YNAO OpenIR  > 丽江天文观测站(南方基地)
SYMBA: An end-to-end VLBI synthetic data generation pipeline Simulating Event Horizon Telescope observations of M 87
Roelofs, F.1; Janssen, M.1; Natarajan, I2; Deane, R.2,3; Davelaar, J.1; Olivares, H.1; Porth, O.4,5; Paine, S. N.6; Bouman, K. L.6,7,8; Tilanus, R. P. J.1,9,10; van Bemmel, I. M.11; Falcke, H.1; Akiyama, K.7,12,13,14; Alberdi, A.15; Alef, W.16; Asada, K.17; Azulay, R.16,18,19; Baczko, A.16; Ball, D.20,21; Balokovic, M.6,7; Barrett, J.13; Bintley, D.22; Blackburn, L.6,7; Boland, W.23; Bower, G. C.24; Bremer, M.25; Brinkerink, C. D.1; Brissenden, R.6,7; Britzen, S.16; Broderick, A. E.26,27,28; Broguiere, D.25; Bronzwaer, T.1; Byun, D.29,30; Carlstrom, J. E.31,32,33,34; Chael, A.35; Chan, C.20,21,36; Chatterjee, S.37; Chatterjee, K.5; Chen, M.24; Chen, Y.38,39; Cho, I29,30; Christian, P.6,20,21; Conway, J. E.40; Cordes, J. M.37; Crew, G. B.13; Cui, Y.41,42; De Laurentis, M.4,43,44; Dempsey, J.22; Desvignes, G.16,80; Dexter, J.45; Doeleman, S. S.6,7; Eatough, R. P.16; Fish, V. L.13; Fomalont, E.12; Fraga-Encinas, R.1; Friberg, P.22; Fromm, C. M.4; Gomez, J. L.15; Galison, P.7,45,46; Gammie, C. F.47,48; Garcia, R.25; Gentaz, O.25; Georgiev, B.27,28; Goddi, C.1,9; Gold, R.4,26,99; Gu, M.38,49; Gurwell, M.6; Hada, K.41,42; Hecht, M. H.13; Hesper, R.50; Ho, L. C.51,52; Ho, P.17; Honma, M.41,42; Huang, C. L.17; Huang, L.38,49; Hughes, D. H.53; Ikeda, S.14,54,55,56; Inoue, M.17; Issaoun, S.1; James, D. J.6,7; Jannuzi, B. T.20,21; Jeter, B.27,28; Jiang, W.38; Johnson, M. D.6,7; Jorstad, S.57,58; Jung, T.29,30; Karami, M.26,27; Karuppusamy, R.16; Kawashima, T.14; Keating, G. K.6; Kettenis, M.11; Kim, J.8,16,29; Kino, M.14,59; Koay, J. Y.17; Koch, P. M.17; Koyama, S.17; Kramer, M.16; Kramer, C.25; Krichbaum, T. P.16; Kuo, C.60; Lauer, T. R.61; Lee, S.29; Li, Y.62; Li, Z.63,64; Lindqvist, M.40; Lico, R.16; Liu, K.16; Liuzzo, E.65; Lo, W.17,66; Lobanov, A. P.16; Loinard, L.67,68; Lonsdale, C.13; Lu, R.16,38,39; MacDonald, N. R.16; Mao JR(毛基荣)69,70,71; Markoff, S.5,72; Marrone, D. P.20,21; Marscher, A. P.57; Marti-Vidal, I18; Matsushita, S.17; Matthews, L. D.13; Medeiros, L.20,21,100; Menten, K. M.16; Mizuno, Y.4; Mizuno, I22; Moran, J. M.6,7; Moriyama, K.13,41; Moscibrodzka, M.1; Mueller, C.1,16; Nagai, H.14,42; Nagar, N. M.73; Nakamura, M.17; Narayan, R.6,7; Narayanan, G.74; Neri, R.25; Ni, C.27,28; Noutsos, A.16; Okino, H.41,75; Ortiz-Leon, G. N.16; Oyama, T.41; Ozel, F.20,21; Palumbo, D. C. M.6,7; Patel, N.6; Pen, U.26,76,77,78; Pesce, D. W.6,7; Pietu, V25; Plambeck, R.79; PopStefanija, A.74; Prather, B.47; Preciado-Lopez, J. A.26; Psaltis, D.20,21; Pu, H.26; Ramakrishnan, V73; Rao, R.24; Rawlings, M. G.22; Raymond, A. W.6,7; Rezzolla, L.4; Ripperda, B.80,81; Rogers, A.13; Ros, E.16; Rose, M.20,21; Roshanineshat, A.20,21; Rottmann, H.16; Roy, A. L.16; Ruszczyk, C.13; Ryan, B. R.82,83; Rygl, K. L. J.65; Sanchez, S.84; Sanchez-Arguelles, D.54,85; Sasada, M.41,86; Savolainen, T.16,87,88; Schloerb, F. P.74; Schuster, K.25; Shao, L.16,52; Shen, Z.38,39; Small, D.11; Sohn, B. Won29,30,89; SooHoo, J.13; Tazaki, F.41; Tiede, P.27,28; Titus, M.13; Toma, K.90,91; Torne, P.16,84; Traianou, E.16; Trent, T.20,21; Trippe, S.92; Tsuda, S.41; van Langevelde, H. J.11,93; van Rossum, D. R.1; Wagner, J.16; Wardle, J.94; Weintroub, J.6,7; Wex, N.16; Wharton, R.16; Wielgus, M.6,7; Wong, G. N.47,82; Wu, Q.95; Young, A.1; Young, K.6; Younsi, Z.4,96; Yuan, F.38,49,97; Yuan, Y.98; Zensus, J. A.16; Zhao, G.29; Zhao, S.1,63; Zhu, Z.46
Source PublicationASTRONOMY & ASTROPHYSICS
2020-04-03
Volume636Pages:19
DOI10.1051/0004-6361/201936622
Contribution Rank第69完成单位
Indexed BySCI
Keywordgalaxies nuclei black hole physics telescopes atmospheric effects techniques high angular resolution techniques interferometric
Abstract

Context. Realistic synthetic observations of theoretical source models are essential for our understanding of real observational data. In using synthetic data, one can verify the extent to which source parameters can be recovered and evaluate how various data corruption effects can be calibrated. These studies are the most important when proposing observations of new sources, in the characterization of the capabilities of new or upgraded instruments, and when verifying model-based theoretical predictions in a direct comparison with observational data. Aims. We present the SYnthetic Measurement creator for long Baseline Arrays (SYMBA), a novel synthetic data generation pipeline for Very Long Baseline Interferometry (VLBI) observations. SYMBA takes into account several realistic atmospheric, instrumental, and calibration effects. Methods. We used SYMBA to create synthetic observations for the Event Horizon Telescope (EHT), a millimetre VLBI array, which has recently captured the first image of a black hole shadow. After testing SYMBA with simple source and corruption models, we study the importance of including all corruption and calibration effects, compared to the addition of thermal noise only. Using synthetic data based on two example general relativistic magnetohydrodynamics (GRMHD) model images of M 87, we performed case studies to assess the image quality that can be obtained with the current and future EHT array for different weather conditions. Results. Our synthetic observations show that the effects of atmospheric and instrumental corruptions on the measured visibilities are significant. Despite these effects, we demonstrate how the overall structure of our GRMHD source models can be recovered robustly with the EHT2017 array after performing calibration steps, which include fringe fitting, a priori amplitude and network calibration, and self-calibration. With the planned addition of new stations to the EHT array in the coming years, images could be reconstructed with higher angular resolution and dynamic range. In our case study, these improvements allowed for a distinction between a thermal and a non-thermal GRMHD model based on salient features in reconstructed images.

Funding ProjectERC Synergy Grant BlackHoleCam: Imaging the Event Horizon of Black Holes[610058] ; New Scientific Frontiers with Precision Radio Interferometry Fellowship - South African Radio Astronomy Observatory (SARAO) ; Academy of Finland[274477] ; Academy of Finland[284495] ; Academy of Finland[312496] ; European Commission Framework Programme Horizon 2020 Research and Innovation action[731016] ; Black Hole Initiative at Harvard University from the John Templeton Foundation[60477] ; Comision Nacional de Investigacio Cientifica y Tecnologica (CONICYT, Chile)[PIA ACT172033] ; Comision Nacional de Investigacio Cientifica y Tecnologica (CONICYT, Chile)[Fondecyt 1171506] ; Comision Nacional de Investigacio Cientifica y Tecnologica (CONICYT, Chile)[BASAL AFB-170002] ; Comision Nacional de Investigacio Cientifica y Tecnologica (CONICYT, Chile)[ALMAconicyt 31140007] ; 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)[279006] ; Consejo Nacional de Ciencia y Tecnologia (CONACYT, Mexico)[281692] ; Direccion General de Asuntos del Personal Academico-Universidad Nacional Autonoma de Mexico (DGAPA-UNAM)[IN112417] ; Generalitat Valenciana postdoctoral grant[APOSTD/2018/177] ; Gordon and Betty Moore Foundation[GBMF-3561] ; Gordon and Betty Moore Foundation[GBMF-5278] ; GenT Program (Generalitat Valenciana)[CIDEGENT/2018/021] ; Jansky Fellowship program of the National Radio Astronomy Observatory (NRAO) ; 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-SSW-SYS008] ; Leverhulme Trust Early Career Research Fellowship ; MEXT/JSPS KAKENHI[18KK0090] ; MEXT/JSPS KAKENHI[JP18K13594] ; MEXT/JSPS KAKENHI[JP18K03656] ; MEXT/JSPS KAKENHI[JP18H03721] ; MEXT/JSPS KAKENHI[18K03709] ; MEXT/JSPS KAKENHI[18H01245] ; MEXT/JSPS KAKENHI[25120007] ; MIT International Science and Technology Initiatives (MISTI) Funds ; Ministry of Science and Technology (MOST) of Taiwan[105-2112-M-001-025-MY3] ; Ministry of Science and Technology (MOST) of Taiwan[106-2112-M-001-011] ; Ministry of Science and Technology (MOST) of Taiwan[106-2119-M-001027] ; Ministry of Science and Technology (MOST) of Taiwan[107-2119-M-001-017] ; Ministry of Science and Technology (MOST) of Taiwan[107-2119-M-001-020] ; Ministry of Science and Technology (MOST) of Taiwan[107-2119-M-110-005] ; National Aeronautics and Space Administration (NASA, Fermi Guest Investigator grant)[80NSSC17K0649] ; NASA through the NASA Hubble Fellowship grant - Space Telescope Science Institute[HST-HF2-51431.001-A] ; NASA[NAS5-26555] ; 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] ; Natural Science Foundation of China[11573051] ; Natural Science Foundation of China[11633006] ; 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 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[2015-R1D1A1A01056807] ; National Research Foundation of Korea[NRF-2015H1D3A1066561] ; Netherlands Organization for Scientific Research (NWO) VICI award[639.043.513] ; Spinoza Prize[SPI 78-409] ; Swedish Research Council[2017-00648] ; Government of Canada through the Department of Innovation, Science and Economic Development ; Province of Ontario through the Ministry of Research, Innovation and Science ; Princeton/Flatiron Postdoctoral Prize Fellowship ; Russian Science Foundation[17-12-01029] ; Spanish Ministerio de Economia y Competitividad[AYA2015-63939-C21-P] ; Spanish Ministerio de Economia y Competitividad[AYA2016-80889-P] ; State Agency for Research of the Spanish MCIU through the Center of Excellence Severo Ochoa award for the Instituto de Astrofisica de Andalucia[SEV-2017-0709] ; National Nuclear Security Administration of the USDOE[89233218CNA000001] ; Italian Ministero dell'Istruzione Universita e Ricerca through the grant Progetti Premiali 2012-iALMA[CUP C52I13000140001] ; European Union's Horizon 2020 research and innovation programme[730562] ; ALMA North America Development Fund ; Academia Sinica ; Chandra[TM6-17006X] ; NSF[ACI-1548562] ; NSF[DBI-0735191] ; NSF[DBI-1265383] ; NSF[DBI-1743442] ; Compute Ontario ; Calcul Quebec ; Compute Canada ; Smithsonian Institution ; National Key R&D Program of China[2017YFA0402700] ; Science and Technologies Facility Council (UK) ; CNRS (Centre National de la Recherche Scientifique, France) ; MPG (Max-Planck-Gesellschaft, Germany) ; IGN (Instituto Geografico Nacional, Spain) ; State of Arizona ; NSF Physics Frontier Center grant[PHY-1125897] ; Kavli Foundation ; [AST-1207704] ; [AST-1207730] ; [AST-1207752] ; [MRI-1228509] ; [OPP-1248097] ; [AST-1310896] ; [AST-1312651] ; [AST-1337663] ; [AST-1440254] ; [AST-1555365] ; [AST-1715061] ; [AST-1615796] ; [AST-1716327] ; [OISE-1743747] ; [AST-1816420]
Funding OrganizationERC Synergy Grant BlackHoleCam: Imaging the Event Horizon of Black Holes[610058] ; New Scientific Frontiers with Precision Radio Interferometry Fellowship - South African Radio Astronomy Observatory (SARAO) ; Academy of Finland[274477, 284495, 312496] ; European Commission Framework Programme Horizon 2020 Research and Innovation action[731016] ; Black Hole Initiative at Harvard University from the John Templeton Foundation[60477] ; Comision Nacional de Investigacio Cientifica y Tecnologica (CONICYT, Chile)[PIA ACT172033, Fondecyt 1171506, BASAL AFB-170002, ALMAconicyt 31140007] ; Consejo Nacional de Ciencia y Tecnologia (CONACYT, Mexico)[104497, 275201, 279006, 281692] ; Direccion General de Asuntos del Personal Academico-Universidad Nacional Autonoma de Mexico (DGAPA-UNAM)[IN112417] ; Generalitat Valenciana postdoctoral grant[APOSTD/2018/177] ; Gordon and Betty Moore Foundation[GBMF-3561, GBMF-5278] ; GenT Program (Generalitat Valenciana)[CIDEGENT/2018/021] ; Jansky Fellowship program of the National Radio Astronomy Observatory (NRAO) ; 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-SSW-SYS008] ; Leverhulme Trust Early Career Research Fellowship ; MEXT/JSPS KAKENHI[18KK0090, JP18K13594, JP18K03656, JP18H03721, 18K03709, 25120007] ; MIT International Science and Technology Initiatives (MISTI) Funds ; Ministry of Science and Technology (MOST) of Taiwan[105-2112-M-001-025-MY3, 106-2112-M-001-011, 106-2119-M-001027, 107-2119-M-001-017, 107-2119-M-001-020, 107-2119-M-110-005] ; National Aeronautics and Space Administration (NASA, Fermi Guest Investigator grant)[80NSSC17K0649] ; NASA through the NASA Hubble Fellowship grant - Space Telescope Science Institute[HST-HF2-51431.001-A] ; NASA[NAS5-26555] ; 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] ; Natural Science Foundation of China[11573051, 11633006, 11650110427, 10625314, 11721303, 11725312, 11933007] ; Natural Sciences and Engineering Research Council of Canada (NSERC) ; National Youth Thousand Talents Program of China ; National Research Foundation of Korea[NRF-2015H1A2A1033752, 2015-R1D1A1A01056807, NRF-2015H1D3A1066561] ; Netherlands Organization for Scientific Research (NWO) VICI award[639.043.513] ; Spinoza Prize[SPI 78-409] ; Swedish Research Council[2017-00648] ; Government of Canada through the Department of Innovation, Science and Economic Development ; Province of Ontario through the Ministry of Research, Innovation and Science ; Princeton/Flatiron Postdoctoral Prize Fellowship ; Russian Science Foundation[17-12-01029] ; Spanish Ministerio de Economia y Competitividad[AYA2015-63939-C21-P, AYA2016-80889-P] ; State Agency for Research of the Spanish MCIU through the Center of Excellence Severo Ochoa award for the Instituto de Astrofisica de Andalucia[SEV-2017-0709] ; National Nuclear Security Administration of the USDOE[89233218CNA000001] ; Italian Ministero dell'Istruzione Universita e Ricerca through the grant Progetti Premiali 2012-iALMA[CUP C52I13000140001] ; European Union's Horizon 2020 research and innovation programme[730562] ; ALMA North America Development Fund ; Academia Sinica ; Chandra[TM6-17006X] ; NSF[ACI-1548562, DBI-0735191, DBI-1265383, DBI-1743442] ; Compute Ontario ; Calcul Quebec ; Compute Canada ; Smithsonian Institution ; National Key R&D Program of China[2017YFA0402700] ; Science and Technologies Facility Council (UK) ; CNRS (Centre National de la Recherche Scientifique, France) ; MPG (Max-Planck-Gesellschaft, Germany) ; IGN (Instituto Geografico Nacional, Spain) ; State of Arizona ; NSF Physics Frontier Center grant[PHY-1125897] ; Kavli Foundation ; [AST-1207704] ; [AST-1207730] ; [AST-1207752] ; [MRI-1228509] ; [OPP-1248097] ; [AST-1310896] ; [AST-1312651] ; [AST-1337663] ; [AST-1440254] ; [AST-1555365] ; [AST-1715061] ; [AST-1615796] ; [AST-1716327] ; [OISE-1743747] ; [AST-1816420]
Language英语
Subject Area天文学 ; 天体物理学 ; 实测天体物理学 ; 射电天文学 ; 星系与宇宙学
MOST Discipline Catalogue理学 ; 理学::天文学
SubtypeArticle
PublisherEDP SCIENCES S A
Publication PlaceAVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE
ISSN0004-6361
URL查看原文
WOS IDWOS:000524552600002
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS KeywordSGR A-ASTERISK ; BLACK-HOLE ; RADIO ; JET ; DISTRIBUTIONS ; CALIBRATION ; MODELS ; INTERFEROMETER ; FIELD ; M87
Citation statistics
Document Type期刊论文
Identifierhttp://ir.ynao.ac.cn/handle/114a53/23045
Collection丽江天文观测站(南方基地)
中国科学院天体结构与演化重点实验室
Corresponding AuthorRoelofs, F.
Affiliation1.Radboud Univ Nijmegen, Dept Astrophys, IMAPP, POB 9010, NL-6500 GL Nijmegen, Netherlands
2.Rhodes Univ, Ctr Radio Astron Tech & Technol, Dept Phys & Elect, ZA-6140 Grahamstown, South Africa
3.Univ Pretoria, Dept Phys, Lynnwood Rd, ZA-0083 Pretoria, South Africa
4.Goethe Univ Frankfurt, Inst Theoret Phys, Max Von Laue Str 1, D-60438 Frankfurt, Germany
5.Univ Amsterdam, Anton Pannekoek Inst Astron, Sci Pk 904, NL-1098 XH Amsterdam, Netherlands
6.Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
7.Harvard Univ, Black Hole Initiat, 20 Garden St, Cambridge, MA 02138 USA
8.CALTECH, 1200 East Calif Blvd, Pasadena, CA 91125 USA
9.Leiden Univ, Leiden Observ Allegro, POB 9513, NL-2300 RA Leiden, Netherlands
10.Netherlands Org Sci Res NWO, Postbus 93138, NL-2509 AC The Hague, Netherlands
11.JIVE, Oude Hoogeveensedijk 4, NL-7991 PD Dwingeloo, Netherlands
12.Natl Radio Astron Observ, 520 Edgemt Rd, Charlottesville, VA 22903 USA
13.MIT, Haystack Observ, 99 Millstone Rd, Westford, MA 01886 USA
14.Natl Astron Observ Japan, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan
15.CSIC, Inst Astrofis Andalucia, Glorieta Astron S-N, E-18008 Granada, Spain
16.Max Planck Inst Radioastron, Auf Hugel 69, D-53121 Bonn, Germany
17.Acad Sinica, Inst Astron & Astrophys, 11F,Astron Math Bldg,AS NTU 1,Sec 4,Roosevelt Rd, Taipei 10617, Taiwan
18.Univ Valencia, Dept Astron & Astrofis, C Dr Moliner 50, E-46100 Valencia, Spain
19.Univ Valencia, Observ Astron, C Catedrat Jose Beltran 2, Valencia 46980, Spain
20.Univ Arizona, Steward Observ, 933 N Cherry Ave, Tucson, AZ 85721 USA
21.Univ Arizona, Dept Astron, 933 N Cherry Ave, Tucson, AZ 85721 USA
22.East Asian Observ, 660 N Aohoku Pl, Hilo, HI 96720 USA
23.NOVA, POB 9513, NL-2300 RA Leiden, Netherlands
24.Acad Sinica, Inst Astron & Astrophys, 645 N Aohoku Pl, Hilo, HI 96720 USA
25.Inst Radioastron Millimetr, 300 Rue Piscine, F-38406 St Martin Dheres, France
26.Perimeter Inst Theoret Phys, 31 Caroline St North, Waterloo, ON N2L 2Y5, Canada
27.Univ Waterloo, Dept Phys & Astron, 200 Univ Ave West, Waterloo, ON N2L 3G1, Canada
28.Univ Waterloo, Waterloo Ctr Astrophys, Waterloo, ON N2L 3G1, Canada
29.Korea Astron & Space Sci Inst, Daedeok Daero 776, Daejeon 34055, South Korea
30.Univ Sci & Technol, Gajeong Ro 217, Daejeon 34113, South Korea
31.Univ Chicago, Kavli Inst Cosmol Phys, 5640 South Ellis Ave, Chicago, IL 60637 USA
32.Univ Chicago, Dept Astron & Astrophys, 5640 South Ellis Ave, Chicago, IL 60637 USA
33.Univ Chicago, Dept Phys, 5640 South Ellis Ave, Chicago, IL 60637 USA
34.Univ Chicago, Enrico Fermi Inst, 5640 South Ellis Ave, Chicago, IL 60637 USA
35.Princeton Univ, Princeton Ctr Theoret Sci, Jadwin Hall, Princeton, NJ 08544 USA
36.Univ Arizona, Data Sci Inst, 1230 N Cherry Ave, Tucson, AZ 85721 USA
37.Cornell Univ, Cornell Ctr Astrophys & Planetary Sci, Ithaca, NY 14853 USA
38.Chinese Acad Sci, Shanghai Astron Observ, 80 Nandan Rd, Shanghai 200030, Peoples R China
39.Chinese Acad Sci, Key Lab Radio Astron, Nanjing 210008, Peoples R China
40.Chalmers Univ Technol, Dept Space Earth & Environm, Onsala Space Observ, S-43992 Onsala, Sweden
41.Natl Astron Observ Japan, Mizusawa VLBI Observ, 2-12 Hoshigaoka, Mizusawa, Iwate 0230861, Japan
42.Grad Univ Adv Studies SOKENDAI, Dept Astron Sci, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan
43.Univ Napoli Federico II, Compl Univ Monte S Angelo, Dipartimento Fis E Pancini, Edificio G,Via Cinthia, I-80126 Naples, Italy
44.Compl Univ Monte S Angelo, Sez Napoli, Ist Nazl Fis Nucl, Edificio G,Via Cinthia, I-80126 Naples, Italy
45.Harvard Univ, Dept Hist Sci, Cambridge, MA 02138 USA
46.Harvard Univ, Dept Phys, Cambridge, MA 02138 USA
47.Univ Illinois, Dept Phys, 1110 West Green St, Urbana, IL 61801 USA
48.Univ Illinois, Dept Astron, 1002 West Green St, Urbana, IL 61801 USA
49.Chinese Acad Sci, Key Lab Res Galaxies & Cosmol, Shanghai 200030, Peoples R China
50.Univ Groningen, Kapteyn Astron Inst, NOVA Sub Mm Instrumentat Grp, Landleven 12, NL-9747 AD Groningen, Netherlands
51.Peking Univ, Sch Phys, Dept Astron, Beijing 100871, Peoples R China
52.Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China
53.Inst Nacl Astrofis Opt & Electr, Apartado Postal 51 & 216, Puebla Pue 72000, Mexico
54.Inst Stat Math, 10-3 Midori Cho, Tachikawa, Tokyo 1908562, Japan
55.Grad Univ Adv Studies SOKENDAI, Dept Stat Sci, 10-3 Midori Cho, Tachikawa, Tokyo 1908562, Japan
56.Univ Tokyo, Kavli Inst Phys & Math Universe, 5-1-5 Kashiwanoha, Kashiwa, Chiba 2778583, Japan
57.Boston Univ, Inst Astrophys Res, 725 Commonwealth Ave, Boston, MA 02215 USA
58.St Petersburg Univ, Astron Inst, Univ Skij Pr 28, St Petersburg 198504, Russia
59.Kogakuin Univ Technol & Engn, Acad Support Ctr, 2665-1 Nakano, Hachioji, Tokyo 1920015, Japan
60.Natl Sun Yat Sen Univ, Phys Dept, 70 Lien Hai Rd, Kaohsiung 80424, Taiwan
61.Natl Opt Astron Observ, 950 North Cherry Ave, Tucson, AZ 85719 USA
62.Chinese Acad Sci, Inst High Energy Phys, Key Lab Particle Astrophys, 19B Yuquan Rd, Beijing, Peoples R China
63.Nanjing Univ, Sch Astron & Space Sci, Nanjing 210023, Peoples R China
64.Nanjing Univ, Key Lab Modern Astron & Astrophys, Nanjing 210023, Peoples R China
65.Italian ALMA Reg Ctr, INAF Ist Radioastron, Via P Gobetti 101, I-40129 Bologna, Italy
66.Natl Taiwan Univ, Dept Phys, 1,Sect 4,Roosevelt Rd, Taipei 10617, Taiwan
67.Univ Nacl Autonoma Mexico, Inst Radioastron & Astrofis, Morelia 58089, Michoacan, Mexico
68.Univ Nacl Autonoma Mexico, Inst Astron, Ciudad De Mexico 04510, Mexico
69.Chinese Acad Sci, Yunnan Observ, Kunming 650011, Yunnan, Peoples R China
70.Chinese Acad Sci, Ctr Astron Megasci, 20A Datun Rd, Beijing 100012, Peoples R China
71.Chinese Acad Sci, Key Lab Struct & Evolut Celestial Objects, Kunming 650011, Yunnan, Peoples R China
72.Univ Amsterdam, Gravitat Astroparticle Phys Amsterdam GRAPPA Inst, Sci Pk 904, NL-1098 XH Amsterdam, Netherlands
73.Univ Concepcion, Astron Dept, Casilla 160-C, Concepcion, Chile
74.Univ Massachusetts, Dept Astron, Amherst, MA 01003 USA
75.Univ Tokyo, Grad Sch Sci, Dept Astron, Bunkyo Ku, 7-3-1 Hongo, Tokyo 1130033, Japan
76.Univ Toronto, Canadian Inst Theoret Astrophys, 60 St George St, Toronto, ON M5S 3H8, Canada
77.Univ Toronto, Dunlap Inst Astron & Astrophys, 50 St George St, Toronto, ON M5S 3H4, Canada
78.Canadian Inst Adv Res, 180 Dundas St West, Toronto, ON M5G 1Z8, Canada
79.Univ Calif Berkeley, Radio Astron Lab, Berkeley, CA 94720 USA
80.Princeton Univ, Dept Astrophys Sci, Peyton Hall, Princeton, NJ 08544 USA
81.Flatiron Inst, Ctr Computat Astrophys, 162 Fifth Ave, New York, NY 10010 USA
82.Los Alamos Natl Lab, CCS 2,POB 1663, Los Alamos, NM 87545 USA
83.Los Alamos Natl Lab, Ctr Theoret Astrophys, Los Alamos, NM 87545 USA
84.IRAM, Inst Radioastron Milimetr, Ave Divina Pastora 7,Local 20, E-18012 Granada, Spain
85.Consejo Nacl Ciencia & Technol, Av Insurgentes Sur 1582, Ciudad De Mexico 03940, Mexico
86.Hiroshima Univ, Hiroshima Astrophys Sci Ctr, 1-3-1 Kagamiyama, Higashihiroshima, Hiroshima 7398526, Japan
87.Aalto Univ, Dept Elect & Nanoengn, PL 15500, Aalto 00076, Finland
88.Aalto Univ, Metsahovi Radio Observ, Metsahovintie 114, Kylmala 02540, Finland
89.Yonsei Univ, Dept Astron, Yonsei Ro 50, Seoul 03722, South Korea
90.Tohoku Univ, Frontier Res Inst Interdisciplinary Sci, Sendai, Miyagi 9808578, Japan
91.Tohoku Univ, Astron Inst, Sendai, Miyagi 9808578, Japan
92.Seoul Natl Univ, Dept Phys & Astron, Seoul 08826, South Korea
93.Leiden Univ, Leiden Observ, Postbus 2300, NL-9513 RA Leiden, Netherlands
94.Brandeis Univ, Dept Phys, 415 South St, Waltham, MA 02453 USA
95.Huazhong Univ Sci & Technol, Sch Phys, Wuhan 430074, Hubei, Peoples R China
96.Univ Coll London, Mullard Space Sci Lab, Dorking RH5 6NT, Surrey, England
97.Univ Chinese Acad Sci, Sch Astron & Space Sci, 19A Yuquan Rd, Beijing 100049, Peoples R China
98.Univ Sci & Technol China, Astron Dept, Hefei 230026, Peoples R China
99.Univ Southern Denmark, CP3-Origins,Campusvej 55, DK-5230 Odense M, Denmark
100.Inst Adv Study, Sch Nat Sci, 1 Einstein Dr, Princeton, NJ 08540 USA
Recommended Citation
GB/T 7714
Roelofs, F.,Janssen, M.,Natarajan, I,et al. SYMBA: An end-to-end VLBI synthetic data generation pipeline Simulating Event Horizon Telescope observations of M 87[J]. ASTRONOMY & ASTROPHYSICS,2020,636:19.
APA Roelofs, F..,Janssen, M..,Natarajan, I.,Deane, R..,Davelaar, J..,...&Zhu, Z..(2020).SYMBA: An end-to-end VLBI synthetic data generation pipeline Simulating Event Horizon Telescope observations of M 87.ASTRONOMY & ASTROPHYSICS,636,19.
MLA Roelofs, F.,et al."SYMBA: An end-to-end VLBI synthetic data generation pipeline Simulating Event Horizon Telescope observations of M 87".ASTRONOMY & ASTROPHYSICS 636(2020):19.
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