Observational Implications of Lowering the LIGO-Virgo Alert Threshold
The recent detection of the binary-neutron-star merger associated with GW170817 by both the Laser Interferometer Gravitational-Wave Observatory (LIGO) and Virgo and the network of electromagnetic-spectrum observing facilities around the world has made the multi-messenger detection of gravitational-w...
| Main Authors: | , , , , , |
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| Format: | Article |
| Language: | English |
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American Astronomical Society
2019
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| Online Access: | https://hdl.handle.net/1721.1/122798 |
| _version_ | 1811092178008539136 |
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| author | Lynch, Ryan Christopher Coughlin, Michael Vitale, Salvatore Stubbs, Christopher W. Katsavounidis, Erik Katsavounidis, Erotokritos |
| author2 | Massachusetts Institute of Technology. Department of Physics |
| author_facet | Massachusetts Institute of Technology. Department of Physics Lynch, Ryan Christopher Coughlin, Michael Vitale, Salvatore Stubbs, Christopher W. Katsavounidis, Erik Katsavounidis, Erotokritos |
| author_sort | Lynch, Ryan Christopher |
| collection | MIT |
| description | The recent detection of the binary-neutron-star merger associated with GW170817 by both the Laser Interferometer Gravitational-Wave Observatory (LIGO) and Virgo and the network of electromagnetic-spectrum observing facilities around the world has made the multi-messenger detection of gravitational-wave (GW) events a reality. These joint detections allow us to probe GW sources in greater detail and provide us with the possibility of confidently establishing events that would not have been detected in GW data alone. In this Letter, we explore the prospects of using the electromagnetic (EM) follow-up of low-significance GW event candidates to increase the sample of confident detections with EM counterparts. We find that the GW-alert threshold change that would roughly double the number of detectable astrophysical events would increase the false-alarm rate (FAR) by more than five orders of magnitude from 1 per 100 years to more than 1000 per year. We find that the localization costs of following up low-significance candidates are marginal, as the same changes to FAR only increase distance/area localizations by less than a factor of 2 and increase volume localization by less than a factor of 4. We argue that EM follow-up thresholds for low-significance candidates should be set on the basis of alert purity (P astro) and not FAR. Ideally, such estimates of P astro would be provided by LIGO-Virgo, but in their absence we provide estimates of the average purity of the GW candidate alerts issued by LIGO-Virgo as a function of FAR for various LIGO-Virgo observing epochs. Keywords: gravitional waves |
| first_indexed | 2024-09-23T15:14:13Z |
| format | Article |
| id | mit-1721.1/122798 |
| institution | Massachusetts Institute of Technology |
| language | English |
| last_indexed | 2024-09-23T15:14:13Z |
| publishDate | 2019 |
| publisher | American Astronomical Society |
| record_format | dspace |
| spelling | mit-1721.1/1227982022-09-29T13:35:00Z Observational Implications of Lowering the LIGO-Virgo Alert Threshold Lynch, Ryan Christopher Coughlin, Michael Vitale, Salvatore Stubbs, Christopher W. Katsavounidis, Erik Katsavounidis, Erotokritos Massachusetts Institute of Technology. Department of Physics MIT Kavli Institute for Astrophysics and Space Research The recent detection of the binary-neutron-star merger associated with GW170817 by both the Laser Interferometer Gravitational-Wave Observatory (LIGO) and Virgo and the network of electromagnetic-spectrum observing facilities around the world has made the multi-messenger detection of gravitational-wave (GW) events a reality. These joint detections allow us to probe GW sources in greater detail and provide us with the possibility of confidently establishing events that would not have been detected in GW data alone. In this Letter, we explore the prospects of using the electromagnetic (EM) follow-up of low-significance GW event candidates to increase the sample of confident detections with EM counterparts. We find that the GW-alert threshold change that would roughly double the number of detectable astrophysical events would increase the false-alarm rate (FAR) by more than five orders of magnitude from 1 per 100 years to more than 1000 per year. We find that the localization costs of following up low-significance candidates are marginal, as the same changes to FAR only increase distance/area localizations by less than a factor of 2 and increase volume localization by less than a factor of 4. We argue that EM follow-up thresholds for low-significance candidates should be set on the basis of alert purity (P astro) and not FAR. Ideally, such estimates of P astro would be provided by LIGO-Virgo, but in their absence we provide estimates of the average purity of the GW candidate alerts issued by LIGO-Virgo as a function of FAR for various LIGO-Virgo observing epochs. Keywords: gravitional waves 2019-11-07T21:23:54Z 2019-11-07T21:23:54Z 2018-07 2018-06 2019-04-26T19:15:45Z Article http://purl.org/eprint/type/JournalArticle 2041-8213 https://hdl.handle.net/1721.1/122798 Lynch, Ryan et al. "Observational Implications of Lowering the LIGO-Virgo Alert Threshold." Astrophysical Journal Letters 821, 2 (July 2018): L24 © 2018 The American Astronomical Society en http://dx.doi.org/10.3847/2041-8213/aacf9f Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. application/pdf American Astronomical Society The Astrophysical Journal Letters |
| spellingShingle | Lynch, Ryan Christopher Coughlin, Michael Vitale, Salvatore Stubbs, Christopher W. Katsavounidis, Erik Katsavounidis, Erotokritos Observational Implications of Lowering the LIGO-Virgo Alert Threshold |
| title | Observational Implications of Lowering the LIGO-Virgo Alert Threshold |
| title_full | Observational Implications of Lowering the LIGO-Virgo Alert Threshold |
| title_fullStr | Observational Implications of Lowering the LIGO-Virgo Alert Threshold |
| title_full_unstemmed | Observational Implications of Lowering the LIGO-Virgo Alert Threshold |
| title_short | Observational Implications of Lowering the LIGO-Virgo Alert Threshold |
| title_sort | observational implications of lowering the ligo virgo alert threshold |
| url | https://hdl.handle.net/1721.1/122798 |
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