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We present a possible observing scenario for the Advanced LIGO and Advanced Virgo gravitational-wave detectors over the next decade, with the intention of providing information to the astronomy community to facilitate planning for multi-messenger astronomy with gravitational waves. We determine the expected sensitivity of the network to transient gravitational-wave signals, and study the capability of the network to determine the sky location of the source. We report our findings for gravitational-wave transients, with particular focus on gravitational-wave signals from the inspiral of binary neutron-star systems, which are considered the most promising for multi-messenger astronomy. The ability to localize the sources of the detected signals depends on the geographical distribution of the detectors and their relative sensitivity, and 90% credible regions can be as large as thousands of square degrees when only two sensitive detectors are operational. Determining the sky position of a significant fraction of detected signals to areas of 5 deg^2 to 20 deg^2 will require at least three detectors of sensitivity within a factor of ~2 of each other and with a broad frequency bandwidth. Should the third LIGO detector be relocated to India as expected, a significant fraction of gravitational-wave signals will be localized to a few square degrees by gravitational-wave observations alone.
B. P. Abbott, R. Abbott, T. D. Abbott, M. R. Abernathy, F. Acernese, K. Ackley, et al. (2016). Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO and Advanced Virgo. LIVING REVIEWS IN RELATIVITY, 19, 1-39 [10.1007/lrr-2016-1].
Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO and Advanced Virgo
B. P. Abbott;R. Abbott;T. D. Abbott;M. R. Abernathy;F. Acernese;K. Ackley;C. Adams;T. Adams;P. Addesso;R. X. Adhikari;V. B. Adya;C. Affeldt;M. Agathos;K. Agatsuma;N. Aggarwal;O. D. Aguiar;A. Ain;P. Ajith;B. Allen;A. Allocca;P. A. Altin;D. V. Amariutei;S. B. Anderson;W. G. Anderson;K. Arai;M. C. Araya;C. C. Arceneaux;J. S. Areeda;N. Arnaud;K. G. Arun;G. Ashton;M. Ast;S. M. Aston;P. Astone;P. Aufmuth;C. Aulbert;S. Babak;P. T. Baker;F. Baldaccini;G. Ballardin;S. W. Ballmer;J. C. Barayoga;S. E. Barclay;B. C. Barish;D. Barker;F. Barone;B. Barr;L. Barsotti;M. Barsuglia;D. Barta;J. Bartlett;I. Bartos;R. Bassiri;A. Basti;J. C. Batch;C. Baune;V. Bavigadda;M. Bazzan;B. Behnke;M. Bejger;C. Belczynski;A. S. Bell;C. J. Bell;B. K. Berger;J. Bergman;G. Bergmann;C. P. L. Berry;D. Bersanetti;A. Bertolini;J. Betzwieser;S. Bhagwat;R. Bhandare;I. A. Bilenko;G. Billingsley;J. Birch;R. Birney;S. Biscans;A. Bisht;M. Bitossi;C. Biwer;M. A. Bizouard;J. K. Blackburn;C. D. Blair;D. Blair;R. M. Blair;S. 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Zhao;M. Zhou;Z. Zhou;X. J. Zhu;M. E. Zucker;S. E. Zuraw;J. Zweizig
2016
Abstract
We present a possible observing scenario for the Advanced LIGO and Advanced Virgo gravitational-wave detectors over the next decade, with the intention of providing information to the astronomy community to facilitate planning for multi-messenger astronomy with gravitational waves. We determine the expected sensitivity of the network to transient gravitational-wave signals, and study the capability of the network to determine the sky location of the source. We report our findings for gravitational-wave transients, with particular focus on gravitational-wave signals from the inspiral of binary neutron-star systems, which are considered the most promising for multi-messenger astronomy. The ability to localize the sources of the detected signals depends on the geographical distribution of the detectors and their relative sensitivity, and 90% credible regions can be as large as thousands of square degrees when only two sensitive detectors are operational. Determining the sky position of a significant fraction of detected signals to areas of 5 deg^2 to 20 deg^2 will require at least three detectors of sensitivity within a factor of ~2 of each other and with a broad frequency bandwidth. Should the third LIGO detector be relocated to India as expected, a significant fraction of gravitational-wave signals will be localized to a few square degrees by gravitational-wave observations alone.
B. P. Abbott, R. Abbott, T. D. Abbott, M. R. Abernathy, F. Acernese, K. Ackley, et al. (2016). Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO and Advanced Virgo. LIVING REVIEWS IN RELATIVITY, 19, 1-39 [10.1007/lrr-2016-1].
B. P. Abbott; R. Abbott; T. D. Abbott; M. R. Abernathy; F. Acernese; K. Ackley; C. Adams; T. Adams; P. Addesso; R. X. Adhikari; V. B. Adya; C. Affeldt...espandi
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11585/865780
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