Published August 1, 2024 | Version Published
Journal Article Open

Observation of Gravitational Waves from the Coalescence of a 2.5–4.5 M⊙ Compact Object and a Neutron Star

Creators

  • 1. ROR icon Max Planck Institute for Gravitational Physics
  • 2. ROR icon California Institute of Technology
  • 3. ROR icon Laser Interferometer Gravitational Wave Observatory
  • 4. ROR icon University of Salerno
  • 5. ROR icon INFN Sezione di Napoli
  • 6. ROR icon University of Warwick
  • 7. ROR icon Pennsylvania State University
  • 8. ROR icon University of Wisconsin–Milwaukee
  • 9. ROR icon Louisiana State University
  • 10. ROR icon Université Catholique de Louvain
  • 11. ROR icon Inter-University Centre for Astronomy and Astrophysics
  • 12. ROR icon Queen Mary University of London
  • 13. ROR icon Sejong University
  • 14. ROR icon National Institute for Space Research
  • 15. ROR icon Stanford University
  • 16. ROR icon University of Rome Tor Vergata
  • 17. ROR icon INFN Sezione di Roma II
  • 18. ROR icon Cardiff University
  • 19. ROR icon University of Antwerp
  • 20. ROR icon International Centre for Theoretical Sciences
  • 21. ROR icon University College Dublin
  • 22. ROR icon National Astronomical Observatory of Japan
  • 23. ROR icon INFN Sezione di Torino
  • 24. ROR icon Friedrich Schiller University Jena
  • 25. ROR icon University of Turin
  • 26. ROR icon University of Glasgow
  • 27. ROR icon University of Western Australia
  • 28. ROR icon Université Savoie Mont Blanc
  • 29. ROR icon University of Naples Federico II
  • 30. ROR icon Australian National University
  • 31. ROR icon Massachusetts Institute of Technology
  • 32. ROR icon Maastricht University
  • 33. ROR icon National Institute for Subatomic Physics
  • 34. ROR icon Université Libre de Bruxelles
  • 35. ROR icon Institut Fresnel
  • 36. ROR icon Laboratoire de Physique des 2 Infinis Irène Joliot-Curie
  • 37. ROR icon University of Tokyo
  • 38. ROR icon University of Barcelona
  • 39. ROR icon Institute for High Energy Physics
  • 40. ROR icon Leibniz University Hannover
  • 41. ROR icon Gran Sasso Science Institute
  • 42. ROR icon University of Florida
  • 43. ROR icon University of Udine
  • 44. ROR icon INFN Sezione di Trieste
  • 45. ROR icon Monterrey Institute of Technology and Higher Education
  • 46. ROR icon Observatoire de la Côte d'Azur
  • 47. ROR icon INFN Sezione di Perugia
  • 48. ROR icon University of Camerino
  • 49. ROR icon University of Washington
  • 50. ROR icon California State University, Fullerton
  • 51. ROR icon Villanova University
  • 52. ROR icon INFN Sezione di Genova
  • 53. ROR icon University of Genoa
  • 54. ROR icon European Gravitational Observatory
  • 55. ROR icon Georgia Institute of Technology
  • 56. ROR icon Chennai Mathematical Institute
  • 57. ROR icon Royal Holloway University of London
  • 58. ROR icon The Graduate University for Advanced Studies, SOKENDAI
  • 59. ROR icon University of Urbino
  • 60. ROR icon INFN Sezione di Firenze
  • 61. ROR icon INFN Sezione di Roma I
  • 62. ROR icon Sapienza University of Rome
  • 63. ROR icon University of Strasbourg
  • 64. ROR icon Embry–Riddle Aeronautical University
  • 65. ROR icon Bar-Ilan University
  • 66. ROR icon Astroparticle and Cosmology Laboratory
  • 67. ROR icon King's College London
  • 68. ROR icon Korea Institute of Science & Technology Information
  • 69. ROR icon Kenyon College
  • 70. ROR icon Osaka University
  • 71. ROR icon Utrecht University
  • 72. ROR icon University of Oregon
  • 73. ROR icon Syracuse University
  • 74. ROR icon Northwestern University
  • 75. ROR icon Wigner Research Centre for Physics
  • 76. ROR icon Concordia University Wisconsin
  • 77. ROR icon Universität Hamburg
  • 78. ROR icon University of Pisa
  • 79. ROR icon INFN Sezione di Pisa
  • 80. ROR icon University of Perugia
  • 81. ROR icon University of Michigan–Ann Arbor
  • 82. ROR icon University of Padua
  • 83. ROR icon INFN Sezione di Padova
  • 84. ROR icon Institute for Plasma Research
  • 85. ROR icon Ghent University
  • 86. ROR icon Polish Academy of Sciences
  • 87. ROR icon University of Sannio
  • 88. ROR icon University of Minnesota
  • 89. ROR icon Claude Bernard University Lyon 1
  • 90. ROR icon University of Strathclyde
  • 91. ROR icon University of the Balearic Islands
  • 92. ROR icon Autonomous University of Barcelona
  • 93. ROR icon Raja Ramanna Centre for Advanced Technology
  • 94. ROR icon University of Amsterdam
  • 95. ROR icon Missouri University of Science and Technology
  • 96. ROR icon Colorado State University
  • 97. ROR icon VU Amsterdam
  • 98. ROR icon Lomonosov Moscow State University
  • 99. ROR icon KU Leuven
  • 100. ROR icon University of Trento
  • 101. ROR icon Trento Institute for Fundamental Physics and Applications
  • 102. ROR icon University of Adelaide
  • 103. ROR icon French National Centre for Scientific Research
  • 104. ROR icon University of Rennes 1
  • 105. ROR icon University of Birmingham
  • 106. ROR icon Washington State University
  • 107. ROR icon University of Liège
  • 108. ROR icon Institute for Theoretical Physics
  • 109. ROR icon Gran Sasso National Laboratory
  • 110. ROR icon Kastler-Brossel Laboratory
  • 111. ROR icon Christopher Newport University
  • 112. ROR icon University of Warsaw
  • 113. ROR icon University of Maryland, College Park
  • 114. ROR icon University of Milano-Bicocca
  • 115. ROR icon INFN Sezione di Milano Bicocca
  • 116. ROR icon Paul Sabatier University
  • 117. ROR icon University of Portsmouth
  • 118. ROR icon Institut Lumière Matière
  • 119. ROR icon University of Santiago de Compostela
  • 120. ROR icon University of Chicago
  • 121. ROR icon Goddard Space Flight Center
  • 122. ROR icon Texas A&M University
  • 123. ROR icon University of Melbourne
  • 124. ROR icon Laboratori Nazionali del Sud
  • 125. ROR icon University of Copenhagen
  • 126. ROR icon Institute for Space Astrophysics and Planetology
  • 127. ROR icon University of Massachusetts Dartmouth
  • 128. ROR icon University of Valencia
  • 129. ROR icon University of British Columbia
  • 130. ROR icon National Cheng Kung University
  • 131. ROR icon National Tsing Hua University
  • 132. ROR icon National Central University
  • 133. ROR icon Charles Sturt University
  • 134. ROR icon Vanderbilt University
  • 135. ROR icon National Chiao Tung University
  • 136. ROR icon The University of Texas at Austin
  • 137. ROR icon Cornell University
  • 138. ROR icon Northeastern University
  • 139. ROR icon Monash University
  • 140. ROR icon Osservatorio Astronomico di Padova
  • 141. ROR icon ARC Centre of Excellence for Gravitational Wave Discovery
  • 142. ROR icon Brera Astronomical Observatory
  • 143. ROR icon Montana State University
  • 144. ROR icon Texas Tech University
  • 145. ROR icon Columbia University
  • 146. ROR icon University of Rhode Island
  • 147. ROR icon The University of Texas Rio Grande Valley
  • 148. ROR icon University of Sassari
  • 149. ROR icon Laboratoire de Physique Corpusculaire de Caen
  • 150. ROR icon University of Parma
  • 151. INFN, Sezione di Milano Bicocca, Gruppo Collegato di Parma, I-43124 Parma, Italy
  • 152. ROR icon Perimeter Institute
  • 153. ROR icon Mines ParisTech
  • 154. ROR icon Indian Institute of Technology Madras
  • 155. Graduate School of Science, Tokyo Institute of Technology, 2-12-1 Ookayama, Meguro-ku, Tokyo 152-8551, Japan
  • 156. ROR icon National Centre for Nuclear Research
  • 157. ROR icon Institut d'Astrophysique de Paris
  • 158. ROR icon Sorbonne University
  • 159. ROR icon Vrije Universiteit Brussel
  • 160. ROR icon Carleton College
  • 161. ROR icon University of Toyama
  • 162. ROR icon Canadian Institute for Theoretical Astrophysics
  • 163. ROR icon University of Cambridge
  • 164. ROR icon Stony Brook University
  • 165. Center for Computational Astrophysics, Flatiron Institute, New York, NY 10010, USA
  • 166. ROR icon Montclair State University
  • 167. ROR icon University of Trieste
  • 168. ROR icon Institute for Nuclear Research
  • 169. ROR icon Center for Particle Physics of Marseilles
  • 170. ROR icon Superconducting and other Innovative Materials and Devices Institute
  • 171. ROR icon University of Basilicata
  • 172. ROR icon Western Washington University
  • 173. ROR icon University of the West of Scotland
  • 174. ROR icon University of Utah
  • 175. ROR icon Eötvös Loránd University
  • 176. ROR icon University of Minho
  • 177. Department of Physics, Graduate School of Science, Osaka Metropolitan University, 3-3-138 Sugimoto-cho, Sumiyoshi-ku, Osaka City, Osaka 558-8585, Japan
  • 178. ROR icon Rochester Institute of Technology
  • 179. ROR icon California State University, Long Beach
  • 180. ROR icon University of Zurich
  • 181. ROR icon University of Szeged
  • 182. ROR icon Indian Institute of Technology Bombay
  • 183. ROR icon Wuhan University
  • 184. ROR icon University of California, Riverside
  • 185. ROR icon Astronomical Observatory of Capodimonte
  • 186. ROR icon University of Nottingham
  • 187. ROR icon Ariel University
  • 188. ROR icon University of Mississippi
  • 189. ROR icon Academia Sinica
  • 190. ROR icon Shanghai Astronomical Observatory
  • 191. ROR icon Chinese University of Hong Kong
  • 192. ROR icon Marquette University
  • 193. ROR icon American University
  • 194. University of Nevada, Las Vegas, Las Vegas, NV 89154, USA
  • 195. ROR icon Fukuoka University
  • 196. ROR icon University of California, Berkeley
  • 197. ROR icon Lancaster University
  • 198. ROR icon Nihon University
  • 199. ROR icon Niigata University
  • 200. ROR icon Tamkang University
  • 201. ROR icon Rutherford Appleton Laboratory
  • 202. ROR icon Chungnam National University
  • 203. ROR icon Scuola Normale Superiore di Pisa
  • 204. ROR icon Peking University
  • 205. ROR icon Aoyama Gakuin University
  • 206. Nambu Yoichiro Institute of Theoretical and Experimental Physics (NITEP), Osaka Metropolitan University, 3-3-138 Sugimoto-cho, Sumiyoshi-ku, Osaka City, Osaka 558-8585, Japan
  • 207. ROR icon Department of Atomic Energy
  • 208. ROR icon University of Białystok
  • 209. ROR icon Jagiellonian University
  • 210. ROR icon University of Southampton
  • 211. ROR icon Ulsan National Institute of Science and Technology
  • 212. ROR icon Chung-Ang University
  • 213. University of Washington Bothell, Bothell, WA 98011, USA
  • 214. ROR icon Aix-Marseille University
  • 215. ROR icon University of Ouagadougou
  • 216. ROR icon Ewha Womans University
  • 217. ROR icon Seoul National University
  • 218. ROR icon Korea Astronomy and Space Science Institute
  • 219. ROR icon Sungkyunkwan University
  • 220. ROR icon High Energy Accelerator Research Organization
  • 221. ROR icon Bard College
  • 222. ROR icon Institute of Mathematics
  • 223. ROR icon Nagoya University
  • 224. ROR icon University of Montreal
  • 225. ROR icon Indian Institute of Science Education and Research Kolkata
  • 226. ROR icon Inje University
  • 227. ROR icon University of Florence
  • 228. ROR icon National Center for High-Performance Computing
  • 229. ROR icon Marshall Space Flight Center
  • 230. ROR icon West Virginia University
  • 231. ROR icon Heidelberg University
  • 232. ROR icon Tongji University
  • 233. ROR icon Institut d'Estudis Espacials de Catalunya
  • 234. ROR icon Institució Catalana de Recerca i Estudis Avançats
  • 235. ROR icon Tsinghua University
  • 236. ROR icon University of Cagliari
  • 237. ROR icon Saha Institute of Nuclear Physics
  • 238. ROR icon Tata Institute of Fundamental Research
  • 239. ROR icon Hobart and William Smith Colleges
  • 240. ROR icon Institut des Hautes Études Scientifiques
  • 241. ROR icon Ryukoku University
  • 242. ROR icon University of Notre Dame
  • 243. ROR icon University of Stavanger
  • 244. ROR icon Hiroshima University
  • 245. ROR icon Laboratory Universe and Theories
  • 246. ROR icon Paris Observatory
  • 247. ROR icon PSL Research University
  • 248. ROR icon University of Paris
  • 249. ROR icon National Institute for Mathematical Sciences
  • 250. ROR icon The Open University of Japan
  • 251. ROR icon Central Glass and Ceramic Research Institute
  • 252. ROR icon National Research Council
  • 253. ROR icon Aristotle University of Thessaloniki
  • 254. ROR icon Yonsei University
  • 255. ROR icon Enrico Fermi Center for Study and Research
  • 256. ROR icon Roma Tre University
  • 257. ROR icon Laboratoire de Physique Subatomique et des Technologies Associées
  • 258. ROR icon University of Antioquia
  • 259. ROR icon Technical University of Madrid
  • 260. ROR icon National Institute of Technology
  • 261. ROR icon University of Ferrara
  • 262. ROR icon Toho University
  • 263. ROR icon Indian Institute of Technology Gandhinagar
  • 264. Laboratoire MSME, Cité Descartes, 5 Boulevard Descartes, Champs-sur-Marne, 77454 Marne-la-Vallée Cedex 2, France
  • 265. ROR icon University of Tsukuba
  • 266. ROR icon Chapman University
  • 267. ROR icon Osaka Institute of Technology
  • 268. ROR icon Arcetri Astrophysical Observatory
  • 269. ROR icon RIKEN
  • 270. ROR icon International School for Advanced Studies
  • 271. ROR icon Goethe University Frankfurt
  • 272. INAF, Osservatorio di Astrofisica e Scienza dello Spazio, I-40129 Bologna, Italy
  • 273. ROR icon São Paulo State University
  • 274. ROR icon Tokyo City University
  • 275. ROR icon Kyoto University
  • 276. ROR icon University of Catania
  • 277. ROR icon National Defense Academy of Japan
  • 278. ROR icon Eindhoven University of Technology
  • 279. Deceased, 2024 February.
  • 280. ROR icon Beijing Normal University

Abstract

We report the observation of a coalescing compact binary with component masses 2.5–4.5 M and 1.2–2.0 M (all measurements quoted at the 90% credible level). The gravitational-wave signal GW230529_181500 was observed during the fourth observing run of the LIGO–Virgo–KAGRA detector network on 2023 May 29 by the LIGO Livingston observatory. The primary component of the source has a mass less than 5 M at 99% credibility. We cannot definitively determine from gravitational-wave data alone whether either component of the source is a neutron star or a black hole. However, given existing estimates of the maximum neutron star mass, we find the most probable interpretation of the source to be the coalescence of a neutron star with a black hole that has a mass between the most massive neutron stars and the least massive black holes observed in the Galaxy. We provisionally estimate a merger rate density of 55^(+127)_(-47) Gpc³ yr ¹ for compact binary coalescences with properties similar to the source of GW230529_181500; assuming that the source is a neutron star–black hole merger, GW230529_181500-like sources may make up the majority of neutron star–black hole coalescences. The discovery of this system implies an increase in the expected rate of neutron star–black hole mergers with electromagnetic counterparts and provides further evidence for compact objects existing within the purported lower mass gap.

Copyright and License

© 2024. The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.

Acknowledgement

This material is based on work supported by NSF's LIGO Laboratory, which is a major facility fully funded by the National Science Foundation. The authors also gratefully acknowledge the support of the Science and Technology Facilities Council (STFC) of the United Kingdom, the Max-Planck-Society (MPS), and the State of Niedersachsen/Germany for support of the construction of Advanced LIGO and construction and operation of the GEO 600 detector. Additional support for Advanced LIGO was provided by the Australian Research Council. The authors gratefully acknowledge the Italian Istituto Nazionale di Fisica Nucleare (INFN), the French Centre National de la Recherche Scientifique (CNRS), and the Netherlands Organization for Scientific Research (NWO) for the construction and operation of the Virgo detector and the creation and support of the EGO consortium. The authors also gratefully acknowledge research support from these agencies, as well as by the Council of Scientific and Industrial Research of India, the Department of Science and Technology, India, the Science & Engineering Research Board (SERB), India, the Ministry of Human Resource Development, India, the Spanish Agencia Estatal de Investigación (AEI), the Spanish Ministerio de Ciencia, Innovación y Universidades, the European Union NextGenerationEU/PRTR (PRTR-C17.I1), the ICSC - CentroNazionale di Ricerca in High Performance Computing, Big Dataand Quantum Computing, funded by the European Union NextGenerationEU, the Comunitat Autonòma de les Illes Balears through the Direcció General de Recerca, Innovació i Transformació Digital with funds from the Tourist Stay Tax Law ITS 2017-006, the Conselleria d’Economia, Hisenda i Innovació the FEDER Operational Program 2021–2027 of the Balearic Islands, the Conselleria d’Innovació Universitats, Ciència i Societat Digital de la Generalitat Valenciana and the CERCA Programme Generalitat de Catalunya, Spain, the National Science Centre of Poland and the European Union—European Regional Development Fund; Foundation for Polish Science (FNP), the Polish Ministry of Science and Higher Education, the Swiss National Science Foundation (SNSF), the Russian Science Foundation, the European Commission, the European Social Funds (ESF), the European Regional Development Funds (ERDF), the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, the Hungarian Scientific Research Fund (OTKA), the French Lyon Institute of Origins (LIO), the Belgian Fonds de la Recherche Scientifique (FRS-FNRS), Actions de Recherche Concertées (ARC) and Fonds Wetenschappelijk Onderzoek—Vlaanderen (FWO), Belgium, the Paris Île-de-France Region, the National Research, Development and Innovation Office Hungary (NKFIH), the National Research Foundation of Korea, the Natural Science and Engineering Research Council Canada, Canadian Foundation for Innovation (CFI), the Brazilian Ministry of Science, Technology, and Innovations, the International Center for Theoretical Physics South American Institute for Fundamental Research (ICTP-SAIFR), the Research Grants Council of Hong Kong, the National Natural Science Foundation of China (NSFC), the Leverhulme Trust, the Research Corporation, the National Science and Technology Council (NSTC), Taiwan, the United States Department of Energy, and the Kavli Foundation. The authors gratefully acknowledge the support of the NSF, STFC, INFN, and CNRS for provision of computational resources. This work was supported by MEXT, JSPS Leading-edge Research Infrastructure Program, JSPS Grant-in-Aid for Specially Promoted Research 26000005, JSPS Grant-in-Aid for Scientific Research on Innovative Areas 2905: JP17H06358, JP17H06361 and JP17H06364, JSPS Core-to-Core Program A. Advanced Research Networks, JSPS Grant-in-Aid for Scientific Research (S) 17H06133 and 20H05639, JSPS Grant-in-Aid for Transformative Research Areas (A) 20A203: JP20H05854, the joint research program of the Institute for Cosmic Ray Research, University of Tokyo, National Research Foundation (NRF), Computing Infrastructure Project of Global Science experimental Data hub Center (GSDC) at KISTI, Korea Astronomy and Space Science Institute (KASI), and Ministry of Science and ICT (MSIT) in Korea, Academia Sinica (AS), AS Grid Center (ASGC) and the National Science and Technology Council (NSTC) in Taiwan under grants including the Rising Star Program and Science Vanguard Research Program, Advanced Technology Center (ATC) of NAOJ, and Mechanical Engineering Center of KEK. We thank the anonymous journal referee for helpful comments.

Software References

Calibration of the LIGO strain data was performed with a GstLAL-based calibration software pipeline (Viets et al. 2018). Data-quality products and event-validation results were computed using the DMT (Zweizig 2006), DQR (LIGO Scientific Collaboration & Virgo Collaboration 2018), DQSEGDB (Fisher et al. 2021), gwdetchar (Urban et al. 2021), hveto (Smith et al. 2011), iDQ (Essick et al. 2020a), Omicron (Robinet et al. 2020), and PythonVirgoTools (Virgo Collaboration 2021) software packages and contributing software tools. Analyses in this catalog relied on software from the LVK Algorithm Library Suite (LIGO Scientific, Virgo, & KAGRA Collaboration 2018). The detection of the signals and subsequent significance evaluations were performed with the GstLAL-based inspiral software pipeline (Messick et al. 2017; Sachdev et al. 2019; Hanna et al. 2020; Cannon et al. 2021), with the MBTA pipeline (Adams et al. 2016; Aubin et al. 2021), and with the PyCBC (Usman et al. 2016; Nitz et al. 2017; Davies et al. 2020) packages. Estimates of the noise spectra and glitch models were obtained using BayesWave (Cornish & Littenberg 2015; Littenberg et al. 2016; Cornish et al. 2021). Low-latency source localization was performed using BAYESTAR (Singer & Price 2016). Source-parameter estimation was primarily performed with the Bilby and Parallel Bilby libraries (Ashton et al. 2019; Romero-Shaw et al. 2020; Smith et al. 2020) using the Dynesty nested sampling package (Speagle 2020). SEOBNRv5PHM waveforms used in parameter estimation were generated using pySEOBNR (Mihaylov et al. 2023). FTI and TIGER waveforms used for testing general relativity were generated using Bilby TGR (Ashton et al. 2024). PESummary was used to post-process and collate parameter estimation results (Hoy & Raymond 2021). The various stages of the parameter estimation analysis were managed with the Asimov library (Williams et al. 2023). Plots were prepared with Matplotlib (Hunter 2007), seaborn (Waskom 2021) and GWpy (Macleod et al. 2021). NumPy (Harris et al. 2020) and SciPy (Virtanen et al. 2020) were used for analyses in the manuscript.

Files

Abac_2024_ApJL_970_L34.pdf

Files (4.8 MB)

Name Size Download all
md5:8592bb6693cfa3a8aaa0382c1c8ac0f1
4.8 MB Preview Download

Additional details

Related works

Is new version of
Discussion Paper: arXiv:2404.04248 (arXiv)
Is supplemented by
Dataset: 10.7935/6k89-7q62 (DOI)

Dates

Accepted
2024-06-25
Available
2024-07-26
Published online

Caltech Custom Metadata

Caltech groups
Astronomy Department, LIGO, TAPIR, Walter Burke Institute for Theoretical Physics, Division of Physics, Mathematics and Astronomy (PMA)
Publication Status
Published