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Article: Prospects for observing and localizing gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA.

Abbott, B P / Abbott, R / Abbott, T D / Abraham, S / Acernese, F / Ackley, K / Adams, C / Adya, V B / Affeldt, C / Agathos, M / Agatsuma, K / Aggarwal, N / Aguiar, O D / Aiello, L / Ain, A / Ajith, P / Akutsu, T / Allen, G / Allocca, A /

Aloy, M A / Altin, P A / Amato, A / Ananyeva, A / Anderson, S B / Anderson, W G / Ando, M / Angelova, S V / Antier, S / Appert, S / Arai, K / Arai, Koya / Arai, Y / Araki, S / Araya, A / Araya, M C / Areeda, J S / Arène, M / Aritomi, N / Arnaud, N / Arun, K G / Ascenzi, S / Ashton, G / Aso, Y / Aston, S M / Astone, P / Aubin, F / Aufmuth, P / AultONeal, K / Austin, C / Avendano, V / Avila-Alvarez, A / Babak, S / Bacon, P / Badaracco, F / Bader, M K M / Bae, S W / Bae, Y B / Baiotti, L / Bajpai, R / Baker, P T / Baldaccini, F / Ballardin, G / Ballmer, S W / Banagiri, S / Barayoga, J C / Barclay, S E / Barish, B C / Barker, D / Barkett, K / Barnum, S / Barone, F / Barr, B / Barsotti, L / Barsuglia, M / Barta, D / Bartlett, J / Barton, M A / Bartos, I / Bassiri, R / Basti, A / Bawaj, M / Bayley, J C / Bazzan, M / Bécsy, B / Bejger, M / Belahcene, I / Bell, A S / Beniwal, D / Berger, B K / Bergmann, G / Bernuzzi, S / Bero, J J / Berry, C P L / Bersanetti, D / Bertolini, A / Betzwieser, J / Bhandare, R / Bidler, J / Bilenko, I A / Bilgili, S A / Billingsley, G / Birch, J / Birney, R / Birnholtz, O / Biscans, S / Biscoveanu, S / Bisht, A / Bitossi, M / Bizouard, M A / Blackburn, J K / Blair, C D / Blair, D G / Blair, R M / Bloemen, S / Bode, N / Boer, M / Boetzel, Y / Bogaert, G / Bondu, F / Bonilla, E / Bonnand, R / Booker, P / Boom, B A / Booth, C D / Bork, R / Boschi, V / Bose, S / Bossie, K / Bossilkov, V / Bosveld, J / Bouffanais, Y / Bozzi, A / Bradaschia, C / Brady, P R / Bramley, A / Branchesi, M / Brau, J E / Briant, T / Briggs, J H / Brighenti, F / Brillet, A / Brinkmann, M / Brisson, V / Brockill, P / Brooks, A F / Brown, D A / Brown, D D / Brunett, S / Buikema, A / Bulik, T / Bulten, H J / Buonanno, A / Buskulic, D / Buy, C / Byer, R L / Cabero, M / Cadonati, L / Cagnoli, G / Cahillane, C / Bustillo, J Calderón / Callister, T A / Calloni, E / Camp, J B / Campbell, W A / Canepa, M / Cannon, K / Cannon, K C / Cao, H / Cao, J / Capocasa, E / Carbognani, F / Caride, S / Carney, M F / Carullo, G / Diaz, J Casanueva / Casentini, C / Caudill, S / Cavaglià, M / Cavalier, F / Cavalieri, R / Cella, G / Cerdá-Durán, P / Cerretani, G / Cesarini, E / Chaibi, O / Chakravarti, K / Chamberlin, S J / Chan, M / Chan, M L / Chao, S / Charlton, P / Chase, E A / Chassande-Mottin, E / Chatterjee, D / Chaturvedi, M / Chatziioannou, K / Cheeseboro, B D / Chen, C S / Chen, H Y / Chen, K H / Chen, X / Chen, Y / Chen, Y R / Cheng, H-P / Cheong, C K / Chia, H Y / Chincarini, A / Chiummo, A / Cho, G / Cho, H S / Cho, M / Christensen, N / Chu, H Y / Chu, Q / Chu, Y K / Chua, S / Chung, K W / Chung, S / Ciani, G / Ciobanu, A A / Ciolfi, R / Cipriano, F / Cirone, A / Clara, F / Clark, J A / Clearwater, P / Cleva, F / Cocchieri, C / Coccia, E / Cohadon, P-F / Cohen, D / Colgan, R / Colleoni, M / Collette, C G / Collins, C / Cominsky, L R / Constancio, M / Conti, L / Cooper, S J / Corban, P / Corbitt, T R / Cordero-Carrión, I / Corley, K R / Cornish, N / Corsi, A / Cortese, S / Costa, C A / Cotesta, R / Coughlin, M W / Coughlin, S B / Coulon, J-P / Countryman, S T / Couvares, P / Covas, P B / Cowan, E E / Coward, D M / Cowart, M J / Coyne, D C / Coyne, R / Creighton, J D E / Creighton, T D / Cripe, J / Croquette, M / Crowder, S G / Cullen, T J / Cumming, A / Cunningham, L / Cuoco, E / Canton, T Dal / Dálya, G / Danilishin, S L / D'Antonio, S / Danzmann, K / Dasgupta, A / Da Silva Costa, C F / Datrier, L E H / Dattilo, V / Dave, I / Davier, M / Davis, D / Daw, E J / DeBra, D / Deenadayalan, M / Degallaix, J / De Laurentis, M / Deléglise, S / Pozzo, W Del / DeMarchi, L M / Demos, N / Dent, T / De Pietri, R / Derby, J / De Rosa, R / De Rossi, C / DeSalvo, R / de Varona, O / Dhurandhar, S / Díaz, M C / Dietrich, T / Fiore, L Di / Giovanni, M Di / Girolamo, T Di / Lieto, A Di / Ding, B / Pace, S Di / Palma, I Di / Renzo, F Di / Dmitriev, A / Doctor, Z / Doi, K / Donovan, F / Dooley, K L / Doravari, S / Dorrington, I / Downes, T P / Drago, M / Driggers, J C / Du, Z / Ducoin, J-G / Dupej, P / Dwyer, S E / Easter, P J / Edo, T B / Edwards, M C / Effler, A / Eguchi, S / Ehrens, P / Eichholz, J / Eikenberry, S S / Eisenmann, M / Eisenstein, R A / Enomoto, Y / Essick, R C / Estelles, H / Estevez, D / Etienne, Z B / Etzel, T / Evans, M / Evans, T M / Fafone, V / Fair, H / Fairhurst, S / Fan, X / Farinon, S / Farr, B / Farr, W M / Fauchon-Jones, E J / Favata, M / Fays, M / Fazio, M / Fee, C / Feicht, J / Fejer, M M / Feng, F / Fernandez-Galiana, A / Ferrante, I / Ferreira, E C / Ferreira, T A / Ferrini, F / Fidecaro, F / Fiori, I / Fiorucci, D / Fishbach, M / Fisher, R P / Fishner, J M / Fitz-Axen, M / Flaminio, R / Fletcher, M / Flynn, E / Fong, H / Font, J A / Forsyth, P W F / Fournier, J-D / Frasca, S / Frasconi, F / Frei, Z / Freise, A / Frey, R / Frey, V / Fritschel, P / Frolov, V V / Fujii, Y / Fukunaga, M / Fukushima, M / Fulda, P / Fyffe, M / Gabbard, H A / Gadre, B U / Gaebel, S M / Gair, J R / Gammaitoni, L / Ganija, M R / Gaonkar, S G / Garcia, A / García-Quirós, C / Garufi, F / Gateley, B / Gaudio, S / Gaur, G / Gayathri, V / Ge, G G / Gemme, G / Genin, E / Gennai, A / George, D / George, J / Gergely, L / Germain, V / Ghonge, S / Ghosh, Abhirup / Ghosh, Archisman / Ghosh, S / Giacomazzo, B / Giaime, J A / Giardina, K D / Giazotto, A / Gill, K / Giordano, G / Glover, L / Godwin, P / Goetz, E / Goetz, R / Goncharov, B / González, G / Castro, J M Gonzalez / Gopakumar, A / Gorodetsky, M L / Gossan, S E / Gosselin, M / Gouaty, R / Grado, A / Graef, C / Granata, M / Grant, A / Gras, S / Grassia, P / Gray, C / Gray, R / Greco, G / Green, A C / Green, R / Gretarsson, E M / Groot, P / Grote, H / Grunewald, S / Gruning, P / Guidi, G M / Gulati, H K / Guo, Y / Gupta, A / Gupta, M K / Gustafson, E K / Gustafson, R / Haegel, L / Hagiwara, A / Haino, S / Halim, O / Hall, B R / Hall, E D / Hamilton, E Z / Hammond, G / Haney, M / Hanke, M M / Hanks, J / Hanna, C / Hannam, M D / Hannuksela, O A / Hanson, J / Hardwick, T / Haris, K / Harms, J / Harry, G M / Harry, I W / Hasegawa, K / Haster, C-J / Haughian, K / Hayakawa, H / Hayama, K / Hayes, F J / Healy, J / 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 / Himemoto, Y / Hinderer, T / Hiranuma, Y / Hirata, N / Hirose, E / Hoak, D / Hochheim, S / Hofman, D / Holgado, A M / Holland, N A / Holt, K / Holz, D E / Hong, Z / Hopkins, P / Horst, C / Hough, J / Howell, E J / Hoy, C G / Hreibi, A / Hsieh, B H / Huang, G Z / Huang, P W / Huang, Y J / Huerta, E A / Huet, D / Hughey, B / Hulko, M / Husa, S / Huttner, S H / Huynh-Dinh, T / Idzkowski, B / Iess, A / Ikenoue, B / Imam, S / Inayoshi, K / Ingram, C / Inoue, Y / Inta, R / Intini, G / Ioka, K / Irwin, B / Isa, H N / Isac, J-M / Isi, M / Itoh, Y / Iyer, B R / Izumi, K / Jacqmin, T / Jadhav, S J / Jani, K / Janthalur, N N / Jaranowski, P / Jenkins, A C / Jiang, J / Johnson, D S / Jones, A W / Jones, D I / Jones, R / Jonker, R J G / Ju, L / Jung, K / Jung, P / Junker, J / Kajita, T / Kalaghatgi, C V / Kalogera, V / Kamai, B / Kamiizumi, M / Kanda, N / Kandhasamy, S / Kang, G W / Kanner, J B / Kapadia, S J / Karki, S / Karvinen, K S / Kashyap, R / Kasprzack, M / Katsanevas, S / Katsavounidis, E / Katzman, W / Kaufer, S / Kawabe, K / Kawaguchi, K / Kawai, N / Kawasaki, T / Keerthana, N V / Kéfélian, F / Keitel, D / Kennedy, R / Key, J S / Khalili, F Y / Khan, H / Khan, I / Khan, S / Khan, Z / Khazanov, E A / Khursheed, M / Kijbunchoo, N / Kim, Chunglee / Kim, C / Kim, J C / Kim, J / Kim, K / Kim, W / Kim, W S / Kim, Y-M / Kimball, C / Kimura, N / King, E J / King, P J / Kinley-Hanlon, M / Kirchhoff, R / Kissel, J S / Kita, N / Kitazawa, H / Kleybolte, L / Klika, J H / Klimenko, S / Knowles, T D / Knyazev, E / Koch, P / Koehlenbeck, S M / Koekoek, G / Kojima, Y / Kokeyama, K / Koley, S / Komori, K / Kondrashov, V / Kong, A K H / Kontos, A / Koper, N / Korobko, M / Korth, W Z / Kotake, K / Kowalska, I / Kozak, D B / Kozakai, C / Kozu, R / Kringel, V / Krishnendu, N / Królak, A / Kuehn, G / Kumar, A / Kumar, P / Kumar, Rahul / Kumar, R / Kumar, S / Kume, J / Kuo, C M / Kuo, H S / Kuo, L / Kuroyanagi, S / Kusayanagi, K / Kutynia, A / Kwak, K / Kwang, S / Lackey, B D / Lai, K H / Lam, T L / Landry, M / Lane, B B / Lang, R N / Lange, J / Lantz, B / Lanza, R K / Lartaux-Vollard, A / Lasky, P D / Laxen, M / Lazzarini, A / Lazzaro, C / Leaci, P / Leavey, S / Lecoeuche, Y K / Lee, C H / Lee, H K / Lee, H M / Lee, H W / Lee, J / Lee, K / Lee, R K / Lehmann, J / Lenon, A / Leonardi, M / Leroy, N / Letendre, N / Levin, Y / Li, J / Li, K J L / Li, T G F / Li, X / Lin, C Y / Lin, F / Lin, F L / Lin, L C C / Linde, F / Linker, S D / Littenberg, T B / Liu, G C / Liu, J / Liu, X / Lo, R K L / Lockerbie, N A / London, L T / Longo, A / Lorenzini, M / Loriette, V / Lormand, M / Losurdo, G / Lough, J D / Lousto, C O / Lovelace, G / Lower, M E / Lück, H / Lumaca, D / Lundgren, A P / Luo, L W / Lynch, R / Ma, Y / Macas, R / Macfoy, S / MacInnis, M / Macleod, D M / Macquet, A / Magaña-Sandoval, F / Zertuche, L Magaña / Magee, R M / Majorana, E / Maksimovic, I / Malik, A / Man, N / Mandic, V / Mangano, V / Mansell, G L / Manske, M / Mantovani, M / Marchesoni, F / Marchio, M / Marion, F / Márka, S / Márka, Z / Markakis, C / Markosyan, A S / Markowitz, A / Maros, E / Marquina, A / Marsat, S / Martelli, F / Martin, I W / Martin, R M / Martynov, D V / Mason, K / Massera, E / Masserot, A / Massinger, T J / Masso-Reid, M / Mastrogiovanni, S / Matas, A / Matichard, F / Matone, L / Mavalvala, N / Mazumder, N / McCann, J J / McCarthy, R / McClelland, D E / McCormick, S / McCuller, L / McGuire, S C / McIver, J / McManus, D J / McRae, T / McWilliams, S T / Meacher, D / Meadors, G D / Mehmet, M / Mehta, A K / Meidam, J / Melatos, A / Mendell, G / Mercer, R A / Mereni, L / Merilh, E L / Merzougui, M / Meshkov, S / Messenger, C / Messick, C / Metzdorff, R / Meyers, P M / Miao, H / Michel, C / Michimura, Y / Middleton, H / Mikhailov, E E / Milano, L / Miller, A L / Miller, A / Millhouse, M / Mills, J C / Milovich-Goff, M C / Minazzoli, O / Minenkov, Y / Mio, N / Mishkin, A / Mishra, C / Mistry, T / Mitra, S / Mitrofanov, V P / Mitselmakher, G / Mittleman, R / Miyakawa, O / Miyamoto, A / Miyazaki, Y / Miyo, K / Miyoki, S / Mo, G / Moffa, D / Mogushi, K / Mohapatra, S R P / Montani, M / Moore, C J / Moraru, D / Moreno, G / Morisaki, S / Moriwaki, Y / Mours, B / Mow-Lowry, C M / Mukherjee, Arunava / Mukherjee, D / Mukherjee, S / Mukund, N / Mullavey, A / Munch, J / Muñiz, E A / Muratore, M / Murray, P G / Nagano, K / Nagano, S / Nagar, A / Nakamura, K / Nakano, H / Nakano, M / Nakashima, R / Nardecchia, I / Narikawa, T / Naticchioni, L / Nayak, R K / Negishi, R / Neilson, J / Nelemans, G / Nelson, T J N / Nery, M / Neunzert, A / Ng, K Y / Ng, S / Nguyen, P / Ni, W T / Nichols, D / Nishizawa, A / Nissanke, S / Nocera, F / North, C / Nuttall, L K / Obergaulinger, M / Oberling, J / O'Brien, B D / Obuchi, Y / O'Dea, G D / Ogaki, W / Ogin, G H / Oh, J J / Oh, S H / Ohashi, M / Ohishi, N / Ohkawa, M / Ohme, F / Ohta, H / Okada, M A / Okutomi, K / Oliver, M / Oohara, K / Ooi, C P / Oppermann, P / Oram, Richard J / O'Reilly, B / Ormiston, R G / Ortega, L F / O'Shaughnessy, R / Oshino, S / Ossokine, S / Ottaway, D J / Overmier, H / Owen, B J / Pace, A E / Pagano, G / Page, M A / Pai, A / Pai, S A / Palamos, J R / Palashov, O / Palomba, C / Pal-Singh, A / Pan, Huang-Wei / Pan, K C / Pang, B / Pang, H F / Pang, P T H / Pankow, C / Pannarale, F / Pant, B C / Paoletti, F / Paoli, A / Papa, M A / Parida, A / Park, J / Parker, W / Pascucci, D / Pasqualetti, A / Passaquieti, R / Passuello, D / Patil, M / Patricelli, B / Pearlstone, B L / Pedersen, C / Pedraza, M / Pedurand, R / Pele, A / Arellano, F E Peña / Penn, S / Perez, C J / Perreca, A / Pfeiffer, H P / Phelps, M / Phukon, K S / Piccinni, O J / Pichot, M / Piergiovanni, F / Pillant, G / Pinard, L / Pinto, I / Pirello, M / Pitkin, M / Poggiani, R / Pong, D Y T / Ponrathnam, S / Popolizio, P / Porter, E K / Powell, J / Prajapati, A K / Prasad, J / Prasai, K / Prasanna, R / Pratten, G / Prestegard, T / Privitera, S / Prodi, G A / Prokhorov, L G / Puncken, O / Punturo, M / Puppo, P / Pürrer, M / Qi, H / Quetschke, V / Quinonez, P J / Quintero, E A / Quitzow-James, R / Raab, F J / Radkins, H / Radulescu, N / Raffai, P / Raja, S / Rajan, C / Rajbhandari, B / Rakhmanov, M / Ramirez, K E / Ramos-Buades, A / Rana, Javed / Rao, K / Rapagnani, P / Raymond, V / Razzano, M / Read, J / Regimbau, T / Rei, L / Reid, S / Reitze, D H / Ren, W / Ricci, F / Richardson, C J / Richardson, J W / Ricker, P M / Riles, K / Rizzo, M / Robertson, N A / Robie, R / Robinet, F / Rocchi, A / Rolland, L / Rollins, J G / Roma, V J / Romanelli, M / Romano, R / Romel, C L / Romie, J H / Rose, K / Rosińska, D / Rosofsky, S G / Ross, M P / Rowan, S / Rüdiger, A / Ruggi, P / Rutins, G / Ryan, K / Sachdev, S / Sadecki, T / Sago, N / Saito, S / Saito, Y / Sakai, K / Sakai, Y / Sakamoto, H / Sakellariadou, M / Sakuno, Y / Salconi, L / Saleem, M / Samajdar, A / Sammut, L / Sanchez, E J / Sanchez, L E / Sanchis-Gual, N / Sandberg, V / Sanders, J R / Santiago, K A / Sarin, N / Sassolas, B / Sathyaprakash, B S / Sato, S / Sato, T / Sauter, O / Savage, R L / Sawada, T / Schale, P / Scheel, M / Scheuer, J / Schmidt, P / Schnabel, R / Schofield, R M S / Schönbeck, A / Schreiber, E / Schulte, B W / Schutz, B F / Schwalbe, S G / Scott, J / Scott, S M / Seidel, E / Sekiguchi, T / Sekiguchi, Y / Sellers, D / Sengupta, A S / Sennett, N / Sentenac, D / Sequino, V / Sergeev, A / Setyawati, Y / Shaddock, D A / Shaffer, T / Shahriar, M S / Shaner, M B / Shao, L / Sharma, P / Shawhan, P / Shen, H / Shibagaki, S / Shimizu, R / Shimoda, T / Shimode, K / Shink, R / Shinkai, H / Shishido, T / Shoda, A / Shoemaker, D H / Shoemaker, D M / ShyamSundar, S / Siellez, K / Sieniawska, M / Sigg, D / Silva, A D / Singer, L P / Singh, N / Singhal, A / Sintes, A M / Sitmukhambetov, S / Skliris, V / Slagmolen, B J J / Slaven-Blair, T J / Smith, J R / Smith, R J E / Somala, S / Somiya, K / Son, E J / Sorazu, B / Sorrentino, F / Sotani, H / Souradeep, T / Sowell, E / Spencer, A P / Srivastava, A K / Srivastava, V / Staats, K / Stachie, C / Standke, M / Steer, D A / Steinke, M / Steinlechner, J / Steinlechner, S / Steinmeyer, D / Stevenson, S P / Stocks, D / Stone, R / Stops, D J / Strain, K A / Stratta, G / Strigin, S E / Strunk, A / Sturani, R / Stuver, A L / Sudhir, V / Sugimoto, R / Summerscales, T Z / Sun, L / Sunil, S / Suresh, J / Sutton, P J / Suzuki, Takamasa / Suzuki, Toshikazu / Swinkels, B L / Szczepańczyk, M J / Tacca, M / Tagoshi, H / Tait, S C / Takahashi, H / Takahashi, R / Takamori, A / Takano, S / Takeda, H / Takeda, M / Talbot, C / Talukder, D / Tanaka, H / Tanaka, Kazuyuki / Tanaka, Kenta / Tanaka, Taiki / Tanaka, Takahiro / Tanioka, S / Tanner, D B / Tápai, M / Martin, E N Tapia San / Taracchini, A / Tasson, J D / Taylor, R / Telada, S / Thies, F / Thomas, M / Thomas, P / Thondapu, S R / Thorne, K A / Thrane, E / Tiwari, Shubhanshu / Tiwari, Srishti / Tiwari, V / Toland, K / Tomaru, T / Tomigami, Y / Tomura, T / Tonelli, M / Tornasi, Z / Torres-Forné, A / Torrie, C I / Töyrä, D / Travasso, F / Traylor, G / Tringali, M C / Trovato, A / Trozzo, L / Trudeau, R / Tsang, K W / Tsang, T T L / Tse, M / Tso, R / Tsubono, K / Tsuchida, S / Tsukada, L / Tsuna, D / Tsuzuki, T / Tuyenbayev, D / Uchikata, N / Uchiyama, T / Ueda, A / Uehara, T / Ueno, K / Ueshima, G / Ugolini, D / Unnikrishnan, C S / Uraguchi, F / Urban, A L / Ushiba, T / Usman, S A / Vahlbruch, H / Vajente, G / Valdes, G / Bakel, N van / Beuzekom, M van / Brand, J F J van den / Broeck, C Van Den / Vander-Hyde, D C / Schaaf, L van der / Heijningen, J V van / Putten, M H P M van / Veggel, A A van / Vardaro, M / Varma, V / Vass, S / Vasúth, M / Vecchio, A / Vedovato, G / Veitch, J / Veitch, P J / Venkateswara, K / Venugopalan, G / Verkindt, D / Vetrano, F / Viceré, A / Viets, A D / Vine, D J / Vinet, J-Y / Vitale, S / Vivanco, Francisco Hernandez / Vo, T / Vocca, H / Vorvick, C / Vyatchanin, S P / Wade, A R / Wade, L E / Wade, M / Walet, R / Walker, M / Wallace, L / Walsh, S / Wang, G / Wang, H / Wang, J / Wang, J Z / Wang, W H / Wang, Y F / Ward, R L / Warden, Z A / Warner, J / Was, M / Watchi, J / Weaver, B / Wei, L-W / Weinert, M / Weinstein, A J / Weiss, R / Wellmann, F / Wen, L / Wessel, E K / Weßels, P / Westhouse, J W / Wette, K / Whelan, J T / Whiting, B F / Whittle, C / Wilken, D M / Williams, D / Williamson, A R / Willis, J L / Willke, B / Wimmer, M H / Winkler, W / Wipf, C C / Wittel, H / Woan, G / Woehler, J / Wofford, J K / Worden, J / Wright, J L / Wu, C M / Wu, D S / Wu, H C / Wu, S R / Wysocki, D M / Xiao, L / Xu, W R / Yamada, T / Yamamoto, H / Yamamoto, Kazuhiro / Yamamoto, Kohei / Yamamoto, T / Yancey, C C / Yang, L / Yap, M J / Yazback, M / Yeeles, D W / Yokogawa, K / Yokoyama, J / Yokozawa, T / Yoshioka, T / Yu, Hang / Yu, Haocun / Yuen, S H R / Yuzurihara, H / Yvert, M / Zadrożny, A K / Zanolin, M / Zeidler, S / Zelenova, T / Zendri, J-P / Zevin, M / Zhang, J / Zhang, L / Zhang, T / Zhao, C / Zhao, Y / Zhou, M / Zhou, Z / Zhu, X J / Zhu, Z H / Zimmerman, A B / Zucker, M E / Zweizig, J

Living reviews in relativity

2020 Volume 23, Issue 1, Page(s) 3

Abstract: We present our current best estimate of the plausible observing scenarios for the Advanced LIGO, Advanced Virgo and KAGRA gravitational-wave detectors over the next several years, with the intention of providing information to facilitate planning for ... ...

Abstract	We present our current best estimate of the plausible observing scenarios for the Advanced LIGO, Advanced Virgo and KAGRA gravitational-wave detectors over the next several years, with the intention of providing information to facilitate planning for multi-messenger astronomy with gravitational waves. We estimate the sensitivity of the network to transient gravitational-wave signals for the third (O3), fourth (O4) and fifth observing (O5) runs, including the planned upgrades of the Advanced LIGO and Advanced Virgo detectors. We study the capability of the network to determine the sky location of the source for gravitational-wave signals from the inspiral of binary systems of compact objects, that is binary neutron star, neutron star-black hole, and binary black hole systems. The ability to localize the sources is given as a sky-area probability, luminosity distance, and comoving volume. The median sky localization area (90% credible region) is expected to be a few hundreds of square degrees for all types of binary systems during O3 with the Advanced LIGO and Virgo (HLV) network. The median sky localization area will improve to a few tens of square degrees during O4 with the Advanced LIGO, Virgo, and KAGRA (HLVK) network. During O3, the median localization volume (90% credible region) is expected to be on the order of
Keywords	covid19
Language	English
Publishing date	2020-09-28
Publishing country	Switzerland
Document type	Journal Article ; Review
ZDB-ID	1416143-6
ISSN	1433-8351
ISSN	1433-8351
DOI	10.1007/s41114-020-00026-9
Database	MEDical Literature Analysis and Retrieval System OnLINE

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Book ; Online: Virgo calibration and reconstruction of the gravitational wave strain during VSR1

The Virgo collaboration / Accadia, T. / Acernese, F. / Antonucci, F. / Aoudia, S. / Arun, K. G. / Astone, P. / Ballardin, G. / Barone, F. / Barsuglia, M. / Bauer, Th. S. / Beker, M. G. / Belletoile, A. / Bigotta, S. / Birindelli, S. / Bitossi, M. / Bizouard, M. A. / Blom, M. / Boccara, C. /

Bondu, F. / Bonelli, L. / Bonnand, R. / Bosi, L. / Braccini, S. / Bradaschia, C. / Brillet, A. / Brisson, V. / Budzynski, R. / Bulik, T. / Bulten, H. J. / Buskulic, D. / Buy, C. / Cagnoli, G. / Calloni, E. / Campagna, E. / Canuel, B. / Carbognani, F. / Cavalier, F. / Cavalieri, R. / Cella, G. / Cesarini, E. / Chassande-Mottin, E. / Chincarini, A. / Cleva, F. / Coccia, E. / Colacino, C. N. / Colas, J. / Colla, A. / Colombini, M. / Corsi, A. / Coulon, J. -P. / Cuoco, E. / D'Antonio, S. / Dari, A. / Dattilo, V. / Davier, M. / Day, R. / De Rosa, R. / del Prete, M. / Di Fiore, L. / Di Lieto, A. / Emilio, M. Di Paolo / Di Virgilio, A. / Dietz, A. / Drago, M. / Fafone, V. / Ferrante, I. / Fidecaro, F. / Fiori, I. / Flaminio, R. / Fournier, J. -D. / Franc, J. / Frasca, S. / Frasconi, F. / Freise, A. / Galimberti, M. / Gammaitoni, L. / Garufi, F. / Gemme, G. / Genin, E. / Gennai, A. / Giazotto, A. / Gouaty, R. / Granata, M. / Greverie, C. / Guidi, G. M. / Heitmann, H. / Hello, P. / Hild, S. / Huet, D. / Jaranowski, P. / Kowalska, I. / Krolak, A. / Leroy, N. / Letendre, N. / Li, T. G. F. / Lorenzini, M. / Loriette, V. / Losurdo, G. / Mackowski, J. M. / Majorana, E. / Maksimovic, I. / Man, N. / Mantovani, M. / Marchesoni, F. / Marion, F. / Marque, J. / Martelli, F. / Masserot, A. / Michel, C. / Milano, L. / Minenkov, Y. / Mohan, M. / Moreau, J. / Morgado, N. / Morgia, A. / Mosca, S. / Moscatelli, V. / Mours, B. / Neri, I. / Nocera, F. / Pagliaroli, G. / Palladino, L. / Palomba, C. / Paoletti, F. / Pardi, S. / Parisi, M. / Pasqualetti, A. / Passaquieti, R. / Passuello, D. / Persichetti, G. / Pichot, M. / Piergiovanni, F. / Pietka, M. / Pinard, L. / Poggiani, R. / Prato, M. / Prodi, G. A. / Punturo, M. / Puppo, P. / Rabaste, O. / Rabeling, D. S. / Rapagnani, P. / Re, V. / Regimbau, T. / Ricci, F. / Robinet, F. / Rocchi, A. / Rolland, L. / Romano, R. / Rosinska, D. / Ruggi, P. / Sassolas, B. / Sentenac, D. / Sturani, R. / Swinkels, B. / Toncelli, A. / Tonelli, M. / Torre, O. / Tournefier, E. / Travasso, F. / Trummer, J. / Vajente, G. / Brand, J. F. J. van den / van der Putten, S. / Vavoulidis, M. / Vedovato, G. / Verkindt, D. / Vetrano, F. / Vicere, A. / Vinet, J. -Y. / Vocca, H. / Was, M. / Yvert, M.

2010

Abstract: Virgo is a kilometer-length interferometer for gravitational waves detection located near Pisa. Its first science run, VSR1, occured from May to October 2007. The aims of the calibration are to measure the detector sensitivity and to reconstruct the time ...

Abstract	Virgo is a kilometer-length interferometer for gravitational waves detection located near Pisa. Its first science run, VSR1, occured from May to October 2007. The aims of the calibration are to measure the detector sensitivity and to reconstruct the time series of the gravitational wave strain h(t). The absolute length calibration is based on an original non-linear reconstruction of the differential arm length variations in free swinging Michelson configurations. It uses the laser wavelength as length standard. This method is used to calibrate the frequency dependent response of the Virgo mirror actuators and derive the detector in-loop response and sensitivity within ~5%. The principle of the strain reconstruction is highlighted and the h(t) systematic errors are estimated. A photon calibrator is used to check the sign of h(t). The reconstructed h(t) during VSR1 is valid from 10 Hz up to 10 kHz with systematic errors estimated to 6% in amplitude. The phase error is estimated to be 70 mrad below 1.9 kHz and 6 micro-seconds above. Comment: 8 pages, 8 figures, proceedings of Amaldi 8 conference, to be published in Journal of Physics Conference Series (JPCS). Second release: correct typos
Keywords	General Relativity and Quantum Cosmology
Subject code	621
Publishing date	2010-02-11
Publishing country	us
Document type	Book ; Online
Database	BASE - Bielefeld Academic Search Engine (life sciences selection)

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Article: Tests of General Relativity with Binary Black Holes from the second LIGO-Virgo Gravitational-Wave Transient Catalog

Collaboration, The LIGO Scientific / Abbott, the Virgo Collaboration R. / Abbott, T. D. / Abraham, S. / Acernese, F. / Ackley, K. / Adams, A. / Adams, C. / Adhikari, R. X. / Adya, V. B. / Affeldt, C. / Agathos, M. / Agatsuma, K. / Aggarwal, N. / Aguiar, O. D. / Aiello, L. / Ain, A. / Ajith, P. / Allen, G. /

Allocca, A. / Altin, P. A. / Amato, A. / Anand, S. / Ananyeva, A. / Anderson, S. B. / Anderson, W. G. / Angelova, S. V. / Ansoldi, S. / Antelis, J. M. / Antier, S. / Appert, S. / Arai, K. / Araya, M. C. / Areeda, J. S. / Arene, M. / Arnaud, N. / Aronson, S. M. / Arun, K. G. / Asali, Y. / Ascenzi, S. / Ashton, G. / Aston, S. M. / Astone, P. / Aubin, F. / Aufmuth, P. / AultONeal, K. / Austin, C. / Avendano, V. / Babak, S. / Badaracco, F. / Bader, M. K. M. / Bae, S. / Baer, A. M. / Bagnasco, S. / Baird, J. / Ball, M. / Ballardin, G. / Ballmer, S. W. / Bals, A. / Balsamo, A. / Baltus, G. / Banagiri, S. / Bankar, D. / Bankar, R. S. / Barayoga, J. C. / Barbieri, C. / Barish, B. C. / Barker, D. / Barneo, P. / Barnum, S. / Barone, F. / Barr, B. / Barsotti, L. / Barsuglia, M. / Barta, D. / Bartlett, J. / Bartos, I. / Bassiri, R. / Basti, A. / Bawaj, M. / Bayley, J. C. / Bazzan, M. / Becher, B. R. / B'ecsy, B. / Bedakihale, V. M. / Bejger, M. / Belahcene, I. / Beniwal, D. / Benjamin, M. G. / Benkel, R. / Bennett, T. F. / Bentley, J. D. / Bergamin, F. / Berger, B. K. / Bergmann, G. / Bernuzzi, S. / Berry, C. P. L. / Bersanetti, D. / Bertolini, A. / Betzwieser, J. / Bhandare, R. / Bhandari, A. V. / Bhattacharjee, D. / Bidler, J. / Bilenko, I. A. / Billingsley, G. / Birney, R. / Birnholtz, O. / Biscans, S. / Bischi, M. / Biscoveanu, S. / Bisht, A. / Bitossi, M. / Bizouard, M.-A. / Blackburn, J. K. / Blackman, J. / Blair, C. D. / Blair, D. G. / Blair, R. M. / Blanch, O. / Bobba, F. / Bode, N. / Boer, M. / Boetzel, Y. / Bogaert, G. / Boldrini, M. / Bondu, F. / Bonilla, E. / Bonnand, R. / Booker, P. / Boom, B. A. / Borhanian, S. / Bork, R. / Boschi, V. / Bose, N. / Bose, S. / Bossilkov, V. / Boudart, V. / Bouffanais, Y. / Bozzi, A. / Bradaschia, C. / Brady, P. R. / Bramley, A. / Branchesi, M. / Brau, J. E. / Breschi, M. / Briant, T. / Briggs, J. H. / Brighenti, F. / Brillet, A. / Brinkmann, M. / Brockill, P. / Brooks, A. F. / Brooks, J. / Brown, D. D. / Brunett, S. / Bruno, G. / Bruntz, R. / Buikema, A. / Bulik, T. / Bulten, H. J. / Buonanno, A. / Buskulic, D. / Byer, R. L. / Cabero, M. / Cadonati, L. / Caesar, M. / Cagnoli, G. / Cahillane, C. / Bustillo, J. Calder'on / Callaghan, J. D. / Callister, T. A. / Calloni, E. / Camp, J. B. / Canepa, M. / Cannon, K. C. / Cao, H. / Cao, J. / Carapella, G. / Carbognani, F. / Carney, M. F. / Carpinelli, M. / Carullo, G. / Carver, T. L. / Diaz, J. Casanueva / Casentini, C. / Caudill, S. / Cavaglia, M. / Cavalier, F. / Cavalieri, R. / Cella, G. / Cerd'a-Dur'an, P. / Cesarini, E. / Chaibi, W. / Chakravarti, K. / Chan, C.-L. / Chan, C. / Chandra, K. / Chanial, P. / Chao, S. / Charlton, P. / Chase, E. A. / Chassande-Mottin, E. / Chatterjee, D. / Chaturvedi, M. / Chatziioannou, K. / Chen, A. / Chen, H. Y. / Chen, X. / Chen, Y. / Cheng, H.-P. / Cheong, C. K. / Chia, H. Y. / Chiadini, F. / Chierici, R. / Chincarini, A. / Chiummo, A. / Cho, G. / Cho, H. 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Abstract: Gravitational waves enable tests of general relativity in the highly dynamical and strong-field regime. Using events detected by LIGO-Virgo up to 1 October 2019, we evaluate the consistency of the data with predictions from the theory. We first establish ...

Abstract	Gravitational waves enable tests of general relativity in the highly dynamical and strong-field regime. Using events detected by LIGO-Virgo up to 1 October 2019, we evaluate the consistency of the data with predictions from the theory. We first establish that residuals from the best-fit waveform are consistent with detector noise, and that the low- and high-frequency parts of the signals are in agreement. We then consider parametrized modifications to the waveform by varying post-Newtonian and phenomenological coefficients, improving past constraints by factors of ${\sim}2$; we also find consistency with Kerr black holes when we specifically target signatures of the spin-induced quadrupole moment. Looking for gravitational-wave dispersion, we tighten constraints on Lorentz-violating coefficients by a factor of ${\sim}2.6$ and bound the mass of the graviton to $m_g \leq 1.76 \times 10^{-23} \mathrm{eV}/c^2$ with 90% credibility. We also analyze the properties of the merger remnants by measuring ringdown frequencies and damping times, constraining fractional deviations away from the Kerr frequency to $\delta \hat{f}_{220} = 0.03^{+0.38}_{-0.35}$ for the fundamental quadrupolar mode, and $\delta \hat{f}_{221} = 0.04^{+0.27}_{-0.32}$ for the first overtone; additionally, we find no evidence for postmerger echoes. Finally, we determine that our data are consistent with tensorial polarizations through a template-independent method. When possible, we assess the validity of general relativity based on collections of events analyzed jointly. We find no evidence for new physics beyond general relativity, for black hole mimickers, or for any unaccounted systematics.
Keywords	covid19
Publisher	ArXiv
Document type	Article
Database	COVID19

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Article ; Online: Properties and astrophysical implications of the 150 Msun binary black hole merger GW190521

Collaboration, The LIGO Scientific / Abbott, the Virgo Collaboration R. / Abbott, T. D. / Abraham, S. / Acernese, F. / Ackley, K. / Adams, C. / Adhikari, R. X. / Adya, V. B. / Affeldt, C. / Agathos, M. / Agatsuma, K. / Aggarwal, N. / Aguiar, O. D. / Aich, A. / Aiello, L. / Ain, A. / Ajith, P. / Akcay, S. /

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Abstract: The gravitational-wave signal GW190521 is consistent with a binary black hole merger source at redshift 0.8 with unusually high component masses, $85^{+21}_{-14}\,M_{\odot}$ and $66^{+17}_{-18}\,M_{\odot}$, compared to previously reported events, and ... ...

Abstract	The gravitational-wave signal GW190521 is consistent with a binary black hole merger source at redshift 0.8 with unusually high component masses, $85^{+21}_{-14}\,M_{\odot}$ and $66^{+17}_{-18}\,M_{\odot}$, compared to previously reported events, and shows mild evidence for spin-induced orbital precession. The primary falls in the mass gap predicted by (pulsational) pair-instability supernova theory, in the approximate range $65 - 120\,M_{\odot}$. The probability that at least one of the black holes in GW190521 is in that range is 99.0%. The final mass of the merger $(142^{+28}_{-16}\,M_{\odot})$ classifies it as an intermediate-mass black hole. Under the assumption of a quasi-circular binary black hole coalescence, we detail the physical properties of GW190521's source binary and its post-merger remnant, including component masses and spin vectors. Three different waveform models, as well as direct comparison to numerical solutions of general relativity, yield consistent estimates of these properties. Tests of strong-field general relativity targeting the merger-ringdown stages of coalescence indicate consistency of the observed signal with theoretical predictions. We estimate the merger rate of similar systems to be $0.13^{+0.30}_{-0.11}\,{\rm Gpc}^{-3}\,\rm{yr}^{-1}$. We discuss the astrophysical implications of GW190521 for stellar collapse, and for the possible formation of black holes in the pair-instability mass gap through various channels: via (multiple) stellar coalescence, or via hierarchical merger of lower-mass black holes in star clusters or in active galactic nuclei. We find it to be unlikely that GW190521 is a strongly lensed signal of a lower-mass black hole binary merger. We also discuss more exotic possible sources for GW190521, including a highly eccentric black hole binary, or a primordial black hole binary.
Keywords	covid19
Publisher	ArXiv
Document type	Article ; Online
DOI	10.3847/2041-8213/aba493
Database	COVID19

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Article: Search for Gravitational Waves Associated with Gamma-Ray Bursts Detected by Fermi and Swift During the LIGO-Virgo Run O3a

Collaboration, The LIGO Scientific / R.Abbott, the Virgo Collaboration / T.D.Abbott, / S.Abraham, / F.Acernese, / K.Ackley, / C.Adams, / R.X.Adhikari, / V.B.Adya, / C.Affeldt, / M.Agathos, / K.Agatsuma, / N.Aggarwal, / O.D.Aguiar, / A.Aich, / L.Aiello, / A.Ain, / P.Ajith, / G.Allen, /

A.Allocca, / P.A.Altin, / A.Amato, / S.Anand, / A.Ananyeva, / S.B.Anderson, / W.G.Anderson, / S.V.Angelova, / S.Ansoldi, / S.Antier, / S.Appert, / K.Arai, / M.C.Araya, / J.S.Areeda, / M.Arene, / N.Arnaud, / S.M.Aronson, / Y.Asali, / S.Ascenzi, / G.Ashton, / M.Assiduo, / S.M.Aston, / P.Astone, / F.Aubin, / P.Aufmuth, / K.AultONeal, / C.Austin, / V.Avendano, / S.Babak, / P.Bacon, / F.Badaracco, / M.K.M.Bader, / S.Bae, / A.M.Baer, / J.Baird, / F.Baldaccini, / G.Ballardin, / S.W.Ballmer, / A.Bals, / A.Balsamo, / G.Baltus, / S.Banagiri, / D.Bankar, / R.S.Bankar, / J.C.Barayoga, / C.Barbieri, / B.C.Barish, / D.Barker, / K.Barkett, / P.Barneo, / F.Barone, / B.Barr, / L.Barsotti, / M.Barsuglia, / D.Barta, / J.Bartlett, / I.Bartos, / R.Bassiri, / A.Basti, / M.Bawaj, / J.C.Bayley, / M.Bazzan, / B.B'ecsy, / M.Bejger, / I.Belahcene, / A.S.Bell, / D.Beniwal, / M.G.Benjamin, / J.D.Bentley, / F.Bergamin, / B.K.Berger, / G.Bergmann, / S.Bernuzzi, / C.P.L.Berry, / D.Bersanetti, / A.Bertolini, / J.Betzwieser, / R.Bhandare, / A.V.Bhandari, / A.Bianchi, / J.Bidler, / E.Biggs, / I.A.Bilenko, / G.Billingsley, / R.Birney, / O.Birnholtz, / S.Biscans, / M.Bischi, / S.Biscoveanu, / A.Bisht, / G.Bissenbayeva, / M.Bitossi, / M.A.Bizouard, / J.K.Blackburn, / J.Blackman, / C.D.Blair, / D.G.Blair, / R.M.Blair, / F.Bobba, / N.Bode, / M.Boer, / Y.Boetzel, / G.Bogaert, / F.Bondu, / E.Bonilla, / R.Bonnand, / P.Booker, / B.A.Boom, / R.Bork, / V.Boschi, / S.Bose, / V.Bossilkov, / J.Bosveld, / Y.Bouffanais, / A.Bozzi, / C.Bradaschia, / P.R.Brady, / A.Bramley, / M.Branchesi, / J.E.Brau, / M.Breschi, / T.Briant, / J.H.Briggs, / F.Brighenti, / A.Brillet, / M.Brinkmann, / P.Brockill, / A.F.Brooks, / J.Brooks, / D.D.Brown, / S.Brunett, / G.Bruno, / R.Bruntz, / A.Buikema, / T.Bulik, / H.J.Bulten, / A.Buonanno, / D.Buskulic, / R.L.Byer, / M.Cabero, / L.Cadonati, / G.Cagnoli, / C.Cahillane, / Bustillo, J.Calder'on / J.D.Callaghan, / T.A.Callister, / E.Calloni, / J.B.Camp, / M.Canepa, / Santoro, G.Caneva / K.C.Cannon, / H.Cao, / J.Cao, / G.Carapella, / F.Carbognani, / S.Caride, / M.F.Carney, / G.Carullo, / T.L.Carver, / Diaz, J.Casanueva / C.Casentini, / J.Castaneda, / S.Caudill, / M.Cavaglia, / F.Cavalier, / R.Cavalieri, / G.Cella, / P.Cerd'a-Dur'an, / E.Cesarini, / O.Chaibi, / K.Chakravarti, / C.Chan, / M.Chan, / S.Chao, / P.Charlton, / E.A.Chase, / E.Chassande-Mottin, / D.Chatterjee, / M.Chaturvedi, / H.Y.Chen, / X.Chen, / Y.Chen, / H.-P.Cheng, / C.K.Cheong, / H.Y.Chia, / F.Chiadini, / R.Chierici, / A.Chincarini, / A.Chiummo, / G.Cho, / H.S.Cho, / M.Cho, / N.Christensen, / Q.Chu, / S.Chua, / K.W.Chung, / S.Chung, / G.Ciani, / P.Ciecielag, / M.Cie'slar, / A.A.Ciobanu, / R.Ciolfi, / F.Cipriano, / A.Cirone, / F.Clara, / J.A.Clark, / P.Clearwater, / S.Clesse, / F.Cleva, / E.Coccia, / P.-F.Cohadon, / D.Cohen, / M.Colleoni, / C.G.Collette, / C.Collins, / M.Colpi, / M.Constancio, / L.Conti, / S.J.Cooper, / P.Corban, / T.R.Corbitt, / I.Cordero-Carri'on, / S.Corezzi, / K.R.Corley, / 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Abstract: We search for gravitational-wave transients associated with gamma-ray bursts detected by the Fermi and Swift satellites during the first part of the third observing run of Advanced LIGO and Advanced Virgo (1 April 2019 15:00 UTC - 1 October 2019 15:00 ... ...

Abstract	We search for gravitational-wave transients associated with gamma-ray bursts detected by the Fermi and Swift satellites during the first part of the third observing run of Advanced LIGO and Advanced Virgo (1 April 2019 15:00 UTC - 1 October 2019 15:00 UTC). 105 gamma-ray bursts were analyzed using a search for generic gravitational-wave transients; 32 gamma-ray bursts were analyzed with a search that specifically targets neutron star binary mergers as short gamma-ray burst progenitors. We describe a method to calculate the probability that triggers from the binary merger targeted search are astrophysical and apply that method to the most significant gamma-ray bursts in that search. We find no significant evidence for gravitational-wave signals associated with the gamma-ray bursts that we followed up, nor for a population of unidentified subthreshold signals. We consider several source types and signal morphologies, and report for these lower bounds on the distance to each gamma-ray burst.
Keywords	covid19
Publisher	ArXiv
Document type	Article
Database	COVID19

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Article ; Online: Gravitational-wave constraints on the equatorial ellipticity of millisecond pulsars

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Abstract: We present a search for continuous gravitational waves from five radio pulsars, comprising three recycled pulsars (PSR J0437-4715, PSR J0711-6830, and PSR J0737-3039A) and two young pulsars: the Crab pulsar (J0534+2200) and the Vela pulsar (J0835-4510). ... ...

Abstract	We present a search for continuous gravitational waves from five radio pulsars, comprising three recycled pulsars (PSR J0437-4715, PSR J0711-6830, and PSR J0737-3039A) and two young pulsars: the Crab pulsar (J0534+2200) and the Vela pulsar (J0835-4510). We use data from the third observing run of Advanced LIGO and Virgo combined with data from their first and second observing runs. For the first time we are able to match (for PSR J0437-4715) or surpass (for PSR J0711-6830) the indirect limits on gravitational-wave emission from recycled pulsars inferred from their observed spin-downs, and constrain their equatorial ellipticities to be less than $10^{-8}$. For each of the five pulsars, we perform targeted searches that assume a tight coupling between the gravitational-wave and electromagnetic signal phase evolution. We also present constraints on PSR J0711-6830, the Crab pulsar and the Vela pulsar from a search that relaxes this assumption, allowing the gravitational-wave signal to vary from the electromagnetic expectation within a narrow band of frequencies and frequency derivatives.
Keywords	covid19
Publisher	ArXiv
Document type	Article ; Online
DOI	10.3847/2041-8213/abb655
Database	COVID19

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Article ; Online: GW190814: Gravitational Waves from the Coalescence of a 23 M$_\odot$ Black Hole with a 2.6 M$_\odot$ Compact Object

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Abstract: We report the observation of a compact binary coalescence involving a 22.2 - 24.3 $M_{\odot}$ black hole and a compact object with a mass of 2.50 - 2.67 $M_{\odot}$ (all measurements quoted at the 90$\%$ credible level). The gravitational-wave signal, ... ...

Abstract	We report the observation of a compact binary coalescence involving a 22.2 - 24.3 $M_{\odot}$ black hole and a compact object with a mass of 2.50 - 2.67 $M_{\odot}$ (all measurements quoted at the 90$\%$ credible level). The gravitational-wave signal, GW190814, was observed during LIGO's and Virgo's third observing run on August 14, 2019 at 21:10:39 UTC and has a signal-to-noise ratio of 25 in the three-detector network. The source was localized to 18.5 deg$^2$ at a distance of $241^{+41}_{-45}$ Mpc; no electromagnetic counterpart has been confirmed to date. The source has the most unequal mass ratio yet measured with gravitational waves, $0.112^{+0.008}_{-0.009}$, and its secondary component is either the lightest black hole or the heaviest neutron star ever discovered in a double compact-object system. The dimensionless spin of the primary black hole is tightly constrained to $\leq 0.07$. Tests of general relativity reveal no measurable deviations from the theory, and its prediction of higher-multipole emission is confirmed at high confidence. We estimate a merger rate density of 1-23 Gpc$^{-3}$ yr$^{-1}$ for the new class of binary coalescence sources that GW190814 represents. Astrophysical models predict that binaries with mass ratios similar to this event can form through several channels, but are unlikely to have formed in globular clusters. However, the combination of mass ratio, component masses, and the inferred merger rate for this event challenges all current models for the formation and mass distribution of compact-object binaries.
Keywords	covid19
Publisher	ArXiv
Document type	Article ; Online
DOI	10.3847/2041-8213/ab960f
Database	COVID19

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Article ; Online: An upper limit on the stochastic gravitational-wave background of cosmological origin.

Abbott, B P / Abbott, R / Acernese, F / Adhikari, R / Ajith, P / Allen, B / Allen, G / Alshourbagy, M / Amin, R S / Anderson, S B / Anderson, W G / Antonucci, F / Aoudia, S / Arain, M A / Araya, M / Armandula, H / Armor, P / Arun, K G / Aso, Y /

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Nature

2009 Volume 460, Issue 7258, Page(s) 990–994

Abstract: A stochastic background of gravitational waves is expected to arise from a superposition of a large number of unresolved gravitational-wave sources of astrophysical and cosmological origin. It should carry unique signatures from the earliest epochs in ... ...

Abstract	A stochastic background of gravitational waves is expected to arise from a superposition of a large number of unresolved gravitational-wave sources of astrophysical and cosmological origin. It should carry unique signatures from the earliest epochs in the evolution of the Universe, inaccessible to standard astrophysical observations. Direct measurements of the amplitude of this background are therefore of fundamental importance for understanding the evolution of the Universe when it was younger than one minute. Here we report limits on the amplitude of the stochastic gravitational-wave background using the data from a two-year science run of the Laser Interferometer Gravitational-wave Observatory (LIGO). Our result constrains the energy density of the stochastic gravitational-wave background normalized by the critical energy density of the Universe, in the frequency band around 100 Hz, to be <6.9 x 10(-6) at 95% confidence. The data rule out models of early Universe evolution with relatively large equation-of-state parameter, as well as cosmic (super)string models with relatively small string tension that are favoured in some string theory models. This search for the stochastic background improves on the indirect limits from Big Bang nucleosynthesis and cosmic microwave background at 100 Hz.
Language	English
Publishing date	2009-08-20
Publishing country	England
Document type	Journal Article
ZDB-ID	120714-3
ISSN	1476-4687 ; 0028-0836
ISSN (online)	1476-4687
ISSN	0028-0836
DOI	10.1038/nature08278
Database	MEDical Literature Analysis and Retrieval System OnLINE

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