Abbott, B. and Abbott, R. and Adhikari, Rana X. and Agresti, J. and Ajith, P. and Allen, B. and Amin, R. and Anderson, S. B. and Anderson, W. G. and Arain, M. and Araya, M. and Armandula, H. and Ashley, M. and Aston, S. and Aufmuth, P. and Aulbert, C. and Babak, S. and Ballmer, S. and Bantilan, H. and Barish, B. C. and Barker, C. and Barker, D. and Barr, B. W. and Barriga, P. and Barton, M. A. and Bayer, K. and Betzwieser, J. and Beyersdorf, P. T. and Bhawal, B. and Bilenko, I. A. and Billingsley, G. and Biswas, R. and Black, E. D. and Blackburn, K. and Blackburn, L. and Blair, D. and Bland, B. and Bogenstahl, J. and Bogue, L. and Bork, R. and Boschi, V. and Bose, S. and Brady, P. R. and Braginsky, V. B. and Brau, J. E. and Brinkmann, M. and Brooks, A. and Brown, D. A. and Bullington, A. and Bunkowski, A. and Buonanno, A. and Burmeister, O. and Busby, D. and Byer, R. L. and Cadonati, L. and Cagnoli, G. and Camp, J. B. and Cannizzo, J. and Cannon, K. and Cantley, C. A. and Cao, J. and Cardenas, L. and Castaldi, G. and Cepeda, C. and Chalkley, E. and Charlton, P. and Chatterji, S. and Chelkowski, S. and Chen, Y. and Chiadini, F. and Christensen, N. and Clark, J. and Cochrane, P. and Cokelaer, T. and Coldwell, R. and Conte, R. and Cook, D. and Corbitt, T. and Coyne, D. and Creighton, J. D. E. and Croce, R. P. and Crooks, D. R. M. and Cruise, A. M. and Cumming, A. and Dalrymple, J. and D'Ambrosio, E. and Danzmann, K. and Davies, G. and Debra, D. and Degallaix, J. and Degree, M. and Demma, T. and Dergachev, V. and Desai, S. and DeSalvo, R. and Dhurandhar, S. and Díaz, M. and Dickson, J. and Di Credico, A. and Diederichs, G. and Dietz, A. and Doomes, E. E. and Drever, R. W. P. and Dumas, J.-C. and Dupuis, R. J. and Dwyer, J. G. and Ehrens, P. and Espinoza, E. and Etzel, T. and Evans, M. and Evans, T. and Fairhurst, S. and Fan, Y. and Fazi, D. and Fejer, M. M. and Finn, L. S. and Fiumara, V. and Fotopoulos, N. and Franzen, A. and Franzen, K. Y. and Freise, A. and Frey, R. and Fricke, T. and Fritschel, P. and Frolov, V. V. and Fyffe, M. and Galdi, V. and Garofoli, J. and Gholami, I. and Giaime, J. A. and Giampanis, S. and Giardina, K. D. and Goda, K. and Goetz, E. and Goggin, L. M. and González, G. and Gossler, S. and Grant, A. and Gras, S. and Gray, C. and Gray, M. and Greenhalgh, J. and Gretarsson, A. M. and Grosso, R. and Grote, H. and Grunewald, S. and Guenther, M. and Gustafson, R. and Hage, B. and Hammer, D. and Hanna, C. and Hanson, J. and Harms, J. and Harry, G. and Harstad, E. and Hayler, T. and Heefner, J. and Heng, I. S. and Heptonstall, A. and Heurs, M. and Hewitson, M. and Hild, S. and Hirose, E. and Hoak, D. and Hosken, D. J. and Hough, J. and Hoyland, D. and Huttner, S. H. and Ingram, D. and Innerhofer, E. and Ito, M. and Itoh, Y. and Ivanov, A. and Johnson, B. and Johnson, W. W. and Jones, D. I. and Jones, G. and Jones, R. and Ju, L. and Kalmus, P. and Kalogera, V. and Kasprzyk, D. and Katsavounidis, E. and Kawabe, K. and Kawamura, S. and Kawazoe, F. and Kells, W. and Keppel, D. G. and Khalili, F. Ya. and Kim, C. and King, P. and Kissel, J. S. and Klimenko, S. and Kokeyama, K. and Kondrashov, V. and Kopparapu, R. K. and Kozak, D. and Krishnan, B. and Kwee, P. and Lam, P. K. and Landry, M. and Lantz, B. and Lazzarini, A. and Lei, M. and Leiner, J. and Leonhardt, V. and Leonor, I. and Libbrecht, K. and Lindquist, P. and Lockerbie, N. A. and Longo, M. and Lormand, M. and Lubinski, M. and Lück, H. and Machenschalk, B. and MacInnis, M. and Mageswaran, M. and Mailand, K. and Malec, M. and Mandic, V. and Marano, S. and Márka, S. and Markowitz, J. and Maros, E. and Martin, I. and Marx, J. N. and Mason, K. and Matone, L. and Matta, V. and Mavalvala, N. and McCarthy, R. and McClelland, D. E. and McGuire, S. C. and McHugh, M. and McKenzie, K. and McWilliams, S. and Meier, T. and Melissinos, A. and Mendell, G. and Mercer, R. A. and Meshkov, S. and Messenger, C. J. and Meyers, D. and Mikhailov, E. and Mitra, S. K. and Mitrofanov, V. P. and Mitselmakher, G. and Mittleman, R. and Miyakawa, O. and Mohanty, S. and Moreno, G. and Mossavi, K. and MowLowry, C. and Moylan, A. and Mudge, D. and Mueller, G. and Mukherjee, S. and Müller-Ebhardt, H. and Munch, J. and Murray, P. and Myers, E. B. and Myers, J. D. and Nash, T. and Newton, G. and Nishizawa, A. and Numata, K. and O'Reilly, B. and O'Shaughnessy, R. and Ottaway, D. J. and Overmier, H. and Owen, B. J. and Pan, Y. and Papa, M. A. and Parameshwaraiah, V. and Patel, P. and Pedraza, M. and Penn, S. and Pierro, V. and Pinto, I. M. and Pitkin, M. and Pletsch, H. J. and Plissi, M. V. and Postiglione, F. and Prix, R. and Quetschke, V. and Raab, F. and Rabeling, D. and Radkins, H. and Rahkola, R. and Rainer, N. and Rakhmanov, M. and Ramsunder, M. and Ray-Majumder, S. and Re, V. and Rehbein, H. and Reid, S. and Reitze, D. H. and Ribichini, L. and Riesen, R. and Riles, K. and Rivera, B. and Robertson, N. A. and Robinson, C. and Robinson, E. L. and Roddy, S. and Rodriguez, A. and Rogan, A. M. and Rollins, J. and Romano, J. D. and Romie, J. and Route, R. and Rowan, S. and Rüdiger, A. and Ruet, L. and Russell, P. and Ryan, K. and Sakata, S. and Samidi, M. and Sancho de la Jordana, L. and Sandberg, V. D. and Sannibale, V. and Saraf, S. and Sarin, P. and Sathyaprakash, B. S. and Sato, S. and Saulson, P. R. and Savage, R. and Savov, P. and Schediwy, S. W. and Schilling, R. and Schnabel, R. and Schofield, R. and Schutz, B. F. and Schwinberg, P. and Scott, S. M. and Searle, A. C. and Sears, B. and Seifert, F. and Sellers, D. and Sengupta, A. S. and Shawhan, P. and Shoemaker, D. H. and Sibley, A. and Siemens, X. and Sigg, D. and Sinha, S. and Sintes, A. M. and Slagmolen, B. J. J. and Slutsky, J. and Smith, J. R. and Smith, M. R. and Somiya, K. and Strain, K. A. and Strom, D. M. and Stuver, A. and Summerscales, T. Z. and Sun, K. -X. and Sung, M. and Sutton, P. J. and Takahashi, H. and Tanner, D. B. and Taylor, R. and Taylor, R. and Thacker, J. and Thorne, K. A. and Thorne, K. S. and Thuering, A. and Tokmakov, K. V. and Torres, C. and Torrie, C. and Traylor, G. and Trias, M. and Tyler, W. and Ugolini, D. and Urbanek, K. and Vahlbruch, H. and Vallisneri, M. and Van Den Broeck, C. and Varvella, M. and Vass, S. and Vecchio, A. and Veitch, J. and Veitch, P. J. and Villar, A. and Vorvick, C. and Vyachanin, S. P. and Waldman, S. J. and Wallace, L. and Ward, H. and Ward, R. and Watts, K. and Weidner, A. and Weinert, M. and Weiss, R. and Wen, S. and Wette, K. and Whelan, J. T. and Whitcomb, S. E. and Whiting, B. F. and Wilkinson, C. and Willems, P. A. and Williams, L. and Willke, B. and Wilmut, I. and Winkler, W. and Wipf, C. C. and Wise, S. and Wiseman, A. G. and Woan, G. and Woods, D. and Wooley, R. and Worden, J. and Wu, W. and Yakushin, I. and Yamamoto, H. and Yan, Z. and Yoshida, S. and Yunes, N. and Zanolin, M. and Zhang, J. and Zhang, L. and Zhao, C. and Zotov, N. and Zucker, M. and zur-Mühlen, H. and Zweizig, J. and Hurley, K. C. and Weinstein, Alan J.
Implications for the origin of GRB 070201 from LIGO observations.
Astrophysical Journal, 681
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We analyzed the available LIGO data coincident with GRB 070201, a short-duration, hard-spectrum gamma-ray burst (GRB) whose electromagnetically determined sky position is coincident with the spiral arms of the Andromeda galaxy (M31). Possible progenitors of such short, hard GRBs include mergers of neutron stars or a neutron star and a black hole, or soft gamma-ray repeater (SGR) flares. These events can be accompanied by gravitational-wave emission. No plausible gravitational-wave candidates were found within a 180s long window around the time of GRB 070201. This result implies that a compact binary progenitor of GRB 070201, with masses in the range 1M☉ < m1 < 3M☉ and 1M☉ < m2 < 40M☉, located in M31 is excluded at > 99% confidence. If the GRB 070201 progenitor was not in M31, then we can exclude a binary neutron star merger progenitor with distance D < 3.5 Mpc, assuming random inclination, at 90% confidence. The result also implies that an unmodeled gravitational-wave burst from GRB 070201 most probably emitted less than 4.4×10^(-4) M☉c^2 (7.9×10^50 ergs) in any 100 ms long period within the signal region if the source was in M31 and radiated isotropically at the same frequency as LIGO's peak sensitivity (f ≈ 150 Hz). This upper limit does not exclude current models of SGRs at the M31 distance.
|Additional Information:||© 2008. The American Astronomical Society.
Received 2007 December 1; accepted 2008 January 6.
We are indebted to the observers of the electromagnetic event, GCN and IPN, for providing us with valuable data and real-time information. We are grateful to Neil Gehrels of NASA/GSFC for his help in reviewing the article.
We are grateful to the GALEX collaboration for providing
the UV image of M31, the SDSS project for providing the optical image of M31, and Google Sky for accelerating the error box position verification.
Color Figures online|
|Funding Agency||Grant Number|
|National Science Foundation||UNSPECIFIED|
|Science and Technology Facilities Council (STFC) (UK)||UNSPECIFIED|
|Max Planck Society||UNSPECIFIED|
|State of Niedersachsen (Germany)||UNSPECIFIED|
|Australian Research Council||UNSPECIFIED|
|Council of Scientiﬁc and Industrial Research (India)||UNSPECIFIED|
|Istituto Nazionale di Fisica Nucleare (Italy)||UNSPECIFIED|
|Ministerio de Educación y Ciencia (Spain)||UNSPECIFIED|
|Conselleria d’Economia,Hisenda i Innovació of the Govern de les Illes Balears||UNSPECIFIED|
|Scottish Universities Physics Alliance||UNSPECIFIED|
|Scottish Funding Council||UNSPECIFIED|
|David and Lucile Packard Foundation||UNSPECIFIED|
|Alfred P. Sloan Foundation||UNSPECIFIED|
|Subject Keywords:||gamma rays: bursts; gravitational waves; methods: data analysis|
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|Usage Policy:||No commercial reproduction, distribution, display or performance rights in this work are provided.|
|Deposited On:||09 Jan 2009 06:07|
|Last Modified:||23 Mar 2015 20:22|
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