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Search for gravitational waves associated with gamma-ray bursts detected by the InterPlanetary Network

We present the results of a search for gravitational waves associated with 223 gamma-ray bursts (GRBs) detected by the InterPlanetary Network (IPN) in 2005-2010 during LIGO's fifth and sixth science runs and Virgo's first, second and third science runs. The IPN satellites provide accurate times of t... Full description

Journal Title: arXiv.org Apr 17, 2014
Main Author: Aasi, J
Other Authors: Abbott, B , Abbott, R , Abbott, T , Abernathy, M , Acernese, F , Ackley, K , Adams, C , Adams, T , Addesso, P , Adhikari, R , Affeldt, C , Agathos, M , Aggarwal, N , Aguiar, O , Ajith, P , Alemic, A , Allen, B , Allocca, A , Amariutei
Format: Electronic Article Electronic Article
Language: English
Subjects:
ID: DOI: 10.1103/PhysRevLett.113.011102
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title: Search for gravitational waves associated with gamma-ray bursts detected by the InterPlanetary Network
format: Article
creator:
  • Aasi, J
  • Abbott, B
  • Abbott, R
  • Abbott, T
  • Abernathy, M
  • Acernese, F
  • Ackley, K
  • Adams, C
  • Adams, T
  • Addesso, P
  • Adhikari, R
  • Affeldt, C
  • Agathos, M
  • Aggarwal, N
  • Aguiar, O
  • Ajith, P
  • Alemic, A
  • Allen, B
  • Allocca, A
  • Amariutei
subjects:
  • Gravitational Waves
  • Neutron Stars
  • Gamma Rays
  • Gamma Ray Bursts
  • Lower Bounds
  • Detectors
  • Gravitational Waves
  • Binary Stars
  • Gravitation
  • Gamma Rays
  • Neutron Stars
  • Searching
  • Coalescing
ispartof: arXiv.org, Apr 17, 2014
description: We present the results of a search for gravitational waves associated with 223 gamma-ray bursts (GRBs) detected by the InterPlanetary Network (IPN) in 2005-2010 during LIGO's fifth and sixth science runs and Virgo's first, second and third science runs. The IPN satellites provide accurate times of the bursts and sky localizations that vary significantly from degree scale to hundreds of square degrees. We search for both a well-modeled binary coalescence signal, the favored progenitor model for short GRBs, and for generic, unmodeled gravitational wave bursts. Both searches use the event time and sky localization to improve the gravitational-wave search sensitivity as compared to corresponding all-time, all-sky searches. We find no evidence of a gravitational-wave signal associated with any of the IPN GRBs in the sample, nor do we find evidence for a population of weak gravitational-wave signals associated with the GRBs. For all IPN-detected GRBs, for which a sufficient duration of quality...
language: eng
source:
identifier: DOI: 10.1103/PhysRevLett.113.011102
fulltext: fulltext_linktorsrc
url: Link


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titleSearch for gravitational waves associated with gamma-ray bursts detected by the InterPlanetary Network
creatorAasi, J ; Abbott, B ; Abbott, R ; Abbott, T ; Abernathy, M ; Acernese, F ; Ackley, K ; Adams, C ; Adams, T ; Addesso, P ; Adhikari, R ; Affeldt, C ; Agathos, M ; Aggarwal, N ; Aguiar, O ; Ajith, P ; Alemic, A ; Allen, B ; Allocca, A ; Amariutei
ispartofarXiv.org, Apr 17, 2014
identifierDOI: 10.1103/PhysRevLett.113.011102
subjectGravitational Waves ; Neutron Stars ; Gamma Rays ; Gamma Ray Bursts ; Lower Bounds ; Detectors ; Gravitational Waves ; Binary Stars ; Gravitation ; Gamma Rays ; Neutron Stars ; Searching ; Coalescing
descriptionWe present the results of a search for gravitational waves associated with 223 gamma-ray bursts (GRBs) detected by the InterPlanetary Network (IPN) in 2005-2010 during LIGO's fifth and sixth science runs and Virgo's first, second and third science runs. The IPN satellites provide accurate times of the bursts and sky localizations that vary significantly from degree scale to hundreds of square degrees. We search for both a well-modeled binary coalescence signal, the favored progenitor model for short GRBs, and for generic, unmodeled gravitational wave bursts. Both searches use the event time and sky localization to improve the gravitational-wave search sensitivity as compared to corresponding all-time, all-sky searches. We find no evidence of a gravitational-wave signal associated with any of the IPN GRBs in the sample, nor do we find evidence for a population of weak gravitational-wave signals associated with the GRBs. For all IPN-detected GRBs, for which a sufficient duration of quality...
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titleSearch for gravitational waves associated with gamma-ray bursts detected by the InterPlanetary Network
descriptionWe present the results of a search for gravitational waves associated with 223 gamma-ray bursts (GRBs) detected by the InterPlanetary Network (IPN) in 2005-2010 during LIGO's fifth and sixth science runs and Virgo's first, second and third science runs. The IPN satellites provide accurate times of the bursts and sky localizations that vary significantly from degree scale to hundreds of square degrees. We search for both a well-modeled binary coalescence signal, the favored progenitor model for short GRBs, and for generic, unmodeled gravitational wave bursts. Both searches use the event time and sky localization to improve the gravitational-wave search sensitivity as compared to corresponding all-time, all-sky searches. We find no evidence of a gravitational-wave signal associated with any of the IPN GRBs in the sample, nor do we find evidence for a population of weak gravitational-wave signals associated with the GRBs. For all IPN-detected GRBs, for which a sufficient duration of quality...
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titleSearch for gravitational waves associated with gamma-ray bursts detected by the InterPlanetary Network
authorAasi, J ; Abbott, B ; Abbott, R ; Abbott, T ; Abernathy, M ; Acernese, F ; Ackley, K ; Adams, C ; Adams, T ; Addesso, P ; Adhikari, R ; Affeldt, C ; Agathos, M ; Aggarwal, N ; Aguiar, O ; Ajith, P ; Alemic, A ; Allen, B ; Allocca, A ; Amariutei
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45Barsotti, L
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48Bartos, I
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atitleSearch for gravitational waves associated with gamma-ray bursts detected by the InterPlanetary Network
jtitlearXiv.org
risdate20140417
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abstractWe present the results of a search for gravitational waves associated with 223 gamma-ray bursts (GRBs) detected by the InterPlanetary Network (IPN) in 2005-2010 during LIGO's fifth and sixth science runs and Virgo's first, second and third science runs. The IPN satellites provide accurate times of the bursts and sky localizations that vary significantly from degree scale to hundreds of square degrees. We search for both a well-modeled binary coalescence signal, the favored progenitor model for short GRBs, and for generic, unmodeled gravitational wave bursts. Both searches use the event time and sky localization to improve the gravitational-wave search sensitivity as compared to corresponding all-time, all-sky searches. We find no evidence of a gravitational-wave signal associated with any of the IPN GRBs in the sample, nor do we find evidence for a population of weak gravitational-wave signals associated with the GRBs. For all IPN-detected GRBs, for which a sufficient duration of quality...
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pubCornell University Library, arXiv.org
doi10.1103/PhysRevLett.113.011102
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date2014-04-17