Перейти к основному содержанию
AkademIndex

Продукты

Для разработчиков

AkademBaseскороОткрытый API экосистемы
Латиница
Русский
Статья

First M87 Event Horizon Telescope Results. III. Data Processing and Calibration

Kazunori AkiyamaBlack Hole Initiative at Harvard University, 20 Garden Street, Cambridge, MA 02138, USAA. AlberdiInstituto de Astrofísica de Andalucía-CSIC, Glorieta de la Astronomía s/n, E-18008 Granada, SpainW. AlefMax-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, GermanyKeiichi AsadaInstitute of Astronomy and Astrophysics, Academia Sinica, 11F of Astronomy-Mathematics Building, AS/NTU No. 1, Sec. 4, Roosevelt Rd, Taipei 10617, Taiwan, R.O.CRebecca AzulayObservatori Astronòmic, Universitat de València, C. Catedrático José Beltrán 2, E-46980 Paterna, València, SpainAnne-Kathrin BaczkoMax-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, GermanyDavid BallSteward Observatory and Department of Astronomy, University of Arizona, 933 N. Cherry Avenue, Tucson, AZ 85721, USAMislav BalokovićBlack Hole Initiative at Harvard University, 20 Garden Street, Cambridge, MA 02138, USAJ. BarrettMassachusetts Institute of Technology Haystack Observatory, 99 Millstone Road, Westford, MA 01886, USADan BintleyEast Asian Observatory, 660 N. A'ohoku Pl., Hilo, HI 96720, USALindy BlackburnCenter for Astrophysics | Harvard & Smithsonian, 60 Garden Street, Cambridge, MA 02138, USAW. BolandNederlandse Onderzoekschool voor Astronomie (NOVA), PO Box 9513, 2300 RA Leiden, The NetherlandsKatherine L. BoumanCenter for Astrophysics | Harvard & Smithsonian, 60 Garden Street, Cambridge, MA 02138, USAGeoffrey C. BowerMichael BremerInstitut de Radioastronomie Millimétrique, 300 rue de la Piscine, F-38406 Saint Martin d'Hères, FranceChristiaan D. BrinkerinkDepartment of Astrophysics, Institute for Mathematics, Astrophysics and Particle Physics (IMAPP), Radboud University, P.O. Box 9010, 6500 GL Nijmegen, The NetherlandsRoger BrissendenBlack Hole Initiative at Harvard University, 20 Garden Street, Cambridge, MA 02138, USAS. BritzenMax-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, GermanyAvery E. BroderickWaterloo Centre for Astrophysics, University of Waterloo, Waterloo, ON N2L 3G1, CanadaDominique BroguièreInstitut de Radioastronomie Millimétrique, 300 rue de la Piscine, F-38406 Saint Martin d'Hères, FranceThomas BronzwaerDepartment of Astrophysics, Institute for Mathematics, Astrophysics and Particle Physics (IMAPP), Radboud University, P.O. Box 9010, 6500 GL Nijmegen, The NetherlandsDo‐Young ByunUniversity of Science and Technology, Gajeong-ro 217, Yuseong-gu, Daejeon 34113, Republic of KoreaJ. E. CarlstromDepartment of Astronomy and Astrophysics, University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637, USAAndrew ChaelBlack Hole Initiative at Harvard University, 20 Garden Street, Cambridge, MA 02138, USAChi‐kwan ChanSteward Observatory and Department of Astronomy, University of Arizona, 933 N. Cherry Avenue, Tucson, AZ 85721, USAShami ChatterjeeCornell Center for Astrophysics and Planetary Science, Cornell University, Ithaca, NY 14853, USAKoushik ChatterjeeAnton Pannekoek Institute for Astronomy, University of Amsterdam, Science Park 904, 1098 XH, Amsterdam, The NetherlandsMing‐Tang ChenXiaopeng ChengIlje ChoKorea Astronomy and Space Science Institute, Daedeok-daero 776, Yuseong-gu, Daejeon 34055, Republic of KoreaPierre ChristianCenter for Astrophysics | Harvard & Smithsonian, 60 Garden Street, Cambridge, MA 02138, USAJ. E. ConwayDepartment of Space, Earth and Environment, Chalmers University of Technology, Onsala Space Observatory, SE-43992 Onsala, SwedenJ. M. CordesCornell Center for Astrophysics and Planetary Science, Cornell University, Ithaca, NY 14853, USAG. CrewMassachusetts Institute of Technology Haystack Observatory, 99 Millstone Road, Westford, MA 01886, USAYuzhu CuiDepartment of Astronomical Science, The Graduate University for Advanced Studies (SOKENDAI), 2-21-1 Osawa, Mitaka, Tokyo 181-8588, JapanJordy DavelaarDepartment of Astrophysics, Institute for Mathematics, Astrophysics and Particle Physics (IMAPP), Radboud University, P.O. Box 9010, 6500 GL Nijmegen, The NetherlandsMariafelicia De LaurentisInstitut für Theoretische Physik, Goethe-Universität Frankfurt, Max-von-Laue-Straße 1, D-60438 Frankfurt am Main, GermanyRoger DeaneCentre for Radio Astronomy Techniques and Technologies, Department of Physics and Electronics, Rhodes University, Grahamstown 6140, South AfricaJessica DempseyEast Asian Observatory, 660 N. A'ohoku Pl., Hilo, HI 96720, USAG. DesvignesMax-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, GermanyJason DexterMax-Planck-Institut für Extraterrestrische Physik, Giessenbachstr. 1, D-85748 Garching, GermanySheperd S. DoelemanBlack Hole Initiative at Harvard University, 20 Garden Street, Cambridge, MA 02138, USARalph P. EatoughMax-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, GermanyH. FalckeDepartment of Astrophysics, Institute for Mathematics, Astrophysics and Particle Physics (IMAPP), Radboud University, P.O. Box 9010, 6500 GL Nijmegen, The NetherlandsVincent L. FishMassachusetts Institute of Technology Haystack Observatory, 99 Millstone Road, Westford, MA 01886, USAEd FomalontNational Radio Astronomy Observatory, 520 Edgemont Rd, Charlottesville, VA 22903, USARaquel Fraga-EncinasDepartment of Astrophysics, Institute for Mathematics, Astrophysics and Particle Physics (IMAPP), Radboud University, P.O. Box 9010, 6500 GL Nijmegen, The NetherlandsPer FribergEast Asian Observatory, 660 N. A'ohoku Pl., Hilo, HI 96720, USAChristian M. FrommInstitut für Theoretische Physik, Goethe-Universität Frankfurt, Max-von-Laue-Straße 1, D-60438 Frankfurt am Main, GermanyJosé L. GómezInstituto de Astrofísica de Andalucía-CSIC, Glorieta de la Astronomía s/n, E-18008 Granada, SpainPeter GalisonBlack Hole Initiative at Harvard University, 20 Garden Street, Cambridge, MA 02138, USACharles F. GammieDepartment of Physics, University of Illinois, 1110 West Green St, Urbana, IL 61801, USARoberto GarcíaInstitut de Radioastronomie Millimétrique, 300 rue de la Piscine, F-38406 Saint Martin d'Hères, FranceOlivier GentazInstitut de Radioastronomie Millimétrique, 300 rue de la Piscine, F-38406 Saint Martin d'Hères, FranceBoris GeorgievDepartment of Physics and Astronomy, University of Waterloo, 200 University Avenue West, Waterloo, ON, N2L 3G1, CanadaC. GoddiLeiden Observatory—Allegro, Leiden University, P.O. Box 9513, 2300 RA Leiden, The NetherlandsRoman GoldInstitut für Theoretische Physik, Goethe-Universität Frankfurt, Max-von-Laue-Straße 1, D-60438 Frankfurt am Main, GermanyMinfeng GuMark GurwellCenter for Astrophysics | Harvard & Smithsonian, 60 Garden Street, Cambridge, MA 02138, USAKazuhiro HadaMizusawa VLBI Observatory, National Astronomical Observatory of Japan, 2-12 Hoshigaoka, Mizusawa, Oshu, Iwate 023-0861, JapanM. H. HechtMassachusetts Institute of Technology Haystack Observatory, 99 Millstone Road, Westford, MA 01886, USARonald HesperNOVA Sub-mm Instrumentation Group, Kapteyn Astronomical Institute, University of Groningen, Landleven 12, 9747 AD Groningen, The NetherlandsLuis C. HoPaul T. P. HoInstitute of Astronomy and Astrophysics, Academia Sinica, 11F of Astronomy-Mathematics Building, AS/NTU No. 1, Sec. 4, Roosevelt Rd, Taipei 10617, Taiwan, R.O.CMareki HonmaMizusawa VLBI Observatory, National Astronomical Observatory of Japan, 2-12 Hoshigaoka, Mizusawa, Oshu, Iwate 023-0861, JapanChih-Wei L. HuangInstitute of Astronomy and Astrophysics, Academia Sinica, 11F of Astronomy-Mathematics Building, AS/NTU No. 1, Sec. 4, Roosevelt Rd, Taipei 10617, Taiwan, R.O.CLei 磊 Huang 黄D. H. HughesInstituto Nacional de Astrofísica, Óptica y Electrónica. Apartado Postal 51 y 216, 72000. Puebla Pue., MéxicoShiro IkedaThe Institute of Statistical Mathematics, 10-3 Midori-cho, Tachikawa, Tokyo, 190-8562, JapanMakoto InoueInstitute of Astronomy and Astrophysics, Academia Sinica, 11F of Astronomy-Mathematics Building, AS/NTU No. 1, Sec. 4, Roosevelt Rd, Taipei 10617, Taiwan, R.O.CSara IssaounDepartment of Astrophysics, Institute for Mathematics, Astrophysics and Particle Physics (IMAPP), Radboud University, P.O. Box 9010, 6500 GL Nijmegen, The NetherlandsD. J. JamesCenter for Astrophysics | Harvard & Smithsonian, 60 Garden Street, Cambridge, MA 02138, USABuell T. JannuziSteward Observatory and Department of Astronomy, University of Arizona, 933 N. Cherry Avenue, Tucson, AZ 85721, USAMichaël JanssenDepartment of Astrophysics, Institute for Mathematics, Astrophysics and Particle Physics (IMAPP), Radboud University, P.O. Box 9010, 6500 GL Nijmegen, The NetherlandsBritton JeterWaterloo Centre for Astrophysics, University of Waterloo, Waterloo, ON N2L 3G1, CanadaWu JiangMichael D. JohnsonBlack Hole Initiative at Harvard University, 20 Garden Street, Cambridge, MA 02138, USASvetlana G. JorstadInstitute for Astrophysical Research, Boston University, 725 Commonwealth Ave., Boston, MA 02215, USATaehyun JungKorea Astronomy and Space Science Institute, Daedeok-daero 776, Yuseong-gu, Daejeon 34055, Republic of KoreaMansour KaramiPerimeter Institute for Theoretical Physics, 31 Caroline Street North, Waterloo, ON, N2L 2Y5, CanadaR. KaruppusamyMax-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, GermanyTomohisa KawashimaNational Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, JapanGarrett K. KeatingCenter for Astrophysics | Harvard & Smithsonian, 60 Garden Street, Cambridge, MA 02138, USAMark KettenisJoint Institute for VLBI ERIC (JIVE), Oude Hoogeveensedijk 4, 7991 PD Dwingeloo, The NetherlandsJae-Young KimMax-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, GermanyJunhan KimSteward Observatory and Department of Astronomy, University of Arizona, 933 N. Cherry Avenue, Tucson, AZ 85721, USAJongsoo KimKorea Astronomy and Space Science Institute, Daedeok-daero 776, Yuseong-gu, Daejeon 34055, Republic of KoreaMotoki KinoKogakuin University of Technology and Engineering, Academic Support Center, 2665-1 Nakano, Hachioji, Tokyo 192-0015, JapanJun Yi KoayInstitute of Astronomy and Astrophysics, Academia Sinica, 11F of Astronomy-Mathematics Building, AS/NTU No. 1, Sec. 4, Roosevelt Rd, Taipei 10617, Taiwan, R.O.CPatrick M. KochInstitute of Astronomy and Astrophysics, Academia Sinica, 11F of Astronomy-Mathematics Building, AS/NTU No. 1, Sec. 4, Roosevelt Rd, Taipei 10617, Taiwan, R.O.CShoko KoyamaInstitute of Astronomy and Astrophysics, Academia Sinica, 11F of Astronomy-Mathematics Building, AS/NTU No. 1, Sec. 4, Roosevelt Rd, Taipei 10617, Taiwan, R.O.CMichael KramerMax-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, GermanyC. KrämerInstitut de Radioastronomie Millimétrique, 300 rue de la Piscine, F-38406 Saint Martin d'Hères, FranceT. P. KrichbaumMax-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, GermanyC. Y. KuoPhysics Department, National Sun Yat-Sen University, No. 70, Lien-Hai Rd, Kaosiung City 80424, Taiwan, R.O.CTod R. LauerNational Optical Astronomy Observatory, 950 North Cherry Ave., Tucson, AZ 85719, USASang-Sung LeeKorea Astronomy and Space Science Institute, Daedeok-daero 776, Yuseong-gu, Daejeon 34055, Republic of KoreaYanrong LiZhiyuan 志远 Li 李M. LindqvistDepartment of Space, Earth and Environment, Chalmers University of Technology, Onsala Space Observatory, SE-43992 Onsala, Sweden
2019en
ABI

Аннотация

Abstract We present the calibration and reduction of Event Horizon Telescope (EHT) 1.3 mm radio wavelength observations of the supermassive black hole candidate at the center of the radio galaxy M87 and the quasar 3C 279, taken during the 2017 April 5–11 observing campaign. These global very long baseline interferometric observations include for the first time the highly sensitive Atacama Large Millimeter/submillimeter Array (ALMA); reaching an angular resolution of 25 μ as, with characteristic sensitivity limits of ∼1 mJy on baselines to ALMA and ∼10 mJy on other baselines. The observations present challenges for existing data processing tools, arising from the rapid atmospheric phase fluctuations, wide recording bandwidth, and highly heterogeneous array. In response, we developed three independent pipelines for phase calibration and fringe detection, each tailored to the specific needs of the EHT. The final data products include calibrated total intensity amplitude and phase information. They are validated through a series of quality assurance tests that show consistency across pipelines and set limits on baseline systematic errors of 2% in amplitude and 1° in phase. The M87 data reveal the presence of two nulls in correlated flux density at ∼3.4 and ∼8.3 G λ and temporal evolution in closure quantities, indicating intrinsic variability of compact structure on a timescale of days, or several light-crossing times for a few billion solar-mass black hole. These measurements provide the first opportunity to image horizon-scale structure in M87.

Идентификаторы

Цитирования и источники

Цитирований: 32Использованных источников: 0
Показатели — AkademScholar · Скоро