H.E.S.S. Follow-up Observations of Binary Black Hole Coalescence Events during the Second and Third Gravitational-wave Observing Runs of Advanced LIGO and Advanced Virgo

Author:

Abdalla H.,Aharonian F.ORCID,Ait Benkhali F.,Angüner E. O.,Ashkar H.ORCID,Backes M.ORCID,Baghmanyan V.,Barbosa Martins V.ORCID,Batzofin R.ORCID,Becherini Y.,Berge D.ORCID,Bernlöhr K.ORCID,Bi B.,Böttcher M.ORCID,Boisson C.ORCID,Bolmont J.,de Bony de Lavergne M.,Brose R.ORCID,Brun F.ORCID,Bulik T.ORCID,Bylund T.ORCID,Cangemi F.,Caroff S.ORCID,Casanova S.ORCID,Chand T.,Chen A.ORCID,Cotter G.ORCID,Damascene Mbarubucyeye J.ORCID,Devin J.,Djannati-Ataï A.,Egberts K.,Ernenwein J.-P.,Fegan S.,Fiasson A.,Fichet de Clairfontaine G.ORCID,Fontaine G.ORCID,Funk S.ORCID,Gabici S.,Giavitto G.ORCID,Giunti L.,Glawion D.ORCID,Glicenstein J. F.ORCID,Grondin M.-H.ORCID,Hinton J. A.,Hörbe M.,Hofmann W.ORCID,Holch T. L.ORCID,Holler M.,Huang ZhiqiuORCID,Huber D.,Jamrozy M.ORCID,Jankowsky F.,Jung-Richardt I.,Kasai E.,Katarzyński K.,Katz U.,Khélifi B.ORCID,Komin Nu.ORCID,Konno R.ORCID,Kosack K.ORCID,Kostunin D.ORCID,Kundu A.ORCID,Lamanna G.,Le Stum S.,Lemière A.,Lemoine-Goumard M.ORCID,Lenain J.-P.ORCID,Leuschner F.ORCID,Lohse T.,Luashvili A.ORCID,Lypova I.,Mackey J.ORCID,Majumdar J.,Malyshev D.ORCID,Marandon V.ORCID,Marchegiani P.ORCID,Martí-Devesa G.ORCID,Marx R.ORCID,Maurin G.,Meintjes P. J.,Mitchell A.ORCID,Mohrmann L.ORCID,Montanari A.ORCID,Moulin E.ORCID,Muller J.ORCID,Murach T.ORCID,de Naurois M.,Nayerhoda A.,Niemiec J.ORCID,Priyana Noel A.,O’Brien P.,Ohm S.ORCID,Olivera-Nieto L.ORCID,de Ona Wilhelmi E.,Ostrowski M.ORCID,Panter M.,Parsons R. D.ORCID,Peron G.,Poireau V.ORCID,Prokhorov D. A.,Prokoph H.,Pühlhofer G.,Punch M.ORCID,Quirrenbach A.,Reichherzer P.ORCID,Renaud M.ORCID,Rieger F.ORCID,Rowell G.ORCID,Rudak B.ORCID,Rueda Ricarte H.ORCID,Ruiz-Velasco E.ORCID,Sahakian V.,Sailer S.,Salzmann H.,Sanchez D. A.,Santangelo A.ORCID,Sasaki M.ORCID,Schüssler F.ORCID,Schutte H. M.ORCID,Schwanke U.ORCID,Senniappan M.ORCID,Shapopi J. N. S.ORCID,Sinha A.ORCID,Sol H.,Specovius A.,Spencer S.ORCID,Stawarz Ł.,Steinmassl S.ORCID,Steppa C.,Sun L.,Takahashi T.,Tanaka T.ORCID,Terrier R.ORCID,Thorpe-Morgan C.,Tsirou M.,Tsuji N.ORCID,Uchiyama Y.,van Eldik C.ORCID,Veh J.ORCID,Vink J.ORCID,Wagner S. J.ORCID,Werner F.,White R.,Wierzcholska A.ORCID,Wong Yu Wun,Zacharias M.ORCID,Zargaryan D.ORCID,Zdziarski A. A.ORCID,Zech A.,Zhu S. J.ORCID,Zouari S.ORCID,Żywucka N.

Abstract

Abstract We report on the observations of four well-localized binary black hole (BBH) mergers by the High Energy Stereoscopic System (H.E.S.S.) during the second and third observing runs of Advanced LIGO and Advanced Virgo, O2 and O3. H.E.S.S. can observe 20 deg2 of the sky at a time and follows up gravitational-wave (GW) events by “tiling” localization regions to maximize the covered localization probability. During O2 and O3, H.E.S.S. observed large portions of the localization regions, between 35% and 75%, for four BBH mergers (GW170814, GW190512_180714, GW190728_064510, and S200224ca). For these four GW events, we find no significant signal from a pointlike source in any of the observations, and we set upper limits on the very high energy (>100 GeV) γ-ray emission. The 1–10 TeV isotropic luminosity of these GW events is below 1045 erg s−1 at the times of the H.E.S.S. observations, around the level of the low-luminosity GRB 190829A. Assuming no changes are made to how follow-up observations are conducted, H.E.S.S. can expect to observe over 60 GW events per year in the fourth GW observing run, O4, of which eight would be observable with minimal latency.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 8 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Cross Observatory Coordination with tilepy: A Novel Tool for Observations of Multimessenger Transient Events;The Astrophysical Journal Supplement Series;2024-08-12

2. H.E.S.S.: The High Energy Stereoscopic System;Handbook of X-ray and Gamma-ray Astrophysics;2024

3. H.E.S.S.: The High Energy Stereoscopic System;Handbook of X-ray and Gamma-ray Astrophysics;2023-12-13

4. GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo during the Second Part of the Third Observing Run;Physical Review X;2023-12-04

5. H.E.S.S.: The High Energy Stereoscopic System;Handbook of X-ray and Gamma-ray Astrophysics;2023-09-30

同舟云学术

1.学者识别学者识别

2.学术分析学术分析

3.人才评估人才评估

"同舟云学术"是以全球学者为主线,采集、加工和组织学术论文而形成的新型学术文献查询和分析系统,可以对全球学者进行文献检索和人才价值评估。用户可以通过关注某些学科领域的顶尖人物而持续追踪该领域的学科进展和研究前沿。经过近期的数据扩容,当前同舟云学术共收录了国内外主流学术期刊6万余种,收集的期刊论文及会议论文总量共计约1.5亿篇,并以每天添加12000余篇中外论文的速度递增。我们也可以为用户提供个性化、定制化的学者数据。欢迎来电咨询!咨询电话:010-8811{复制后删除}0370

www.globalauthorid.com

TOP

Copyright © 2019-2024 北京同舟云网络信息技术有限公司
京公网安备11010802033243号  京ICP备18003416号-3