High-energy electromagnetic offline follow-up of LIGO-Virgo gravitational-wave binary coalescence candidate events

Blackburn, L., Briggs, M.S., Camp, J., Christensen, N., Connaughton, V., Jenke, P., Remillard, R.A. and Veitch, J. (2015) High-energy electromagnetic offline follow-up of LIGO-Virgo gravitational-wave binary coalescence candidate events. Astrophysical Journal Supplement Series, 217(1), 8. (doi: 10.1088/0067-0049/217/1/8)

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Abstract

We present two different search methods for electromagnetic counterparts to gravitational-wave (GW) events from ground-based detectors using archival NASA high-energy data from the Fermi Gamma-ray Burst Monitor (GBM) and RXTE All-sky Monitor (ASM) instruments. To demonstrate the methods, we use a limited number of representative GW background noise events produced by a search for binary neutron star coalescence over the last two months of the LIGO-Virgo S6/VSR3 joint science run. Time and sky location provided by the GW data trigger a targeted search in the high-energy photon data. We use two custom pipelines: one to search for prompt gamma-ray counterparts in GBM, and the other to search for a variety of X-ray afterglow model signals in ASM. We measure the efficiency of the joint pipelines to weak gamma-ray burst counterparts, and a family of model X-ray afterglows. By requiring a detectable signal in either electromagnetic instrument coincident with a GW event, we are able to reject a large majority of GW candidates. This reduces the signal-to-noise ratio of the loudest surviving GW background event by around 15–20%.

Item Type:Articles
Status:Published
Refereed:Yes
Glasgow Author(s) Enlighten ID:Veitch, Dr John
Authors: Blackburn, L., Briggs, M.S., Camp, J., Christensen, N., Connaughton, V., Jenke, P., Remillard, R.A., and Veitch, J.
College/School:College of Science and Engineering > School of Physics and Astronomy
Journal Name:Astrophysical Journal Supplement Series
Publisher:American Astronomical Society
ISSN:0067-0049
ISSN (Online):1538-4365
Published Online:05 March 2015

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