YNAO OpenIR  > 星系类星体研究组
Selective Dynamical Imaging of Interferometric Data
Farah, Joseph1,2; Galison, Peter3,4,5; Akiyama, Kazunori3,6,7; Bouman, Katherine L.3,8,9; Bower, Geoffrey C.10; Chael, Andrew11,12; Fuentes, Antonio13; Gómez, José L.14; Honma, Mareki15,16,17; Johnson, Michael D.3,8; Kofuji, Yutaro15,17; Marrone, Daniel P.18; Moriyama, Kotaro6,15; Narayan, Ramesh3,8; Pesce, Dominic W.3,8; Tiede, Paul19,20; Wielgus, Maciek21; Zhao, Guang-Yao13; Alberdi, Antxon13; Alef, Walter21; Algaba, Juan Carlos22; Anantua, Richard3,8; Asada, Keiichi23; Azulay, Rebecca21,24,25; Baczko, Anne-Kathrin21; Ball, David18; Baloković, Mislav3,8; Barrett, John6; Benson, Bradford A.26,27; Bintley, Dan28; Blackburn, Lindy3,8; Blundell, Raymond8; Boland, Wilfred29; Boyce, Hope30,31; Bremer, Michael32; Brinkerink, Christiaan D.33; Brissenden, Roger3,8; Britzen, Silke21; Broderick, Avery E.19,20,34; Broguiere, Dominique32; Bronzwaer, Thomas33; Bustamente, Sandra35; Byun, Do-Young36,37; Carlstrom, John E.27,38,39,40; Chan, Chi-kwan18,41; Chatterjee, Koushik42; Chatterjee, Shami43; Chen, Ming-Tang10; Chen, Yongjun44,45; Cho, Ilje14; Christian, Pierre46; Conway, John E.47; Cordes, James M.43; Crawford, Thomas M.27,38; Crew, Geoffrey B.6; Cruz-Osorio, Alejandro48; Cui, Yuzhu15,16; Davelaar, Jordy33,49,50; Laurentis, Mariafelicia De48,51,52; Deane, Roger53,54,55; Dempsey, Jessica28; Desvignes, Gregory56; Doeleman, Sheperd S.3,8; Eatough, Ralph P.21,57; Falcke, Heino33; Fish, Vincent L.6; Fomalont, Ed58; Ford, H. Alyson18; Fraga-Encinas, Raquel33; Friberg, Per28; Fromm, Christian M.3,8,48; Gammie, Charles F.59,60; Garc'a, Roberto32; Gentaz, Olivier32; Goddi, Ciriaco33,61; Gold, Roman34,62; Gómez-Ruiz, Arturo I.63,64; Gu, Minfeng44,65; Gurwell, Mark8; Hada, Kazuhiro15,16; Haggard, Daryl30,31; Hecht, Michael H.6; Hesper, Ronald66; Ho, Luis C.67,68; Ho, Paul23; Huang, Chih-Wei L.23; Huang, Lei44,65; Hughes, David H.63; Ikeda, Shiro7,69,70,71; Inoue, Makoto23; Issaoun, Sara33; James, David J.3,8; Jannuzi, Buell T.18; Janssen, Michael21; Jeter, Britton19,20; Jiang, Wu44; Jimenez-Rosales, Alejandra33; Jorstad, Svetlana72; Jung, Taehyun36,37; Karami, Mansour19,34; Karuppusamy, Ramesh21; Kawashima, Tomohisa73; Keating, Garrett K.8; Kettenis, Mark74; Kim, Dong-Jin21; Kim, Jae-Young21,36; Kim, Jongsoo36; Kim, Junhan9,18; Kino, Motoki7,75; Koay, Jun Yi23; Koch, Patrick M.23; Koyama, Shoko23; Kramer, Carsten32; Kramer, Michael21; Krichbaum, Thomas P.21; Kuo, Cheng-Yu23,76; Lauer, Tod R.77; Lee, Sang-Sung36; Levis, Aviad9; Li, Yan-Rong78; Li, Zhiyuan79,80; Lico, Rocco13,21,81; Lindahl, Greg8; Lindqvist, Michael47; Liu, Jun21; Liu, Kuo21; Liuzzo, Elisabetta81; Lo, Wen-Ping23,82; Lobanov, Andrei P.21; Loinard, Laurent83,84; Lonsdale, Colin6; Lu, Ru-Sen21,44,45; MacDonald, Nicholas R.21; Mao JR(毛基荣)85,86,87; Marchili, Nicola21,81; Markoff, Sera42,88; Marscher, Alan P.72; Martí-Vidal, Iván24,25; Matsushita, Satoki23; Matthews, Lynn D.6; Medeiros, Lia18,89; Menten, Karl M.21; Mizuno, Izumi28; Mizuno, Yosuke48,90; Moran, James M.3,8; Moscibrodzka, Monika33; Müller, Cornelia21,33; Mejas, Alejandro Mus24,25; Musoke, Gibwa33,42; Nagai, Hiroshi7,16; Nagar, Neil M.91; Nakamura, Masanori23,92; Narayanan, Gopal35; Natarajan, Iniyan53,55,93; Nathanail, Antonios48; Neilsen, Joey94; Neri, Roberto32; Ni, Chunchong19,20; Noutsos, Aristeidis21; Nowak, Michael A.95; Okino, Hiroki15,17; Olivares, Héctor33; Ortiz-León, Gisela N.21; Oyama, Tomoaki15; zel, Feryal18; Palumbo, Daniel C. M.3,8; Park, Jongho23; Patel, Nimesh8; Pen, Ue-Li34,96,97,98; Piétu, Vincent32; Plambeck, Richard99; PopStefanija, Aleksandar35; Porth, Oliver42,48; Pötzl, Felix M.21; Prather, Ben59; Preciado-López, Jorge A.34; Psaltis, Dimitrios18; Pu, Hung-Yi23,34,100; Ramakrishnan, Venkatessh91; Rao, Ramprasad10; Rawlings, Mark G.28; Raymond, Alexander W.3,8; Rezzolla, Luciano48,101,102; Ripperda, Bart50,103; Roelofs, Freek8,33; Rogers, Alan6; Ros, Eduardo21; Rose, Mel18; Roshanineshat, Arash18; Rottmann, Helge21; Roy, Alan L.21; Ruszczyk, Chet6; Rygl, Kazi L. J.81; Sánchez, Salvador104; Sánchez-Arguelles, David63,105; Sasada, Mahito15,106; Savolainen, Tuomas21,107,108; Schloerb, F. Peter35; Schuster, Karl-Friedrich32; Shao, Lijing21,68; Shen, Zhiqiang44,45; Small, Des74; Sohn, Bong Won36,37,109; SooHoo, Jason6; Sun, He9; Tazaki, Fumie15; Tetarenko, Alexandra J.28; Tilanus, Remo P. J.18,33,110,111; Titus, Michael6; Toma, Kenji112,113; Torne, Pablo21,104; Traianou, Efthalia14,21; Trent, Tyler18; Trippe, Sascha114; Bemmel, Ilse van74; Langevelde, Huib Jan van74,115; Rossum, Daniel R. van33; Wagner, Jan21; Ward-Thompson, Derek116; Wardle, John117; Weintroub, Jonathan3,8; Wex, Norbert21; Wharton, Robert21; Wiik, Kaj118; Wong, George N.59; Wu, Qingwen119; Yoon, Doosoo42; Young, André33; Young, Ken8; Younsi, Ziri48,120; Yuan, Feng44,65,121; Yuan, Ye-Fei122; Zensus, J. Anton21; Zhao, Shan-Shan44
Source PublicationASTROPHYSICAL JOURNAL LETTERS
2022-05-01
Volume930Issue:2
DOI10.3847/2041-8213/ac6615
Contribution Rank第87完成单位
Indexed BySCI
Abstract

Recent developments in very long baseline interferometry (VLBI) have made it possible for the Event Horizon Telescope (EHT) to resolve the innermost accretion flows of the largest supermassive black holes on the sky. The sparse nature of the EHT's (u, v)-coverage presents a challenge when attempting to resolve highly time-variable sources. We demonstrate that the changing (u, v)-coverage of the EHT can contain regions of time over the course of a single observation that facilitate dynamical imaging. These optimal time regions typically have projected baseline distributions that are approximately angularly isotropic and radially homogeneous. We derive a metric of coverage quality based on baseline isotropy and density that is capable of ranking array configurations by their ability to produce accurate dynamical reconstructions. We compare this metric to existing metrics in the literature and investigate their utility by performing dynamical reconstructions on synthetic data from simulated EHT observations of sources with simple orbital variability. We then use these results to make recommendations for imaging the 2017 EHT Sgr A* data set.

Funding ProjectNational Science Foundation[OISE-1743747] ; National Science Foundation[AST-1816420] ; National Science Foundation[AST-1716536] ; National Science Foundation[AST-1440254] ; National Science Foundation[AST1935980] ; Gordon and Betty Moore Foundation[GBMF-5278] ; Gordon and Betty Moore Foundation[GBMF-3561] ; Black Hole Initiative - John Templeton Foundation ; Gordon and Betty Moore Foundation ; NASA Hubble Fellowship - Space Telescope Science Institute[HST-HF2-51431.001-A] ; NASA Hubble Fellowship - Space Telescope Science Institute[NAS5-26555] ; Academy of Finland[274477] ; Academy of Finland[284495] ; Academy of Finland[312496] ; Academy of Finland[315721] ; Agencia Nacional de Investigacin y Desarrollo (ANID), Chile[NCN19058] ; Fondecyt[3190878] ; Alexander von Humboldt Stiftung ; Alfred P. Sloan Research Fellowship ; Allegro ; European ALMA Regional Centre node in the Netherlands ; NL astronomy research network NOVA ; University of Amsterdam ; Leiden University ; Radboud University ; Black Hole Initiative at Harvard University through the John Templeton Foundation[60477] ; China Scholarship Council ; Consejo Nacional de Ciencia y Tecnologia (CONACYT, Mexico)[U0004-246083] ; Consejo Nacional de Ciencia y Tecnologia (CONACYT, Mexico)[U0004-259839] ; Consejo Nacional de Ciencia y Tecnologia (CONACYT, Mexico)[F0003-272050] ; Consejo Nacional de Ciencia y Tecnologia (CONACYT, Mexico)[M0037-279006] ; Consejo Nacional de Ciencia y Tecnologia (CONACYT, Mexico)[F0003-281692] ; Consejo Nacional de Ciencia y Tecnologia (CONACYT, Mexico)[104497] ; Consejo Nacional de Ciencia y Tecnologia (CONACYT, Mexico)[275201] ; Consejo Nacional de Ciencia y Tecnologia (CONACYT, Mexico)[263356] ; Delaney Family via the Delaney Family John A. Wheeler Chair at Perimeter Institute ; Direccin General de Asuntos del Personal Acadmico-Universidad Nacional Autnoma de Mxico (DGAPA-UNAM)[IN112417] ; Direccin General de Asuntos del Personal Acadmico-Universidad Nacional Autnoma de Mxico (DGAPA-UNAM)[IN112820] ; European Research Council Synergy Grant BlackHoleCam: Imaging the Event Horizon of Black Holes[610058] ; Generalitat Valenciana[APOSTD/2018/177] ; GenT Program[CIDEGENT/2018/021] ; MICINN[PID2019-108995GBC22] ; European Research Council[884631] ; Istituto Nazionale di Fisica Nucleare (INFN) sezione di Napoli, iniziative specifiche TEONGRAV ; two Dutch National Supercomputers, Cartesius and Snellius (NWO)[2021.013] ; International Max Planck Research School for Astronomy and Astrophysics at the University of Bonn ; Joint Princeton/Flatiron Postdoctoral Fellowship ; Joint Columbia/Flatiron Postdoctoral Fellowship ; Simons Foundation ; Japanese Government (Monbukagakusho: MEXT) Scholarship ; Japan Society for the Promotion of Science (JSPS)[JP17J08829] ; Key Research Program of Frontier Sciences, Chinese Academy of Sciences (CAS)[QYZDJ-SSW-SLH057] ; Key Research Program of Frontier Sciences, Chinese Academy of Sciences (CAS)[QYZDJ-SSWSYS008] ; Key Research Program of Frontier Sciences, Chinese Academy of Sciences (CAS)[ZDBS-LY-SLH011] ; Leverhulme Trust Early Career Research Fellowship ; Max-Planck-Gesellschaft (MPG) ; Max Planck Partner Group of the MPG ; CAS ; MEXT/JSPS KAKENHI[18KK0090] ; MEXT/JSPS KAKENHI[JP21H01137] ; MEXT/JSPS KAKENHI[JP18H03721] ; MEXT/JSPS KAKENHI[18K03709] ; MEXT/JSPS KAKENHI[18H01245] ; MEXT/JSPS KAKENHI[25120007] ; Malaysian Fundamental Research Grant Scheme (FRGS)[FRGS/1/2019/STG02/UM/02/6] ; MIT International Science and Technology Initiatives (MISTI) Funds ; Ministry of Education (MoE) of Taiwan Yushan Young Scholar Program ; Physics Division, National Center for Theoretical Sciences of Taiwan ; National Aeronautics and Space Administration (NASA)[80NSSC20K1567] ; National Aeronautics and Space Administration (NASA)[80NSSC20K0527] ; National Aeronautics and Space Administration (NASA)[80NSSC20K0645] ; National Institute of Natural Sciences (NINS) of Japan ; National Key Research and Development Program of China[2016YFA0400704] ; National Key Research and Development Program of China[2016YFA0400702] ; National Science Foundation (NSF)[AST-0096454] ; National Science Foundation (NSF)[AST-0352953] ; National Science Foundation (NSF)[AST-0521233] ; National Science Foundation (NSF)[AST-0705062] ; National Science Foundation (NSF)[AST-0905844] ; National Science Foundation (NSF)[AST-0922984] ; National Science Foundation (NSF)[AST-1126433] ; National Science Foundation (NSF)[AST-1140030] ; National Science Foundation (NSF)[DGE-1144085] ; National Science Foundation (NSF)[AST-1207704] ; National Science Foundation (NSF)[AST-1207730] ; National Science Foundation (NSF)[AST-1207752] ; National Science Foundation (NSF)[MRI-1228509] ; National Science Foundation (NSF)[OPP-1248097] ; National Science Foundation (NSF)[AST-1310896] ; National Science Foundation (NSF)[AST-1555365] ; National Science Foundation (NSF)[AST-1615796] ; National Science Foundation (NSF)[AST-1715061] ; National Science Foundation (NSF)[AST-1716327] ; National Science Foundation (NSF)[AST-1903847] ; National Science Foundation (NSF)[AST-2034306] ; National Science Foundation (NSF)[OPP-1852617] ; Natural Science Foundation of China[11650110427] ; Natural Science Foundation of China[10625314] ; Natural Science Foundation of China[11721303] ; Natural Science Foundation of China[11725312] ; Natural Science Foundation of China[11933007] ; Natural Science Foundation of China[11991052] ; Natural Science Foundation of China[11991053] ; NWO[OCENW.KLEIN.113] ; China Postdoctoral Science Foundation[2020M671266] ; Natural Sciences and Engineering Research Council of Canada (NSERC) ; National Youth Thousand Talents Program of China ; National Research Foundation of Korea[NRF-2015H1A2A1033752] ; National Research Foundation of Korea[2015R1D1A1A01056807] ; National Research Foundation of Korea[NRF-2015H1D3A1066561] ; National Research Foundation of Korea[2019R1F1A1059721] ; Netherlands Organization for Scientific Research (NWO) VICI award[639.043.513] ; Spinoza Prize[SPI 78-409] ; New Scientific Frontiers with Precision Radio Interferometry Fellowship - South African Radio Astronomy Observatory (SARAO) ; Swedish Research Council[2017-00648] ; Perimeter Institute for Theoretical Physics (Government of Canada through the Department of Innovation, Science and Economic Development) ; Perimeter Institute for Theoretical Physics (Province of Ontario through the Ministry of Research, Innovation and Science) ; Spanish Ministerio de Ciencia e Innovacin[PGC2018-098915-B-C21] ; Spanish Ministerio de Ciencia e Innovacin[AYA2016-80889P] ; Spanish Ministerio de Ciencia e Innovacin[PID2019-108995GB-C21] ; Spanish Ministerio de Ciencia e Innovacin[PID2020-117404GB-C21] ; State Agency for Research of the Spanish MCIU through the Center of Excellence Severo Ochoa award[SEV-2017-0709] ; Toray Science Foundation ; Consejera de Economa, Conocimiento, Empresas y Universidad of the Junta de Andaluca[P18-FR1769] ; Consejo Superior de Investigaciones Cientficas[2019AEP112] ; M2FINDERS project - European Research Council (ERC) under the European Unions Horizon 2020 Research and Innovation Programme[101018682] ; US Department of Energy (USDOE) through the Los Alamos National Laboratory[89233218CNA000001] ; European Unions Horizon 2020 research and innovation program[730562 RadioNet] ; Shanghai Pilot Program for Basic Research, Chinese Academy of Science, Shanghai Branch[JCYJ-SHFY-2021-013] ; ALMA North America Development Fund ; Academia Sinica ; Chandra[DD7-18089X] ; Chandra[TM617006X] ; GenT Program (Generalitat Valenciana)[CIDEGENT/2018/021] ; NSF[ACI-1548562] ; NSF[DBI-0735191] ; NSF[DBI-1265383] ; NSF[DBI-1743442] ; CyVerse ; Compute Ontario ; Calcul Quebec ; Compute Canada ; Swedish Research Council (VR) ; Virtual Institute of Accretion (VIA) postdoctoral fellowships from the Netherlands Research School for Astronomy (NOVA) ; Smithsonian Institution ; Ministry of Finance of China ; National Key R&D Program of China[2017YFA0402700] ; Science and Technologies Facility Council (UK) ; National Research Foundation of Korea (NRF) - Ministry of Education[NRF-2021R1A6A3A01086420] ; Ministry of Finance in China ; CNRS (Centre National de la Recherche Scientifique, France) ; MPG (MaxPlanck-Gesellschaft, Germany) ; IGN (Instituto Geogrfico Nacional, Spain) ; State of Arizona ; NSF ; Kavli Institute of Cosmological Physics at the University of Chicago ; NASA - Space Telescope Science Institute[NAS5-26555] ; NASA - Space Telescope Science Institute[HST-HF2-51494.001] ; Ministry of Science and Technology (MOST) of Taiwan[103-2119-M001-010-MY2] ; Ministry of Science and Technology (MOST) of Taiwan[105-2112-M-001-025-MY3] ; Ministry of Science and Technology (MOST) of Taiwan[105-2119-M-001042] ; Ministry of Science and Technology (MOST) of Taiwan[106-2112-M-001-011] ; Ministry of Science and Technology (MOST) of Taiwan[106-2119-M-001-013] ; Ministry of Science and Technology (MOST) of Taiwan[106-2119-M001-027] ; Ministry of Science and Technology (MOST) of Taiwan[106-2923-M-001-005] ; Ministry of Science and Technology (MOST) of Taiwan[107-2119-M-001-017] ; Ministry of Science and Technology (MOST) of Taiwan[1072119-M-001-020] ; Ministry of Science and Technology (MOST) of Taiwan[107-2119-M-001-041] ; Ministry of Science and Technology (MOST) of Taiwan[107-2119-M-110-005] ; The Ministry of Science and Technology (MOST) of Taiwan[107-2923-M-001-009] ; The Ministry of Science and Technology (MOST) of Taiwan[108-2112-M-001-048] ; The Ministry of Science and Technology (MOST) of Taiwan[108-2112-M-001051] ; The Ministry of Science and Technology (MOST) of Taiwan[108-2923-M-001-002] ; The Ministry of Science and Technology (MOST) of Taiwan[109-2112-M-001-025] ; The Ministry of Science and Technology (MOST) of Taiwan[109-2124-M001-005] ; The Ministry of Science and Technology (MOST) of Taiwan[109-2923-M-001-001] ; The Ministry of Science and Technology (MOST) of Taiwan[110-2112-M-003-007-MY2] ; The Ministry of Science and Technology (MOST) of Taiwan[110-2112-M-001-033] ; The Ministry of Science and Technology (MOST) of Taiwan[110-2124-M-001-007] ; The Ministry of Science and Technology (MOST) of Taiwan[110-2923-M001-001] ; International Max Planck Research School for Astronomy and Astrophysics at the University of Cologne ; Chinese Academy of Sciences
Funding OrganizationNational Science Foundation[OISE-1743747, AST-1816420, AST-1716536, AST-1440254, AST1935980] ; Gordon and Betty Moore Foundation[GBMF-5278, GBMF-3561] ; Black Hole Initiative - John Templeton Foundation ; Gordon and Betty Moore Foundation ; NASA Hubble Fellowship - Space Telescope Science Institute[HST-HF2-51431.001-A, NAS5-26555] ; Academy of Finland[274477, 284495, 312496, 315721] ; Agencia Nacional de Investigacin y Desarrollo (ANID), Chile[NCN19058] ; Fondecyt[3190878] ; Alexander von Humboldt Stiftung ; Alfred P. Sloan Research Fellowship ; Allegro ; European ALMA Regional Centre node in the Netherlands ; NL astronomy research network NOVA ; University of Amsterdam ; Leiden University ; Radboud University ; Black Hole Initiative at Harvard University through the John Templeton Foundation[60477] ; China Scholarship Council ; Consejo Nacional de Ciencia y Tecnologia (CONACYT, Mexico)[U0004-246083, U0004-259839, F0003-272050, M0037-279006, F0003-281692, 104497, 275201, 263356] ; Delaney Family via the Delaney Family John A. Wheeler Chair at Perimeter Institute ; Direccin General de Asuntos del Personal Acadmico-Universidad Nacional Autnoma de Mxico (DGAPA-UNAM)[IN112417, IN112820] ; European Research Council Synergy Grant BlackHoleCam: Imaging the Event Horizon of Black Holes[610058] ; Generalitat Valenciana[APOSTD/2018/177] ; GenT Program[CIDEGENT/2018/021] ; MICINN[PID2019-108995GBC22] ; European Research Council[884631] ; Istituto Nazionale di Fisica Nucleare (INFN) sezione di Napoli, iniziative specifiche TEONGRAV ; two Dutch National Supercomputers, Cartesius and Snellius (NWO)[2021.013] ; International Max Planck Research School for Astronomy and Astrophysics at the University of Bonn ; Joint Princeton/Flatiron Postdoctoral Fellowship ; Joint Columbia/Flatiron Postdoctoral Fellowship ; Simons Foundation ; Japanese Government (Monbukagakusho: MEXT) Scholarship ; Japan Society for the Promotion of Science (JSPS)[JP17J08829] ; Key Research Program of Frontier Sciences, Chinese Academy of Sciences (CAS)[QYZDJ-SSW-SLH057, QYZDJ-SSWSYS008, ZDBS-LY-SLH011] ; Leverhulme Trust Early Career Research Fellowship ; Max-Planck-Gesellschaft (MPG) ; Max Planck Partner Group of the MPG ; CAS ; MEXT/JSPS KAKENHI[18KK0090, JP21H01137, JP18H03721, 18K03709, 18H01245, 25120007] ; Malaysian Fundamental Research Grant Scheme (FRGS)[FRGS/1/2019/STG02/UM/02/6] ; MIT International Science and Technology Initiatives (MISTI) Funds ; Ministry of Education (MoE) of Taiwan Yushan Young Scholar Program ; Physics Division, National Center for Theoretical Sciences of Taiwan ; National Aeronautics and Space Administration (NASA)[80NSSC20K1567, 80NSSC20K0527, 80NSSC20K0645] ; National Institute of Natural Sciences (NINS) of Japan ; National Key Research and Development Program of China[2016YFA0400704, 2016YFA0400702] ; National Science Foundation (NSF)[AST-0096454, AST-0352953, AST-0521233, AST-0705062, AST-0905844, AST-0922984, AST-1126433, AST-1140030, DGE-1144085, AST-1207704, AST-1207730, AST-1207752, MRI-1228509, OPP-1248097, AST-1310896, AST-1555365, AST-1615796, AST-1715061, AST-1716327, AST-1903847, AST-2034306, OPP-1852617] ; Natural Science Foundation of China[11650110427, 10625314, 11721303, 11725312, 11933007, 11991052, 11991053] ; NWO[OCENW.KLEIN.113] ; China Postdoctoral Science Foundation[2020M671266] ; Natural Sciences and Engineering Research Council of Canada (NSERC) ; National Youth Thousand Talents Program of China ; National Research Foundation of Korea[NRF-2015H1A2A1033752, 2015R1D1A1A01056807, NRF-2015H1D3A1066561, 2019R1F1A1059721] ; Netherlands Organization for Scientific Research (NWO) VICI award[639.043.513] ; Spinoza Prize[SPI 78-409] ; New Scientific Frontiers with Precision Radio Interferometry Fellowship - South African Radio Astronomy Observatory (SARAO) ; Swedish Research Council[2017-00648] ; Perimeter Institute for Theoretical Physics (Government of Canada through the Department of Innovation, Science and Economic Development) ; Perimeter Institute for Theoretical Physics (Province of Ontario through the Ministry of Research, Innovation and Science) ; Spanish Ministerio de Ciencia e Innovacin[PGC2018-098915-B-C21, AYA2016-80889P, PID2019-108995GB-C21, PID2020-117404GB-C21] ; State Agency for Research of the Spanish MCIU through the Center of Excellence Severo Ochoa award[SEV-2017-0709] ; Toray Science Foundation ; Consejera de Economa, Conocimiento, Empresas y Universidad of the Junta de Andaluca[P18-FR1769] ; Consejo Superior de Investigaciones Cientficas[2019AEP112] ; M2FINDERS project - European Research Council (ERC) under the European Unions Horizon 2020 Research and Innovation Programme[101018682] ; US Department of Energy (USDOE) through the Los Alamos National Laboratory[89233218CNA000001] ; European Unions Horizon 2020 research and innovation program[730562 RadioNet] ; Shanghai Pilot Program for Basic Research, Chinese Academy of Science, Shanghai Branch[JCYJ-SHFY-2021-013] ; ALMA North America Development Fund ; Academia Sinica ; Chandra[DD7-18089X, TM617006X] ; GenT Program (Generalitat Valenciana)[CIDEGENT/2018/021] ; NSF[ACI-1548562, DBI-0735191, DBI-1265383, DBI-1743442] ; CyVerse ; Compute Ontario ; Calcul Quebec ; Compute Canada ; Swedish Research Council (VR) ; Virtual Institute of Accretion (VIA) postdoctoral fellowships from the Netherlands Research School for Astronomy (NOVA) ; Smithsonian Institution ; Ministry of Finance of China ; National Key R&D Program of China[2017YFA0402700] ; Science and Technologies Facility Council (UK) ; National Research Foundation of Korea (NRF) - Ministry of Education[NRF-2021R1A6A3A01086420] ; Ministry of Finance in China ; CNRS (Centre National de la Recherche Scientifique, France) ; MPG (MaxPlanck-Gesellschaft, Germany) ; IGN (Instituto Geogrfico Nacional, Spain) ; State of Arizona ; NSF ; Kavli Institute of Cosmological Physics at the University of Chicago ; NASA - Space Telescope Science Institute[NAS5-26555, HST-HF2-51494.001] ; Ministry of Science and Technology (MOST) of Taiwan[103-2119-M001-010-MY2, 105-2112-M-001-025-MY3, 105-2119-M-001042, 106-2112-M-001-011, 106-2119-M-001-013, 106-2119-M001-027, 106-2923-M-001-005, 107-2119-M-001-017, 1072119-M-001-020, 107-2119-M-001-041, 107-2119-M-110-005] ; The Ministry of Science and Technology (MOST) of Taiwan[107-2923-M-001-009, 108-2112-M-001-048, 108-2112-M-001051, 108-2923-M-001-002, 109-2112-M-001-025, 109-2124-M001-005, 109-2923-M-001-001, 110-2112-M-003-007-MY2, 110-2112-M-001-033, 110-2124-M-001-007, 110-2923-M001-001] ; International Max Planck Research School for Astronomy and Astrophysics at the University of Cologne ; Chinese Academy of Sciences
Language英语
Subject Area天文学 ; 射电天文学 ; 星系与宇宙学
MOST Discipline Catalogue理学 ; 理学::天文学
SubtypeArticle
PublisherIOP Publishing Ltd
Publication PlaceTEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
ISSN2041-8205
URL查看原文
WOS IDWOS:000794024000001
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS KeywordSCALE STRUCTURE ; HORIZON ; M87 ; SHADOW ; ALGORITHM ; MASS
Citation statistics
Document Type期刊论文
Version出版稿
Identifierhttp://ir.ynao.ac.cn/handle/114a53/25181
Collection星系类星体研究组
中国科学院天体结构与演化重点实验室
Corresponding AuthorFarah, Joseph
Affiliation1.Las Cumbres Observatory, 6740 Cortona Drive, Suite 102, Goleta, CA 93117-5575, USA; josephfarah@ucsb.edu;
2.Department of Physics, University of California, Santa Barbara, CA 93106-9530, USA;
3.Black Hole Initiative at Harvard University, 20 Garden Street, Cambridge, MA 02138, USA;
4.Department of History of Science, Harvard University, Cambridge, MA 02138, USA;
5.Department of Physics, Harvard University, Cambridge, MA 02138, USA;
6.Massachusetts Institute of Technology Haystack Observatory, 99 Millstone Road, Westford, MA 01886, USA;
7.National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan;
8.Center for Astrophysics ∣ Harvard & Smithsonian, 60 Garden Street, Cambridge, MA 02138, USA;
9.California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125, USA;
10.Institute of Astronomy and Astrophysics, Academia Sinica, 645 N. A'ohoku Place, Hilo, HI 96720, USA;
11.Princeton Center for Theoretical Science, Jadwin Hall, Princeton University, Princeton, NJ 08544, USA;
12.NASA Hubble Fellowship Program, Einstein Fellow;
13.Instituto de Astrofísica de Andalucía-CSIC, Glorieta de la Astronomía s/n, E-18008 Granada, Spain;
14.Instituto de Astrofísica de Andalucía-CíSIC, Glorieta de la Astronomía s/n, E-18008 Granada, Spain;
15.Mizusawa VLBI Observatory, National Astronomical Observatory of Japan, 2-12 Hoshigaoka, Mizusawa, Oshu, Iwate 023-0861, Japan;
16.Department of Astronomical Science, The Graduate University for Advanced Studies (SOKENDAI), 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan;
17.Department of Astronomy, Graduate School of Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan;
18.Steward Observatory and Department of Astronomy, University of Arizona, 933 N. Cherry Ave., Tucson, AZ 85721, USA;
19.Department of Physics and Astronomy, University of Waterloo, 200 University Avenue W, Waterloo, ON N2L 3G1, Canada;
20.Waterloo Centre for Astrophysics, University of Waterloo, Waterloo, ON N2L 3G1, Canada;
21.Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany;
22.Department of Physics, Faculty of Science, University of Malaya, 50603 Kuala Lumpur, Malaysia;
23.Institute of Astronomy and Astrophysics, Academia Sinica, 11F of Astronomy-Mathematics Building, AS/NTU No. 1, Sec. 4, Roosevelt Rd., Taipei 10617, Taiwan, R.O.C.;
24.Departament d'Astronomia i Astrofísica, Universitat de València, C. Dr. Moliner 50, E-46100 Burjassot, València, Spain;
25.Observatori Astronòmic, Universitat de València, C. Catedrático José Beltrán 2, E-46980 Paterna, València, Spain;
26.Fermi National Accelerator Laboratory, MS209, P.O. Box 500, Batavia, IL 60510, USA;
27.Department of Astronomy and Astrophysics, University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637, USA;
28.East Asian Observatory, 660 N. A'ohoku Place, Hilo, HI 96720, USA;
29.Nederlandse Onderzoekschool voor Astronomie (NOVA), PO Box 9513, 2300 RA Leiden, The Netherlands;
30.Department of Physics, McGill University, 3600 rue University, Montréal, QC H3A 2T8, Canada;
31.McGill Space Institute, McGill University, 3550 rue University, Montréal, QC H3A 2A7, Canada;
32.Institut de Radioastronomie Millimétrique, 300 rue de la Piscine, F-38406 Saint Martin d'Hères, France;
33.Department of Astrophysics, Institute for Mathematics, Astrophysics and Particle Physics (IMAPP), Radboud University, P.O. Box 9010, 6500 GL Nijmegen, The Netherlands;
34.Perimeter Institute for Theoretical Physics, 31 Caroline Street N, Waterloo, ON N2L 2Y5, Canada;
35.Department of Astronomy, University of Massachusetts, Amherst, Amherst, MA 01003, USA;
36.Korea Astronomy and Space Science Institute, Daedeok-daero 776, Yuseong-gu, Daejeon 34055, Republic of Korea;
37.University of Science and Technology, Gajeong-ro 217, Yuseong-gu, Daejeon 34113, Republic of Korea;
38.Kavli Institute for Cosmological Physics, University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637, USA;
39.Department of Physics, University of Chicago, 5720 South Ellis Avenue, Chicago, IL 60637, USA;
40.Enrico Fermi Institute, University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637, USA;
41.Data Science Institute, University of Arizona, 1230 N. Cherry Ave., Tucson, AZ 85721, USA;
42.Anton Pannekoek Institute for Astronomy, University of Amsterdam, Science Park 904, 1098 XH, Amsterdam, The Netherlands;
43.Cornell Center for Astrophysics and Planetary Science, Cornell University, Ithaca, NY 14853, USA;
44.Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai 200030, People's Republic of China;
45.Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, Nanjing 210008, People's Republic of China;
46.Physics Department, Fairfield University, 1073 North Benson Road, Fairfield, CT 06824, USA;
47.Department of Space, Earth and Environment, Chalmers University of Technology, Onsala Space Observatory, SE-43992 Onsala, Sweden;
48.Institut für Theoretische Physik, Goethe-Universität Frankfurt, Max-von-Laue-Straße 1, D-60438 Frankfurt am Main, Germany;
49.Department of Astronomy and Columbia Astrophysics Laboratory, Columbia University, 550 W. 120th Street, New York, NY 10027, USA;
50.Center for Computational Astrophysics, Flatiron Institute, 162 Fifth Avenue, New York, NY 10010, USA;
51.Dipartimento di Fisica
52.INFN Sez. di Napoli, Compl. Univ. di Monte S. Angelo, Edificio G, Via Cinthia, I-80126, Napoli, Italy;
53.Wits Centre for Astrophysics, University of the Witwatersrand, 1 Jan Smuts Avenue, Braamfontein, Johannesburg 2050, South Africa;
54.Department of Physics, University of Pretoria, Hatfield, Pretoria 0028, South Africa;
55.Centre for Radio Astronomy Techniques and Technologies, Department of Physics and Electronics, Rhodes University, Makhanda 6140, South Africa;
56.LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de Paris, 5 place Jules Janssen, F-92195 Meudon, France;
57.National Astronomical Observatories, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing 100101, People's Republic of China;
58.National Radio Astronomy Observatory, 520 Edgemont Rd., Charlottesville, VA 22903, USA;
59.Department of Physics, University of Illinois, 1110 West Green Street, Urbana, IL 61801, USA;
60.Department of Astronomy, University of Illinois at Urbana-Champaign, 1002 West Green Street, Urbana, IL 61801, USA;
61.INAF—Osservatorio Astronomico di Cagliari, Via della Scienza 5, I-09047, Selargius, CA, Italy;
62.CP3-Origins, University of Southern Denmark, Campusvej 55, DK-5230 Odense M, Denmark;
63.Instituto Nacional de Astrofísica, Óptica y Electrónica. Apartado Postal 51 y 216, 72000. Puebla Pue., México;
64.Consejo Nacional de Ciencia y Tecnologìa, Av. Insurgentes Sur 1582, 03940, Ciudad de México, México;
65.Key Laboratory for Research in Galaxies and Cosmology, Chinese Academy of Sciences, Shanghai 200030, People's Republic of China;
66.NOVA Sub-mm Instrumentation Group, Kapteyn Astronomical Institute, University of Groningen, Landleven 12, 9747 AD Groningen, The Netherlands;
67.Department of Astronomy, School of Physics, Peking University, Beijing 100871, People's Republic of China;
68.Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing 100871, People's Republic of China;
69.The Institute of Statistical Mathematics, 10-3 Midori-cho, Tachikawa, Tokyo 190-8562, Japan;
70.Department of Statistical Science, The Graduate University for Advanced Studies (SOKENDAI), 10-3 Midori-cho, Tachikawa, Tokyo 190-8562, Japan;
71.Kavli Institute for the Physics and Mathematics of the Universe, The University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa 277-8583, Japan;
72.Institute for Astrophysical Research, Boston University, 725 Commonwealth Ave., Boston, MA 02215, USA;
73.Institute for Cosmic Ray Research, The University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa, Chiba 277-8582, Japan;
74.Joint Institute for VLBI ERIC (JIVE), Oude Hoogeveensedijk 4, 7991 PD Dwingeloo, The Netherlands;
75.Kogakuin University of Technology & Engineering, Academic Support Center, 2665-1 Nakano, Hachioji, Tokyo 192-0015, Japan;
76.Physics Department, National Sun Yat-Sen University, No. 70, Lien-Hai Road, Kaosiung City 80424, Taiwan, R.O.C.;
77.National Optical Astronomy Observatory, 950 N. Cherry Ave., Tucson, AZ 85719, USA;
78.Key Laboratory for Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, 19B Yuquan Road, Shijingshan District, Beijing, People's Republic of China;
79.School of Astronomy and Space Science, Nanjing University, Nanjing 210023, People's Republic of China;
80.Key Laboratory of Modern Astronomy and Astrophysics, Nanjing University, Nanjing 210023, People's Republic of China;
81.Italian ALMA Regional Centre, INAF-Istituto di Radioastronomia, Via P. Gobetti 101, I-40129 Bologna, Italy;
82.Department of Physics, National Taiwan University, No.1, Sect.4, Roosevelt Rd., Taipei 10617, Taiwan, R.O.C;
83.Instituto de Radioastronomía y Astrofísica, Universidad Nacional Autónoma de México, Morelia 58089, México;
84.Instituto de Astronomía, Universidad Nacional Autónoma de México, CdMx 04510, México;
85.Yunnan Observatories, Chinese Academy of Sciences, 650011 Kunming, Yunnan Province, People's Republic of China;
86.Center for Astronomical Mega-Science, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing, 100012, People's Republic of China;
87.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, 650011 Kunming, People's Republic of China;
88.Gravitation Astroparticle Physics Amsterdam (GRAPPA) Institute, University of Amsterdam, Science Park 904, 1098 XH Amsterdam, The Netherlands;
89.School of Natural Sciences, Institute for Advanced Study, 1 Einstein Drive, Princeton, NJ 08540, USA;
90.Tsung-Dao Lee Institute and School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai, 200240, People's Republic of China;
91.Astronomy Department, Universidad de Concepción, Casilla 160-C, Concepción, Chile;
92.National Institute of Technology, Hachinohe College, 16-1 Uwanotai, Tamonoki, Hachinohe City, Aomori 039-1192, Japan;
93.South African Radio Astronomy Observatory, Observatory 7925, Cape Town, South Africa;
94.Villanova University, Mendel Science Center Rm. 263B, 800 E. Lancaster Ave., Villanova PA 19085;
95.Physics Department, Washington University CB 1105, St. Louis, MO 63130, USA;
96.Canadian Institute for Theoretical Astrophysics, University of Toronto, 60 St. George Street, Toronto, ON M5S 3H8, Canada;
97.Dunlap Institute for Astronomy and Astrophysics, University of Toronto, 50 St. George Street, Toronto, ON M5S 3H4, Canada;
98.Canadian Institute for Advanced Research, 180 Dundas St. W, Toronto, ON M5G 1Z8, Canada;
99.Radio Astronomy Laboratory, University of California, Berkeley, CA 94720, USA;
100.Department of Physics, National Taiwan Normal University, No. 88, Sec. 4, Tingzhou Rd., Taipei 116, Taiwan, R.O.C.;
101.Frankfurt Institute for Advanced Studies, Ruth-Moufang-Strasse 1, D-60438 Frankfurt, Germany;
102.School of Mathematics, Trinity College, Dublin 2, Ireland;
103.Department of Astrophysical Sciences, Peyton Hall, Princeton University, Princeton, NJ 08544, USA;
104.Instituto de Radioastronomía Milimétrica, IRAM, Avenida Divina Pastora 7, Local 20, E-18012, Granada, Spain;
105.Consejo Nacional de Ciencia y Tecnología, Av. Insurgentes Sur 1582, 03940, Ciudad de México, México;
106.Hiroshima Astrophysical Science Center, Hiroshima University, 1-3-1 Kagamiyama, Higashi-Hiroshima, Hiroshima 739-8526, Japan;
107.Aalto University Department of Electronics and Nanoengineering, PL 15500, FI-00076 Aalto, Finland;
108.Aalto University Metsähovi Radio Observatory, Metsähovintie 114, FI-02540 Kylmälä, Finland;
109.Department of Astronomy, Yonsei University, Yonsei-ro 50, Seodaemun-gu, 03722 Seoul, Republic of Korea;
110.Leiden Observatory—Allegro, Leiden University, P.O. Box 9513, 2300 RA Leiden, The Netherlands;
111.Netherlands Organisation for Scientific Research (NWO), Postbus 93138, 2509 AC Den Haag, The Netherlands;
112.Frontier Research Institute for Interdisciplinary Sciences, Tohoku University, Sendai 980-8578, Japan;
113.Astronomical Institute, Tohoku University, Sendai 980-8578, Japan;
114.Department of Physics and Astronomy, Seoul National University, Gwanak-gu, Seoul 08826, Republic of Korea;
115.Leiden Observatory, Leiden University, Postbus 2300, 9513 RA Leiden, The Netherlands;
116.Jeremiah Horrocks Institute, University of Central Lancashire, Preston PR1 2HE, UK;
117.Physics Department, Brandeis University, 415 South Street, Waltham, MA 02453, USA;
118.Tuorla Observatory, Department of Physics and Astronomy, University of Turku, Finland;
119.School of Physics, Huazhong University of Science and Technology, Wuhan, Hubei, 430074, People's Republic of China;
120.Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey, RH5 6NT, UK;
121.School of Astronomy and Space Sciences, University of Chinese Academy of Sciences, No. 19A Yuquan Road, Beijing 100049, People's Republic of China;
122.Astronomy Department, University of Science and Technology of China, Hefei 230026, People's Republic of China
Recommended Citation
GB/T 7714
Farah, Joseph,Galison, Peter,Akiyama, Kazunori,et al. Selective Dynamical Imaging of Interferometric Data[J]. ASTROPHYSICAL JOURNAL LETTERS,2022,930(2).
APA Farah, Joseph.,Galison, Peter.,Akiyama, Kazunori.,Bouman, Katherine L..,Bower, Geoffrey C..,...&Zhao, Shan-Shan.(2022).Selective Dynamical Imaging of Interferometric Data.ASTROPHYSICAL JOURNAL LETTERS,930(2).
MLA Farah, Joseph,et al."Selective Dynamical Imaging of Interferometric Data".ASTROPHYSICAL JOURNAL LETTERS 930.2(2022).
Files in This Item:
File Name/Size DocType Version Access License
Selective Dynamical (12138KB)期刊论文出版稿开放获取CC BY-NC-SAView Application Full Text
Related Services
Recommend this item
Bookmark
Usage statistics
Export to Endnote
Google Scholar
Similar articles in Google Scholar
[Farah, Joseph]'s Articles
[Galison, Peter]'s Articles
[Akiyama, Kazunori]'s Articles
Baidu academic
Similar articles in Baidu academic
[Farah, Joseph]'s Articles
[Galison, Peter]'s Articles
[Akiyama, Kazunori]'s Articles
Bing Scholar
Similar articles in Bing Scholar
[Farah, Joseph]'s Articles
[Galison, Peter]'s Articles
[Akiyama, Kazunori]'s Articles
Terms of Use
No data!
Social Bookmark/Share
File name: Selective Dynamical Imaging of Interferometric Data.pdf
Format: Adobe PDF
All comments (0)
No comment.
 

Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.