An all-sky search for long-duration gravitational wave transients with initial LIGO

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dc.contributor.author Sengupta, Anand
dc.date.accessioned 2015-12-16T09:40:10Z
dc.date.available 2015-12-16T09:40:10Z
dc.date.issued 2015-11
dc.identifier.citation Sengupta, Anand et al., “An all-sky search for long-duration gravitational wave transients with initial LIGO”, arXiv, Cornell University Library, DOI: arXiv:1511.04398v1, Nov. 2015. en_US
dc.identifier.other http://arxiv.org/abs/1511.04398v1
dc.identifier.uri https://repository.iitgn.ac.in/handle/123456789/2004
dc.description.abstract We present the results of a search for long-duration gravitational wave transients in two sets of data collected by the LIGO Hanford and LIGO Livingston detectors between November 5, 2005 and September 30, 2007, and July 7, 2009 and October 20, 2010, with a total observational time of 283.0 days and 132.9 days, respectively. The search targets gravitational wave transients of duration 10 - 500 seconds in a frequency band of 40 - 1000 Hz, with minimal assumptions about the signal waveform, polarization, source direction, or time of occurrence. All candidate triggers were consistent with the expected background; as a result we set 90% confidence upper limits on the rate of long-duration gravitational wave transients for different types of gravitational wave signals. We also report upper limits on the source rate density per year per Mpc^3 for specific signal models. These are the first results from an all-sky search for unmodeled long-duration transient gravitational waves. en_US
dc.description.statementofresponsibility by Anand Sengupta et.al.
dc.language.iso en_US en_US
dc.publisher Cornell University Library en_US
dc.subject General Relativity and Quantum Cosmology (gr-qc) en_US
dc.subject Cosmology and Nongalactic Astrophysics (astro-ph.CO) en_US
dc.subject Instrumentation and Methods for Astrophysics (astro-ph.IM) en_US
dc.title An all-sky search for long-duration gravitational wave transients with initial LIGO en_US
dc.type Preprint en_US


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