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First M87 Event Horizon Telescope Results. IV. Imaging the Central Supermassive Black Hole

The Astrophysical Journal Letters · 2019 · Vol. 875(1) · pp. L4–L4
Kazunori AkiyamaA. AlberdiW. AlefKeiichi AsadaRebecca AzulayAnne-Kathrin BaczkoDavid BallMislav BalokovićJohn BarrettDan BintleyLindy BlackburnW. BolandKatherine L. BoumanGeoffrey C. BowerMichael BremerChristiaan D. BrinkerinkRoger BrissendenS. BritzenAvery E. BroderickDominique BroguièreThomas BronzwaerDo‐Young ByunJ. E. CarlstromAndrew ChaelChi‐kwan ChanShami ChatterjeeKoushik ChatterjeeMing‐Tang ChenXiaopeng ChengIlje ChoPierre ChristianJ. E. ConwayJ. M. CordesG. CrewYuzhu CuiJordy DavelaarMariafelicia De LaurentisRoger DeaneJessica DempseyG. DesvignesJason DexterSheperd S. DoelemanRalph P. EatoughH. FalckeVincent L. FishEd FomalontRaquel Fraga-EncinasWilliam T. FreemanPer FribergChristian M. FrommJosé L. GómezPeter GalisonCharles F. GammieRoberto GarcíaOlivier GentazBoris GeorgievC. GoddiRoman GoldMinfeng GuMark GurwellKazuhiro HadaM. H. HechtRonald HesperLuis C. HoPaul T. P. HoMareki HonmaChih-Wei L. HuangLei 磊 Huang 黄D. H. HughesShiro IkedaMakoto InoueSara IssaounD. J. JamesBuell T. JannuziMichaël JanssenBritton JeterWu JiangMichael D. JohnsonSvetlana G. JorstadTaehyun JungMansour KaramiR. KaruppusamyTomohisa KawashimaGarrett K. KeatingMark KettenisJae-Young KimJunhan KimJongsoo KimMotoki KinoJun Yi KoayPatrick M. KochShoko KoyamaM. KrämerC. KrämerT. P. KrichbaumCheng‐Yu KuoTod R. LauerSang-Sung LeeYan-Rong LiZhiyuan 志远 Li 李M. LindqvistKuo LiuElisabetta LiuzzoWen-Ping LoA. P. LobanovLaurent LoinardC. J. LonsdaleRu-Sen LuNicholas R. MacDonaldJirong 基荣 Mao 毛Sera MarkoffDaniel P. MarroneAlan P. MarscherI. Martí‐VidalSatoki MatsushitaLynn D. MatthewsLia MedeirosK. M. MentenYosuke MizunoIzumi MizunoJ. M. MoranKotaro MoriyamaMonika MościbrodzkaCornelia MüllerHiroshi NagaiNeil M. NagarMasanori NakamuraRamesh NarayanGopal NarayananIniyan NatarajanR. NeriChunchong NiA. NoutsosHiroki OkinoHéctor OlivaresTomoaki OyamaFeryal ÖzelDaniel C. M. PalumboNimesh PatelUe‐Li PenDominic W. PesceVincent PiétuR. L. PlambeckAleksandar PopStefanijaOliver PorthBen PratherJorge A. Preciado-LópezDimitrios PsaltisHung-Yi PuVenkatessh RamakrishnanRamprasad RaoMark G. RawlingsAlexander W. RaymondLuciano RezzollaBart RipperdaFreek RoelofsA. E. E. RogersE. RosMel RoseArash RoshanineshatHelge RottmannA. L. RoyChet RuszczykBenjamin R. RyanK. L. J. RyglSalvador SánchezDavid Sánchez-ArgüellesMahito SasadaT. SavolainenF. Peter SchloerbK. SchüsterLijing ShaoZhi-Qiang ShenDes SmallBong Won SohnJason SoohooFumie TazakiPaul TiedeR. P. J. TilanusMichael S. TitusKenji TomaPablo TornéTyler TrentSascha TrippeShuichiro TsudaIlse van BemmelHuib Jan van LangeveldeDaniel R. van RossumJan WagnerJ. F. C. WardleJonathan WeintroubNorbert WexRobert WhartonMaciek WielgusGeorge N. WongQingwen 庆文 Wu 吴André YoungKen YoungZiri YounsiFeng 峰 Yuan 袁Ye-Fei 业飞 Yuan 袁J. A. ZensusGuang-Yao ZhaoShan-Shan ZhaoZiyan ZhuJoseph FarahZheng Meyer-ZhaoDaniel MichalikAndrew NadolskiHiroaki NishiokaNicolas PradelRurik A. PrimianiKamal SouccarLaura VertatschitschPaul Yamaguchi

Abstract

Abstract We present the first Event Horizon Telescope (EHT) images of M87, using observations from April 2017 at 1.3 mm wavelength. These images show a prominent ring with a diameter of ∼40 μ as, consistent with the size and shape of the lensed photon orbit encircling the “shadow” of a supermassive black hole. The ring is persistent across four observing nights and shows enhanced brightness in the south. To assess the reliability of these results, we implemented a two-stage imaging procedure. In the first stage, four teams, each blind to the others’ work, produced images of M87 using both an established method (CLEAN) and a newer technique (regularized maximum likelihood). This stage allowed us to avoid shared human bias and to assess common features among independent reconstructions. In the second stage, we reconstructed synthetic data from a large survey of imaging parameters and then compared the results with the corresponding ground truth images. This stage allowed us to select parameters objectively to use when reconstructing images of M87. Across all tests in both stages, the ring diameter and asymmetry remained stable, insensitive to the choice of imaging technique. We describe the EHT imaging procedures, the primary image features in M87, and the dependence of these features on imaging assumptions.

Astrophysical Phenomena and ObservationsAstrophysics and Cosmic PhenomenaRadio Astronomy Observations and TechnologySupermassive black holePhysicsShadow (psychology)TelescopeAsymmetryBrightnessGalaxyAstrophysicsArtificial intelligenceOptics

Funding

  • National Science Foundation
  • Smithsonian Institution
  • U.S. Department of Energy
  • National Aeronautics and Space Administration
  • John Templeton Foundation
  • Gordon and Betty Moore Foundation
  • Kavli Foundation
  • Harvard University
  • University of Chicago
  • University of Arizona
  • Innovation, Science and Economic Development Canada
  • Compute Canada
  • Ministerio de Ciencia, Innovación y Universidades
  • National Radio Astronomy Observatory
  • Associated Universities
  • International Max Planck Research School for Environmental, Cellular and Molecular Microbiology
  • Government of Canada
  • Leverhulme Trust
  • European Commission
  • National Research Foundation
  • Department of Science and Technology, Ministry of Science and Technology, India
  • Ministry of Education, Culture, Sports, Science and Technology
  • National Natural Science Foundation of China
  • Academia Sinica
  • Academy of Finland
  • Chinese Academy of Sciences
  • Consejo Nacional de Ciencia y Tecnología
  • Nederlandse Organisatie voor Wetenschappelijk Onderzoek
  • Ministerio de Economía y Competitividad
  • Generalitat Valenciana
  • Nuclear Safety and Security Commission
  • Korea Institute of Science and Technology
  • Korea Institute of Science and Technology Information
  • Korea Astronomy and Space Science Institute
  • National Research Foundation of Korea
  • Max-Planck-Gesellschaft
  • Vetenskapsrådet
  • China Scholarship Council
  • European Southern Observatory
  • Centre National de la Recherche Scientifique
  • Universidad Nacional Autónoma de México
  • National Astronomical Observatory of Japan
  • Russian Science Foundation
  • Ministero dello Sviluppo Economico
  • Iran Telecommunication Research Center
  • Recruitment Program of Global Experts
  • Istituto Nazionale di Fisica Nucleare
  • Instituto de Astrofísica de Andalucía
  • Institut Périmètre de physique théorique
  • Korea Research Environment Open Network
  • Toray Science Foundation
  • National Nuclear Security Administration
  • Natural Sciences and Engineering Research Council of Canada
  • Japan Society for the Promotion of Science
  • Comisión Nacional de Investigación Científica y Tecnológica
  • Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México
  • National Institutes of Natural Sciences
  • National Key Research and Development Program of China
  • National Institute of Information and Communications Technology
  • Office of International Science and Engineering
  • Los Alamos National Laboratory
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References
First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole
The Astrophysical Journal Letters · 2019 · 3,995 citations
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The Astrophysical Journal Letters · 2019 · 1,045 citations
First M87 Event Horizon Telescope Results. III. Data Processing and Calibration
The Astrophysical Journal Letters · 2019 · 853 citations
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