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Cited by 481

The DOI matches its Crossref record; 2 of the 2 references it cites were found in a registry or an index.

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

Open access
Martynov, D. V., Hall, E. D., Abbott, B. P., Abbott, R., Abbott, T. D., Adams, C., Adhikari, R. X., Anderson, R. A., Anderson, S. B., Arai, K., Arain, M. A., Aston, S. M., Austin, L., Ballmer, S. W., Barbet, M., Barker, D., Barr, B., Barsotti, L., Bartlett, J., Barton, M. A., Bartos, I., Batch, J. C., Bell, A. S., Belopolski, I., Bergman, J., Betzwieser, J., Billingsley, G., Birch, J., Biscans, S., Biwer, C., Black, E., Blair, C. D., Bogan, C., Bond, C., Bork, R., Bridges, D. O., Brooks, A. F., Brown, D. D., Carbone, L., Celerier, C., Ciani, G., Clara, F., Cook, D., Countryman, S. T., Cowart, M. J., Coyne, D. C., Cumming, A., Cunningham, L., Damjanic, M., Dannenberg, R., Danzmann, K., Costa, C. F. Da Silva, Daw, E. J., DeBra, D., DeRosa, R. T., DeSalvo, R., Dooley, K. L., Doravari, S., Driggers, J. C., Dwyer, S. E., Effler, A., Etzel, T., Evans, M., Evans, T. M., Factourovich, M., Fair, H., Feldbaum, D., Fisher, R. P., Foley, S., Frede, M., Freise, A., Fritschel, P., Frolov, V. V., Fulda, P., Fyffe, M., Galdi, V., Giaime, J. A., Giardina, K. D., Gleason, J. R., Goetz, R., Gras, S., Gray, C., Greenhalgh, R. J. S., Grote, H., Guido, C. J., Gushwa, K. E., Gustafson, E. K., Gustafson, R., Hammond, G., Hanks, J., Hanson, J., Hardwick, T., Harry, G. M., Haughian, K., Heefner, J., Heintze, M. C., Heptonstall, A. W., Hoak, D., Hough, J., Ivanov, A., Izumi, K., Jacobson, M., James, E., Jones, R., Kandhasamy, S., Karki, S., Kasprzack, M., Kaufer, S., Kawabe, K., Kells, W., Kijbunchoo, N., King, E. J., King, P. J., Kinzel, D. L., Kissel, J. S., Kokeyama, K., Korth, W. Z., Kuehn, G., Kwee, P., Landry, M., Lantz, B., Le Roux, A., Levine, B. M., Lewis, J. B., Lhuillier, V., Lockerbie, N. A., Lormand, M., Lubinski, M. J., Lundgren, A. P., MacDonald, T., MacInnis, M., Macleod, D. M., Mageswaran, M., Mailand, K., Márka, S., Márka, Z., Markosyan, A. S., Maros, E., Martin, I. W., Martin, R. M., Marx, J. N., Mason, K., Massinger, T. J., Matichard, F., Mavalvala, N., McCarthy, R., McClelland, D. E., McCormick, S., McIntyre, G., McIver, J., Merilh, E. L., Meyer, M. S., Meyers, P. M., Miller, J., Mittleman, R., Moreno, G., Mueller, C. L., Mueller, G., Mullavey, A., Munch, J., Murray, P. G., Nuttall, L. K., Oberling, J., O’Dell, J., Oppermann, P., Oram, Richard J., O’Reilly, B., Osthelder, C., Ottaway, D. J., Overmier, H., Palamos, J. R., Paris, H. R., Parker, W., Patrick, Z., Pele, A., Penn, S., Phelps, M., Pickenpack, M., Pierro, V., Pinto, I., Poeld, J., Principe, M., Prokhorov, L., Puncken, O., Quetschke, V., Quintero, E. A., Raab, F. J., Radkins, H., Raffai, P., Ramet, C. R., Reed, C. M., Reid, S., Reitze, D. H., Robertson, N. A., Rollins, J. G., Roma, V. J., Romie, J. H., Rowan, S., Ryan, K., Sadecki, T., Sanchez, E. J., Sandberg, V., Sannibale, V., Savage, R. L., Schofield, R. M. S., Schultz, B., Schwinberg, P., Sellers, D., Sevigny, A., Shaddock, D. A., Shao, Z., Shapiro, B., Shawhan, P., Shoemaker, D. H., Sigg, D., Slagmolen, B. J. J., Smith, J. R., Smith, M. R., Smith-Lefebvre, N. D., Sorazu, B., Staley, A., Stein, A. J., Stochino, A., Strain, K. A., Taylor, R., Thomas, M., Thomas, P., Thorne, K. A., Thrane, E., Tokmakov, K. V., Torrie, C. I., Traylor, G., Vajente, G., Valdes, G., van Veggel, A. A., Vargas, M., Vecchio, A., Veitch, P. J., Venkateswara, K., Vo, T., Vorvick, C., Waldman, S. J., Walker, M., Ward, R. L., Warner, J., Weaver, B., Weiss, R., Welborn, T., Weßels, P., Wilkinson, C., Willems, P. A., Williams, L., Willke, B., Wilmut, I., Winkelmann, L., Wipf, C. C., Worden, J., Wu, G., Yamamoto, H., Yancey, C. C., Yu, H., Zhang, L., Zucker, M. E., Zweizig, J.·2016·Physical Review D
DOI 10.1103/physrevd.93.112004
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Abstract

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 ${10}^{\ensuremath{-}23}/\sqrt{\mathrm{Hz}}$ 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 $30\text{ }\text{ }{M}_{\ensuremath{\bigodot}}$ 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.

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Authors
Martynov, D. V., Hall, E. D., Abbott, B. P., Abbott, R., Abbott, T. D., Adams, C., Adhikari, R. X., Anderson, R. A., Anderson, S. B., Arai, K., Arain, M. A., Aston, S. M., Austin, L., Ballmer, S. W., Barbet, M., Barker, D., Barr, B., Barsotti, L., Bartlett, J., Barton, M. A., Bartos, I., Batch, J. C., Bell, A. S., Belopolski, I., Bergman, J., Betzwieser, J., Billingsley, G., Birch, J., Biscans, S., Biwer, C., Black, E., Blair, C. D., Bogan, C., Bond, C., Bork, R., Bridges, D. O., Brooks, A. F., Brown, D. D., Carbone, L., Celerier, C., Ciani, G., Clara, F., Cook, D., Countryman, S. T., Cowart, M. J., Coyne, D. C., Cumming, A., Cunningham, L., Damjanic, M., Dannenberg, R., Danzmann, K., Costa, C. F. D. S., Daw, E. J., DeBra, D., DeRosa, R. T., DeSalvo, R., Dooley, K. L., Doravari, S., Driggers, J. C., Dwyer, S. E., Effler, A., Etzel, T., Evans, M., Evans, T. M., Factourovich, M., Fair, H., Feldbaum, D., Fisher, R. P., Foley, S., Frede, M., Freise, A., Fritschel, P., Frolov, V. V., Fulda, P., Fyffe, M., Galdi, V., Giaime, J. A., Giardina, K. D., Gleason, J. R., Goetz, R., Gras, S., Gray, C., Greenhalgh, R. J. S., Grote, H., Guido, C. J., Gushwa, K. E., Gustafson, E. K., Gustafson, R., Hammond, G., Hanks, J., Hanson, J., Hardwick, T., Harry, G. M., Haughian, K., Heefner, J., Heintze, M. C., Heptonstall, A. W., Hoak, D., Hough, J., Ivanov, A., Izumi, K., Jacobson, M., James, E., Jones, R., Kandhasamy, S., Karki, S., Kasprzack, M., Kaufer, S., Kawabe, K., Kells, W., Kijbunchoo, N., King, E. J., King, P. J., Kinzel, D. L., Kissel, J. S., Kokeyama, K., Korth, W. Z., Kuehn, G., Kwee, P., Landry, M., Lantz, B., Le Roux, A., Levine, B. M., Lewis, J. B., Lhuillier, V., Lockerbie, N. A., Lormand, M., Lubinski, M. J., Lundgren, A. P., MacDonald, T., MacInnis, M., Macleod, D. M., Mageswaran, M., Mailand, K., Márka, S., Márka, Z., Markosyan, A. S., Maros, E., Martin, I. W., Martin, R. M., Marx, J. N., Mason, K., Massinger, T. J., Matichard, F., Mavalvala, N., McCarthy, R., McClelland, D. E., McCormick, S., McIntyre, G., McIver, J., Merilh, E. L., Meyer, M. S., Meyers, P. M., Miller, J., Mittleman, R., Moreno, G., Mueller, C. L., Mueller, G., Mullavey, A., Munch, J., Murray, P. G., Nuttall, L. K., Oberling, J., O’Dell, J., Oppermann, P., Oram, R. J., O’Reilly, B., Osthelder, C., Ottaway, D. J., Overmier, H., Palamos, J. R., Paris, H. R., Parker, W., Patrick, Z., Pele, A., Penn, S., Phelps, M., Pickenpack, M., Pierro, V., Pinto, I., Poeld, J., Principe, M., Prokhorov, L., Puncken, O., Quetschke, V., Quintero, E. A., Raab, F. J., Radkins, H., Raffai, P., Ramet, C. R., Reed, C. M., Reid, S., Reitze, D. H., Robertson, N. A., Rollins, J. G., Roma, V. J., Romie, J. H., Rowan, S., Ryan, K., Sadecki, T., Sanchez, E. J., Sandberg, V., Sannibale, V., Savage, R. L., Schofield, R. M. S., Schultz, B., Schwinberg, P., Sellers, D., Sevigny, A., Shaddock, D. A., Shao, Z., Shapiro, B., Shawhan, P., Shoemaker, D. H., Sigg, D., Slagmolen, B. J. J., Smith, J. R., Smith, M. R., Smith-Lefebvre, N. D., Sorazu, B., Staley, A., Stein, A. J., Stochino, A., Strain, K. A., Taylor, R., Thomas, M., Thomas, P., Thorne, K. A., Thrane, E., Tokmakov, K. V., Torrie, C. I., Traylor, G., Vajente, G., Valdes, G., van Veggel, A. A., Vargas, M., Vecchio, A., Veitch, P. J., Venkateswara, K., Vo, T., Vorvick, C., Waldman, S. J., Walker, M., Ward, R. L., Warner, J., Weaver, B., Weiss, R., Welborn, T., Weßels, P., Wilkinson, C., Willems, P. A., Williams, L., Willke, B., Wilmut, I., Winkelmann, L., Wipf, C. C., Worden, J., Wu, G., Yamamoto, H., Yancey, C. C., Yu, H., Zhang, L., Zucker, M. E., & Zweizig, J.
Venue
Physical Review D
Publisher
American Physical Society (APS)
Published
2016-06-02
Volume
93
Issue
11
ISSN
  • 2470-0010 (ISSN-L)
  • 2470-0029
DOI
10.1103/physrevd.93.112004
OpenAlex
W2339792708
Cited by
481
References
2
FWCI
27.67
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Sensitivity of the Advanced LIGO detectors at the beginning of gravitational wave astronomy. https://app.cochat.ai/papers/10.1103/physrevd.93.112004
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Martynov, D. V., Hall, E. D., Abbott, B. P., Abbott, R., Abbott, T. D., Adams, C., Adhikari, R. X., Anderson, R. A., Anderson, S. B., Arai, K., Arain, M. A., Aston, S. M., Austin, L., Ballmer, S. W., Barbet, M., Barker, D., Barr, B., Barsotti, L., Bartlett, J., . . . Zweizig, J. (2016). Sensitivity of the Advanced LIGO detectors at the beginning of gravitational wave astronomy. Physical Review D. https://doi.org/10.1103/physrevd.93.112004

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