Characterization of the LIGO detectors during their sixth science run
In 2009-2010, the Laser Interferometer Gravitational-Wave Observatory (LIGO) operated together with international partners Virgo and GEO600 as a network to search for gravitational waves (GWs) of astrophysical origin. The sensitivity of these detectors was limited by a combination of noise sources i...
| Main Authors: | , , , |
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| Other Authors: | |
| Format: | Article |
| Published: |
IOP Publishing
2019
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| Online Access: | https://hdl.handle.net/1721.1/121230 |