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Improving LIGO calibration accuracy by tracking and compensating for slow temporal variations

Tuyenbayev, D. and Karki, S. and Betzwieser, J. and Cahillane, C. and Goetz, E. and Izumi, K. and Kandhasamy, S. and Kissel, J. S. and Mendell, G. and Wade, M. and Weinstein, A. J. and Savage, R. L. (2017) Improving LIGO calibration accuracy by tracking and compensating for slow temporal variations. Classical and Quantum Gravity, 34 (1). Art. No. 015002. ISSN 0264-9381. http://resolver.caltech.edu/CaltechAUTHORS:20170112-122943086

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Abstract

Calibration of the second-generation LIGO interferometric gravitational-wave detectors employs a method that uses injected periodic modulations to track and compensate for slow temporal variations in the differential length response of the instruments. These detectors utilize feedback control loops to maintain resonance conditions by suppressing differential arm length variations. We describe how the sensing and actuation functions of these servo loops are parameterized and how the slow variations in these parameters are quantified using the injected modulations. We report the results of applying this method to the LIGO detectors and show that it significantly reduces systematic errors in their calibrated outputs.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1088/0264-9381/34/1/015002DOIArticle
http://iopscience.iop.org/article/10.1088/0264-9381/34/1/015002/metaPublisherArticle
https://arxiv.org/abs/1608.05134arXivDiscussion Paper
ORCID:
AuthorORCID
Weinstein, A. J.0000-0002-0928-6784
Additional Information:© 2016 IOP Publishing Ltd. Received 8 August 2016, revised 21 October 2016; Accepted for publication 1 November 2016; Published 6 December 2016. LIGO was constructed by the California Institute of Technology and Massachusetts Institute of Technology with funding from the National Science Foundation (NSF) and operates under cooperative agreement PHY-0757058. This work was supported by the following NSF grants: HRD-1242090 for D Tuyenbayev, PHY-1607336 for S Karki, PHY-1404139 for S Kandhasamy and PHY-1607178 for M Wade. Fellowship support for S Karki and D Tuyenbayev from the LIGO Laboratory and for D Tuyenbayev from the UTRGV College of Sciences are also gratefully acknowledged. This paper carries LIGO Document Number LIGO-P1600063.
Group:LIGO
Funders:
Funding AgencyGrant Number
NSFPHY-0757058
NSFHRD-1242090
NSFPHY-1607336
NSFPHY-1404139
NSFPHY-1607178
LIGO LaboratoryUNSPECIFIED
UTRGV College of SciencesUNSPECIFIED
Other Numbering System:
Other Numbering System NameOther Numbering System ID
LIGO DocumentLIGO-P1600063
Record Number:CaltechAUTHORS:20170112-122943086
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20170112-122943086
Official Citation:D Tuyenbayev et al 2017 Class. Quantum Grav. 34 015002
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:73475
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:18 Jan 2017 20:46
Last Modified:18 Jan 2017 21:13

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