The Advanced LIGO photon calibrators

The two interferometers of the Laser Interferometry Gravitational-wave Observatory (LIGO) recently detected gravitational waves from the mergers of binary black hole systems. Accurate calibration of the output of these detectors was crucial for the observation of these events and the extraction of p...
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Autor*in:	Karki, S [verfasserIn] Tuyenbayev, D Kandhasamy, S Abbott, B. P Abbott, T. D Anders, E. H Berliner, J Betzwieser, J Cahillane, C Canete, L Conley, C Daveloza, H. P De Lillo, N Gleason, J. R Goetz, E Izumi, K Kissel, J. S Mendell, G Quetschke, V Rodruck, M Sachdev, S Sadecki, T Schwinberg, P. B Sottile, A Wade, M Weinstein, A. J West, M Savage, R. L

Format:	Artikel
Sprache:	Englisch

Erschienen:	2016

Rechteinformationen:	Nutzungsrecht: © Author(s)

Übergeordnetes Werk:	Enthalten in: Review of scientific instruments - Melville, NY : AIP, 1930, 87(2016), 11
Übergeordnetes Werk:	volume:87 ; year:2016 ; number:11

Links:	Volltext Link aufrufen

DOI / URN:	10.1063/1.4967303

Katalog-ID:	OLC1984136739

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700	1		\|a Gleason, J. R \|4 oth
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allfields	10.1063/1.4967303 doi PQ20161201 (DE-627)OLC1984136739 (DE-599)GBVOLC1984136739 (PRQ)c693-db8a6d95ad9f707ec08b0a1f5f7980911a1ffdaa8f2f76f07aaee0455e13eb8c0 (KEY)0016010520160000087001100000advancedligophotoncalibrators DE-627 ger DE-627 rakwb eng 530 620 DE-600 Karki, S verfasserin aut The Advanced LIGO photon calibrators 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier The two interferometers of the Laser Interferometry Gravitational-wave Observatory (LIGO) recently detected gravitational waves from the mergers of binary black hole systems. Accurate calibration of the output of these detectors was crucial for the observation of these events and the extraction of parameters of the sources. The principal tools used to calibrate the responses of the second-generation (Advanced) LIGO detectors to gravitational waves are systems based on radiation pressure and referred to as photon calibrators. These systems, which were completely redesigned for Advanced LIGO, include several significant upgrades that enable them to meet the calibration requirements of second-generation gravitational wave detectors in the new era of gravitational-wave astronomy. We report on the design, implementation, and operation of these Advanced LIGO photon calibrators that are currently providing fiducial displacements on the order of 1 0 − 18 m / Hz with accuracy and precision of better than 1%. Nutzungsrecht: © Author(s) Tuyenbayev, D oth Kandhasamy, S oth Abbott, B. P oth Abbott, T. D oth Anders, E. H oth Berliner, J oth Betzwieser, J oth Cahillane, C oth Canete, L oth Conley, C oth Daveloza, H. P oth De Lillo, N oth Gleason, J. R oth Goetz, E oth Izumi, K oth Kissel, J. S oth Mendell, G oth Quetschke, V oth Rodruck, M oth Sachdev, S oth Sadecki, T oth Schwinberg, P. B oth Sottile, A oth Wade, M oth Weinstein, A. J oth West, M oth Savage, R. L oth Enthalten in Review of scientific instruments Melville, NY : AIP, 1930 87(2016), 11 (DE-627)129509175 (DE-600)209865-9 (DE-576)014915782 0034-6748 nnns volume:87 year:2016 number:11 http://dx.doi.org/10.1063/1.4967303 Volltext http://dx.doi.org/10.1063/1.4967303 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY GBV_ILN_21 GBV_ILN_47 GBV_ILN_59 GBV_ILN_70 GBV_ILN_170 GBV_ILN_2219 GBV_ILN_2279 GBV_ILN_4306 GBV_ILN_4310 AR 87 2016 11
spelling	10.1063/1.4967303 doi PQ20161201 (DE-627)OLC1984136739 (DE-599)GBVOLC1984136739 (PRQ)c693-db8a6d95ad9f707ec08b0a1f5f7980911a1ffdaa8f2f76f07aaee0455e13eb8c0 (KEY)0016010520160000087001100000advancedligophotoncalibrators DE-627 ger DE-627 rakwb eng 530 620 DE-600 Karki, S verfasserin aut The Advanced LIGO photon calibrators 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier The two interferometers of the Laser Interferometry Gravitational-wave Observatory (LIGO) recently detected gravitational waves from the mergers of binary black hole systems. Accurate calibration of the output of these detectors was crucial for the observation of these events and the extraction of parameters of the sources. The principal tools used to calibrate the responses of the second-generation (Advanced) LIGO detectors to gravitational waves are systems based on radiation pressure and referred to as photon calibrators. These systems, which were completely redesigned for Advanced LIGO, include several significant upgrades that enable them to meet the calibration requirements of second-generation gravitational wave detectors in the new era of gravitational-wave astronomy. We report on the design, implementation, and operation of these Advanced LIGO photon calibrators that are currently providing fiducial displacements on the order of 1 0 − 18 m / Hz with accuracy and precision of better than 1%. Nutzungsrecht: © Author(s) Tuyenbayev, D oth Kandhasamy, S oth Abbott, B. P oth Abbott, T. D oth Anders, E. H oth Berliner, J oth Betzwieser, J oth Cahillane, C oth Canete, L oth Conley, C oth Daveloza, H. P oth De Lillo, N oth Gleason, J. R oth Goetz, E oth Izumi, K oth Kissel, J. S oth Mendell, G oth Quetschke, V oth Rodruck, M oth Sachdev, S oth Sadecki, T oth Schwinberg, P. B oth Sottile, A oth Wade, M oth Weinstein, A. J oth West, M oth Savage, R. L oth Enthalten in Review of scientific instruments Melville, NY : AIP, 1930 87(2016), 11 (DE-627)129509175 (DE-600)209865-9 (DE-576)014915782 0034-6748 nnns volume:87 year:2016 number:11 http://dx.doi.org/10.1063/1.4967303 Volltext http://dx.doi.org/10.1063/1.4967303 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY GBV_ILN_21 GBV_ILN_47 GBV_ILN_59 GBV_ILN_70 GBV_ILN_170 GBV_ILN_2219 GBV_ILN_2279 GBV_ILN_4306 GBV_ILN_4310 AR 87 2016 11
allfields_unstemmed	10.1063/1.4967303 doi PQ20161201 (DE-627)OLC1984136739 (DE-599)GBVOLC1984136739 (PRQ)c693-db8a6d95ad9f707ec08b0a1f5f7980911a1ffdaa8f2f76f07aaee0455e13eb8c0 (KEY)0016010520160000087001100000advancedligophotoncalibrators DE-627 ger DE-627 rakwb eng 530 620 DE-600 Karki, S verfasserin aut The Advanced LIGO photon calibrators 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier The two interferometers of the Laser Interferometry Gravitational-wave Observatory (LIGO) recently detected gravitational waves from the mergers of binary black hole systems. Accurate calibration of the output of these detectors was crucial for the observation of these events and the extraction of parameters of the sources. The principal tools used to calibrate the responses of the second-generation (Advanced) LIGO detectors to gravitational waves are systems based on radiation pressure and referred to as photon calibrators. These systems, which were completely redesigned for Advanced LIGO, include several significant upgrades that enable them to meet the calibration requirements of second-generation gravitational wave detectors in the new era of gravitational-wave astronomy. We report on the design, implementation, and operation of these Advanced LIGO photon calibrators that are currently providing fiducial displacements on the order of 1 0 − 18 m / Hz with accuracy and precision of better than 1%. Nutzungsrecht: © Author(s) Tuyenbayev, D oth Kandhasamy, S oth Abbott, B. P oth Abbott, T. D oth Anders, E. H oth Berliner, J oth Betzwieser, J oth Cahillane, C oth Canete, L oth Conley, C oth Daveloza, H. P oth De Lillo, N oth Gleason, J. R oth Goetz, E oth Izumi, K oth Kissel, J. S oth Mendell, G oth Quetschke, V oth Rodruck, M oth Sachdev, S oth Sadecki, T oth Schwinberg, P. B oth Sottile, A oth Wade, M oth Weinstein, A. J oth West, M oth Savage, R. L oth Enthalten in Review of scientific instruments Melville, NY : AIP, 1930 87(2016), 11 (DE-627)129509175 (DE-600)209865-9 (DE-576)014915782 0034-6748 nnns volume:87 year:2016 number:11 http://dx.doi.org/10.1063/1.4967303 Volltext http://dx.doi.org/10.1063/1.4967303 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY GBV_ILN_21 GBV_ILN_47 GBV_ILN_59 GBV_ILN_70 GBV_ILN_170 GBV_ILN_2219 GBV_ILN_2279 GBV_ILN_4306 GBV_ILN_4310 AR 87 2016 11
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allfieldsSound	10.1063/1.4967303 doi PQ20161201 (DE-627)OLC1984136739 (DE-599)GBVOLC1984136739 (PRQ)c693-db8a6d95ad9f707ec08b0a1f5f7980911a1ffdaa8f2f76f07aaee0455e13eb8c0 (KEY)0016010520160000087001100000advancedligophotoncalibrators DE-627 ger DE-627 rakwb eng 530 620 DE-600 Karki, S verfasserin aut The Advanced LIGO photon calibrators 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier The two interferometers of the Laser Interferometry Gravitational-wave Observatory (LIGO) recently detected gravitational waves from the mergers of binary black hole systems. Accurate calibration of the output of these detectors was crucial for the observation of these events and the extraction of parameters of the sources. The principal tools used to calibrate the responses of the second-generation (Advanced) LIGO detectors to gravitational waves are systems based on radiation pressure and referred to as photon calibrators. These systems, which were completely redesigned for Advanced LIGO, include several significant upgrades that enable them to meet the calibration requirements of second-generation gravitational wave detectors in the new era of gravitational-wave astronomy. We report on the design, implementation, and operation of these Advanced LIGO photon calibrators that are currently providing fiducial displacements on the order of 1 0 − 18 m / Hz with accuracy and precision of better than 1%. Nutzungsrecht: © Author(s) Tuyenbayev, D oth Kandhasamy, S oth Abbott, B. P oth Abbott, T. D oth Anders, E. H oth Berliner, J oth Betzwieser, J oth Cahillane, C oth Canete, L oth Conley, C oth Daveloza, H. P oth De Lillo, N oth Gleason, J. R oth Goetz, E oth Izumi, K oth Kissel, J. S oth Mendell, G oth Quetschke, V oth Rodruck, M oth Sachdev, S oth Sadecki, T oth Schwinberg, P. B oth Sottile, A oth Wade, M oth Weinstein, A. J oth West, M oth Savage, R. L oth Enthalten in Review of scientific instruments Melville, NY : AIP, 1930 87(2016), 11 (DE-627)129509175 (DE-600)209865-9 (DE-576)014915782 0034-6748 nnns volume:87 year:2016 number:11 http://dx.doi.org/10.1063/1.4967303 Volltext http://dx.doi.org/10.1063/1.4967303 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY GBV_ILN_21 GBV_ILN_47 GBV_ILN_59 GBV_ILN_70 GBV_ILN_170 GBV_ILN_2219 GBV_ILN_2279 GBV_ILN_4306 GBV_ILN_4310 AR 87 2016 11
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spellingShingle	Karki, S ddc 530 The Advanced LIGO photon calibrators
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title	The Advanced LIGO photon calibrators
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title_sort	advanced ligo photon calibrators
title_auth	The Advanced LIGO photon calibrators
abstract	The two interferometers of the Laser Interferometry Gravitational-wave Observatory (LIGO) recently detected gravitational waves from the mergers of binary black hole systems. Accurate calibration of the output of these detectors was crucial for the observation of these events and the extraction of parameters of the sources. The principal tools used to calibrate the responses of the second-generation (Advanced) LIGO detectors to gravitational waves are systems based on radiation pressure and referred to as photon calibrators. These systems, which were completely redesigned for Advanced LIGO, include several significant upgrades that enable them to meet the calibration requirements of second-generation gravitational wave detectors in the new era of gravitational-wave astronomy. We report on the design, implementation, and operation of these Advanced LIGO photon calibrators that are currently providing fiducial displacements on the order of 1 0 − 18 m / Hz with accuracy and precision of better than 1%.
abstractGer	The two interferometers of the Laser Interferometry Gravitational-wave Observatory (LIGO) recently detected gravitational waves from the mergers of binary black hole systems. Accurate calibration of the output of these detectors was crucial for the observation of these events and the extraction of parameters of the sources. The principal tools used to calibrate the responses of the second-generation (Advanced) LIGO detectors to gravitational waves are systems based on radiation pressure and referred to as photon calibrators. These systems, which were completely redesigned for Advanced LIGO, include several significant upgrades that enable them to meet the calibration requirements of second-generation gravitational wave detectors in the new era of gravitational-wave astronomy. We report on the design, implementation, and operation of these Advanced LIGO photon calibrators that are currently providing fiducial displacements on the order of 1 0 − 18 m / Hz with accuracy and precision of better than 1%.
abstract_unstemmed	The two interferometers of the Laser Interferometry Gravitational-wave Observatory (LIGO) recently detected gravitational waves from the mergers of binary black hole systems. Accurate calibration of the output of these detectors was crucial for the observation of these events and the extraction of parameters of the sources. The principal tools used to calibrate the responses of the second-generation (Advanced) LIGO detectors to gravitational waves are systems based on radiation pressure and referred to as photon calibrators. These systems, which were completely redesigned for Advanced LIGO, include several significant upgrades that enable them to meet the calibration requirements of second-generation gravitational wave detectors in the new era of gravitational-wave astronomy. We report on the design, implementation, and operation of these Advanced LIGO photon calibrators that are currently providing fiducial displacements on the order of 1 0 − 18 m / Hz with accuracy and precision of better than 1%.
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container_issue	11
title_short	The Advanced LIGO photon calibrators
url	http://dx.doi.org/10.1063/1.4967303
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author2	Tuyenbayev, D Kandhasamy, S Abbott, B. P Abbott, T. D Anders, E. H Berliner, J Betzwieser, J Cahillane, C Canete, L Conley, C Daveloza, H. P De Lillo, N Gleason, J. R Goetz, E Izumi, K Kissel, J. S Mendell, G Quetschke, V Rodruck, M Sachdev, S Sadecki, T Schwinberg, P. B Sottile, A Wade, M Weinstein, A. J West, M Savage, R. L
author2Str	Tuyenbayev, D Kandhasamy, S Abbott, B. P Abbott, T. D Anders, E. H Berliner, J Betzwieser, J Cahillane, C Canete, L Conley, C Daveloza, H. P De Lillo, N Gleason, J. R Goetz, E Izumi, K Kissel, J. S Mendell, G Quetschke, V Rodruck, M Sachdev, S Sadecki, T Schwinberg, P. B Sottile, A Wade, M Weinstein, A. J West, M Savage, R. L
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doi_str	10.1063/1.4967303
up_date	2024-07-03T23:19:18.678Z
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