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

被引：5

作者：

Abdalla, H. ^{[1
]}

Aharonian, F. ^{[2
,3
,4
]}

Benkhali, F. Ait ^{[3
]}

Anguner, E. O. ^{[5
]}

Ashkar, H. ^{[6
]}

Backes, M. ^{[1
,7
]}

Baghmanyan, V ^{[8
]}

Martins, V. Barbosa ^{[9
]}

Batzofin, R. ^{[10
]}

Becherini, Y. ^{[11
]}

Berge, D. ^{[9
]}

Bernlohr, K. ^{[3
]}

Bi, B. ^{[12
]}

Bottcher, M. ^{[7
]}

Boisson, C. ^{[13
]}

Bolmont, J. ^{[14
]}

de Lavergne, M. de Bony ^{[15
]}

Brose, R. ^{[2
]}

Brun, F. ^{[6
]}

Bulik, T. ^{[16
]}

Bylund, T. ^{[11
]}

Cangemi, F. ^{[14
]}

Caroff, S. ^{[14
]}

Casanova, S. ^{[8
]}

Chand, T. ^{[7
]}

Chen, A. ^{[10
]}

Cotter, G. ^{[17
]}

Mbarubucyeye, J. Damascene ^{[9
]}

Devin, J. ^{[18
]}

Djannati-Atai, A. ^{[19
]}

Egberts, K. ^{[20
]}

Ernenwein, J-P ^{[5
]}

Fegan, S. ^{[21
]}

Fiasson, A. ^{[15
]}

de Clairfontaine, G. Fichet ^{[13
]}

Fontaine, G. ^{[21
]}

Funk, S. ^{[22
]}

Gabici, S. ^{[19
]}

Giavitto, G. ^{[9
]}

Giunti, L. ^{[6
,19
]}

Glawion, D. ^{[22
]}

Glicenstein, J. F. ^{[6
]}

Grondin, M-H ^{[18
]}

Hinton, J. A. ^{[3
]}

Horbe, M. ^{[17
]}

Hofmann, W. ^{[3
]}

Holch, T. L. ^{[9
]}

Holler, M. ^{[23
]}

Huang, Zhiqiu ^{[3
]}

Huber, D. ^{[23
]}

机构：

[1] Univ Namibia, Dept Phys, Private Bag 13301, Windhoek 10005, Namibia

[2] Dublin Inst Adv Studies, 31 Fitzwilliam Pl, Dublin 2, Ireland

[3] Max Planck Inst Kernphys, POB 103980, D-69029 Heidelberg, Germany

[4] RAU, High Energy Astrophys Lab, 123 Hovsep Emin St, Yerevan 0051, Armenia

[5] Aix Marseille Univ, CPPM, CNRS IN2P3, Marseille, France

[6] Univ Paris Saclay, CEA, IRFU, F-91191 Gif Sur Yvette, France

[7] North West Univ, Ctr Space Res, ZA-2520 Potchefstroom, South Africa

[8] Inst Fizyki Jadrowej PAN, Ul Radzikowskiego 152, PL-31342 Krakow, Poland

[9] DESY, D-15738 Zeuthen, Germany

[10] Univ Witwatersrand, Sch Phys, 1 Jan Smuts Ave, ZA-2050 Johannesburg, South Africa

[11] Linnaeus Univ, Dept Phys & Elect Engn, SE-35195 Vaxjo, Sweden

[12] Univ Tubingen, Inst Astron & Astrophys, Sand 1, D-72076 Tubingen, Germany

[13] Univ Paris, Univ PSL, Observ Paris, Lab Univers & Theories,CNRS, F-92190 Meudon, France

[14] Sorbonne Univ, Univ Paris Diderot, Sorbonne Paris Cite, CNRS IN2P3,Lab Phys Nucl & Hautes Energies,LPNHE, 4 Pl Jussieu, F-75252 Paris, France

[15] Univ Savoie Mt Blanc, Lab Annecy Phys Particules, CNRS, IN2P3, F-74000 Annecy, France

[16] Univ Warsaw, Astron Observ, Al Ujazdowskie 4, PL-00478 Warsaw, Poland

[17] Univ Oxford, Dept Phys, Denys Wilkinson Bldg,Keble Rd, Oxford OX1 3RH, England

[18] Univ Bordeaux, Ctr Etud Nucl Bordeaux Gradignan, CNRS IN2P3, F-33175 Gradignan, France

[19] Univ Paris, Astroparticule & Cosmol, CNRS, F-75013 Paris, France

[20] Univ Potsdam, Inst Phys & Astron, Karl Liebknecht Str 24-25, D-14476 Potsdam, Germany

[21] Ecole Polytech, Lab Leprince Ringuet, CNRS, Inst Polytech Paris, F-91128 Palaiseau, France

[22] Friedrich Alexander Univ Erlangen Nurnberg, Erlangen Ctr Astroparticle Phys, Erwin Rommel Str 1, D-91058 Erlangen, Germany

[23] Leopold Franzens Univ Innsbruck, Inst Astro & Teilchenphys, A-6020 Innsbruck, Austria

[24] Uniwersytet Jagiellonski, Obserwatorium Astron, Ul Orla 171, PL-30244 Krakow, Poland

[25] Heidelberg Univ, Landessternwarte, D-69117 Heidelberg, Germany

[26] Nicolaus Copernicus Univ, Fac Phys Astron & Informat, Inst Astron, Grudziadzka 5, PL-87100 Torun, Poland

[27] Humboldt Univ, Inst Phys, Newtonstr 15, D-12489 Berlin, Germany

[28] Univ Free State, Dept Phys, POB 339, ZA-9300 Bloemfontein, South Africa

[29] Univ Leicester, Dept Phys & Astron, Univ Rd, Leicester LE1 7RH, Leics, England

[30] Univ Amsterdam, Anton Pannekoek Inst Astron, GRAPPA, Sci Pk 904, NL-1098 XH Amsterdam, Netherlands

[31] Univ Montpellier, Lab Univers & Particules Montpellier, CNRS IN2P3, CC 72,Pl Eugene Bataillon, F-34095 Montpellier 5, France

[32] Univ Adelaide, Sch Phys Sci, Adelaide, SA 5005, Australia

[33] Polish Acad Sci, Nicolaus Copernicus Astron Ctr, Ul Bartycka 18, PL-00716 Warsaw, Poland

[34] Yerevan Phys Inst, 2 Alikhanian Bros St, Yerevan 375036, Armenia

[35] Univ Tokyo, Univ Tokyo Inst Adv Study UTIAS, Kavli Inst Phys & Math Universe WPI, 5-1-5 Kashiwa No Ha, Kashiwa, Chiba 2778583, Japan

[36] Konan Univ, Dept Phys, Higashinada Ku, 8-9-1 Okamoto, Kobe, Hyogo 6588501, Japan

[37] RIKEN, 2-1 Hirosawa, Wako, Saitama 3510198, Japan

[38] Rikkyo Univ, Dept Phys, Toshima Ku, 3-34-1 Nishi Ikebukuro, Tokyo 1718501, Japan

来源：

ASTROPHYSICAL JOURNAL | 2021年 / 923卷 / 01期

基金：

日本学术振兴会; 新加坡国家研究基金会; 奥地利科学基金会; 澳大利亚研究理事会; 英国科学技术设施理事会;

关键词：

GAMMA-RAY BURSTS; GW170817; DISCS;

D O I：

10.3847/1538-4357/ac2e04

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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 deg(2) 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) gamma-ray emission. The 1-10 TeV isotropic luminosity of these GW events is below 10(45) 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.

引用

页数：15

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