Search for Gravitational Waves Associated with γ-ray Bursts Detected by the Interplanetary Network

Search for Gravitational Waves Associated with γ-ray Bursts Detected by the Interplanetary Network. Aasi, J., Abbott, B., P., Abbott, R., Abbott, T., Abernathy, M., R., Acernese, F., Ackley, K., Adams, C., Adams, T., Addesso, P., Adhikari, R., X., Affeldt, C., Agathos, M., Aggarwal, N., Aguiar, O., D., Ajith, P., Alemic, A., Allen, B., Allocca, A., Amariutei, D., Andersen, M., Anderson, R., A., Anderson, S., B., Anderson, W., G., Arai, K., Araya, M., C., Arceneaux, C., Areeda, J., S., Ast, S., Aston, S., M., Astone, P., Aufmuth, P., Augustus, H., Aulbert, C., Aylott, B., E., Babak, S., Baker, P., T., Ballardin, G., Ballmer, S., W., Barayoga, J., C., Barbet, M., Barish, B., C., Barker, D., Barone, F., Barr, B., Barsotti, L., Barsuglia, M., Barton, M., A., Bartos, I., Bassiri, R., Basti, A., Batch, J., C., Bauchrowitz, J., Bauer, T., S., Baune, C., Bavigadda, V., Behnke, B., Bejger, M., Beker, M., G., Belczynski, C., Bell, A., S., Bell, C., Bergmann, G., Bersanetti, D., Bertolini, A., Betzwieser, J., Bilenko, I., A., Billingsley, G., Birch, J., Biscans, S., Bitossi, M., Biwer, C., Bizouard, M., A., Black, E., Blackburn, J., K., Blackburn, L., Blair, D., Bloemen, S., Bock, O., Bodiya, T., P., Boer, M., Bogaert, G., Bogan, C., Bond, C., Bondu, F., Bonelli, L., Bonnand, R., Bork, R., Born, M., Boschi, V., Bose, S., Bosi, L., Bradaschia, C., Brady, P., R., Braginsky, V., B., Branchesi, M., Brau, J., E., Briant, T., Bridges, D., O., Brillet, A., Brinkmann, M., Brisson, V., Brooks, A., F., Brown, D., A., Brown, D., D., Brückner, F., Buchman, S., Buikema, A., Bulik, T., Bulten, H., J., Buonanno, A., Burman, R., Buskulic, D., Buy, C., Cadonati, L., Cagnoli, G., Calderón Bustillo, J., Calloni, E., Camp, J., B., Campsie, P., Cannon, K., C., Canuel, B., Cao, J., Capano, C., D., Carbognani, F., Carbone, L., Caride, S., Castaldi, G., Caudill, S., Cavaglià, M., Cavalier, F., Cavalieri, R., Celerier, C., Cella, G., Cepeda, C., Cesarini, E., Chakraborty, R., Chalermsongsak, T., Chamberlin, S., J., Chao, S., Charlton, P., Chassande-Mottin, E., Chen, X., Chen, Y., Chincarini, A., Chiummo, A., Cho, H., S., Cho, M., Chow, J., H., Christensen, N., Chu, Q., Chua, S., S., Y., Chung, S., Ciani, G., Clara, F., Clark, D., E., Clark, J., A., Clayton, J., H., Cleva, F., Coccia, E., Cohadon, P., Colla, A., Collette, C., Colombini, M., Cominsky, L., Constancio, M., Conte, A., Cook, D., Corbitt, T., R., Cornish, N., Corsi, A., Costa, C., A., Coughlin, M., W., Coulon, J., Countryman, S., Couvares, P., Coward, D., M., Cowart, M., J., Coyne, D., C., Coyne, R., Craig, K., Creighton, J., D., E., Croce, R., P., Crowder, S., G., Cumming, A., Cunningham, L., Cuoco, E., Cutler, C., Dahl, K., Dal Canton, T., Damjanic, M., Danilishin, S., L., D’Antonio, S., Danzmann, K., Dattilo, V., Daveloza, H., Davier, M., Davies, G., S., Daw, E., J., Day, R., Dayanga, T., DeBra, D., Debreczeni, G., Degallaix, J., Deléglise, S., Del Pozzo, W., Denker, T., Dent, T., Dereli, H., Dergachev, V., De Rosa, R., DeRosa, R., T., DeSalvo, R., Dhurandhar, S., Díaz, M., Dickson, J., Di Fiore, L., Di Lieto, A., Di Palma, I., Di Virgilio, A., Dolique, V., Dominguez, E., 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., Eberle, T., Edo, T., Edwards, M., Effler, A., Eggenstein, H., Ehrens, P., Eichholz, J., Eikenberry, S., S., Endrőczi, G., Essick, R., Etzel, T., Evans, M., Evans, T., Factourovich, M., Fafone, V., Fairhurst, S., Fan, X., Fang, Q., Farinon, S., Farr, B., Farr, W., M., Favata, M., Fazi, D., Fehrmann, H., Fejer, M., M., Feldbaum, D., Feroz, F., Ferrante, I., Ferreira, E., C., Ferrini, F., Fidecaro, F., Finn, L., S., Fiori, I., Fisher, R., P., Flaminio, R., Fournier, J., Franco, S., Frasca, S., Frasconi, F., Frede, M., Frei, Z., Freise, A., Frey, R., Fricke, T., T., Fritschel, P., Frolov, V., V., Fulda, P., Fyffe, M., Gair, J., R., Gammaitoni, L., Gaonkar, S., Garufi, F., Gehrels, N., Gemme, G., Gendre, B., Genin, E., Gennai, A., Ghosh, S., Giaime, J., A., Giardina, K., D., Giazotto, A., Gleason, J., Goetz, E., Goetz, R., Gondan, L., González, G., Gordon, N., Gorodetsky, M., L., Gossan, S., Goßler, S., Gouaty, R., Gräf, C., Graff, P., B., Granata, M., Grant, A., Gras, S., Gray, C., Greenhalgh, R., J., S., Gretarsson, A., M., Groot, P., Grote, H., Grover, K., Grunewald, S., Guidi, G., M., Guido, C., J., Gushwa, K., Gustafson, E., K., Gustafson, R., Ha, J., Hall, E., D., Hamilton, W., Hammer, D., Hammond, G., Hanke, M., Hanks, J., Hanna, C., Hannam, M., D., Hanson, J., Harms, J., Harry, G., M., Harry, I., W., Harstad, E., D., Hart, M., Hartman, M., T., Haster, C., Haughian, K., Heidmann, A., Heintze, M., Heitmann, H., Hello, P., Hemming, G., Hendry, M., Heng, I., S., Heptonstall, A., W., Heurs, M., Hewitson, M., Hild, S., Hoak, D., Hodge, K., A., Hofman, D., Holt, K., Hopkins, P., Horrom, T., Hoske, D., Hosken, D., J., Hough, J., Howell, E., J., Hu, Y., Huerta, E., Hughey, B., Husa, S., Huttner, S., H., Huynh, M., Huynh-Dinh, T., Idrisy, A., Ingram, D., R., Inta, R., Islas, G., Isogai, T., Ivanov, A., Iyer, B., R., Izumi, K., Jacobson, M., Jang, H., Jaranowski, P., Ji, Y., Jiménez-Forteza, F., Johnson, W., W., Jones, D., I., Jones, R., Jonker, R., J., G., Ju, L., K., H., Kalmus, P., Kalogera, V., Kandhasamy, S., Kang, G., Kanner, J., B., Karlen, J., Kasprzack, M., Katsavounidis, E., Katzman, W., Kaufer, H., Kaufer, S., Kaur, T., Kawabe, K., Kawazoe, F., Kéfélian, F., Keiser, G., M., Keitel, D., Kelley, D., B., Kells, W., Keppel, D., G., Khalaidovski, A., Khalili, F., Y., Khazanov, E., A., Kim, C., Kim, K., Kim, N., G., Kim, N., Kim, S., Kim, Y., King, E., J., King, P., J., Kinzel, D., L., Kissel, J., S., Klimenko, S., Kline, J., Koehlenbeck, S., Kokeyama, K., Kondrashov, V., Koranda, S., Korth, W., Z., Kowalska, I., Kozak, D., B., Kringel, V., Krishnan, B., Królak, A., Kuehn, G., Kumar, A., Kumar, D., N., Kumar, P., Kumar, R., Kuo, L., Kutynia, A., Lam, P., K., Landry, M., Lantz, B., Larson, S., Lasky, P., D., Lazzarini, A., Lazzaro, C., Leaci, P., Leavey, S., Lebigot, E., O., Lee, C., H., Lee, H., K., Lee, H., M., Lee, J., Lee, P., J., Leonardi, M., Leong, J., R., Leonor, I., Le Roux, A., Leroy, N., Letendre, N., Levin, Y., Levine, B., Lewis, J., Li, T., G., F., Libbrecht, K., Libson, A., Lin, A., C., Littenberg, T., B., Lockerbie, N., A., Lockett, V., Lodhia, D., Loew, K., Logue, J., Lombardi, A., L., Lopez, E., Lorenzini, M., Loriette, V., Lormand, M., Losurdo, G., Lough, J., Lubinski, M., J., Lück, H., Lundgren, A., P., Ma, Y., Macdonald, E., P., MacDonald, T., Machenschalk, B., MacInnis, M., Macleod, D., M., Magaña-Sandoval, F., Magee, R., Mageswaran, M., Maglione, C., Mailand, K., Majorana, E., Maksimovic, I., Malvezzi, V., Man, N., Manca, G., M., Mandel, I., Mandic, V., Mangano, V., Mangini, N., M., Mansell, G., Mantovani, M., Marchesoni, F., Marion, F., Márka, S., Márka, Z., Markosyan, A., Maros, E., Marque, J., Martelli, F., Martin, I., W., Martin, R., M., Martinelli, L., Martynov, D., Marx, J., N., Mason, K., Masserot, A., Massinger, T., J., Matichard, F., Matone, L., Mavalvala, N., May, G., Mazumder, N., Mazzolo, G., McCarthy, R., McClelland, D., E., McGuire, S., C., McIntyre, G., McIver, J., McLin, K., Meacher, D., Meadors, G., D., Mehmet, M., Meidam, J., Meinders, M., Melatos, A., Mendell, G., Mercer, R., A., Meshkov, S., Messenger, C., Meyer, M., S., Meyers, P., M., Mezzani, F., Miao, H., Michel, C., Mikhailov, E., E., Milano, L., Miller, J., Minenkov, Y., Mingarelli, C., M., F., Mishra, C., Mitra, S., Mitrofanov, V., P., Mitselmakher, G., Mittleman, R., Moe, B., Moggi, A., Mohan, M., Mohapatra, S., R., P., Moraru, D., Moreno, G., Morgado, N., Morriss, S., R., Mossavi, K., Mours, B., Mow-Lowry, C., M., Mueller, C., L., Mueller, G., Mukherjee, S., Mullavey, A., Munch, J., Murphy, D., Murray, P., G., Mytidis, A., Nagy, M., F., Nardecchia, I., Naticchioni, L., Nayak, R., K., Necula, V., Nelemans, G., Neri, I., Neri, M., Newton, G., Nguyen, T., Nielsen, A., B., Nissanke, S., Nitz, A., H., Nocera, F., Nolting, D., Normandin, M., E., N., Nuttall, L., K., Ochsner, E., O’Dell, J., Oelker, E., Oh, J., J., Oh, S., H., Ohme, F., Omar, S., Oppermann, P., Oram, R., O’Reilly, B., Ortega, W., O’Shaughnessy, R., Osthelder, C., Ottaway, D., J., Ottens, R., S., Overmier, H., Owen, B., J., Padilla, C., Pai, A., Palashov, O., Palomba, C., Pan, H., Pan, Y., Pankow, C., Paoletti, F., Papa, M., A., Paris, H., Pasqualetti, A., Passaquieti, R., Passuello, D., Pedraza, M., Pele, A., Penn, S., Perreca, A., Phelps, M., Pichot, M., Pickenpack, M., Piergiovanni, F., Pierro, V., Pinard, L., Pinto, I., M., Pitkin, M., Poeld, J., Poggiani, R., Poteomkin, A., Powell, J., Prasad, J., Predoi, V., Premachandra, S., Prestegard, T., Price, L., R., Prijatelj, M., Privitera, S., Prodi, G., A., Prokhorov, L., Puncken, O., Punturo, M., Puppo, P., Pürrer, M., Qin, J., Quetschke, V., Quintero, E., Quitzow-James, R., Raab, F., J., Rabeling, D., S., Rácz, I., Radkins, H., Raffai, P., Raja, S., Rajalakshmi, G., Rakhmanov, M., Ramet, C., Ramirez, K., Rapagnani, P., Raymond, V., Razzano, M., Re, V., Recchia, S., Reed, C., M., Regimbau, T., Reid, S., Reitze, D., H., Reula, O., Rhoades, E., Ricci, F., Riesen, R., Riles, K., Robertson, N., A., Robinet, F., Rocchi, A., Roddy, S., B., Rolland, L., Rollins, J., G., Romano, R., Romanov, G., Romie, J., H., Rosińska, D., Rowan, S., Rüdiger, A., Ruggi, P., Ryan, K., Salemi, F., Sammut, L., Sandberg, V., Sanders, J., R., Sankar, S., Sannibale, V., Santiago-Prieto, I., Saracco, E., Sassolas, B., Sathyaprakash, B., S., Saulson, P., R., Savage, R., Scheuer, J., Schilling, R., Schilman, M., Schmidt, P., Schnabel, R., Schofield, R., M., S., Schreiber, E., Schuette, D., Schutz, B., F., Scott, J., Scott, S., M., Sellers, D., Sengupta, A., S., Sentenac, D., Sequino, V., Sergeev, A., Shaddock, D., A., Shah, S., Shahriar, M., S., Shaltev, M., Shao, Z., Shapiro, B., Shawhan, P., Shoemaker, D., H., Sidery, T., L., Siellez, K., Siemens, X., Sigg, D., Simakov, D., Singer, A., Singer, L., Singh, R., Sintes, A., M., Slagmolen, B., J., J., Slutsky, J., Smith, J., R., Smith, M., R., Smith, R., J., E., Smith-Lefebvre, N., D., Son, E., J., Sorazu, B., Souradeep, T., Staley, A., Stebbins, J., Steinke, M., Steinlechner, J., Steinlechner, S., Stephens, B., C., Steplewski, S., Stevenson, S., Stone, R., Stops, D., Strain, K., A., Straniero, N., Strigin, S., Sturani, R., Stuver, A., L., Summerscales, T., Z., Susmithan, S., Sutton, P., J., Swinkels, B., Tacca, M., Talukder, D., Tanner, D., B., Tao, J., Tarabrin, S., P., Taylor, R., Tellez, G., Thirugnanasambandam, M., P., Thomas, M., Thomas, P., Thorne, K., A., Thorne, K., S., Thrane, E., Tiwari, V., Tokmakov, K., V., Tomlinson, C., Tonelli, M., Torres, C., V., Torrie, C., I., Travasso, F., Traylor, G., Tse, M., Tshilumba, D., Tuennermann, H., Ugolini, D., Unnikrishnan, C., S., Urban, A., L., Usman, S., A., Vahlbruch, H., Vajente, G., Valdes, G., Vallisneri, M., van Beuzekom, M., van den Brand, J., F., J., Van Den Broeck, C., van der Sluys, M., V., van Heijningen, J., van Veggel, A., A., Vass, S., Vasúth, M., Vaulin, R., Vecchio, A., Vedovato, G., Veitch, J., Veitch, P., J., Venkateswara, K., Verkindt, D., Vetrano, F., Viceré, A., Vincent-Finley, R., Vinet, J., Vitale, S., Vo, T., Vocca, H., Vorvick, C., Vousden, W., D., Vyachanin, S., P., Wade, A., R., Wade, L., Wade, M., Walker, M., Wallace, L., Walsh, S., Wang, M., Wang, X., Ward, R., L., Was, M., Weaver, B., Wei, L., Weinert, M., Weinstein, A., J., Weiss, R., Welborn, T., Wen, L., Wessels, P., West, M., Westphal, T., Wette, K., Whelan, J., T., White, D., J., Whiting, B., F., Wiesner, K., Wilkinson, C., Williams, K., Williams, L., Williams, R., Williams, T., D., Williamson, A., R., Willis, J., L., Willke, B., Wimmer, M., Winkler, W., Wipf, C., C., Wiseman, A., G., Wittel, H., Woan, G., Wolovick, N., Worden, J., Wu, Y., Yablon, J., Yakushin, I., Yam, W., Yamamoto, H., Yancey, C., C., Yang, H., Yoshida, S., Yvert, M., Zadrożny, A., Zanolin, M., Zendri, J., Zhang, F., Zhang, L., Zhao, C., Zhu, H., Zhu, X., J., Zucker, M., E., Zuraw, S., Zweizig, J., Aptekar, R., L., Atteia, J., L., Cline, T., Connaughton, V., Frederiks, D., D., Golenetskii, S., V., Hurley, K., Krimm, H., A., Marisaldi, M., Pal’shin, V., D., Palmer, D., Svinkin, D., S., Terada, Y., & von Kienlin, A. Physical Review Letters, 113(1):011102, 6, 2014.

Paper

Website abstract bibtex

We present the results of a search for gravitational waves associated with 223 gamma-ray bursts (GRBs) detected by the InterPlanetary Network (IPN) in 2005-2010 during LIGO's fifth and sixth science runs and Virgo's first, second and third science runs. The IPN satellites provide accurate times of the bursts and sky localizations that vary significantly from degree scale to hundreds of square degrees. We search for both a well-modeled binary coalescence signal, the favored progenitor model for short GRBs, and for generic, unmodeled gravitational wave bursts. Both searches use the event time and sky localization to improve the gravitational-wave search sensitivity as compared to corresponding all-time, all-sky searches. We find no evidence of a gravitational-wave signal associated with any of the IPN GRBs in the sample, nor do we find evidence for a population of weak gravitational-wave signals associated with the GRBs. For all IPN-detected GRBs, for which a sufficient duration of quality gravitational-wave data is available, we place lower bounds on the distance to the source in accordance with an optimistic assumption of gravitational-wave emission energy of $10^-2M_\odotc^2$ at 150 Hz, and find a median of 13 Mpc. For the 27 short-hard GRBs we place 90% confidence exclusion distances to two source models: a binary neutron star coalescence, with a median distance of 12Mpc, or the coalescence of a neutron star and black hole, with a median distance of 22 Mpc. Finally, we combine this search with previously published results to provide a population statement for GRB searches in first-generation LIGO and Virgo gravitational-wave detectors, and a resulting examination of prospects for the advanced gravitational-wave detectors.

@article{
 title = {Search for Gravitational Waves Associated with γ-ray Bursts Detected by the Interplanetary Network},
 type = {article},
 year = {2014},
 identifiers = {[object Object]},
 pages = {011102},
 volume = {113},
 websites = {http://arxiv.org/abs/1403.6639,http://link.aps.org/doi/10.1103/PhysRevLett.113.011102},
 month = {6},
 day = {30},
 id = {735caa00-ebd4-3397-830b-5fa403ed6526},
 created = {2014-07-01T10:32:17.000Z},
 accessed = {2014-11-06},
 file_attached = {true},
 profile_id = {dd509e7c-4027-3bb0-8868-37d2bd3fe939},
 last_modified = {2015-09-07T12:41:18.000Z},
 tags = {GRBs,GW,IPN,LIGO,S5,S6,Virgo},
 read = {true},
 starred = {true},
 authored = {true},
 confirmed = {true},
 hidden = {false},
 citation_key = {Aasi:2014iia},
 genre = {High Energy Astrophysical Phenomena; General Relativity and Quantum Cosmology},
 abstract = {We present the results of a search for gravitational waves associated with 223 gamma-ray bursts (GRBs) detected by the InterPlanetary Network (IPN) in 2005-2010 during LIGO's fifth and sixth science runs and Virgo's first, second and third science runs. The IPN satellites provide accurate times of the bursts and sky localizations that vary significantly from degree scale to hundreds of square degrees. We search for both a well-modeled binary coalescence signal, the favored progenitor model for short GRBs, and for generic, unmodeled gravitational wave bursts. Both searches use the event time and sky localization to improve the gravitational-wave search sensitivity as compared to corresponding all-time, all-sky searches. We find no evidence of a gravitational-wave signal associated with any of the IPN GRBs in the sample, nor do we find evidence for a population of weak gravitational-wave signals associated with the GRBs. For all IPN-detected GRBs, for which a sufficient duration of quality gravitational-wave data is available, we place lower bounds on the distance to the source in accordance with an optimistic assumption of gravitational-wave emission energy of $10^-2M_\odotc^2$ at 150 Hz, and find a median of 13 Mpc. For the 27 short-hard GRBs we place 90% confidence exclusion distances to two source models: a binary neutron star coalescence, with a median distance of 12Mpc, or the coalescence of a neutron star and black hole, with a median distance of 22 Mpc. Finally, we combine this search with previously published results to provide a population statement for GRB searches in first-generation LIGO and Virgo gravitational-wave detectors, and a resulting examination of prospects for the advanced gravitational-wave detectors.},
 bibtype = {article},
 author = {Aasi, J and Abbott, B. P. and Abbott, R. and Abbott, T and Abernathy, M. R. and Acernese, F and Ackley, K and Adams, C. and Adams, T and Addesso, P and Adhikari, R. X. and Affeldt, C and Agathos, M and Aggarwal, N and Aguiar, O. D. and Ajith, P and Alemic, A and Allen, B. and Allocca, A. and Amariutei, D. and Andersen, M. and Anderson, R. A. and Anderson, S. B. and Anderson, W. G. and Arai, K. and Araya, M. C. and Arceneaux, C. and Areeda, J. S. and Ast, S. and Aston, S. M. and Astone, P. and Aufmuth, P. and Augustus, H. and Aulbert, C. and Aylott, B. E. and Babak, S. and Baker, P. T. and Ballardin, G. and Ballmer, S. W. and Barayoga, J. C. and Barbet, M. and Barish, B. C. and Barker, D. and Barone, F. and Barr, B. and Barsotti, L. and Barsuglia, M. and Barton, M. A. and Bartos, I. and Bassiri, R. and Basti, A. and Batch, J. C. and Bauchrowitz, J. and Bauer, Th. S. and Baune, C. and Bavigadda, V. and Behnke, B. and Bejger, M. and Beker, M. G. and Belczynski, C. and Bell, A. S. and Bell, C. and Bergmann, G. and Bersanetti, D. and Bertolini, A. and Betzwieser, J. and Bilenko, I. A. and Billingsley, G. and Birch, J. and Biscans, S. and Bitossi, M. and Biwer, C. and Bizouard, M. A. and Black, E. and Blackburn, J. K. and Blackburn, L. and Blair, D. and Bloemen, S. and Bock, O. and Bodiya, T. P. and Boer, M. and Bogaert, G. and Bogan, C. and Bond, C. and Bondu, F. and Bonelli, L. and Bonnand, R. and Bork, R. and Born, M. and Boschi, V. and Bose, Sukanta and Bosi, L. and Bradaschia, C. and Brady, P. R. and Braginsky, V. B. and Branchesi, M. and Brau, J. E. and Briant, T. and Bridges, D. O. and Brillet, A. and Brinkmann, M. and Brisson, V. and Brooks, A. F. and Brown, D. A. and Brown, D. D. and Brückner, F. and Buchman, S. and Buikema, A. and Bulik, T. and Bulten, H. J. and Buonanno, A. and Burman, R. and Buskulic, D. and Buy, C. and Cadonati, L. and Cagnoli, G. and Calderón Bustillo, J. and Calloni, E. and Camp, J. B. and Campsie, P. and Cannon, K. C. and Canuel, B. and Cao, J. and Capano, C. D. and Carbognani, F. and Carbone, L. and Caride, S. and Castaldi, G. and Caudill, S. and Cavaglià, M. and Cavalier, F. and Cavalieri, R. and Celerier, C. and Cella, G. and Cepeda, C. and Cesarini, E. and Chakraborty, R. and Chalermsongsak, T. and Chamberlin, S. J. and Chao, S. and Charlton, P. and Chassande-Mottin, E. and Chen, X. and Chen, Y. and Chincarini, A. and Chiummo, A. and Cho, H. S. and Cho, M. and Chow, J. H. and Christensen, N. and Chu, Q. and Chua, S. S. Y. and Chung, S. and Ciani, G. and Clara, F. and Clark, D. E. and Clark, J. A. and Clayton, J. H. and Cleva, F. and Coccia, E. and Cohadon, P.-F. and Colla, A. and Collette, C. and Colombini, M. and Cominsky, L. and Constancio, M. and Conte, A. and Cook, D. and Corbitt, T. R. and Cornish, N. and Corsi, A. and Costa, C. A. and Coughlin, M. W. and Coulon, J.-P. and Countryman, S. and Couvares, P. and Coward, D. M. and Cowart, M. J. and Coyne, D. C. and Coyne, R. and Craig, K. and Creighton, J. D. E. and Croce, R. P. and Crowder, S. G. and Cumming, A. and Cunningham, L. and Cuoco, E. and Cutler, C. and Dahl, K. and Dal Canton, T. and Damjanic, M. and Danilishin, S. L. and D’Antonio, S. and Danzmann, K. and Dattilo, V. and Daveloza, H. and Davier, M. and Davies, G. S. and Daw, E. J. and Day, R. and Dayanga, T. and DeBra, D. and Debreczeni, G. and Degallaix, J. and Deléglise, S. and Del Pozzo, W. and Denker, T. and Dent, T. and Dereli, H. and Dergachev, V. and De Rosa, R. and DeRosa, R. T. and DeSalvo, R. and Dhurandhar, S. and Díaz, M. and Dickson, J. and Di Fiore, L. and Di Lieto, A. and Di Palma, I. and Di Virgilio, A. and Dolique, V. and Dominguez, E. and Donovan, F. and Dooley, K. L. and Doravari, S. and Douglas, R. and Downes, T. P. and Drago, M. and Drever, R. W. P. and Driggers, J. C. and Du, Z. and Ducrot, M. and Dwyer, S. and Eberle, T. and Edo, T. and Edwards, M. and Effler, A. and Eggenstein, H.-B. and Ehrens, P. and Eichholz, J. and Eikenberry, S. S. and Endrőczi, G. and Essick, R. and Etzel, T. and Evans, M. and Evans, T. and Factourovich, M. and Fafone, V. and Fairhurst, S. and Fan, X. and Fang, Q. and Farinon, S. and Farr, B. and Farr, W. M. and Favata, M. and Fazi, D. and Fehrmann, H. and Fejer, M. M. and Feldbaum, D. and Feroz, F. and Ferrante, I. and Ferreira, E. C. and Ferrini, F. and Fidecaro, F. and Finn, L. S. and Fiori, I. and Fisher, R. P. and Flaminio, R. and Fournier, J.-D. and Franco, S. and Frasca, S. and Frasconi, F. and Frede, M. and Frei, Z. and Freise, A. and Frey, R. and Fricke, T. T. and Fritschel, P. and Frolov, V. V. and Fulda, P. and Fyffe, M. and Gair, J. R. and Gammaitoni, L. and Gaonkar, S. and Garufi, F. and Gehrels, N. and Gemme, G. and Gendre, B. and Genin, E. and Gennai, A. and Ghosh, S. and Giaime, J. A. and Giardina, K. D. and Giazotto, A. and Gleason, J. and Goetz, E. and Goetz, R. and Gondan, L. and González, G. and Gordon, N. and Gorodetsky, M. L. and Gossan, S. and Goßler, S. and Gouaty, R. and Gräf, C. and Graff, P. B. and Granata, M. and Grant, A. and Gras, S. and Gray, C. and Greenhalgh, R. J. S. and Gretarsson, A. M. and Groot, P. and Grote, H. and Grover, K. and Grunewald, S. and Guidi, G. M. and Guido, C. J. and Gushwa, K. and Gustafson, E. K. and Gustafson, R. and Ha, J. and Hall, E. D. and Hamilton, W. and Hammer, D. and Hammond, G. and Hanke, M. and Hanks, J. and Hanna, C. and Hannam, M. D. and Hanson, J. and Harms, J. and Harry, G. M. and Harry, I. W. and Harstad, E. D. and Hart, M. and Hartman, M. T. and Haster, C.-J. and Haughian, K. and Heidmann, A. and Heintze, M. and Heitmann, H. and Hello, P. and Hemming, G. and Hendry, M. and Heng, I. S. and Heptonstall, A. W. and Heurs, M. and Hewitson, M. and Hild, S. and Hoak, D. and Hodge, K. A. and Hofman, D. and Holt, K. and Hopkins, P. and Horrom, T. and Hoske, D. and Hosken, D. J. and Hough, J. and Howell, E. J. and Hu, Y. and Huerta, E. and Hughey, B. and Husa, S. and Huttner, S. H. and Huynh, M. and Huynh-Dinh, T. and Idrisy, A. and Ingram, D. R. and Inta, R. and Islas, G. and Isogai, T. and Ivanov, A. and Iyer, B. R. and Izumi, K. and Jacobson, M. and Jang, H. and Jaranowski, P. and Ji, Y. and Jiménez-Forteza, F. and Johnson, W. W. and Jones, D. I. and Jones, R. and Jonker, R. J. G. and Ju, L. and K., Haris and Kalmus, P. and Kalogera, V. and Kandhasamy, S. and Kang, G. and Kanner, J. B. and Karlen, J. and Kasprzack, M. and Katsavounidis, E. and Katzman, W. and Kaufer, H. and Kaufer, S. and Kaur, T. and Kawabe, K. and Kawazoe, F. and Kéfélian, F. and Keiser, G. M. and Keitel, D. and Kelley, D. B. and Kells, W. and Keppel, D. G. and Khalaidovski, A. and Khalili, F. Y. and Khazanov, E. A. and Kim, C. and Kim, K. and Kim, N. G. and Kim, N. and Kim, S. and Kim, Y.-M. and King, E. J. and King, P. J. and Kinzel, D. L. and Kissel, J. S. and Klimenko, S. and Kline, J. and Koehlenbeck, S. and Kokeyama, K. and Kondrashov, V. and Koranda, S. and Korth, W. Z. and Kowalska, I. and Kozak, D. B. and Kringel, V. and Krishnan, B. and Królak, A. and Kuehn, G. and Kumar, A. and Kumar, D. Nanda and Kumar, P. and Kumar, R. and Kuo, L. and Kutynia, A. and Lam, P. K. and Landry, M. and Lantz, B. and Larson, S. and Lasky, P. D. and Lazzarini, A. and Lazzaro, C. and Leaci, P. and Leavey, S. and Lebigot, E. O. and Lee, C. H. and Lee, H. K. and Lee, H. M. and Lee, J. and Lee, P. J. and Leonardi, M. and Leong, J. R. and Leonor, I. and Le Roux, A. and Leroy, N. and Letendre, N. and Levin, Y. and Levine, B. and Lewis, J. and Li, T. G. F. and Libbrecht, K. and Libson, A. and Lin, A. C. and Littenberg, T. B. and Lockerbie, N. A. and Lockett, V. and Lodhia, D. and Loew, K. and Logue, J. and Lombardi, A. L. and Lopez, E. and Lorenzini, M. and Loriette, V. and Lormand, M. and Losurdo, G. and Lough, J. and Lubinski, M. J. and Lück, H. and Lundgren, A. P. and Ma, Y. and Macdonald, E. P. and MacDonald, T. and Machenschalk, B. and MacInnis, M. and Macleod, D. M. and Magaña-Sandoval, F. and Magee, R. and Mageswaran, M. and Maglione, C. and Mailand, K. and Majorana, E. and Maksimovic, I. and Malvezzi, V. and Man, N. and Manca, G. M. and Mandel, I. and Mandic, V. and Mangano, V. and Mangini, N. M. and Mansell, G. and Mantovani, M. and Marchesoni, F. and Marion, F. and Márka, S. and Márka, Z. and Markosyan, A. and Maros, E. and Marque, J. and Martelli, F. and Martin, I. W. and Martin, R. M. and Martinelli, L. and Martynov, D. and Marx, J. N. and Mason, K. and Masserot, A. and Massinger, T. J. and Matichard, F. and Matone, L. and Mavalvala, N. and May, G. and Mazumder, N. and Mazzolo, G. and McCarthy, R. and McClelland, D. E. and McGuire, S. C. and McIntyre, G. and McIver, J. and McLin, K. and Meacher, D. and Meadors, G. D. and Mehmet, M. and Meidam, J. and Meinders, M. and Melatos, A. and Mendell, G. and Mercer, R. A. and Meshkov, S. and Messenger, C. and Meyer, M. S. and Meyers, P. M. and Mezzani, F. and Miao, H. and Michel, C. and Mikhailov, E. E. and Milano, L. and Miller, J. and Minenkov, Y. and Mingarelli, C. M. F. and Mishra, C. and Mitra, S. and Mitrofanov, V. P. and Mitselmakher, G. and Mittleman, R. and Moe, B. and Moggi, A. and Mohan, M. and Mohapatra, S. R. P. and Moraru, D. and Moreno, G. and Morgado, N. and Morriss, S. R. and Mossavi, K. and Mours, B. and Mow-Lowry, C. M. and Mueller, C. L. and Mueller, G. and Mukherjee, S. and Mullavey, A. and Munch, J. and Murphy, D. and Murray, P. G. and Mytidis, A. and Nagy, M. F. and Nardecchia, I. and Naticchioni, L. and Nayak, R. K. and Necula, V. and Nelemans, G. and Neri, I. and Neri, M. and Newton, G. and Nguyen, T. and Nielsen, A. B. and Nissanke, S. and Nitz, A. H. and Nocera, F. and Nolting, D. and Normandin, M. E. N. and Nuttall, L. K. and Ochsner, E. and O’Dell, J. and Oelker, E. and Oh, J. J. and Oh, S. H. and Ohme, F. and Omar, S. and Oppermann, P. and Oram, R. and O’Reilly, B. and Ortega, W. and O’Shaughnessy, R. and Osthelder, C. and Ottaway, D. J. and Ottens, R. S. and Overmier, H. and Owen, B. J. and Padilla, C. and Pai, A. and Palashov, O. and Palomba, C. and Pan, H. and Pan, Y. and Pankow, C. and Paoletti, F. and Papa, M. A. and Paris, H. and Pasqualetti, A. and Passaquieti, R. and Passuello, D. and Pedraza, M. and Pele, A. and Penn, S. and Perreca, A. and Phelps, M. and Pichot, M. and Pickenpack, M. and Piergiovanni, F. and Pierro, V. and Pinard, L. and Pinto, I. M. and Pitkin, M. and Poeld, J. and Poggiani, R. and Poteomkin, A. and Powell, J. and Prasad, J. and Predoi, V. and Premachandra, S. and Prestegard, T. and Price, L. R. and Prijatelj, M. and Privitera, S. and Prodi, G. 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C. and Yang, H. and Yoshida, S. and Yvert, M. and Zadrożny, A. and Zanolin, M. and Zendri, J.-P. and Zhang, Fan and Zhang, L. and Zhao, C. and Zhu, H. and Zhu, X. J. and Zucker, M. E. and Zuraw, S. and Zweizig, J. and Aptekar, R. L. and Atteia, J. L. and Cline, T. and Connaughton, V. and Frederiks, D. D. and Golenetskii, S. V. and Hurley, K. and Krimm, H. A. and Marisaldi, M. and Pal’shin, V. D. and Palmer, D. and Svinkin, D. S. and Terada, Y. and von Kienlin, A.},
 journal = {Physical Review Letters},
 number = {1}
}

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R.","Willis, J., L.","Willke, B.","Wimmer, M.","Winkler, W.","Wipf, C., C.","Wiseman, A., G.","Wittel, H.","Woan, G.","Wolovick, N.","Worden, J.","Wu, Y.","Yablon, J.","Yakushin, I.","Yam, W.","Yamamoto, H.","Yancey, C., C.","Yang, H.","Yoshida, S.","Yvert, M.","Zadrożny, A.","Zanolin, M.","Zendri, J.","Zhang, F.","Zhang, L.","Zhao, C.","Zhu, H.","Zhu, X., J.","Zucker, M., E.","Zuraw, S.","Zweizig, J.","Aptekar, R., L.","Atteia, J., L.","Cline, T.","Connaughton, V.","Frederiks, D., D.","Golenetskii, S., V.","Hurley, K.","Krimm, H., A.","Marisaldi, M.","Pal’shin, V., D.","Palmer, D.","Svinkin, D., S.","Terada, Y.","von Kienlin, A."],"year":2014,"bibtype":"article","biburl":null,"bibdata":{"title":"Search for Gravitational Waves Associated with γ-ray Bursts Detected by the Interplanetary Network","type":"article","year":"2014","identifiers":"[object Object]","pages":"011102","volume":"113","websites":"http://arxiv.org/abs/1403.6639,http://link.aps.org/doi/10.1103/PhysRevLett.113.011102","month":"6","day":"30","id":"735caa00-ebd4-3397-830b-5fa403ed6526","created":"2014-07-01T10:32:17.000Z","accessed":"2014-11-06","file_attached":"true","profile_id":"dd509e7c-4027-3bb0-8868-37d2bd3fe939","last_modified":"2015-09-07T12:41:18.000Z","tags":"GRBs,GW,IPN,LIGO,S5,S6,Virgo","read":"true","starred":"true","authored":"true","confirmed":"true","hidden":false,"citation_key":"Aasi:2014iia","genre":"High Energy Astrophysical Phenomena; General Relativity and Quantum Cosmology","abstract":"We present the results of a search for gravitational waves associated with 223 gamma-ray bursts (GRBs) detected by the InterPlanetary Network (IPN) in 2005-2010 during LIGO's fifth and sixth science runs and Virgo's first, second and third science runs. The IPN satellites provide accurate times of the bursts and sky localizations that vary significantly from degree scale to hundreds of square degrees. We search for both a well-modeled binary coalescence signal, the favored progenitor model for short GRBs, and for generic, unmodeled gravitational wave bursts. Both searches use the event time and sky localization to improve the gravitational-wave search sensitivity as compared to corresponding all-time, all-sky searches. We find no evidence of a gravitational-wave signal associated with any of the IPN GRBs in the sample, nor do we find evidence for a population of weak gravitational-wave signals associated with the GRBs. For all IPN-detected GRBs, for which a sufficient duration of quality gravitational-wave data is available, we place lower bounds on the distance to the source in accordance with an optimistic assumption of gravitational-wave emission energy of $10^-2M_\\odotc^2$ at 150 Hz, and find a median of 13 Mpc. For the 27 short-hard GRBs we place 90% confidence exclusion distances to two source models: a binary neutron star coalescence, with a median distance of 12Mpc, or the coalescence of a neutron star and black hole, with a median distance of 22 Mpc. Finally, we combine this search with previously published results to provide a population statement for GRB searches in first-generation LIGO and Virgo gravitational-wave detectors, and a resulting examination of prospects for the advanced gravitational-wave detectors.","bibtype":"article","author":"Aasi, J and Abbott, B. P. and Abbott, R. and Abbott, T and Abernathy, M. R. and Acernese, F and Ackley, K and Adams, C. and Adams, T and Addesso, P and Adhikari, R. X. and Affeldt, C and Agathos, M and Aggarwal, N and Aguiar, O. D. and Ajith, P and Alemic, A and Allen, B. and Allocca, A. and Amariutei, D. and Andersen, M. and Anderson, R. A. and Anderson, S. B. and Anderson, W. G. and Arai, K. and Araya, M. C. and Arceneaux, C. and Areeda, J. S. and Ast, S. and Aston, S. M. and Astone, P. and Aufmuth, P. and Augustus, H. and Aulbert, C. and Aylott, B. E. and Babak, S. and Baker, P. T. and Ballardin, G. and Ballmer, S. W. and Barayoga, J. C. and Barbet, M. and Barish, B. C. and Barker, D. and Barone, F. and Barr, B. and Barsotti, L. and Barsuglia, M. and Barton, M. A. and Bartos, I. and Bassiri, R. and Basti, A. and Batch, J. C. and Bauchrowitz, J. and Bauer, Th. S. and Baune, C. and Bavigadda, V. and Behnke, B. and Bejger, M. and Beker, M. G. and Belczynski, C. and Bell, A. S. and Bell, C. and Bergmann, G. and Bersanetti, D. and Bertolini, A. and Betzwieser, J. and Bilenko, I. A. and Billingsley, G. and Birch, J. and Biscans, S. and Bitossi, M. and Biwer, C. and Bizouard, M. A. and Black, E. and Blackburn, J. K. and Blackburn, L. and Blair, D. and Bloemen, S. and Bock, O. and Bodiya, T. 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S. and Terada, Y. and von Kienlin, A.","journal":"Physical Review Letters","number":"1","bibtex":"@article{\n title = {Search for Gravitational Waves Associated with γ-ray Bursts Detected by the Interplanetary Network},\n type = {article},\n year = {2014},\n identifiers = {[object Object]},\n pages = {011102},\n volume = {113},\n websites = {http://arxiv.org/abs/1403.6639,http://link.aps.org/doi/10.1103/PhysRevLett.113.011102},\n month = {6},\n day = {30},\n id = {735caa00-ebd4-3397-830b-5fa403ed6526},\n created = {2014-07-01T10:32:17.000Z},\n accessed = {2014-11-06},\n file_attached = {true},\n profile_id = {dd509e7c-4027-3bb0-8868-37d2bd3fe939},\n last_modified = {2015-09-07T12:41:18.000Z},\n tags = {GRBs,GW,IPN,LIGO,S5,S6,Virgo},\n read = {true},\n starred = {true},\n authored = {true},\n confirmed = {true},\n hidden = {false},\n citation_key = {Aasi:2014iia},\n genre = {High Energy Astrophysical Phenomena; General Relativity and Quantum Cosmology},\n abstract = {We present the results of a search for gravitational waves associated with 223 gamma-ray bursts (GRBs) detected by the InterPlanetary Network (IPN) in 2005-2010 during LIGO's fifth and sixth science runs and Virgo's first, second and third science runs. The IPN satellites provide accurate times of the bursts and sky localizations that vary significantly from degree scale to hundreds of square degrees. We search for both a well-modeled binary coalescence signal, the favored progenitor model for short GRBs, and for generic, unmodeled gravitational wave bursts. Both searches use the event time and sky localization to improve the gravitational-wave search sensitivity as compared to corresponding all-time, all-sky searches. We find no evidence of a gravitational-wave signal associated with any of the IPN GRBs in the sample, nor do we find evidence for a population of weak gravitational-wave signals associated with the GRBs. For all IPN-detected GRBs, for which a sufficient duration of quality gravitational-wave data is available, we place lower bounds on the distance to the source in accordance with an optimistic assumption of gravitational-wave emission energy of $10^-2M_\\odotc^2$ at 150 Hz, and find a median of 13 Mpc. For the 27 short-hard GRBs we place 90% confidence exclusion distances to two source models: a binary neutron star coalescence, with a median distance of 12Mpc, or the coalescence of a neutron star and black hole, with a median distance of 22 Mpc. Finally, we combine this search with previously published results to provide a population statement for GRB searches in first-generation LIGO and Virgo gravitational-wave detectors, and a resulting examination of prospects for the advanced gravitational-wave detectors.},\n bibtype = {article},\n author = {Aasi, J and Abbott, B. P. and Abbott, R. and Abbott, T and Abernathy, M. R. and Acernese, F and Ackley, K and Adams, C. and Adams, T and Addesso, P and Adhikari, R. X. and Affeldt, C and Agathos, M and Aggarwal, N and Aguiar, O. D. and Ajith, P and Alemic, A and Allen, B. and Allocca, A. and Amariutei, D. and Andersen, M. and Anderson, R. A. and Anderson, S. B. and Anderson, W. G. and Arai, K. and Araya, M. C. and Arceneaux, C. and Areeda, J. S. and Ast, S. and Aston, S. M. and Astone, P. and Aufmuth, P. and Augustus, H. and Aulbert, C. and Aylott, B. E. and Babak, S. and Baker, P. T. and Ballardin, G. and Ballmer, S. W. and Barayoga, J. C. and Barbet, M. and Barish, B. C. and Barker, D. and Barone, F. and Barr, B. and Barsotti, L. and Barsuglia, M. and Barton, M. A. and Bartos, I. and Bassiri, R. and Basti, A. and Batch, J. C. and Bauchrowitz, J. and Bauer, Th. S. and Baune, C. and Bavigadda, V. and Behnke, B. and Bejger, M. and Beker, M. G. and Belczynski, C. and Bell, A. S. and Bell, C. and Bergmann, G. and Bersanetti, D. and Bertolini, A. and Betzwieser, J. and Bilenko, I. A. and Billingsley, G. and Birch, J. and Biscans, S. and Bitossi, M. and Biwer, C. and Bizouard, M. A. and Black, E. and Blackburn, J. K. and Blackburn, L. and Blair, D. and Bloemen, S. and Bock, O. and Bodiya, T. P. and Boer, M. and Bogaert, G. and Bogan, C. and Bond, C. and Bondu, F. and Bonelli, L. and Bonnand, R. and Bork, R. and Born, M. and Boschi, V. and Bose, Sukanta and Bosi, L. and Bradaschia, C. and Brady, P. R. and Braginsky, V. B. and Branchesi, M. and Brau, J. E. and Briant, T. and Bridges, D. O. and Brillet, A. and Brinkmann, M. and Brisson, V. and Brooks, A. F. and Brown, D. A. and Brown, D. D. and Brückner, F. and Buchman, S. and Buikema, A. and Bulik, T. and Bulten, H. J. and Buonanno, A. and Burman, R. and Buskulic, D. and Buy, C. and Cadonati, L. and Cagnoli, G. and Calderón Bustillo, J. and Calloni, E. and Camp, J. B. and Campsie, P. and Cannon, K. C. and Canuel, B. and Cao, J. and Capano, C. D. and Carbognani, F. and Carbone, L. and Caride, S. and Castaldi, G. and Caudill, S. and Cavaglià, M. and Cavalier, F. and Cavalieri, R. and Celerier, C. and Cella, G. and Cepeda, C. and Cesarini, E. and Chakraborty, R. and Chalermsongsak, T. and Chamberlin, S. 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S. and Terada, Y. and von Kienlin, A.},\n journal = {Physical Review Letters},\n number = {1}\n}","author_short":["Aasi, J.","Abbott, B., P.","Abbott, R.","Abbott, T.","Abernathy, M., R.","Acernese, F.","Ackley, K.","Adams, C.","Adams, T.","Addesso, P.","Adhikari, R., X.","Affeldt, C.","Agathos, M.","Aggarwal, N.","Aguiar, O., D.","Ajith, P.","Alemic, A.","Allen, B.","Allocca, A.","Amariutei, D.","Andersen, M.","Anderson, R., A.","Anderson, S., B.","Anderson, W., G.","Arai, K.","Araya, M., C.","Arceneaux, C.","Areeda, J., S.","Ast, S.","Aston, S., M.","Astone, P.","Aufmuth, P.","Augustus, H.","Aulbert, C.","Aylott, B., E.","Babak, S.","Baker, P., T.","Ballardin, G.","Ballmer, S., W.","Barayoga, J., C.","Barbet, M.","Barish, B., C.","Barker, D.","Barone, F.","Barr, B.","Barsotti, L.","Barsuglia, M.","Barton, M., A.","Bartos, I.","Bassiri, R.","Basti, A.","Batch, J., C.","Bauchrowitz, J.","Bauer, T., S.","Baune, C.","Bavigadda, V.","Behnke, B.","Bejger, M.","Beker, M., G.","Belczynski, 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