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We present a new method which accounts for changes in the properties of gravitational-wave detector noise over time in the PyCBC search for gravitational waves from compact binary coalescences. We use information from LIGO data quality streams that m
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::00dc8840977de18e1217eaff8b860d05
http://arxiv.org/abs/2204.03091
http://arxiv.org/abs/2204.03091