1. Implications for the Origin of GRB 051103 from LIGO Observations
- Author
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The LIGO Scientific Collaboration, Abadie, J., Abbott, B. P., Abbott, T. D., Abbott, R., Abernathy, M., Adams, C., Adhikari, R., Affeldt, C., Ajith, P., Allen, B., Allen, G. S., Ceron, E. Amador, Amariutei, D., Amin, R. S., Anderson, S. B., Anderson, W. G., Arai, K., Arain, M. A., Araya, M. C., Aston, S. M., Atkinson, D., Aufmuth, P., Aulbert, C., Aylott, B. E., Babak, S., Baker, P., Ballmer, S., Barker, D., Barnum, S., Barr, B., Barriga, P., Barsotti, L., Barton, M. A., Bartos, I., Bassiri, R., Bastarrika, M., Bauchrowitz, J., Behnke, B., Bell, A. S., Belopolski, I., Benacquista, M., Bertolini, A., Betzwieser, J., Beveridge, N., Beyersdorf, P. T., Bilenko, I. A., Billingsley, G., Birch, J., Biswas, R., Black, E., Blackburn, J. K., Blackburn, L., Blair, D., Bland, B., Bock, O., Bodiya, T. P., Bogan, C., Bondarescu, R., Bork, R., Born, M., Bose, S., Boyle, M., Brady, P. R., Braginsky, V. B., Brau, J. E., Breyer, J., Bridges, D. O., Brinkmann, M., Britzger, M., Brooks, A. F., Brown, D. A., Brummitt, A., Buonanno, A., Burguet-Castell, J., Burmeister, O., Byer, R. L., Cadonati, L., Camp, J. B., Campsie, P., Cannizzo, J., Cannon, K., Cao, J., Capano, C., Caride, S., Caudill, S., Cavaglia, M., Cepeda, C., Chalermsongsak, T., Chalkley, E., Charlton, P., Chelkowski, S., Chen, Y., Christensen, N., Chua, S. S. Y., Chung, S., Chung, C. T. Y., Clara, F., Clark, D., Clark, J., Clayton, J. H., Conte, R., Cook, D., Corbitt, T. R. C., Cornish, N., Costa, C. A., Coughlin, M., Coward, D. M., Coyne, D. C., Creighton, J. D. E., Creighton, T. D., Cruise, A. M., Cumming, A., Cunningham, L., Culter, R. M., Dahl, K., Danilishin, S. L., Dannenberg, R., Danzmann, K., Das, K., Daudert, B., Daveloza, H., Davies, G., Daw, E. J., Dayanga, T., DeBra, D., Degallaix, J., Dent, T., Dergachev, V., DeRosa, R., DeSalvo, R., Dhurandhar, S., Di Palma, I., Diaz, M., Donovan, F., Dooley, K. L., Dorsher, S., Douglas, E. S. D., Drever, R. W. P., Driggers, J. C., Dumas, J. -C., Dwyer, S., Eberle, T., Edgar, M., Edwards, M., Effler, A., Ehrens, P., Engel, R., Etzel, T., Evans, M., Evans, T., Factourovich, M., Fairhurst, S., Fan, Y., Farr, B. F., Fazi, D., Fehrmann, H., Feldbaum, D., Finn, L. S., Flanigan, M., Foley, S., Forsi, E., Fotopoulos, N., Frede, M., Frei, M., Frei, Z., Freise, A., Frey, R., Fricke, T. T., Friedrich, D., Fritschel, P., Frolov, V. V., Fulda, P., Fyffe, M., Garcia, J., Garofoli, J. A., Gholami, I., Ghosh, S., Giaime, J. A., Giampanis, S., Giardina, K. D., Gill, C., Goetz, E., Goggin, L. M., Gonzalez, G., Gorodetsky, M. L., Gossler, S., Graef, C., Grant, A., Gras, S., Gray, C., Greenhalgh, R. J. S., Gretarsson, A. M., Grosso, R., Grote, H., Grunewald, S., Guido, C., Gupta, R., Gustafson, E. K., Gustafson, R., Hage, B., Hallam, J. M., Hammer, D., Hammond, G., Hanks, J., Hanna, C., Hanson, J., Harms, J., Harry, G. M., Harry, I. W., Harstad, E. D., Hartman, M. T., Haughian, K., Hayama, K., Heefner, J., Hendry, M. A., Heng, I. S., Heptonstall, A. W., Herrera, V., Hewitson, M., Hild, S., Hoak, D., Hodge, K. A., Holt, K., Hong, T., Hooper, S., Hosken, D. J., Hough, J., Howell, E. J., Hughey, B., Husa, S., Huttner, S. H., Ingram, D. R., Inta, R., Isogai, T., Ivanov, A., Johnson, W. W., Jones, D. I., Jones, G., Jones, R., Ju, L., Kalmus, P., Kalogera, V., Kandhasamy, S., Kanner, J. B., Katsavounidis, E., Katzman, W., Kawabe, K., Kawamura, S., Kawazoe, F., Kells, W., Kelner, M., Keppel, D. G., Khalaidovski, A., Khalili, F. Y., Khazanov, E. A., Kim, N., Kim, H., King, P. J., Kinzel, D. L., Kissel, J. S., Klimenko, S., Kondrashov, V., Kopparapu, R., Koranda, S., Korth, W. Z., Kozak, D., Kringel, V., Krishnamurthy, S., Krishnan, B., Kuehn, G., Kumar, R., Kwee, P., Landry, M., Lantz, B., Lastzka, N., Lazzarini, A., Leaci, P., Leong, J., Leonor, I., Li, J., Lindquist, P. E., Lockerbie, N. A., Lodhia, D., Lormand, M., Lu, P., Luan, J., Lubinski, M., Luck, H., Lundgren, A. P., Macdonald, E., Machenschalk, B., MacInnis, M., Mageswaran, M., Mailand, K., Mandel, I., Mandic, V., Marandi, A., Marka, S., Marka, Z., Maros, E., Martin, I. W., Martin, R. M., Marx, J. N., Mason, K., Matichard, F., Matone, L., Matzner, R. A., Mavalvala, N., McCarthy, R., McClelland, D. E., McGuire, S. C., McIntyre, G., McIver, J., McKechan, D. J. A., Meadors, G., Mehmet, M., Meier, T., Melatos, A., Melissinos, A. C., Mendell, G., Mercer, R. A., Meshkov, S., Messenger, C., Meyer, M. S., Miao, H., Miller, J., Mino, Y., Mitrofanov, V. P., Mitselmakher, G., Mittleman, R., Miyakawa, O., Moe, B., Moesta, P., Mohanty, S. D., Moraru, D., Moreno, G., Mossavi, K., Mow-Lowry, C. M., Mueller, G., Mukherjee, S., Mullavey, A., Muller-Ebhardt, H., Munch, J., Murphy, D., Murray, P. G., Nash, T., Nawrodt, R., Nelson, J., Newton, G., Nishizawa, A., Nolting, D., Nuttall, L., O'Reilly, B., O'Shaughnessy, R., Ochsner, E., O'Dell, J., Ogin, G. H., Oldenburg, R. G., Osthelder, C., Ott, C. D., Ottaway, D. J., Ottens, R. S., Overmier, H., Owen, B. J., Page, A., Pan, Y., Pankow, C., Papa, M. A., Patel, P., Pedraza, M., Pekowsky, L., Penn, S., Peralta, C., Perreca, A., Phelps, M., Pickenpack, M., Pinto, I. M., Pitkin, M., Pletsch, H. J., Plissi, M. V., Podkaminer, J., Pold, J., Postiglione, F., Predoi, V., Price, L. R., Prijatelj, M., Principe, M., Privitera, S., Prix, R., Prokhorov, L., Puncken, O., Quetschke, V., Raab, F. J., Radkins, H., Raffai, P., Rakhmanov, M., Ramet, C. R., Rankins, B., Mohapatra, S. R. P., Raymond, V., Redwine, K., Reed, C. M., Reed, T., Reid, S., Reitze, D. H., Riesen, R., Riles, K., Roberts, P., Robertson, N. A., Robinson, C., Robinson, E. L., Roddy, S., Rollins, J., Romano, J. D., Romie, J. H., Rover, C., Rowan, S., Rudiger, A., Ryan, K., Sakata, S., Sakosky, M., Salemi, F., Salit, M., Sammut, L., de la Jordana, L. Sancho, Sandberg, V., Sannibale, V., SantamarÌa, L., Santiago-Prieto, I., Santostasi, G., Saraf, S., Sathyaprakash, B. S., Sato, S., Saulson, P. R., Savage, R., Schilling, R., Schlamminger, S., Schnabel, R., Schofield, R. M. S., Schulz, B., Schutz, B. F., Schwinberg, P., Scott, J., Scott, S. M., Searle, A. C., Seifert, F., Sellers, D., Sengupta, A. S., Sergeev, A., Shaddock, D. A., Shaltev, M., Shapiro, B., Shawhan, P., Weerathunga, T. Shihan, Shoemaker, D. H., Sibley, A., Siemens, X., Sigg, D., Singer, A., Singer, L., Sintes, A. M., Skelton, G., Slagmolen, B. J. J., Slutsky, J., Smith, R., Smith, J. R., Smith, M. R., Smith, N. D., Somiya, K., Sorazu, B., Soto, J., Speirits, F. C., Stein, A. J., Steinlechner, J., Steinlechner, S., Steplewski, S., Stefszky, M., Stochino, A., Stone, R., Strain, K. A., Strigin, S., Stroeer, A. S., Stuver, A. L., Summerscales, T. Z., Sung, M., Susmithan, S., Sutton, P. J., Szokoly, G. P., Talukder, D., Tanner, D. B., Tarabrin, S. P., Taylor, J. R., Taylor, R., Thomas, P., Thorne, K. A., Thorne, K. S., Thrane, E., Thuring, A., Tokmakov, K. V., Torres, C., Torrie, C. I., Traylor, G., Trias, M., Tseng, K., Ugolini, D., Urbanek, K., Vahlbruch, H., Vaishnav, B., Vallisneri, M., Broeck, C. Van Den, van der Sluys, M. V., van Veggel, A. A., Vass, S., Vaulin, R., Vecchio, A., Veitch, J., Veitch, P. J., Veltkamp, C., Villar, A. E., Vorvick, C., Vyachanin, S. P., Waldman, S. J., Wallace, L., Wanner, A., Ward, R. L., Wei, P., Weinert, M., Weinstein, A. J., Weiss, R., Wen, L., Wen, S., Wessels, P., West, M., Westphal, T., Wette, K., Whelan, J. T., Whitcomb, S. E., White, D., Whiting, B. F., Wilkinson, C., Willems, P. A., Williams, H. R., Williams, L., Willke, B., Winkelmann, L., Winkler, W., Wipf, C. C., Wiseman, A. G., Woan, G., Wooley, R., Worden, J., Yablon, J., Yakushin, I., Yamamoto, K., Yamamoto, H., Yang, H., Yeaton-Massey, D., Yoshida, S., Yu, P., Zanolin, M., Zhang, L., Zhang, Z., Zhao, C., Zotov, N., Zucker, M. E., Zweizig, J., Bizouard, M. A., Dietz, A., Guidi, G. M., Was, M., Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), LIGO, LVC Collaboration, The, Pinto, I. M., and Principe, M.
- Subjects
[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE] ,Astrophysics::High Energy Astrophysical Phenomena ,SCIENCE RUN ,Soft gamma repeater ,FOS: Physical sciences ,Astrophysics ,General Relativity and Quantum Cosmology (gr-qc) ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Compact star ,Magnetar ,01 natural sciences ,ENERGETICS ,General Relativity and Quantum Cosmology ,gamma-ray burst: individual (GRB 051103) ,stars: magnetars ,SEARCH ,0103 physical sciences ,magnetars [stars] ,Astrophysics::Solar and Stellar Astrophysics ,SHORT-DURATION ,010303 astronomy & astrophysics ,QC ,Astrophysics::Galaxy Astrophysics ,QB ,REPEATER ,Physics ,GAMMA-RAY BURSTS ,High Energy Astrophysical Phenomena (astro-ph.HE) ,Spiral galaxy ,individual (GRB 051103) [gamma-ray burst] ,010308 nuclear & particles physics ,Gravitational wave ,[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE] ,Astronomy and Astrophysics ,individual (GRB 051103) ,gravitational waves ,stars: magnetars [gamma-ray burst] ,LIGO ,GIANT FLARES ,Neutron star ,JET BREAKS ,GRB-051103 ,Space and Planetary Science ,GRAVITATIONAL-WAVE BURSTS ,[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc] ,Gamma-ray burst ,Astrophysics - High Energy Astrophysical Phenomena - Abstract
We present the results of a LIGO search for gravitational waves (GWs) associated with GRB 051103, a short-duration hard-spectrum gamma-ray burst (GRB) whose electromagnetically determined sky position is coincident with the spiral galaxy M81, which is 3.6 Mpc from Earth. Possible progenitors for short-hard GRBs include compact object mergers and soft gamma repeater (SGR) giant flares. A merger progenitor would produce a characteristic GW signal that should be detectable at the distance of M81, while GW emission from an SGR is not expected to be detectable at that distance. We found no evidence of a GW signal associated with GRB 051103. Assuming weakly beamed gamma-ray emission with a jet semi-angle of 30 deg we exclude a binary neutron star merger in M81 as the progenitor with a confidence of 98%. Neutron star-black hole mergers are excluded with > 99% confidence. If the event occurred in M81 our findings support the the hypothesis that GRB 051103 was due to an SGR giant flare, making it the most distant extragalactic magnetar observed to date., 8 pages, 3 figures. For a repository of data used in the publication, go to: https://dcc.ligo.org/cgi-bin/DocDB/ShowDocument?docid=15166 . Also see the announcement for this paper on ligo.org at: http://www.ligo.org/science/Publication-GRB051103/index.php
- Published
- 2012