Full band All-sky search for periodic gravitational waves in the O1 LIGO data

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dc.contributor.author Sengupta, Anand
dc.date.accessioned 2018-03-01T09:00:43Z
dc.date.available 2018-03-01T09:00:43Z
dc.date.issued 2018-02
dc.identifier.citation Sengupta, Anand et al., “Full band All-sky search for periodic gravitational waves in the O1 LIGO data”, arXiv, Cornell University Library, DOI: arXiv:1802.05241, Feb. 2018. en_US
dc.identifier.uri https://repository.iitgn.ac.in/handle/123456789/3498
dc.identifier.uri http://arxiv.org/abs/1802.05241
dc.description.abstract We report on a new all-sky search for periodic gravitational waves in the frequency band 475-2000 Hz and with a frequency time derivative in the range of [-1.0e-8, +1e-9] Hz/s. Potential signals could be produced by a nearby spinning and slightly non-axisymmetric isolated neutron star in our galaxy. This search uses the data from Advanced LIGO's first observational run O1. No gravitational wave signals were observed, and upper limits were placed on their strengths. For completeness, results from the separately published low frequency search 20-475 Hz are included as well. Our lowest upper limit on worst-case (linearly polarized) strain amplitude h_0 is 4e-25 near 170 Hz, while at the high end of our frequency range we achieve a worst-case upper limit of 1.3e-24. For a circularly polarized source (most favorable orientation), the smallest upper limit obtained is ~1.5e-25. en_US
dc.description.statementofresponsibility Anand Sengupta et al.,
dc.language.iso en en_US
dc.publisher Cornell University Library en_US
dc.title Full band All-sky search for periodic gravitational waves in the O1 LIGO data en_US
dc.type Preprint en_US


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