additional, Shimwell, T., additional, Storey, M., additional, Sweetnam, T., additional, Troup, E., additional, Turner, B., additional, Tuthill, J., additional, Tzioumis, A., additional, Voronkov, M. A., additional, Westmeier, T., additional, and Wilson, C. D., additional
Published: 2015
Full Text: View/download PDF

35. ASKAP H i imaging of the galaxy group IC 1459

Author: Serra, P., primary, Koribalski, B., additional, Kilborn, V., additional, Allison, J. R., additional, Amy, S. W., additional, Ball, L., additional, Bannister, K., additional, Bell, M. E., additional, Bock, D. C.-J., additional, Bolton, R., additional, Bowen, M., additional, Boyle, B., additional, Broadhurst, S., additional, Brodrick, D., additional, Brothers, M., additional, Bunton, J. D., additional, Chapman, J., additional, Cheng, W., additional, Chippendale, A. P., additional, Chung, Y., additional, Cooray, F., additional, Cornwell, T., additional, DeBoer, D., additional, Diamond, P., additional, Forsyth, R., additional, Gough, R., additional, Gupta, N., additional, Hampson, G. A., additional, Harvey-Smith, L., additional, Hay, S., additional, Hayman, D. B., additional, Heywood, I., additional, Hotan, A. W., additional, Hoyle, S., additional, Humphreys, B., additional, Indermuehle, B., additional, Jacka, C., additional, Jackson, C. A., additional, Jackson, S., additional, Jeganathan, K., additional, Johnston, S., additional, Joseph, J., additional, Kamphuis, P., additional, Leach, M., additional, Lenc, E., additional, Lensson, E., additional, Mackay, S., additional, Marquarding, M., additional, Marvil, J., additional, McClure-Griffiths, N., additional, McConnell, D., additional, Meyer, M., additional, Mirtschin, P., additional, Neuhold, S., additional, Ng, A., additional, Norris, R. P., additional, O'Sullivan, J., additional, Pathikulangara, J., additional, Pearce, S., additional, Phillips, C., additional, Popping, A., additional, Qiao, R. Y., additional, Reynolds, J. E., additional, Roberts, P., additional, Sault, R. J., additional, Schinckel, A. E. T., additional, Shaw, R., additional, Shimwell, T. W., additional, Staveley-Smith, L., additional, Storey, M., additional, Sweetnam, A. W., additional, Troup, E., additional, Tzioumis, A., additional, Voronkov, M. A., additional, Westmeier, T., additional, Whiting, M., additional, Wilson, C., additional, Wong, O. I., additional, and Wu, X., additional
Published: 2015
Full Text: View/download PDF

36. The Murchison Widefield Array Correlator

Author: Ord, S. M., primary, Crosse, B., additional, Emrich, D., additional, Pallot, D., additional, Wayth, R. B., additional, Clark, M. A., additional, Tremblay, S. E., additional, Arcus, W., additional, Barnes, D., additional, Bell, M., additional, Bernardi, G., additional, Bhat, N. D. R., additional, Bowman, J. D., additional, Briggs, F., additional, Bunton, J. D., additional, Cappallo, R. J., additional, Corey, B. E., additional, Deshpande, A. A., additional, deSouza, L., additional, Ewell-Wice, A., additional, Feng, L., additional, Goeke, R., additional, Greenhill, L. J., additional, Hazelton, B. J., additional, Herne, D., additional, Hewitt, J. N., additional, Hindson, L., additional, Hurley-Walker, N., additional, Jacobs, D., additional, Johnston-Hollitt, M., additional, Kaplan, D. L., additional, Kasper, J. C., additional, Kincaid, B. B., additional, Koenig, R., additional, Kratzenberg, E., additional, Kudryavtseva, N., additional, Lenc, E., additional, Lonsdale, C. J., additional, Lynch, M. J., additional, McKinley, B., additional, McWhirter, S. R., additional, Mitchell, D. A., additional, Morales, M. F., additional, Morgan, E., additional, Oberoi, D., additional, Offringa, A., additional, Pathikulangara, J., additional, Pindor, B., additional, Prabu, T., additional, Procopio, P., additional, Remillard, R. A., additional, Riding, J., additional, Rogers, A. E. E., additional, Roshi, A., additional, Salah, J. E., additional, Sault, R. J., additional, Udaya Shankar, N., additional, Srivani, K. S., additional, Stevens, J., additional, Subrahmanyan, R., additional, Tingay, S. J., additional, Waterson, M., additional, Webster, R. L., additional, Whitney, A. R., additional, Williams, A., additional, Williams, C. L., additional, and Wyithe, J. S. B., additional
Published: 2015
Full Text: View/download PDF

37. Illuminating the past 8 billion years of cold gas towards two gravitationally lensed quasars.

Author: Allison, J. R., Moss, V. A., Macquart, J.-P., Curran, S. J., Duchesne, S. W., Mahony, E. K., Sadler, E. M., Whiting, M. T., Bannister, K. W., Chippendale, A. P., Edwards, P. G., Harvey-Smith, L., Heywood, I., Indermuehle, B. T., Lenc, E., Marvil, J., McConnell, D., and Sault, R. J.
Subjects: COLD gases, GRAVITATIONAL lenses, QUASARS, ABSORPTION, RADIO interference
Abstract: Using the Boolardy Engineering Test Array of the Australian Square Kilometre Array Pathfinder (ASKAP BETA), we have carried out the first z = 0-1 survey for H I and OH absorption towards the gravitationally lensed quasars PKS B1830-211 and MG J0414+0534. Although we detected all previously reported intervening systems towards PKS B1830-211, in the case of MG J0414+0534, three systems were not found, indicating that the original identifications may have been confused with radio frequency interference. Given the sensitivity of our data, we find that our detection yield is consistent with the expected frequency of intervening H I systems estimated from previous surveys for 21-cm emission in nearby galaxies and z - 3 damped Lyman α absorbers. We find spectral variability in the z = 0.886 face-on spiral galaxy towards PKS B1830-211 from observations undertaken with the Westerbork Synthesis Radio Telescope in 1997/1998 and ASKAP BETA in 2014/2015. The H I equivalent width varies by a few per cent over approximately yearly time-scales. This long-term spectral variability is correlated between the north-east and south-west images of the core, and with the total flux density of the source, implying that it is observationally coupled to intrinsic changes in the quasar. The absence of any detectable variability in the ratio of H I associated with the two core images is in stark contrast to the behaviour previously seen in the molecular lines. We therefore infer that coherent opaque H I structures in this galaxy are larger than the parsec-scale molecular clouds found at mm-wavelengths. [ABSTRACT FROM AUTHOR]
Published: 2017
Full Text: View/download PDF

38. VLA MULTI-WAVELENGTH MICROWAVE OBSERVATIONS OF SATURN'S C AND B RINGS.

Author: Zhang, Z., Hayes, A. G., de Pater, I., Dunn, D. E., Janssen, M. A., Nicholson, P. D., Cuzzi, J. N., Butler, B. J., Sault, R. J., and Chatterjee, S.
Subjects: WAVELENGTHS, RINGS of Saturn
Published: 2017

39. LOCALIZATION AND BROADBAND FOLLOW-UP OF THE GRAVITATIONAL-WAVE TRANSIENT GW 150914

Author: Abbott1, B. P., Abbott1, R., Abbott2, T. D., Abernathy1, M. R., Acernese3, F., 4, Ackley5, K., Adams6, C., Adams7, T., Addesso3, P., Adhikari1, R. X., Adya8, V. B., Affeldt8, C., Agathos9, M., Agatsuma9, K., Aggarwal10, N., Aguiar11, O. D., Aiello12, L., Ain14, A., Ajith15, P., Allen8, B., 17, 16, Allocca18, A., Altin20, P. A., Anderson1, S. B., Anderson16, W. G., Arai1, K., Araya1, M. C., Arceneaux21, C. C., Areeda22, J. S., Arnaud23, N., Arun24, K. G., Ascenzi13, S., Ashton26, G., Ast27, M., Aston6, S. M., Astone28, P., Aufmuth8, P., Aulbert8, C., Babak29, S., Bacon30, P., Bader9, M. K. M., Baker31, P. T., Baldaccini32, F., Ballardin34, G., Ballmer35, S. W., Barayoga1, J. C., Barclay36, S. E., Barish1, B. C., Barker37, D., Barone3, F., Barr36, B., Barsotti10, L., Barsuglia30, M., Barta38, D., Barthelmy39, S., Bartlett37, J., Bartos40, I., Bassiri41, R., Basti18, A., Batch37, J. C., Baune8, C., Bavigadda34, V., Bazzan42, M., Behnke29, B., Bejger44, M., Bell36, A. S., Bell36, C. J., Berger1, B. K., Bergman37, J., Bergmann8, G., Berry45, C. P. L., Bersanetti46, D., Bertolini9, A., Betzwieser6, J., Bhagwat35, S., Bhandare48, R., Bilenko49, I. A., Billingsley1, G., Birch6, J., Birney50, R., Biscans10, S., Bisht8, A., Bitossi34, M., Biwer35, C., Bizouard23, M. A., Blackburn1, J. K., Blair51, C. D., Blair51, D. G., Blair37, R. M., Bloemen52, S., Bock8, O., Bodiya10, T. P., Boer53, M., Bogaert53, G., Bogan8, C., Bohe29, A., Bojtos54, P., Bond45, C., Bondu55, F., Bonnand7, R., Boom9, B. A., Bork1, R., Boschi18, V., Bose14, S., Bouffanais30, Y., Bozzi34, A., Bradaschia19, C., Brady16, P. R., Braginsky49, V. B., Branchesi57, M., Brau59, J. E., Briant60, T., Brillet53, A., Brinkmann8, M., Brisson23, V., Brockill16, P., Brooks1, A. F., Brown35, D. A., Brown45, D. D., Brown10, N. M., Buchanan2, C. C., Buikema10, A., Bulik61, T., Bulten9, H. J., Buonanno29, A., Buskulic7, D., Buy30, C., Byer41, R. L., Cadonati64, L., Cagnoli65, G., Cahillane1, C., Bustillo64, J. C., Callister1, T., Calloni4, E., Camp39, J. B., Cannon69, K. C., Cao70, J., Capano8, C. D., Capocasa30, E., Carbognani34, F., Caride71, S., Diaz23, J. C., Casentini13, C., Caudill16, S., Cavagliá21, M., Cavalier23, F., Cavalieri34, R., Cella19, G., Cepeda1, C. B., Baiardi57, L. C., Cerretani18, G., Cesarini13, E., Chakraborty1, R., Chalermsongsak1, T., Chamberlin72, S. J., Chan36, M., Chao73, S., Charlton74, P., Chassande Mottin30, E., Chen75, H. Y., Chen76, Y., Cheng73, C., Chincarini47, A., Chiummo34, A., Cho77, H. S., Cho63, M., Chow20, J. H., Christensen78, N., Chu51, Q., Chua60, S., Chung51, S., Ciani5, G., Clara37, F., Clark64, J. A., Cleva53, F., Coccia12, E., 25, 13, Cohadon60, P. F., Colla28, A., Collette80, C. G., Cominsky81, L., M. Constancio J. r., 11, Conte28, A., Conti43, L., Cook37, D., Corbitt2, T. R., Cornish31, N., Corsi71, A., Cortese34, S., Costa11, C. A., Coughlin78, M. W., Coughlin82, S. B., Coulon53, J. P., Countryman40, S. T., Couvares1, P., Cowan64, E. E., Coward51, D. M., Cowart6, M. J., Coyne1, D. C., Coyne71, R., Craig36, K., Creighton16, J. D. E., Cripe2, J., Crowder83, S. G., Cumming36, A., Cunningham36, L., Cuoco34, E., Dal Canton8, T., Danilishin36, S. L., D'Antonio13, S., Danzmann8, K., Darman84, N. S., Dattilo34, V., Dave48, I., Daveloza85, H. P., Davier23, M., Davies36, G. S., Daw86, E. J., Day34, R., Debra41, D., Debreczeni38, G., Degallaix66, J., De Laurentis4, M., Deléglise60, S., Del Pozzo45, W., Denker8, T., Dent8, T., Dereli53, H., Dergachev1, V., Derosa6, R. T., De Rosa4, R., Desalvo87, R., Dhurandhar14, S., Díaz85, M. C., Di Fiore4, L., Di Giovanni28, M., Di Lieto18, A., Di Pace28, S., Di Palma8, I., Di Virgilio19, A., Dojcinoski88, G., Dolique66, V., Donovan10, F., Dooley21, K. L., Doravari6, S., 8, Douglas36, R., Downes16, T. P., Drago8, M., 90, 89, Drever1, R. W. P., Driggers37, J. C., Du70, Z., Ducrot7, M., Dwyer37, S. E., Edo86, T. B., Edwards78, M. C., Effler6, A., Eggenstein8, H. B., Ehrens1, P., Eichholz5, J., Eikenberry5, S. S., Engels76, W., Essick10, R. C., Etzel1, T., Evans10, M., Evans6, T. M., Everett72, R., Factourovich40, M., Fafone12, V., Fair35, H., Fairhurst91, S., Fan70, X., Fang51, Q., Farinon47, S., Farr75, B., Farr45, W. M., Favata88, M., Fays91, M., Fehrmann8, H., Fejer41, M. M., Ferrante18, I., Ferreira11, E. C., Ferrini34, F., Fidecaro18, F., Fiori34, I., Fiorucci30, D., Fisher35, R. P., Flaminio66, R., Fletcher36, M., Fournier53, J. D., Franco23, S., Frasca28, S., Frasconi19, F., Frei54, Z., Freise45, A., Frey59, R., Frey23, V., Fricke8, T. T., Fritschel10, P., Frolov6, V. V., Fulda5, P., Fyffe6, M., Gabbard21, H. A. G., Gair93, J. R., Gammaitoni32, L., Gaonkar14, S. G., Garufi4, F., Gatto30, A., Gaur94, G., Gehrels39, N., Gemme47, G., Gendre53, B., Genin34, E., Gennai19, A., George48, J., Gergely96, L., Germain7, V., Ghosh15, A., Ghosh9, S., Giaime2, J. A., 6, Giardina6, K. D., Giazotto19, A., Gill97, K., Glaefke36, A., Goetz98, E., Goetz5, R., Gondan54, L., González2, G., Castro18, J. M. G., Gopakumar99, A., Gordon36, N. A., Gorodetsky49, M. L., Gossan1, S. E., Gosselin34, M., Gouaty7, R., Graef36, C., Graff63, P. B., Granata66, M., Grant36, A., Gras10, S., Gray37, C., Greco57, G., Green45, A. C., Groot52, P., Grote8, H., Grunewald29, S., Guidi57, G. M., Guo70, X., Gupta14, A., Gupta95, M. K., Gushwa1, K. E., Gustafson1, E. K., Gustafson98, R., Hacker22, J. J., Hall56, B. R., Hall1, E. D., Hammond36, G., Haney99, M., Hanke8, M. M., Hanks37, J., Hanna72, C., Hannam91, M. D., Hanson6, J., Hardwick2, T., Haris106, K., Harms57, J., Harry100, G. M., Harry29, I. W., Hart36, M. J., Hartman5, M. T., Haster45, C. J., Haughian36, K., Heidmann60, A., Heintze5, M. C., Heitmann53, H., Hello23, P., Hemming34, G., Hendry36, M., Heng36, I. S., Hennig36, J., Heptonstall1, A. W., Heurs8, M., Hild36, S., Hoak101, D., Hodge1, K. A., Hofman66, D., Hollitt102, S. E., Holt6, K., Holz75, D. E., Hopkins91, P., Hosken102, D. J., Hough36, J., Houston36, E. A., Howell51, E. J., Hu36, Y. M., Huang73, S., Huerta82, E. A., 103, Huet23, D., Hughey97, B., Husa67, S., Huttner36, S. H., Huynh Dinh6, T., Idrisy72, A., Indik8, N., Ingram37, D. R., Inta71, R., Isa36, H. N., Isac60, J. M., Isi1, M., Islas22, G., Isogai10, T., Iyer15, B. R., Izumi37, K., Jacqmin60, T., Jang77, H., Jani64, K., Jaranowski104, P., Jawahar105, S., Jiménez Forteza67, F., Johnson2, W. W., Jones26, D. I., Jones36, R., Jonker9, R. J. G., Ju51, L., Kalaghatgi24, C. V., Kalogera82, V., Kandhasamy21, S., Kang77, G., Kanner1, J. B., Karki59, S., Kasprzack2, M., 34, 23, Katsavounidis10, E., Katzman6, W., Kaufer17, S., Kaur51, T., Kawabe37, K., Kawazoe8, F., Kéfélian53, F., Kehl69, M. S., Keitel8, D., Kelley35, D. B., Kells1, W., Kennedy86, R., Key85, J. S., Khalaidovski8, A., Khalili49, F. Y., Khan12, I., Khan91, S., Khan95, Z., Khazanov107, E. A., Kijbunchoo37, N., Kim77, C., Kim108, J., Kim109, K., Kim77, N., Kim41, N., Kim108, Y. M., King102, E. J., King37, P. J., Kinzel6, D. L., Kissel37, J. S., Kleybolte27, L., Klimenko5, S., Koehlenbeck8, S. M., Kokeyama2, K., Koley9, S., Kondrashov1, V., Kontos10, A., Korobko27, M., Korth1, W. Z., Kowalska61, I., Kozak1, D. B., Kringel8, V., Królak110, A., 111, Krueger17, C., Kuehn8, G., Kumar69, P., Kuo73, L., Kutynia110, A., Lackey35, B. D., Landry37, M., Lange112, J., Lantz41, B., Lasky113, P. D., Lazzarini1, A., Lazzaro43, C., Leaci28, P., 79, 29, Leavey36, S., Lebigot30, E. O., Lee108, C. H., Lee109, H. K., Lee114, H. M., Lee36, K., Lenon35, A., Leonardi89, M., Leong8, J. R., Leroy23, N., Letendre7, N., Levin113, Y., Levine37, B. M., Li1, T. G. F., Libson10, A., Littenberg115, T. B., Lockerbie105, N. A., Logue36, J., Lombardi101, A. L., Lord35, J. E., Lorenzini12, M., Loriette116, V., Lormand6, M., Losurdo58, G., Lough8, J. D., Lück8, H., Lundgren8, A. P., Luo78, J., Lynch10, R., Ma51, Y., Macdonald41, T., Machenschalk8, B., Macinnis10, M., Macleod2, D. M., Magaña Sandoval35, F., Magee56, R. M., Mageswaran1, M., Majorana28, E., Maksimovic116, I., Malvezzi13, V., Man53, N., Mandel45, I., Mandic83, V., Mangano36, V., Mansell20, G. L., Manske16, M., Mantovani34, M., Marchesoni33, F., 117, Marion7, F., Márka40, S., Márka40, Z., Markosyan41, A. S., Maros1, E., Martelli57, F., Martellini53, L., Martin36, I. W., Martin5, R. M., Martynov1, D. V., Marx1, J. N., Mason10, K., Masserot7, A., Massinger35, T. J., Masso Reid36, M., Matichard10, F., Matone40, L., Mavalvala10, N., Mazumder56, N., Mazzolo8, G., Mccarthy37, R., Mcclelland20, D. E., Mccormick6, S., Mcguire118, S. C., Mcintyre1, G., Mciver1, J., Mcmanus20, D. J., Mcwilliams103, S. T., Meacher72, D., Meadors8, G. D., Meidam9, J., Melatos84, A., Mendell37, G., Mendoza Gandara8, D., Mercer16, R. A., Merilh37, E., Merzougui53, M., Meshkov1, S., Messenger36, C., Messick72, C., Meyers83, P. M., Mezzani28, F., Miao45, H., Michel66, C., Middleton45, H., Mikhailov119, E. E., Milano4, L., Miller10, J., Millhouse31, M., Minenkov13, Y., Ming8, J., Mirshekari120, S., Mishra15, C., Mitra14, S., Mitrofanov49, V. P., Mitselmakher5, G., Mittleman10, R., Moggi19, A., Mohan34, M., Mohapatra10, S. R. P., Montani57, M., Moore88, B. C., Moore121, C. J., Moraru37, D., Moreno37, G., Morriss85, S. R., Mossavi8, K., Mours7, B., Mow Lowry45, C. M., Mueller5, C. L., Mueller5, G., Muir91, A. W., Mukherjee15, A., Mukherjee16, D., Mukherjee85, S., Mukund14, N., Mullavey6, A., Munch102, J., Murphy40, D. J., Murray36, P. G., Mytidis5, A., Nardecchia13, I., Naticchioni28, L., Nayak122, R. K., Necula5, V., Nedkova101, K., Nelemans9, G., Neri46, M., Neunzert98, A., Newton36, G., Nguyen20, T. T., Nielsen8, A. B., Nissanke9, S., Nitz8, A., Nocera34, F., Nolting6, D., Normandin85, M. E. N., Nuttall35, L. K., Oberling37, J., Ochsner16, E., O'Dell123, J., Oelker10, E., Ogin124, G. H., Oh125, J. J., Oh125, S. H., Ohme91, F., Oliver67, M., Oppermann8, P., Oram6, R. J., O'Reilly6, B., O'Shaughnessy112, R., Ottaway102, D. J., Ottens5, R. S., Overmier6, H., Owen71, B. J., Pai106, A., Pai48, S. A., Palamos59, J. R., Palashov107, O., Palliyaguru71, N., Palomba28, C., Pal Singh27, A., Pan73, H., Pankow82, C., Pannarale91, F., Pant48, B. C., Paoletti19, F., Paoli34, A., Papa8, M. A., 29, 16, Paris41, H. R., Parker6, W., Pascucci36, D., Pasqualetti34, A., Passaquieti18, R., Passuello19, D., Patricelli18, B., Patrick41, Z., Pearlstone36, B. L., Pedraza1, M., Pedurand66, R., Pekowsky35, L., Pele6, A., Penn126, S., Perreca1, A., Phelps36, M., Piccinni28, O., Pichot53, M., Piergiovanni57, F., Pierro87, V., Pillant34, G., Pinard66, L., Pinto87, I. M., Pitkin36, M., Poggiani18, R., Popolizio34, P., Post8, A., Powell36, J., Prasad14, J., Predoi91, V., Premachandra113, S. S., Prestegard83, T., Price1, L. R., Prijatelj34, M., Principe87, M., Privitera29, S., Prodi89, G. A., Prokhorov49, L., Puncken8, O., Punturo33, M., Puppo28, P., Pürrer29, M., Qi16, H., Qin51, J., Quetschke85, V., Quintero1, E. A., Quitzow James59, R., Raab37, F. J., Rabeling20, D. S., Radkins37, H., Raffai54, P., Raja48, S., Rakhmanov85, M., Rapagnani28, P., Raymond29, V., Razzano18, M., Re25, V., Read22, J., Reed37, C. M., Regimbau53, T., Rei47, L., Reid50, S., Reitze1, D. H., 5, Rew119, H., Reyes35, S. D., Ricci28, F., Riles98, K., Robertson1, N. A., Robie36, R., Robinet23, F., Rocchi13, A., Rolland7, L., Rollins1, J. G., Roma59, V. J., Romano3, R., Romanov119, G., Romie6, J. H., Rosińska44, D., 127, Rowan36, S., Rüdiger8, A., Ruggi34, P., Ryan37, K., Sachdev1, S., Sadecki37, T., Sadeghian16, L., Salconi34, L., Saleem106, M., Salemi8, F., Samajdar122, A., Sammut84, L., 113, Sanchez1, E. J., Sandberg37, V., Sandeen82, B., Sanders35, J. R., Sassolas66, B., Sathyaprakash91, B. S., Saulson35, P. R., Sauter98, O., Savage37, R. L., Sawadsky17, A., Schale59, P., Schilling8, R., Schmidt8, J., Schmidt1, P., Schnabel27, R., Schofield59, R. M. S., Schönbeck27, A., Schreiber8, E., Schuette8, D., Schutz29, B. F., Scott36, J., Scott20, S. M., Sellers6, D., Sentenac34, D., Sequino13, V., Sergeev107, A., Serna22, G., Setyawati9, Y., Sevigny37, A., Shaddock20, D. A., Shah9, S., Shahriar82, M. S., Shaltev8, M., Shao1, Z., Shapiro41, B., Shawhan63, P., Sheperd16, A., Shoemaker10, D. H., Shoemaker64, D. M., Siellez53, K., Siemens16, X., Sigg37, D., Silva11, A. D., Simakov8, D., Singer1, A., Singh8, A., Singh2, R., Singhal12, A., Sintes67, A. M., Slagmolen20, B. J. J., Smith22, J. R., Smith1, N. D., Smith1, R. J. E., Son125, E. J., Sorazu36, B., Sorrentino47, F., Souradeep14, T., Srivastava95, A. K., Staley40, A., Steinke8, M., Steinlechner36, J., Steinlechner36, S., Steinmeyer8, D., Stephens16, B. C., Stone85, R., Strain36, K. A., Straniero66, N., Stratta57, G., Strauss78, N. A., Strigin49, S., Sturani120, R., Stuver6, A. L., Summerscales128, T. Z., Sun84, L., Sutton91, P. J., Swinkels34, B. L., Szczepańczyk97, M. J., Tacca30, M., Talukder59, D., Tanner5, D. B., Tápai96, M., Tarabrin8, S. P., Taracchini29, A., Taylor1, R., Theeg8, T., Thirugnanasambandam1, M. P., Thomas45, E. G., Thomas6, M., Thomas37, P., Thorne6, K. A., Thorne76, K. S., Thrane113, E., Tiwari12, S., Tiwari91, V., Tokmakov105, K. V., Tomlinson86, C., Tonelli18, M., Torres85, C. V., Torrie1, C. I., Töyrä45, D., Travasso32, F., Traylor6, G., Trifirò21, D., Tringali89, M. C., Trozzo19, L., 129, Tse10, M., Turconi53, M., Tuyenbayev85, D., Ugolini130, D., Unnikrishnan99, C. S., Urban16, A. L., Usman35, S. A., Vahlbruch17, H., Vajente1, G., Valdes85, G., van Bakel9, N., van Beuzekom9, M., van den Brand9, J. F. J., Van Den Broeck9, C., Vander Hyde22, D. C., van der Schaaf9, L., van Heijningen9, J. V., van Veggel36, A. A., Vardaro42, M., Vass1, S., Vasúth38, M., Vaulin10, R., Vecchio45, A., Vedovato43, G., Veitch45, J., Veitch102, P. J., Venkateswara131, K., Verkindt7, D., Vetrano57, F., Viceré57, A., Vinciguerra45, S., Vine50, D. J., Vinet53, J. Y., Vitale10, S., Vo35, T., Vocca32, H., Vorvick37, C., Voss5, D., Vousden45, W. D., Vyatchanin49, S. P., Wade20, A. R., Wade132, L. E., Wade132, M., Walker2, M., Wallace1, L., Walsh8, S., Wang12, G., Wang45, H., Wang45, M., Wang70, X., Wang51, Y., Ward20, R. L., Warner37, J., Was7, M., Weaver37, B., Wei53, L. W., Weinert8, M., Weinstein1, A. J., Weiss10, R., Welborn6, T., Wen51, L., Weßels8, P., Westphal8, T., Wette8, K., Whelan8, J. T., 112, White86, D. J., Whiting5, B. F., Williams1, R. D., Williamson91, A. R., Willis133, J. L., Willke8, B., Wimmer8, M. H., Winkler8, W., Wipf1, C. C., Wittel8, H., Woan36, G., Worden37, J., Wright36, J. L., Wu6, G., Yablon82, J., Yam10, W., Yamamoto1, H., Yancey63, C. C., Yap20, M. J., Yu10, H., Yvert7, M., Zadrożny110, A., Zangrando43, L., Zanolin97, M., Zendri43, J. P., Zevin82, M., Zhang10, F., Zhang1, L., Zhang119, M., Zhang112, Y., Zhao51, C., Zhou82, M., Zhou82, Z., Zhu51, X. J., Zucker1, M. E., Zuraw101, S. E., Zweizig1, J., Allison134, J., 135, Bannister134, K., Bell134, M. E., Chatterjee136, S., Chippendale134, A. P., Edwards134, P. G., Harvey Smith134, L., Ian, Heywood134, 137, Hotan138, A., Indermuehle134, B., Marvil134, J., Mcconnell134, D., Murphy135, T., 139, Popping135, A., 140, Reynolds134, J., Sault84, R. J., 134, Voronkov134, M. A., Whiting134 (The Australian Square Kilometer Array Pathfinder, M. T., Castro Tirado141, A. J., 142, Cunniffe141, R., Jelínek143, M., Tello141, J. C., Oates141, S. R., Hu141, Y. D., Kubánek144, P., Guziy145, S., Castellón146, A., García Cerezo142, A., Muñoz142, V. F., Pérez del Pulgar142, C., Castillo Carrión147, S., Castro Cerón148, J. M., Hudec143, R., 149, Caballero García150, M. D., Páta149, P., Vitek149, S., Adame151, J. A., Konig151, S., Rendón141, F., 151, Mateo Sanguino152, T. de J., Fernández Muñoz153, R., Yock154, P. C., Rattenbury154, N., Allen155, W. H., Querel156, R., Jeong141, S., 157, Park157, I. H., Bai158, J., Cui159, C. h., Fan158, Y., Wang158, C. h., Hiriart160, D., Lee161, W. H., Claret141, A., Sánchez Ramírez141, R., Pandey162, S. B., Mediavilla163, T., Sabau Graziati164, L., Abbott165, T. M. C., Abdalla137, F. B., 166, Allam167, S., Annis167, J., Armstrong168, R., Benoit Lévy166, A., 169, 170, Berger171, E., Bernstein172, R. A., Bertin169, E., 170, Brout173, D., Buckley Geer167, E., Burke174, D. L., 175, Capozzi176, D., Carretero177, J., 178, Castander177, F. J., Chornock179, R., Cowperthwaite171, P. S., Crocce177, M., Cunha174, C. E., D'Andrea26, C. B., 176, da Costa180, L. N., Desai181, S., 182, Diehl167, H. T., Dietrich181, J. P., Doctor183, Z., Drlica Wagner167, A., Drout171, M. R., Eifler173, T. F., 184, Estrada167, J., Evrard98, A. E., Fernandez178, E., Finley167, D. A., Flaugher167, B., Foley185, R. J., 186, Fong187, W. F., Fosalba177, P., Fox188, D. B., Frieman167, J., 183, Fryer189, C. L., Gaztanaga177, E., Gerdes190, D. W., Goldstein191, D. A., 192, Gruen174, D., Gruendl185, R. A., 193, Gutierrez167, G., Herner167, K., Honscheid194, K., 195, James165, D. J., Johnson193, M. D., Johnson193, M. W. G., Karliner186, I., Kasen192, D., 196, Kent167, S., Kessler183, R., Kim192, A. G., Kind185, M. C., Kuehn197, K., Kuropatkin167, N., Lahav166, O., Li198, T. S., Lima180, M., 199, Lin167, H., Maia180, M. A. G., Margutti200, R., Marriner167, J., Martini194, P., 201, Matheson202, T., Melchior168, P., Metzger203, B. D., Miller190, C. J., 204, Miquel178, R., 205, Neilsen167, E., Nichol176, R. C., Nord167, B., Nugent192, P., Ogando180, R., Petravick193, D., Plazas184, A. A., Quataert206, E., Roe192, N., Romer207, A. K., Roodman174, A., Rosell180, A. C., Rykoff174, E. S., Sako173, M., Sanchez208, E., Scarpine167, V., Schindler175, R., Schubnell190, M., Scolnic183, D., Sevilla Noarbe185, I., 208, Sheldon209, E., Smith187, N., Smith165, R. C., Soares Santos167, M., Sobreira180, F., Stebbins167, A., Suchyta173, E., Swanson193, M. E. C., Tarle190, G., Thaler186, J., Thomas176, D., Thomas192, R. C., Tucker167, D. L., Vikram210, V., Walker165, A. R., Wechsler41, R. H., 174, 175, Wester167, W., Yanny167, B., Zhang98, Y., Zuntz211, J., Connaughton212, V., Burns213, E., Goldstein214, A., 378, Briggs215, M. S., Zhang216, B. B., 217, Hui214, C. M., Jenke216, P., Wilson Hodge214, C. A., Bhat216, P. N., Bissaldi218, E., Cleveland212, W., Fitzpatrick216, G., Giles219, M. M., Gibby219, M. H., Greiner220, J., von Kienlin220, A., Kippen221, R. M., Mcbreen222, S., Mailyan216, B., Meegan216, C. A., Paciesas212, W. S., Preece215, R. D., Roberts222, O., Sparke223, L., Stanbro213, M., Toelge220, K., Veres216, P., Yu220, H. F., 224, Blackburn171, L., Ackermann225, M., Ajello226, M., Albert227, A., Anderson228, B., 229, Atwood230, W. B., Axelsson231, M., 232, Baldini227, L., 233, Barbiellini234, G., 235, Bastieri236, D., 237, Bellazzini238, R., Bissaldi239, E., Blandford227, R. D., Bloom227, E. D., Bonino, Raffaella, Bottacini227, E., Brandt242, T. J., Bruel243, P., Buson242, S., 244, 245, Caliandro227, G. A., 246, Cameron227, R. A., Caragiulo239, M., 247, Caraveo248, P. A., Cavazzuti249, E., Charles227, E., Chekhtman250, A., Chiang227, J., Chiaro237, G., Ciprini249, S., 251, Cohen Tanugi252, J., Cominsky253, L. R., Costanza239, F., Cuoco240, A., 241, D'Ammando254, F., 255, de Palma239, F., 256, Desiante240, R., 257, Digel227, S. W., Di Lalla238, N., Di Mauro227, M., Di Venere239, L., Domínguez226, A., Drell227, P. S., Dubois227, R., Favuzzi239, C., Ferrara242, E. C., Franckowiak227, A., Fukazawa258, Y., Funk259, S., Fusco239, P., Gargano239, F., Gasparrini249, D., Giglietto239, N., Giommi249, P., Giordano239, F., Giroletti254, M., Glanzman227, T., Godfrey227, G., Gomez Vargas260, G. A., 261, Green242, D., 262, Grenier263, I. A., Grove264, J. E., Guiriec242, S., Hadasch265, D., Harding242, A. K., Hays242, E., Hewitt266, J. W., Hill227, A. B., 267, Horan243, D., Jogler227, T., Jóhannesson268, G., Johnson227, A. S., Kensei258, S., Kocevski242, D., Kuss238, M., La Mura237, G., 265, Larsson229, S., 231, Latronico240, L., Li269, J., Li229, L., Longo234, F., Loparco239, F., Lovellette264, M. N., Lubrano251, P., Magill262, J., Maldera240, S., Manfreda238, A., Marelli248, M., Mayer225, M., Mazziotta239, M. N., Mcenery242, J. E., Meyer228, M., Michelson227, P. F., Mirabal242, N., Mizuno270, T., Moiseev245, A. A., Monzani227, M. E., Moretti271, E., Morselli261, A., Moskalenko227, I. V., Negro240, M., Nuss252, E., Ohsugi270, T., Omodei227, N., Orienti254, M., Orlando227, E., Ormes272, J. F., Paneque227, D., 271, Perkins242, J. S., Pesce Rollins227, M., 238, Piron252, F., Pivato238, G., Porter227, T. A., Racusin242, J. L., Rainò239, S., Rando236, R., Razzaque273, S., Reimer227, A., Reimer227, O., Salvetti248, D., Saz Parkinson230, P. M., 274, 275, Sgrò238, C., Simone239, D., Siskind276, E. J., Spada238, F., Spandre238, G., Spinelli239, P., Suson277, D. J., Tajima227, H., 278, Thayer227, J. B., Thompson242, D. J., Tibaldo279, L., Torres269, D. F., 280, Troja242, E., Uchiyama281, Y., Venters242, T. M., Vianello227, G., Wood264, K. S., Wood227, M., Zhu262, S., Zimmer228, S., Brocato282, E., Cappellaro283, E., Covino284, S., Grado285, A., Nicastro286, L., Palazzi286, E., Pian286, E., 287, Amati286, L., Antonelli282, L. A., 288, Capaccioli289, M., D'Avanzo284, P., D'Elia282, V., Getman285, F., Giuffrida282, G., Iannicola282, G., Limatola285, L., Lisi282, M., Marinoni282, S., Marrese282, P., 283, Melandri284, A., Piranomonte282, S., Possenti290, A., Pulone282, L., Rossi286, A., Stamerra287, A., 291, Stella282, L., Testa282, V., Tomasella283, L., Yang283 (The GRAvitational Wave Inaf TeAm, S., Bazzano292, A., Bozzo293, E., Brandt294, S., Courvoisier293, T. J. L., Ferrigno293, C., Hanlon295, L., Kuulkers296, E., Laurent297, P., Mereghetti298, S., Roques299, J. P., Savchenko300, V., Ubertini292, P., Kasliwal301, M. M., Singer39, L. P., Cao301, Y., Duggan301, G., Kulkarni301, S. R., Bhalerao14, V., Miller184, A. A., 301, 379, Barlow301, T., Bellm301, E., Manulis302, I., Rana14, J., Laher303, R., Masci303, F., Surace303, J., Rebbapragada184, U., Cook301, D., Van Sistine16, A., Sesar304, B., Perley305, D., Ferreti306, R., Prince301, T., Kendrick307, R., Horesh302 (The Intermediate Palomar Transient Factory, A., Hurley308, K., Golenetskii309, S. V., Aptekar309, R. L., Frederiks309, D. D., Svinkin309, D. S., Rau220, A., Zhang220, X., Smith230, D. M., Cline39, T., 380, Krimm245, H., 310, Abe311, F., Doi312, M., Fujisawa313, K., Kawabata314, K. S., Morokuma312, T., Motohara312, K., Tanaka315, M., Ohta316, K., Yanagisawa317, K., Yoshida314, M., Baltay318, C., Rabinowitz318, D., Ellman318, N., Rostami318, S., Bersier319, D. F., Bode319, M. F., Collins319, C. A., Copperwheat319, C. M., Darnley319, M. J., Galloway320, D. K., 321, Gomboc322, A., 323, Kobayashi319, S., Mazzali319, P., Mundell324, C. G., Piascik319, A. S., Don, Pollacco325, Steele319, I. A., Ulaczyk325, K., Broderick326, J. W., Fender327, R. P., Jonker52, P. G., 328, Rowlinson135, A., 326, 329, Stappers211, B. W., Wijers329 (The Low Frequency Array, R. A. M. J., Lipunov330, V., Gorbovskoy330, E., Tyurina330, N., Kornilov330, V., Balanutsa330, P., Kuznetsov330, A., Buckley331, D., Rebolo332, R., Serra Ricart332, M., Israelian332, G., Budnev333, N. M., Gress333, O., Ivanov333, K., Poleshuk333, V., Tlatov334, A., Yurkov335, V., Kawai336, N., Serino337, M., Negoro338, H., Nakahira339, S., Mihara337, T., Tomida340, H., Ueno340, S., Tsunemi341, H., Matsuoka337, M., Croft342, S., 343, Feng344, L., Franzen345, T. M. O., Gaensler135, B. M., 139, 346, Johnston Hollitt347, M., Kaplan16, D. L., Morales131, M. F., Tingay135, S. J., 345, 348, Wayth135, R. B., 345, Williams345 (The Murchison Wide field Array, A., Smartt349, S. J., Chambers350, K. C., Smith349, K. W., Huber350, M. E., Young349, D. R., Wright349, D. E., Schultz350, A., Denneau350, L., Flewelling350, H., Magnier350, E. A., Primak350, N., Rest351, A., Sherstyuk350, A., Stalder350, B., Stubbs352, C. W., Tonry350, J., Waters350, C., Willman350, M., 353, F. Olivares E., 354, Campbell355, H., Kotak349, R., Sollerman306, J., Smith26, M., Dennefeld356, M., Anderson357, J. P., Botticella285, M. T., Chen220, T. W., Valle285, M. D., Elias Rosa283, N., Fraser355, M., Inserra349, C., Kankare349, E., Kupfer301, T., Harmanen358, J., Galbany353, L., 359, Le Guillou360, L., 361, Lyman325, J. D., Maguire349, K., Mitra361, A., Nicholl171, M., Razza353, A., Terreran283, G., 349, Valenti362, S., 363, Gal Yam364, A., Ćwiek110, A., Ćwiok365, M., Mankiewicz366, L., Opiela366, R., Zaremba365, M., Żarnecki365, A. F., Onken20, C. A., Scalzo20, R. A., Schmidt20, B. P., Wolf20, C., Yuan20, F., Evans367, P. A., Kennea72, J. A., Burrows72, D. N., Campana284, S., Cenko39, S. B., 368, Giommi288, P., Marshall39, F. E., Nousek72, J., O'Brien367, P., Osborne367, J. P., Palmer369, D., Perri282, M., Siegel72, M., Tagliaferri284, G., Klotz370, A., Turpin370, D., Laugier53, R., Beroiz85, M., 371, Peñuela85, T., 372, Macri373, L. M., Oelkers373, R. J., Lambas374, D. G., Vrech374, R., Cabral374, J., Colazo374, C., Dominguez374, M., Sanchez374, B., Gurovich374, S., Lares374, M., Marshall373, J. L., Depoy373, D. L., Padilla375, N., Pereyra85, N. A., Benacquista85, M., Tanvir367, N. R., Wiersema367, K., Levan325, A. J., Steeghs325, D., Hjorth305, J., Fynbo305, J. P. U., Malesani305, D., Milvang Jensen305, B., Watson305, D., Irwin355, M., Fernandez355, C. G., Mcmahon355, R. G., Banerji355, M., Gonzalez Solares355, E., Schulze353, S., 375, de Ugarte Postigo305, A., 376, Thoene376, C. C., Cano377, Z., Rosswog306, S., (Astro)-Particles Physics, 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., Barthelmy, S., Bartlett, J., Bartos, I., Bassiri, R., Basti, A., Batch, J. C., Baune, C., Bavigadda, V., Bazzan, M., Behnke, B., Bejger, M., Bell, A. S., Bell, C. J., Berger, B. K., Bergman, J., 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., Bodiya, T. P., Boer, M., Bogaert, G., Bogan, C., Bohe, A., Bojtos, P., 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., Brooks, A. F., Brown, D. A., Brown, D. D., Brown, N. M., Buchanan, C. C., Buikema, A., Bulik, T., Bulten, H. J., Buonanno, A., Buskulic, D., Buy, C., Byer, R. L., Cadonati, L., Cagnoli, G., Cahillane, C., Bustillo, J. C., Callister, T., Calloni, Enrico, Camp, J. B., Cannon, K. C., Cao, J., Capano, C. D., Capocasa, E., Carbognani, F., Caride, S., Diaz, J. C., Casentini, C., Caudill, S., Cavagliá, M., Cavalier, F., Cavalieri, R., Cella, G., Cepeda, C. B., Baiardi, L. C., Cerretani, G., Cesarini, E., Chakraborty, R., Chalermsongsak, T., Chamberlin, S. J., Chan, M., Chao, S., Charlton, P., Chassande Mottin, E., 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., Dattilo, V., Dave, I., Daveloza, H. P., Davier, M., Davies, G. S., Daw, E. J., Day, R., Debra, D., Debreczeni, G., Degallaix, J., DE LAURENTIS, Martina, Deléglise, S., Del Pozzo, W., Denker, T., Dent, T., Dereli, H., Dergachev, V., Derosa, R. T., DE ROSA, Rosario, Desalvo, R., Dhurandhar, S., Díaz, M. C., Di Fiore, L., Di Giovanni, M., Di Lieto, A., Di Pace, S., Di Palma, I., Di Virgilio, A., Dojcinoski, G., Dolique, V., Donovan, F., Dooley, K. L., Doravari, S., Douglas, R., 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., 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., Ferrante, I., Ferreira, E. C., Ferrini, F., Fidecaro, F., Fiori, I., Fiorucci, D., Fisher, R. P., Flaminio, R., Fletcher, M., Fournier, J. D., Franco, S., Frasca, S., Frasconi, F., Frei, Z., Freise, A., Frey, R., Frey, V., Fricke, T. T., Fritschel, P., Frolov, V. V., Fulda, P., Fyffe, M., Gabbard, H. A. G., Gair, J. R., Gammaitoni, L., Gaonkar, S. G., Garufi, Fabio, Gatto, A., Gaur, G., Gehrels, N., Gemme, G., Gendre, B., Genin, E., Gennai, A., George, J., Gergely, L., Germain, V., Ghosh, A., 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. G., Gopakumar, A., Gordon, N. A., Gorodetsky, M. L., Gossan, S. E., Gosselin, M., Gouaty, R., 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., Haris, K., 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., Heptonstall, A. W., Heurs, M., Hild, S., Hoak, D., Hodge, K. A., Hofman, D., Hollitt, S. E., Holt, K., Holz, D. E., Hopkins, P., Hosken, D. J., 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., Idrisy, A., Indik, N., Ingram, D. R., Inta, R., Isa, H. N., Isac, J. M., Isi, M., Islas, G., Isogai, T., Iyer, B. R., Izumi, K., Jacqmin, T., Jang, H., Jani, K., Jaranowski, P., Jawahar, S., Jiménez Forteza, F., Johnson, W. W., Jones, D. I., Jones, R., Jonker, R. J. G., Ju, L., Kalaghatgi, C. V., Kalogera, V., Kandhasamy, S., Kang, G., Kanner, J. B., Karki, S., Kasprzack, M., Katsavounidis, E., Katzman, W., Kaufer, S., Kaur, T., Kawabe, K., Kawazoe, F., Kéfélian, F., Kehl, M. S., Keitel, D., Kelley, D. B., Kells, W., Kennedy, R., Key, J. S., Khalaidovski, A., Khalili, F. Y., Khan, I., Khan, S., Khan, Z., Khazanov, E. A., Kijbunchoo, N., Kim, C., Kim, J., Kim, K., Kim, N., Kim, Y. M., King, E. J., King, P. J., Kinzel, D. L., Kissel, J. S., Kleybolte, L., Klimenko, S., Koehlenbeck, S. M., Kokeyama, K., Koley, S., Kondrashov, V., Kontos, A., Korobko, M., Korth, W. Z., Kowalska, I., Kozak, D. B., Kringel, V., Królak, A., Krueger, C., Kuehn, G., Kumar, P., Kuo, L., Kutynia, A., Lackey, B. D., Landry, M., Lange, J., Lantz, B., Lasky, P. D., 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., Levine, B. M., Li, T. G. F., Libson, A., Littenberg, T. B., Lockerbie, N. A., Logue, J., Lombardi, A. L., Lord, J. E., Lorenzini, M., Loriette, V., Lormand, M., Losurdo, G., Lough, J. D., Lück, H., Lundgren, A. P., Luo, J., Lynch, R., Ma, Y., Macdonald, T., Machenschalk, B., Macinnis, M., Macleod, D. M., Magaña Sandoval, F., Magee, R. M., Mageswaran, 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., Martin, R. M., Martynov, D. V., Marx, J. N., Mason, K., Masserot, A., Massinger, T. J., Masso Reid, M., Matichard, F., Matone, L., Mavalvala, N., Mazumder, N., Mazzolo, G., Mccarthy, R., Mcclelland, D. E., Mccormick, S., Mcguire, S. C., Mcintyre, G., Mciver, J., Mcmanus, D. J., Mcwilliams, S. T., Meacher, D., Meadors, G. D., Meidam, J., Melatos, A., Mendell, G., Mendoza Gandara, D., Mercer, R. A., Merilh, E., Merzougui, M., Meshkov, S., Messenger, C., Messick, C., Meyers, P. M., Mezzani, F., Miao, H., Michel, C., Middleton, H., Mikhailov, E. E., Milano, Leopoldo, 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, C. L., Mueller, G., Muir, A. W., Mukherjee, A., 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., Necula, V., Nedkova, K., Nelemans, G., 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, R. J., O'Reilly, B., O'Shaughnessy, R., Ottaway, D. J., Ottens, R. S., Overmier, H., Owen, B. J., Pai, A., Pai, S. A., Palamos, J. R., Palashov, O., Palliyaguru, N., 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., Phelps, M., Piccinni, O., Pichot, M., Piergiovanni, F., Pierro, V., Pillant, G., Pinard, L., Pinto, I. M., Pitkin, M., Poggiani, R., Popolizio, P., Post, A., Powell, J., Prasad, J., Predoi, V., Premachandra, S. S., Prestegard, T., Price, L. R., Prijatelj, M., Principe, M., Privitera, S., Prodi, G. A., Prokhorov, L., Puncken, O., Punturo, M., Puppo, P., Pürrer, M., Qi, H., Qin, J., Quetschke, V., Quintero, E. A., Quitzow James, R., Raab, F. J., Rabeling, D. S., Radkins, H., Raffai, P., Raja, S., 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., 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., 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., 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., Sentenac, D., Sequino, V., Sergeev, A., Serna, G., Setyawati, Y., Sevigny, A., Shaddock, D. A., Shah, S., Shahriar, M. S., Shaltev, M., Shao, Z., Shapiro, B., Shawhan, P., Sheperd, A., Shoemaker, D. H., Shoemaker, D. M., Siellez, K., Siemens, X., Sigg, D., Silva, A. D., Simakov, D., Singer, A., 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., 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., Thorne, K. S., Thrane, E., Tiwari, S., Tiwari, V., Tokmakov, K. V., Tomlinson, C., Tonelli, M., 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., 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., 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., Welborn, T., Wen, L., Weßels, P., Westphal, T., Wette, K., Whelan, J. T., White, D. J., 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., Worden, J., Wright, J. L., Wu, G., Yablon, J., Yam, W., Yamamoto, H., Yancey, C. C., Yap, M. J., Yu, H., Yvert, M., Zadrożny, A., Zangrando, L., Zanolin, M., Zendri, J. P., Zevin, M., Zhang, F., Zhang, L., Zhang, M., Zhang, Y., Zhao, C., Zhou, M., Zhou, Z., Zhu, X. J., Zucker, M. E., Zuraw, S. E., Zweizig, J., Allison, J., Bannister, K., Bell, M. E., Chatterjee, S., Chippendale, A. P., Edwards, P. G., Harvey Smith, L., Heywood, Ian, Hotan, A., Indermuehle, B., Marvil, J., Mcconnell, D., Murphy, T., Popping, A., Reynolds, J., Sault, R. J., Voronkov, M. A., Whiting, M. T., Castro Tirado, A. J., Cunniffe, R., Jelínek, M., Tello, J. C., Oates, S. R., Hu, Y. D., Kubánek, P., Guziy, S., Castellón, A., García Cerezo, A., Muñoz, V. F., Pérez Del Pulgar, C., Castillo Carrión, S., Castro Cerón, J. M., Hudec, R., Caballero García, M. D., Páta, P., Vitek, S., Adame, J. A., Konig, S., Rendón, F., Mateo Sanguino, T. De J., Fernández Muñoz, R., Yock, P. C., Rattenbury, N., Allen, W. H., Querel, R., Jeong, S., Park, I. H., Bai, J., Cui, C. h., Fan, Y., Wang, C. h., Hiriart, D., Lee, W. H., Claret, A., Sánchez Ramírez, R., Pandey, S. B., Mediavilla, T., Sabau Graziati, L., Abbott, T. M. C., Abdalla, F. B., Allam, S., Annis, J., Armstrong, R., Benoit Lévy, A., Berger, E., Bernstein, R. A., Bertin, E., Brout, D., Buckley Geer, E., Burke, D. L., Capozzi, D., Carretero, J., Castander, F. J., Chornock, R., Cowperthwaite, P. S., Crocce, M., Cunha, C. E., D'Andrea, C. B., Da Costa, L. N., Desai, S., Diehl, H. T., Dietrich, J. P., Doctor, Z., Drlica Wagner, A., Drout, M. R., Eifler, T. F., Estrada, J., Evrard, A. E., Fernandez, E., Finley, D. A., Flaugher, B., Foley, R. J., Fong, W. F., Fosalba, P., Fox, D. B., Frieman, J., Fryer, C. L., Gaztanaga, E., Gerdes, D. W., Goldstein, D. A., Gruen, D., Gruendl, R. A., Gutierrez, G., Herner, K., Honscheid, K., James, D. J., Johnson, M. D., Johnson, M. W. G., Karliner, I., Kasen, D., Kent, S., Kessler, R., Kim, A. G., Kind, M. C., Kuehn, K., Kuropatkin, N., Lahav, O., Li, T. S., Lima, M., Lin, H., Maia, M. A. G., Margutti, R., Marriner, J., Martini, P., Matheson, T., Melchior, P., Metzger, B. D., Miller, C. J., Miquel, R., Neilsen, E., Nichol, R. C., Nord, B., Nugent, P., Ogando, R., Petravick, D., Plazas, A. A., Quataert, E., Roe, N., Romer, A. K., Roodman, A., Rosell, A. C., Rykoff, E. S., Sako, M., Sanchez, E., Scarpine, V., Schindler, R., Schubnell, M., Scolnic, D., Sevilla Noarbe, I., Sheldon, E., Smith, N., Smith, R. C., Soares Santos, M., Sobreira, F., Stebbins, A., Suchyta, E., Swanson, M. E. C., Tarle, G., Thaler, J., Thomas, D., Thomas, R. C., Tucker, D. L., Vikram, V., Walker, A. R., Wechsler, R. H., Wester, W., Yanny, B., Zuntz, J., Connaughton, V., Burns, E., Goldstein, A., Briggs, M. S., Zhang, B. B., Hui, C. M., Jenke, P., Wilson Hodge, C. A., Bhat, P. N., Bissaldi, E., Cleveland, W., Fitzpatrick, G., Giles, M. M., Gibby, M. H., Greiner, J., Von Kienlin, A., Kippen, R. M., Mcbreen, S., Mailyan, B., Meegan, C. A., Paciesas, W. S., Preece, R. D., Roberts, O., Sparke, L., Stanbro, M., Toelge, K., Veres, P., Yu, H. F., Blackburn, L., Ackermann, M., Ajello, M., Albert, A., Anderson, B., Atwood, W. B., Axelsson, M., Baldini, L., Barbiellini, G., Bastieri, D., Bellazzini, R., Blandford, R. D., Bloom, E. D., Bonino, R., Bottacini, E., Brandt, T. J., Bruel, P., Buson, S., Caliandro, G. A., Cameron, R. A., Caragiulo, M., Caraveo, P. A., Cavazzuti, E., Charles, E., Chekhtman, A., Chiang, J., Chiaro, G., Ciprini, S., Cohen Tanugi, J., Cominsky, L. R., Costanza, F., Cuoco, A., D'Ammando, F., De Palma, F., Desiante, R., Digel, S. W., Di Lalla, N., Di Mauro, M., Di Venere, L., Domínguez, A., Drell, P. S., Dubois, R., Favuzzi, C., Ferrara, E. C., Franckowiak, A., Fukazawa, Y., Funk, S., Fusco, P., Gargano, F., Gasparrini, D., Giglietto, N., Giommi, P., Giordano, F., Giroletti, M., Glanzman, T., Godfrey, G., Gomez Vargas, G. A., Green, D., Grenier, I. A., Grove, J. E., Guiriec, S., Hadasch, D., Harding, A. K., Hays, E., Hewitt, J. W., Hill, A. B., Horan, D., Jogler, T., Jóhannesson, G., Johnson, A. S., Kensei, S., Kocevski, D., Kuss, M., La Mura, G., Larsson, S., Latronico, L., Li, J., Li, L., Longo, F., Loparco, F., Lovellette, M. N., Lubrano, P., Magill, J., Maldera, S., Manfreda, A., Marelli, M., Mayer, M., Mazziotta, M. N., Mcenery, J. E., Meyer, M., Michelson, P. F., Mirabal, N., Mizuno, T., Moiseev, A. A., Monzani, M. E., Moretti, E., Morselli, A., Moskalenko, I. V., Negro, M., Nuss, E., Ohsugi, T., Omodei, N., Orienti, M., Orlando, E., Ormes, J. F., Paneque, D., Perkins, J. S., Pesce Rollins, M., Piron, F., Pivato, G., Porter, T. A., Racusin, J. L., Rainò, S., Rando, R., Razzaque, S., Reimer, A., Reimer, O., Salvetti, D., Parkinson, P. M. Saz, Sgrò, C., Simone, D., Siskind, E. J., Spada, F., Spandre, G., Spinelli, P., Suson, D. J., Tajima, H., Thayer, J. B., Thompson, D. J., Tibaldo, L., Torres, D. F., Troja, E., Uchiyama, Y., Venters, T. M., Vianello, G., Wood, K. S., Wood, M., Zhu, S., Zimmer, S., Brocato, E., Cappellaro, E., Covino, S., Grado, A., Nicastro, L., Palazzi, E., Pian, E., Amati, L., Antonelli, L. A., Capaccioli, M., D'Avanzo, P., D'Elia, V., Getman, F., Giuffrida, G., Iannicola, G., Limatola, L., Lisi, M., Marinoni, S., Marrese, P., Melandri, A., Piranomonte, S., Possenti, A., Pulone, L., Rossi, A., Stamerra, A., Stella, L., Testa, V., Tomasella, L., Yang, S., Bazzano, A., Bozzo, E., Brandt, S., Courvoisier, T. J. L., Ferrigno, C., Hanlon, L., Kuulkers, E., Laurent, P., Mereghetti, S., Roques, J. P., Savchenko, V., Ubertini, P., Kasliwal, M. M., Singer, L. P., Cao, Y., Duggan, G., Kulkarni, S. R., Bhalerao, V., Miller, A. A., Barlow, T., Bellm, E., Manulis, I., Rana, J., Laher, R., Masci, F., Surace, J., Rebbapragada, U., Sistine, A. Van, Sesar, B., Perley, D., Ferreti, R., Prince, T., Kendrick, R., Horesh, A., Hurley, K., Golenetskii, S. V., Aptekar, R. L., Frederiks, D. D., Svinkin, D. S., Rau, A., Zhang, X., Smith, D. M., Cline, T., Krimm, H., Abe, F., Doi, M., Fujisawa, K., Kawabata, K. S., Morokuma, T., Motohara, K., Tanaka, M., Ohta, K., Yanagisawa, K., Yoshida, M., Baltay, C., Rabinowitz, D., Ellman, N., Rostami, S., Bersier, D. F., Bode, M. F., Collins, C. A., Copperwheat, C. M., Darnley, M. J., Galloway, Duncan K., Gomboc, A., Kobayashi, S., Mazzali, P., Mundell, C. G., Piascik, A. S., Pollacco, Don, Steele, I. A., Ulaczyk, K., Broderick, J. W., Fender, R. P., Jonker, P. G., Rowlinson, A., Stappers, B. W., Wijers, R. A. M. J., Lipunov, V., Gorbovskoy, E., Tyurina, N., Kornilov, V., Balanutsa, P., Kuznetsov, A., Buckley, D., Rebolo, R., Serra Ricart, M., Israelian, G., Budnev, N. M., Gress, O., Ivanov, K., Poleshuk, V., Tlatov, A., Yurkov, V., Kawai, N., Serino, M., Negoro, H., Nakahira, S., Mihara, T., Tomida, H., Ueno, S., Tsunemi, H., Matsuoka, M., Croft, S., Feng, L., Franzen, T. M. O., Gaensler, B. M., Johnston Hollitt, M., Kaplan, D. L., Morales, M. F., Tingay, S. J., Wayth, R. B., Williams, A., Smartt, S. J., Chambers, K. C., Smith, K. W., Huber, M. E., Young, D. R., Wright, D. E., Schultz, A., Denneau, L., Flewelling, H., Magnier, E. A., Primak, N., Rest, A., Sherstyuk, A., Stalder, B., Stubbs, C. W., Tonry, J., Waters, C., Willman, M., Olivares, E. F., Campbell, H., Kotak, R., Sollerman, J., Smith, M., Dennefeld, M., Anderson, J. P., Botticella, M. T., Chen, T. W., Valle, M. D., Elias Rosa, N., Fraser, M., Inserra, C., Kankare, E., Kupfer, T., Harmanen, J., Galbany, L., Guillou, L. Le, Lyman, J. D., Maguire, K., Mitra, A., Nicholl, M., Razza, A., Terreran, G., Valenti, S., Gal Yam, A., Ćwiek, A., Ćwiok, M., Mankiewicz, L., Opiela, R., Zaremba, M., Żarnecki, A. F., Onken, C. A., Scalzo, R. A., Schmidt, B. P., Wolf, C., Yuan, F., Evans, P. A., Kennea, J. A., Burrows, D. N., Campana, S., Cenko, S. B., Marshall, F. E., Nousek, J., O'Brien, P., Osborne, J. P., Palmer, D., Perri, M., Siegel, M., Tagliaferri, G., Klotz, A., Turpin, D., Laugier, R., Beroiz, M., Peñuela, T., Macri, L. M., Oelkers, R. J., Lambas, D. G., Vrech, R., Cabral, J., Colazo, C., Dominguez, M., Sanchez, B., Gurovich, S., Lares, M., Marshall, J. L., Depoy, D. L., Padilla, N., Pereyra, N. A., Benacquista, M., Tanvir, N. R., Wiersema, K., Levan, A. J., Steeghs, D., Hjorth, J., Fynbo, J. P. U., Malesani, D., Milvang Jensen, B., Watson, D., Irwin, M., Fernandez, C. G., Mcmahon, R. G., Banerji, M., Gonzalez Solares, E., Schulze, S., De Ugarte Postigo, A., Thoene, C. C., Cano, Z., Rosswog, S., Institut Lumière Matière [Villeurbanne] ( ILM ), Université Claude Bernard Lyon 1 ( UCBL ), Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique ( CNRS ), Laboratoire des matériaux avancés ( LMA ), 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 Leprince-Ringuet ( LLR ), Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -École polytechnique ( X ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire Univers et Particules de Montpellier ( LUPM ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Montpellier 2 - Sciences et Techniques ( UM2 ) -Université de Montpellier ( UM ), Laboratoire de Physique Nucléaire et de Hautes Énergies ( LPNHE ), Université Pierre et Marie Curie - Paris 6 ( UPMC ) -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 ), 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 ), 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 ), LIGO, VIRGO, FERMI LAT, PESSTO, Institut Lumière Matière [Villeurbanne] (ILM), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS), Laboratoire des matériaux avancés (LMA), 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 Leprince-Ringuet (LLR), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Univers et Particules de Montpellier (LUPM), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Université Pierre et Marie Curie - Paris 6 (UPMC)-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), 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), 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), The LIGO Scientific Collaboration, The Virgo Collaboration, The Australian Square Kilometer Array, Pathfinder (ASKAP) Collaboration, The BOOTES Collaboration, The Dark Energy Survey and the Dark Energy Camera GW-EM Collaborations, The Fermi GBM Collaboration, The Fermi LAT Collaboration, The GRAvitational Wave Inaf TeAm (GRAWITA), The Intermediate Palomar Transient Factory (iPTF) Collaboration, The InterPlanetary Network, The J-GEM Collaboration, The La Silla--QUEST Survey, The Liverpool Telescope Collaboration, The Low Frequency Array (LOFAR) Collaboration, The MASTER Collaboration, The MAXI Collaboration, The Murchison Wide-field Array (MWA) Collaboration, The Pan-STARRS Collaboration, The PESSTO Collaboration, The Pi of the Sky Collaboration, The SkyMapper Collaboration, The Swift Collaboration, The TAROT, Zadko, Algerian National Observatory, C2PU Collaboration, The TOROS Collaboration, The VISTA Collaboration, Calloni, E., De Laurentis, M., De Rosa, R., Garufi, F., Milano, L., Longo, Francesco, Centre National de la Recherche Scientifique (CNRS)-École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC), 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), Université Nice Sophia Antipolis (... - 2019) (UNS), 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), Université de Rennes 1 (UR1), Université de Rennes (UNIV-RENNES)-Université de Rennes (UNIV-RENNES)-Centre National de la Recherche Scientifique (CNRS), Chassande-Mottin, E., Cohadon, P. -. F., M. Constancio J. r., Coulon, J. -. P., D’Antonio, S., Eggenstein, H. -. B., Fournier, J. -. D., A., Gatto, Haster, C. -. J., Huynh-Dinh, T., Isac, J. -. M., Jiménez-Forteza, F., Kim, Y. -. M., Magaña-Sandoval, F., Masso-Reid, M., Mendoza-Gandara, D., C., Michel, Mow-Lowry, C. M., O’Dell, J., O’Reilly, B., O’Shaughnessy, R., Pal-Singh, A., Quitzow-James, R., A., Singh, van Bakel, N., van Beuzekom, M., van den Brand, J. F. J., Vander-Hyde, D. C., van der Schaaf, L., van Heijningen, J. V., van Veggel, A. A., Vinet, J. -. Y., M., Wade, Wei, L. -. W., Wessels, P., Zendri, J. -. P., the Virgo Collaboration, Harvey-Smith, L., Ian, Heywood, The Australian Square Kilometer Array Pathfinder (ASKAP) Collaboration, Castro-Tirado, A. J., Hu, Y. -. D., García-Cerezo, A., Pérez del Pulgar, C., Castillo-Carrión, S., Caballero-García, M. D., Mateo Sanguino, T. de J., Fernández-Muñoz, R., Sánchez-Ramírez, R., Sabau-Graziati, L., Benoit-Lévy, A., Buckley-Geer, E., D’Andrea, C. B., da Costa, L. N., Drlica-Wagner, A., Fong, W. -. F., Sevilla-Noarbe, I., Soares-Santos, M., The Dark Energy Survey, the Dark Energy Camera GW-EM Collaborations, Zhang, B. -. B., Wilson-Hodge, C. A., von Kienlin, A., Yu, H. -. F., Cohen-Tanugi, J., D’Ammando, F., de Palma, F., Gomez-Vargas, G. A., Pesce-Rollins, M., Saz Parkinson, P. M., D’Avanzo, P., D’Elia, V., Courvoisier, T. J. -. L., The INTEGRAL Collaboration, Van Sistine, A., The La Silla–QUEST Survey, Galloway, D. K., Don, Pollacco, Serra-Ricart, M., Johnston-Hollitt, M., F. Olivares E., Chen, T. -. W., Elias-Rosa, N., Le Guillou, L., Gal-Yam, A., O’Brien, P., The, Tarot, Zadko, Algerian National Observatory, C2pu, Collaboration, Milvang-Jensen, B., Gonzalez-Solares, E., Postigo, A. de U., High Energy Astrophys. & Astropart. Phys (API, FNWI), CALTECH, Louisiana State Univ, Univ Salerno, Complesso Univ Monte S.Angelo, Univ Florida, LIGO Livingston Observ, Univ Savoie Mont Blanc, Max Planck Inst Gravitat Phys, Nikhef, MIT, Inst Nacl Pesquisas Espaciais, Gran Sasso Sci Inst, Ist Nazl Fis Nucl, 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 Saclay, Chennai Math Inst, Univ Roma Tor Vergata, Univ Southampton, Univ Hamburg, Universidade de São Paulo (USP), Montana State Univ, Univ Perugia, Eur Gravitat Observ EGO, Syracuse Univ, Univ Glasgow, LIGO Hanford Observ, RMKI, NASA, Columbia Univ, Stanford Univ, Univ Padua, CAMK PAN, Univ Birmingham, Univ Genoa, RRCAT, Lomonosov Moscow State Univ, Univ West Scotland, Univ Western Australia, Radboud Univ Nijmegen, Univ Cote Azur, MTA Eotvos Univ, Univ Rennes 1, Washington State Univ, Univ Urbino Carlo Bo, Univ Oregon, ENS PSL Res Univ, Warsaw Univ, Vrije Univ Amsterdam, Univ Maryland, Georgia Inst Technol, Univ Claude Bernard Lyon 1, Univ Illes Balears, Univ Naples Federico II, Univ Toronto, Tsinghua Univ, Texas Tech Univ, Penn State Univ, Natl Tsing Hua Univ, Charles Sturt Univ, Univ Chicago, Korea Inst Sci & Technol Informat, Carleton Coll, Univ Roma La Sapienza, Univ Brussels, Sonoma State Univ, Northwestern Univ, Univ Minnesota, Univ Melbourne, Univ Texas Rio Grande Valley, Univ Sheffield, Univ Sannio Benevento, Montclair State Univ, Univ Trento, Cardiff Univ, Natl Astron Observ Japan, Univ Edinburgh, Indian Inst Technol, Inst Plasma Res, Univ Szeged, Embry Riddle Aeronaut Univ, Univ Michigan, Amer Univ, Univ Massachusetts, Univ Adelaide, W Virginia Univ, Univ Bialystok, Univ Strathclyde, IISER TVM, Inst Appl Phys, Pusan Natl Univ, Hanyang Univ, NCBJ, IM PAN, Rochester Inst Technol, Monash Univ, Seoul Natl Univ, Univ Alabama, CNRS, 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, Hobart & William Smith Coll, Univ Zielona Gora, Andrews Univ, Univ Siena, Trinity Univ, Univ Washington, Kenyon Coll, Abilene Christian Univ, CSIRO Astron & Space Sci, ARC Ctr Excellence All Sky Astrophys CAASTRO, Cornell Ctr Astrophys & Planetary Sci, Rhodes Univ, Univ Sydney, CSIC, Univ Malaga, Acad Sci Czech Republ, Nikolaev Natl Univ, ISDEFE SMOS FOS ESA ESAC, Czech Tech Univ, Estn Sondeos Atmosfer ESAt El Arenosillo CEDEA IN, Univ Huelva, UMA CSIC, Univ Auckland, Vintage Lane Observ, Natl Inst Water & Atmospher Res, Sungkyunkwan Univ, Chinese Acad Sci, Univ Nacl Autonoma Mexico, Aryabhatta Res Inst Observat Sci, Univ Cadiz, Inst Nacl Tecn Aerospacial INTA, Natl Opt Astron Observ, UCL, Fermilab Natl Accelerator Lab, Princeton Univ, UPMC Univ Paris 06, Harvard Smithsonian Ctr Astrophys, Carnegie Observ, Univ Penn, SLAC Natl Accelerator Lab, Univ Portsmouth, IEEC CSIC, Barcelona Inst Sci & Technol, Ohio Univ, Lab Interinst eAstron LIneA, Excellence Cluster Universe, Univ Munich, Univ Illinois, Univ Arizona, Los Alamos Natl Lab, Univ Calif Berkeley, Ohio State Univ, Australian Astron Observ, Texas A&M Univ, NYU, Inst Catalana Recerca & Estudis Avancats, Univ Sussex, Ctr Invest Energet Medioambientales & Tecnol, Brookhaven Natl Lab, Argonne Natl Lab, Univ Manchester, Univ Space Res Assoc, Jacobs Technol Inc, Max Planck Inst Extraterr Phys, Natl Univ Ireland Univ Coll Dublin, NASA Headquarters, Tech Univ Munich, Deutsch Elektr Synchrotron DESY, Clemson Univ, Stockholm Univ, AlbaNova, Univ Calif Santa Cruz, KTH Royal Inst Technol, Tokyo Metropolitan Univ, Univ Trieste, Univ Turin, Ecole Polytech, Univ Maryland Baltimore Cty, Consorzio Interuniv Fis Spaziale CIFS, Univ Bari, Politecn Bari, INAF Ist Astrofis Spaziale & Fis Cosm, Agenzia Spaziale Italiana ASI Sci Data Ctr, George Mason Univ, US Navy, Univ Montpellier, INAF Ist Radioastron, Univ Bologna, Univ Telemat Pegaso, Univ Udine, Hiroshima Univ, Erlangen Ctr Astroparticle Phys, Pontificia Univ Catolica Chile, Naval Res Lab, Leopold Franzens Univ Innsbruck, Univ North Florida, Univ Iceland, Inst Space Sci IEEC CSIC, Max Planck Inst Phys & Astrophys, Univ Denver, Univ Johannesburg, Univ Hong Kong, NYCB Real Time Comp Inc, Purdue Univ Calumet, Nagoya Univ, Max Planck Inst Kernphys, Inst Catalana Recerca & Estudis Avancats ICREA, Dept Phys, INAF Osservatorio Astron Roma, INAF Osservatorio Astron Padova, INAF Osservatorio Astron Brera, INAF Osservatorio Astron Capodimonte, INAF Ist Astrofis Spaziale & Fis Cosm Bologna, Scuola Normale Super Pisa, ASI Sci Data Ctr, INAF ORA Osservatorio Astron Cagliari, INAF Osservatorio Astron Torino, INAF Inst Space Astrophys & Planetol, Univ Geneva, DTU Space Natl Space Inst Elektrovej, Eur Space Astron Ctr ESA ESAC, IASF Milano, Univ Toulouse, Weizmann Inst Sci, Max Planck Inst Astron, Niels Bohr Inst, Lockheed Martin Space Syst Co, Ioffe Phys Tech Inst, Univ Tokyo, Yamaguchi Univ, Kyoto Univ, Yale Univ, Liverpool JMU, Univ Nova Gorica, Univ Ljubljana, Univ Bath, Univ Warwick, Netherlands Inst Radio Astron, Univ Oxford, SRON Netherlands Inst Space Res, Univ Amsterdam, South African Astron Observ, Inst Astrofis Canarias, Irkutsk State Univ, Main Pulkovo Observ RAS, Blagoveschensk State Pedag Univ, Tokyo Inst Technol, RIKEN, Nihon Univ, Japan Aerosp Explorat Agcy, Japan Aerosp Explorat Agcy JAXA, Osaka Univ, Eureka Sci Inc, Curtin Univ, Victoria Univ Wellington, and Ist Nazl Astrofis
Subjects: Astronomy, ADVANCED LIGO, 01 natural sciences, General Relativity and Quantum Cosmology, localization, GW150914, localization, EM follow-up, Observatory, Broadband, BURSTS, GeneralLiterature_REFERENCE(e.g.,dictionaries,encyclopedias,glossaries), 010303 astronomy & astrophysics, gravitational wave, QC, media_common, QB, Physics, astro-ph.HE, High Energy Astrophysical Phenomena (astro-ph.HE), gravitational waves, [PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], methods: observational, Astrophysics - High Energy Astrophysical Phenomena, Cosmology and Gravitation, [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], gravitational waves – methods: observational, media_common.quotation_subject, gr-qc, Astrophysics::High Energy Astrophysical Phenomena, GW150914, FOS: Physical sciences, ENERGY CAMERA SEARCH, General Relativity and Quantum Cosmology (gr-qc), NEUTRON-STAR MERGERS, Gravitational waves, [ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], Binary black hole, observational, Astronomy and Astrophysics, Space and Planetary Science [gravitational waves, methods], 0103 physical sciences, GW151226, observational [Methods], EM follow-up, STFC, RADIO, 010308 nuclear & particles physics, Gravitational wave, ST/I001123/1, RCUK, [ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], COUNTERPARTS, Astronomy and Astrophysic, LIGO, Neutron star, Space and Planetary Science, Sky, ST/L000709/1, EMISSION
Abstract: A gravitational-wave (GW) transient was identified in data recorded by the Advanced Laser Interferometer Gravitational-wave Observatory (LIGO) detectors on 2015 September 14. The event, initially designated G184098 and later given the name GW150914, is described in detail elsewhere. By prior arrangement, preliminary estimates of the time, significance, and sky location of the event were shared with 63 teams of observers covering radio, optical, near-infrared, X-ray, and gamma-ray wavelengths with ground- and space-based facilities. In this Letter we describe the low-latency analysis of the GW data and present the sky localization of the first observed compact binary merger. We summarize the follow-up observations reported by 25 teams via private Gamma-ray Coordinates Network circulars, giving an overview of the participating facilities, the GW sky localization coverage, the timeline and depth of the observations. As this event turned out to be a binary black hole merger, there is little expectation of a detectable electromagnetic (EM) signature. Nevertheless, this first broadband campaign to search for a counterpart of an Advanced LIGO source represents a milestone and highlights the broad capabilities of the transient astronomy community and the observing strategies that have been developed to pursue neutron star binary merger events. Detailed investigations of the EM data and results of the EM follow-up campaign are being disseminated in papers by the individual teams., Comment: For Supplement, see https://arxiv.org/abs/1604.07864
Published: 2016

Catalog

Books, media, physical & digital resources

See catalog results

Searchworks

Select search scope, currently: Articles Catalog books, media & more in Jio Institute collections Articles journal articles & other e-resources

Search

Search Constraints

Refine your results

Search Limiters

Topic

Publication Year Range

Language

Publication Type

Journal

Database

Publisher

39 results on '"Sault, R. J."'

Search Results

Catalog

Select search scope, currently: Articles

Catalog

books, media & more in Jio Institute collections

Articles

journal articles & other e-resources