Sensitivity of the Advanced LIGO detectors at the beginning of gravitational wave astronomy

التفاصيل البيبلوغرافية
العنوان: Sensitivity of the Advanced LIGO detectors at the beginning of gravitational wave astronomy
المؤلفون: Ligo, The Scientific Collaboration, Martynov, D. V., Hall, E. D., Abbott, B. P., Abbott, R., Abbott, T. D., Abernathy, M. R., Ackley, K., Adams, C., Addesso, P., Adhikari, R. X., Adya, V. B., Affeldt, C., Aggarwal, N., Aguiar, O. D., Ain, A., Ajith, P., Allen, B., Altin, P. A., Anderson, R. A., Anderson, S. B., Anderson, W. G., Arai, K., Arain, M. A., Araya, M. C., Arceneaux, C. C., Areeda, J. S., Arun, K. G., Ashton, G., Ast, M., Aston, S. M., Aufmuth, P., Aulbert, C., Babak, S., Baker, P. T., Ballmer, S. W., Barayoga, J. C., Barclay, S. E., Barish, B. C., Barker, D., Barr, B., Barsotti, L., Bartlett, J., Bartos, I., Bassiri, R., Batch, J. C., Baune, C., Belgin, M., Bell, A. S., Belopolski, I., Berger, B. K., Bergmann, G., Berry, C. P. L., Bhagwat, S., Bhandare, R., Bilenko, I. A., Billingsley, G., Birch, J., Birney, R., Biscans, S., Bisht, A., Biwer, C., Blackburn, J. K., Blair, C. D., Blair, D. G., Blair, R. M., Bock, O., Bogan, C., Bohe, A., Bond, C., Bork, R., Bose, S., Brady, P. R., Braginsky, V. B., Branco, V., Brau, J. E., Brinkmann, M., Brockill, P., Broida, J. E., Brooks, A. F., Brown, D. A., Brown, D. D., Brown, N. M., Brunett, S., Buchanan, C. C., Buikema, A., Buonanno, A., Byer, R. L., Cabero, M., Cadonati, L., Cahillane, C., Calderon Bustillo, J., Callister, T., Camp, J. B., Cannon, K. C., Cao, J., Capano, C. D., Caride, S., Caudill, S., Cavaglia, M., Cepeda, C. B., Chan, M., Chao, S., Charlton, P., Cheeseboro, B. D., Chen, H. Y., Chen, Y., Cheng, C., Cho, H. S., Cho, M., Chow, J. H., Christensen, N., Chu, Q., Chung, S., Ciani, G., Clara, F., Clark, J. A., Collette, C. G., Cominsky, L., Constancio, M., Cook, D., Corbitt, T. R., Cornish, N., Corpuz, A. A., Corsi, A., Costa, C. A., Coughlin, M. W., Coughlin, S. B., Countryman, S. T., Couvares, P., Cowan, E. E., Coward, D. M., Cowart, M. J., Coyne, D. C., Coyne, R., Craig, K., Creighton, J. D. E., Cripe, J., Crowder, S. G., Cumming, A., Cunningham, L., Dal Canton, T., Damjanic, M., Danilishin, S. L., Danzmann, K., Darman, N. S., Dasgupta, A., Da Silva Costa, C. F., Dave, I., Davies, G. S., Daw, E. J., Day, B., De, S., Debra, D., Del Pozzo, W., Denker, T., Dent, T., Dergachev, V., Derosa, R. T., Desalvo, R., Devine, R. C., Dhurandhar, S., Diaz, M. C., Di Palma, I., Donovan, F., Dooley, K. L., Doravari, S., Douglas, R., Downes, T. P., Drago, M., Drever, R. W. P., Driggers, J. C., Dwyer, S. E., Edo, T. B., Edwards, M. C., Effler, A., Eggenstein, H. -B, Ehrens, P., Eichholz, J., Eikenberry, S. S., Engels, W., Essick, R. C., Etzel, T., Evans, M., Evans, T. M., Everett, R., Factourovich, M., Fair, H., Fairhurst, S., Fan, X., Fang, Q., Ben Farr, Farr, W. M., Favata, M., Fays, M., Fehrmann, H., Fejer, M. M., Fenyvesi, E., Ferreira, E. C., Fisher, R. P., Fletcher, M., Foley, S., Forsyth, S. S., Frei, Z., Freise, A., Frey, R., Fritschel, P., Frolov, V. V., Fulda, P., Fyffe, M., Gabbard, H. A. G., Gair, J. R., Gaonkar, S. G., Gaur, G., Gehrels, N., Geng, P., George, J., Gergely, L., Ghosh, Abhirup, Ghosh, Archisman, Giaime, J. A., Giardina, K. D., Gill, K., Glaefke, A., Goetz, E., Goetz, R., Gondan, L., Gonzalez, G., Gopakumar, A., Gordon, N. A., Gorodetsky, M. L., Gossan, S. E., Graef, C., Graff, P. B., Grant, A., Gras, S., Gray, C., Green, A. C., Greenhalgh, J., Grote, H., Grunewald, S., Guo, X., Gupta, A., Gupta, M. K., Gushwa, K. E., Gustafson, E. K., Gustafson, R., Hacker, J. J., Hall, B. R., Hammond, G., Haney, M., Hanke, M. M., Hanks, J., Hanna, C., Hannam, M. D., Hanson, J., Hardwick, T., Harry, G. M., Harry, I. W., Hart, M. J., Hartman, M. T., Haster, C. -J, Haughian, K., Heefner, J., Heintze, M. C., Hendry, M., Heng, I. S., Hennig, J., Henry, J., Heptonstall, A. W., Heurs, M., Hild, S., Hoak, D., Holt, K., Holz, D. E., Hopkins, P., Hough, J., Houston, E. A., Howell, E. J., Hu, Y. M., Huang, S., Huerta, E. A., Hughey, B., Husa, S., Huttner, S. H., Huynh-Dinh, T., Indik, N., Ingram, D. R., Inta, R., Isa, H. N., Isi, M., Isogai, T., Iyer, B. R., Izumi, K., James, E., Jang, H., Jani, K., Jawahar, S., Jian, L., Jimenez-Forteza, F., Johnson, W. W., Jones, D. I., Jones, R., Ju, L., K, Haris, Kalaghatgi, C. V., Kalogera, V., Kandhasamy, S., Kang, G., Kanner, J. B., Kapadia, S. J., Karki, S., Karvinen, K. S., Kasprzack, M., Katsavounidis, E., Katzman, W., Kaufer, S., Kaur, T., Kawabe, K., Kehl, M. S., Keitel, D., Kelley, D. B., Kells, W., Kennedy, R., Key, J. S., Khalili, F. Y., Khan, S., Khan, Z., Khazanov, E. A., Kijbunchoo, N., Kim, Chi-Woong, Kim, Chunglee, Kim, J., Kim, K., Kim, N., Kim, W., Kim, Y. -M, Kimbrell, S. J., King, E. J., King, P. J., Kissel, J. S., Klein, B., Kleybolte, L., Klimenko, S., Koehlenbeck, S. M., Kondrashov, V., Kontos, A., Korobko, M., Korth, W. Z., Kozak, D. B., Kringel, V., Krishnan, B., Krueger, C., Kuehn, G., Kumar, P., Kumar, R., Kuo, L., Kwee, P., Lackey, B. D., Landry, M., Lange, J., Lantz, B., Lasky, P. D., Laxen, M., Lazzarini, A., Leavey, S., Lebigot, E. O., Lee, C. H., Lee, H. K., Lee, H. M., Lee, K., Lenon, A., Leong, J. R., Levin, Y., Lewis, J. B., Li, T. G. F., Libson, A., Littenberg, T. B., Lockerbie, N. A., Loew, K. M., Lombardi, A. L., London, L. T., Lord, J. E., Lormand, M., Luck, H., Lundgren, A. P., Lynch, R., Ma, Y., Machenschalk, B., Macinnis, M., Macleod, D. M., Magana-Sandoval, F., Magana Zertuche, L., Magee, R. M., Mandel, I., Mandic, V., Mangano, V., Mansell, G. L., Manske, M., Marka, S., Marka, Z., Markosyan, A. S., Maros, E., Martin, I. W., Marx, J. N., Mason, K., Massinger, T. J., Masso-Reid, M., Matichard, F., Matone, L., Mavalvala, N., Mazumder, N., Mccarthy, R., Mcclelland, D. E., Mccormick, S., Mcguire, S. C., Mcintyre, G., Mciver, J., Mcmanus, D. J., Mcrae, T., Mcwilliams, S. T., Meadors, G. D., Melatos, A., Mendell, G., Mercer, R. A., Merilh, E. L., Meshkov, S., Messenger, C., Messick, C., Meyer, M., Meyers, P. M., Miao, H., Middleton, H., Mikhailov, E. E., Miller, A. L., Miller, A., Miller, B. B., Miller, J., Millhouse, M., Ming, J., Mirshekari, S., Mishra, C., Mitra, S., Mitrofanov, V. P., Mitselmakher, G., Mittleman, R., Mohapatra, S. R. P., Moore, B. C., Moore, C. J., Moraru, D., Moreno, G., Morriss, S. R., Mossavi, K., Mow-Lowry, C. M., Mueller, G., Muir, A. W., Mukherjee, Arunava, Mukherjee, D., Mukherjee, S., Mukund, N., Mullavey, A., Munch, J., Murphy, D. J., Murray, P. G., Mytidis, A., Nayak, R. K., Nedkova, K., Nelson, T. J. N., Neunzert, A., Newton, G., Nguyen, T. T., Nielsen, A. B., Nitz, A., Nolting, D., Normandin, M. E. N., Nuttall, L. K., Oberling, J., Ochsner, E., O, J., Oelker, E., Ogin, G. H., Oh, J. J., Oh, S. H., Ohme, F., Oliver, M., Oppermann, P., Oram, Richard J., O Reilly, B., O Shaughnessy, R., Ott, C. D., Ottaway, D. J., Overmier, H., Owen, B. J., Pai, A., Pai, S. A., Palamos, J. R., Palashov, O., Pal-Singh, A., Pan, H., Pankow, C., Pannarale, F., Pant, B. C., Papa, M. A., Paris, H. R., Parker, W., Pascucci, D., Patrick, Z., Pearlstone, B. L., Pedraza, M., Pekowsky, L., Pele, A., Penn, S., Perreca, A., Perri, L. M., Phelps, M., Pierro, V., Pinto, I. M., Pitkin, M., Poe, M., Post, A., Powell, J., Prasad, J., Pratt, J., Predoi, V., Prestegard, T., Price, L. R., Prijatelj, M., Principe, M., Privitera, S., Prix, R., Prokhorov, L., Puncken, O., Purrer, M., Qi, H., Qin, J., Qiu, S., Quetschke, V., Quintero, E. A., Quitzow-James, R., Raab, F. J., Rabeling, D. S., Radkins, H., Raffai, P., Raja, S., Rajan, C., Rakhmanov, M., Raymond, V., Read, J., Reed, C. M., Reid, S., Reitze, D. H., Rew, H., Reyes, S. D., Rhoades, E., Riles, K., Rizzo, M., Robertson, N. A., Robie, R., Rollins, J. G., Roma, V. J., Romano, J. D., Romanov, G., Romie, J. H., Rowan, S., Rudiger, A., Ryan, K., Sachdev, S., Sadecki, T., Sadeghian, L., Sakellariadou, M., Saleem, M., Salemi, F., Samajdar, A., Sammut, L., Sanchez, E. J., Sandberg, V., Sandeen, B., Sanders, J. R., Sathyaprakash, B. S., Saulson, P. R., Sauter, O. E. S., Savage, R. L., Sawadsky, A., Schale, P., Schilling, R., Schmidt, E., Schmidt, J., Schmidt, P., Schnabel, R., Schofield, R. M. S., Schonbeck, A., Schreiber, E., Schuette, D., Schulz, B., Schutz, B. F., Schwinberg, P., Scott, J., Scott, S. M., Sellers, D., Sengupta, A. S., Sergeev, A., Shaddock, D. A., Shaffer, T., Shahriar, M. S., Shaltev, M., Shapiro, B., Shawhan, P., Sheperd, A., Shoemaker, D. H., Shoemaker, D. M., Siemens, X., Sigg, D., Silva, A. D., Singer, A., Singer, L. P., Singh, A., Singh, R., Sintes, A. M., Slagmolen, B. J. J., Smith, J. R., Smith, N. D., Smith, R. J. E., Son, E. J., Sorazu, B., Souradeep, T., Srivastava, A. K., Staley, A., Stein, A., Steinke, M., Steinlechner, J., Steinlechner, S., Steinmeyer, D., Stephens, B. C., Stiles, D., Stone, M. C., Stone, R., Strain, K. A., Strauss, N. A., Strigin, S., Sturani, R., Stuver, A. L., Summerscales, T. Z., Sun, L., Sunil, S., Sutton, P. J., Talukder, D., Tanner, D. B., Tapai, M., Tarabrin, S. P., Taracchini, A., Taylor, R., Theeg, T., Thirugnanasambandam, M. P., Thomas, E. G., Thomas, M., Thomas, P., Thorne, K. A., Thorne, K. S., Thrane, E., Tiwari, V., Tokmakov, K. V., Toland, K., Tomlinson, C., Tornasi, Z., Torres, C. V., Torrie, C. I., Toyra, D., Traylor, G., Trifiro, D., Tse, M., Tuyenbayev, D., Ugolini, D., Unnikrishnan, C. S., Urban, A. L., Usman, S. A., Vahlbruch, H., Vajente, G., Valdes, G., Vander-Hyde, D. C., Veggel, A. A., Vargas, M., Vass, S., Vaulin, R., Vecchio, A., Veitch, J., Veitch, P. J., Venkateswara, K., Vinciguerra, S., Vine, D. J., Vitale, S., Vo, T., Vorvick, C., Voss, D. V., Vousden, W. D., Vyatchanin, S. P., Wade, A. R., Wade, L. E., Wade, M., Waldman, S., Walker, M., Wallace, L., Walsh, S., Wang, H., Wang, M., Wang, X., Wang, Y., Ward, R. L., Warner, J., Weaver, B., Weinert, M., Weinstein, A. J., Weiss, R., Wen, L., Wessels, P., Westphal, T., Wette, K., Whelan, J. T., White, D. J., Whiting, B. F., Willems, P., Williams, R. D., Williamson, A. R., Willis, J. L., Willke, B., Wimmer, M. H., Winkelmann, L., Winkler, W., Wipf, C. C., Wittel, H., Woan, G., Woehler, J., Worden, J., Wright, J. L., Wu, D. S., Wu, G., Yablon, J., Yam, W., Yamamoto, H., Yancey, C. C., Yu, H., Zanolin, M., Zevin, M., Zhang, L., Zhang, M., Zhang, Y., Zhao, C., Zhou, M., Zhou, Z., Zhu, X. J., Zucker, M. E., Zuraw, S. E., Zweizig, J.
المساهمون: The LIGO Scientific Collaboration, LSC Instrument Group, The, Galdi, V., Pierro, V., Pinto, I. M., Principe, M.
المصدر: NASA Astrophysics Data System
Physical Review D
بيانات النشر: American Physical Society (APS), 2016.
سنة النشر: 2016
مصطلحات موضوعية: Physics - Instrumentation and Detectors, Gravitational-wave observatory, Physics and Astronomy (miscellaneous), Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Astrophysics, 01 natural sciences, Gravitational-wave astronomy, General Relativity and Quantum Cosmology, Binary black hole, optical coatings, 0103 physical sciences, Astronomical interferometer, 010306 general physics, Instrumentation and Methods for Astrophysics (astro-ph.IM), QC, QB, Physics, 010308 nuclear & particles physics, Gravitational wave, Astronomy, Instrumentation and Detectors (physics.ins-det), interferometry, LIGO, Neutron star, Interferometry, Astrophysics - Instrumentation and Methods for Astrophysics
الوصف: The Laser Interferometer Gravitational Wave Observatory (LIGO) consists of two widely separated 4 km laser interferometers designed to detect gravitational waves from distant astrophysical sources in the frequency range from 10 Hz to 10 kHz. The first observation run of the Advanced LIGO detectors started in September 2015 and ended in January 2016. A strain sensitivity of better than 10^(-23) sqrt(Hz) was achieved around 100 Hz. Understanding both the fundamental and the technical noise sources was critical for increasing the astrophysical strain sensitivity. The average distance at which coalescing binary black hole systems with individual masses of 30 M⊙ could be detected above a signal-to-noise ratio (SNR) of 8 was 1.3 Gpc, and the range for binary neutron star inspirals was about 75 Mpc. With respect to the initial detectors, the observable volume of the Universe increased by a factor 69 and 43, respectively. These improvements helped Advanced LIGO to detect the gravitational wave signal from the binary black hole coalescence, known as GW150914.
وصف الملف: application/pdf
تدمد: 2470-0029
2470-0010
1550-2368
1550-7998
الوصول الحر: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::366751ee628c0fba13817af3a8e951b9Test
https://doi.org/10.1103/physrevd.93.112004Test
حقوق: OPEN
رقم الانضمام: edsair.doi.dedup.....366751ee628c0fba13817af3a8e951b9
قاعدة البيانات: OpenAIRE
الوصف
تدمد:24700029
24700010
15502368
15507998