Application of a zero-latency whitening filter to compact binary coalescence gravitational-wave searches

Leo Tsukada, Kipp Cannon, Chad Hanna, Drew Keppel, Duncan Meacher, Cody Messick

Research output: Contribution to journalArticle

Abstract

Joint electromagnetic and gravitational-wave (GW) observation is a major goal of both the GW astronomy and electromagnetic astronomy communities for the coming decade. One way to accomplish this goal is to direct follow-up of GW candidates. Prompt electromagnetic emission may fade quickly, therefore it is desirable to have GW detection happen as quickly as possible. A leading source of latency in GW detection is the whitening of the data. We examine the performance of a zero-latency whitening filter in a detection pipeline for compact binary coalescence (CBC) GW signals. We find that the filter reproduces signal-to-noise ratio (SNR) sufficiently consistent with the results of the original high-latency and phase-preserving filter for both noise and artificial GW signals (called "injections"). Additionally, we demonstrate that these two whitening filters show excellent agreement in χ2 value, a discriminator for GW signals.

Original languageEnglish (US)
Article number103009
JournalPhysical Review D
Volume97
Issue number10
DOIs
StatePublished - May 15 2018

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gravitational waves
coalescing
filters
astronomy
electromagnetism
discriminators
preserving
electromagnetic radiation
signal to noise ratios
injection

All Science Journal Classification (ASJC) codes

  • Physics and Astronomy (miscellaneous)

Cite this

Tsukada, Leo ; Cannon, Kipp ; Hanna, Chad ; Keppel, Drew ; Meacher, Duncan ; Messick, Cody. / Application of a zero-latency whitening filter to compact binary coalescence gravitational-wave searches. In: Physical Review D. 2018 ; Vol. 97, No. 10.
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Application of a zero-latency whitening filter to compact binary coalescence gravitational-wave searches. / Tsukada, Leo; Cannon, Kipp; Hanna, Chad; Keppel, Drew; Meacher, Duncan; Messick, Cody.

In: Physical Review D, Vol. 97, No. 10, 103009, 15.05.2018.

Research output: Contribution to journalArticle

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