Berger, Beverly K. (2018) Identification and mitigation of Advanced LIGO noise sources. Journal of Physics: Conference Series, 957 . Art. No. 012004. ISSN 1742-6596. https://resolver.caltech.edu/CaltechAUTHORS:20190117-092518932
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Abstract
In order to increase the reach of the astrophysical searches, various sources of instrumental and environmental noise must be identified and ameliorated. Here we discuss efforts to understand the origin of noise manifested as short-duration bursts (glitches) and/or range-impacting features at LIGO Hanford. Several examples found at LIGO Hanford Observatory in O1 and O2 were identified including glitches due to an air compressor, ringing phone, airplanes, and an incorrect servo setting, and a decrease in detector sensitivity due to truck traffic.
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| Additional Information: | © 2018 Published under licence by IOP Publishing Ltd. Content from this work may be used under the terms of the Creative Commons Attribution 3.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI. Published under licence by IOP Publishing Ltd. I would like to thank S. Dwyer, J. McIver, B. O'Reily, and J. Smith for valuable comments. LIGO was constructed by the California Institute of Technology and Massachusetts Institute of Technology with funding from the National Science Foundation and operates under cooperative agreement PHY-0757058. This paper carries the LIGO Document Number P1700343. | ||||||
| Group: | LIGO | ||||||
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| Record Number: | CaltechAUTHORS:20190117-092518932 | ||||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20190117-092518932 | ||||||
| Official Citation: | Beverly K. Berger 2018 J. Phys.: Conf. Ser. 957 012004 | ||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | ||||||
| ID Code: | 92338 | ||||||
| Collection: | CaltechAUTHORS | ||||||
| Deposited By: | Tony Diaz | ||||||
| Deposited On: | 22 Jan 2019 22:29 | ||||||
| Last Modified: | 03 Oct 2019 20:43 |
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