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First M87 Event Horizon Telescope Results. II. Array and Instrumentation

The Astrophysical Journal Letters · 2019 · Vol. 875(1) · pp. L2–L2
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-EncinasPer 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 OlivaresGisela N. Ortiz-LeónTomoaki 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 ZhuJuan Carlos AlgabaAlexander AllardiRodrigo AmesticaU. BachChristopher BeaudoinB. A. BensonRyan BertholdJ. BlanchardR. BlundellSandra BustamenteR. J. CappalloEdgar Castillo-DomínguezChih-Cheng ChangShu-Hao ChangSong-Chu ChangChung-Chen ChenRyan ChilsonTim C. ChuterRodrigo Córdova RosadoI. M. CoulsonT. M. CrawfordJoseph CrowleyJohn DavidM. DeromeMatthew R. DexterSven DornbuschKevin A. DudevoirSergio A. DzibChris EckertN. R. EricksonW. EverettAaron FaberJoseph FarahVernon FathThomas W. FolkersDavid C. ForbesR. FreundArturo I. Gómez-RuizDavid M. GaleF. GaoGertie GeertsemaD. A. GrahamChristopher H. GreerRonald GrossleinFrédéric GuethN. W. HalversonChih-Chiang HanKuo-Chang HanH. JinchiYutaka HasegawaJ. W. HenningA. Hernández-GómezR. Herrero‐IllanaS. HeyminckAkihiko HirotaJames HogeYau-De HuangC. M. Violette ImpellizzeriHomin JiangA. KambleRyan KeislerKimihiro KimuraYusuke KonoDerek KuboJohn KurodaRichard LacasseRobert A. LaingE. M. LeitchChao-Te LiL. C.-C. LinChing-Tang LiuKuan-Yu LiuLi-Ming LuR. G. MarsonPierre Martin-CocherKyle MassingillCallie MatulonisMartin P. McCollStephen R. McWhirterHugo MessiasZheng Meyer-ZhaoDaniel MichalikAlfredo MontañaWilliam MontgomerieMatias Mora-KleinD. MudersAndrew NadolskiS. NavarroChi H. NguyenHiroaki NishiokaTimothy NortonGeorge NystromHideo OgawaPeter OshiroTomoaki OyamaS. PadinHarriet ParsonsScott PaineJ. PeñalverN. PhillipsMichael PoirierNicolas PradelRurik A. PrimianiPhilippe RaffinA. RahlinGeorge ReilandC. RisacherIgnacio RuizAlejandro F. Sáez-MadaínRemi SassellaP. SchellartPaul ShawKevin M. SilvaHotaka ShiokawaDavid R. SmithW. M. SnowKamal SouccarDon SousaT. K. SridharanRanjani SrinivasanWilliam StahmA. A. StarkKyle StorySjoerd T. TimmerLaura VertatschitschCraig WaltherTa-Shun WeiN. WhitehornA. R. WhitneyD. P. WoodyJ. G. A. WouterlootMelvin WrightPaul YamaguchiChen-Yu YuMilagros ZeballosL. M. Ziurys

Abstract

Abstract The Event Horizon Telescope (EHT) is a very long baseline interferometry (VLBI) array that comprises millimeter- and submillimeter-wavelength telescopes separated by distances comparable to the diameter of the Earth. At a nominal operating wavelength of ∼1.3 mm, EHT angular resolution ( λ / D ) is ∼25 μ as, which is sufficient to resolve nearby supermassive black hole candidates on spatial and temporal scales that correspond to their event horizons. With this capability, the EHT scientific goals are to probe general relativistic effects in the strong-field regime and to study accretion and relativistic jet formation near the black hole boundary. In this Letter we describe the system design of the EHT, detail the technology and instrumentation that enable observations, and provide measures of its performance. Meeting the EHT science objectives has required several key developments that have facilitated the robust extension of the VLBI technique to EHT observing wavelengths and the production of instrumentation that can be deployed on a heterogeneous array of existing telescopes and facilities. To meet sensitivity requirements, high-bandwidth digital systems were developed that process data at rates of 64 gigabit s −1 , exceeding those of currently operating cm-wavelength VLBI arrays by more than an order of magnitude. Associated improvements include the development of phasing systems at array facilities, new receiver installation at several sites, and the deployment of hydrogen maser frequency standards to ensure coherent data capture across the array. These efforts led to the coordination and execution of the first Global EHT observations in 2017 April, and to event-horizon-scale imaging of the supermassive black hole candidate in M87.

Astrophysical Phenomena and ObservationsAstrophysics and Cosmic PhenomenaPulsars and Gravitational Waves ResearchVery-long-baseline interferometryPhysicsEvent horizonTelescopeHydrogen maserSupermassive black holeMillimeterInstrumentation (computer programming)Angular resolution (graph drawing)Maser

Funding

  • National Science Foundation
  • Smithsonian Institution
  • U.S. Department of Energy
  • National Aeronautics and Space Administration
  • John Templeton Foundation
  • Gordon and Betty Moore Foundation
  • Massachusetts Institute of Technology
  • Harvard University
  • University of Chicago
  • University of Arizona
  • Innovation, Science and Economic Development Canada
  • Compute Canada
  • Strong
  • 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
  • Academia Sinica
  • Chinese Academy of Sciences
  • Consejo Nacional de Ciencia y Tecnología
  • Nederlandse Organisatie voor Wetenschappelijk Onderzoek
  • Ministerio de Economía y Competitividad
  • Generalitat Valenciana
  • 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
  • Recruitment Program of Global Experts
  • Istituto Nazionale di Fisica Nucleare
  • Instituto de Astrofísica de Andalucía
  • Institut Périmètre de physique théorique
  • 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
  • Office of Polar Programs
  • Los Alamos National Laboratory
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References
<i>The Mathematical Theory of Black Holes</i>
Physics Today · 1984 · 2,183 citations
Observation of Gravitational Waves from a Binary Black Hole Merger
Physical Review Letters · 2016 · 13,779 citations
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