Abstract
The Event Horizon Telescope (EHT) Collaboration has recently produced the first resolved images of the central supermassive black hole in the giant elliptical galaxy M87. Here we report on tests of the consistency and accuracy of the general relativistic radiative transfer codes used within the collaboration to model M87∗ and Sgr A∗. We compare and evaluate (1) deflection angles for equatorial null geodesics in a Kerr spacetime; (2) images calculated from a series of simple, parameterized matter distributions in the Kerr metric using simplified emissivities and absorptivities; (3) for a subset of codes, images calculated from general relativistic magnetohydrodynamics simulations using different realistic synchrotron emissivities and absorptivities; (4) observables for the 2017 configuration of EHT, including visibility amplitudes and closure phases. The error in total flux is of order 1% when the codes are run with production numerical parameters. The dominant source of discrepancies for small camera distances is the location and detailed setup of the software "camera"that each code uses to produce synthetic images. We find that when numerical parameters are suitably chosen and the camera is sufficiently far away the images converge and that for given transfer coefficients, numerical uncertainties are unlikely to limit parameter estimation for the current generation of EHT observations. The purpose of this paper is to describe a verification and comparison of EHT radiative transfer codes. It is not to verify EHT models more generally.
Original language | English (US) |
---|---|
Article number | 148 |
Journal | Astrophysical Journal |
Volume | 897 |
Issue number | 2 |
DOIs | |
State | Published - Jul 10 2020 |
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science
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Verification of Radiative Transfer Schemes for the EHT. / Eatough, Ralphp; Gold, Roman; Broderick, Avery E.; Younsi, Ziri; Fromm, Christian M.; Gammie, Charles F.; Mościbrodzka, Monika; Pu, Hung Yi; Bronzwaer, Thomas; Davelaar, Jordy; Dexter, Jason; Ball, David; Chan, Chi Kwan; Kawashima, Tomohisa; Mizuno, Yosuke; Ripperda, Bart; Akiyama, Kazunori; Alberdi, Antxon; Alef, Walter; Asada, Keiichi; Azulay, Rebecca; Baczko, Anne Kathrin; Baloković, Mislav; Barrett, John; Bintley, Dan; Blackburn, Lindy; Boland, Wilfred; Bouman, Katherine L.; Bower, Geoffrey C.; Bremer, Michael; Brinkerink, Christiaan D.; Brissenden, Roger; Britzen, Silke; Broguiere, Dominique; Byun, Do Young; Carlstrom, John E.; Chael, Andrew; Chatterjee, Koushik; Chatterjee, Shami; Chen, Ming Tang; Chen, Yongjun; Cho, Ilje; Christian, Pierre; Conway, John E.; Cordes, James M.; Crew, Geoffrey B.; Cui, Yuzhu; Laurentis, Mariafelicia De; Deane, Roger; Dempsey, Jessica; Desvignes, Gregory; Doeleman, Sheperd S.; Eatough, Ralphp; Falcke, Heino; Fish, Vincent L.; Fomalont, Ed; Fraga-Encinas, Raquel; Freeman, Bill; Friberg, Per; Gómez, José L.; Galison, Peter; García, Roberto; Gentaz, Olivier; Georgiev, Boris; Goddi, Ciriaco; Gu, Minfeng; Gurwell, Mark; Hada, Kazuhiro; Hecht, Michael H.; Hesper, Ronald; Ho, Luis C.; Ho, Paul; Honma, Mareki; Huang, Chih Wei L.; Huang, Lei; Hughes, David H.; Inoue, Makoto; Issaoun, Sara; James, David J.; Jannuzi, Buell T.; Janssen, Michael; Jeter, Britton; Jiang, Wu; Jimenez-Rosales, Alejandra; Johnson, Michael D.; Jorstad, Svetlana; Jung, Taehyun; Karami, Mansour; Karuppusamy, Ramesh; Keating, Garrett K.; Kettenis, Mark; Kim, Jae Young; Kim, Junhan; Kim, Jongsoo; Kino, Motoki; Koay, Jun Yi; Koch, Patrick M.; Koyama, Shoko; Kramer, Michael; Kramer, Carsten; Krichbaum, Thomas P.; Kuo, Cheng Yu; Lauer, Tod R.; Lee, Sang Sung; Li, Yan Rong; Li, Zhiyuan; Lico, Rocco; Lindqvist, Michael; Liu, Kuo; Liuzzo, Elisabetta; Lo, Wen Ping; Lobanov, Andrei P.; Loinard, Laurent; Lonsdale, Colin; Lu, Ru Sen; Macdonald, Nicholas R.; Markoff, Sera; Mao, Jirong; Marrone, Daniel P.; Marscher, Alan P.; Martí-Vidal, Iván; Matsushita, Satoki; Matthews, Lynn D.; Medeiros, Lia; Menten, Karl M.; Mizuno, Izumi; Moran, James M.; Moriyama, Kotaro; Müller, Cornelia; Nagai, Hiroshi; Nakamura, Masanori; Nagar, Neil M.; Narayan, Ramesh; Narayanan, Gopal; Natarajan, Iniyan; Neri, Roberto; Ni, Chunchong; Noutsos, Aristeidis; Okino, Hiroki; Ortiz-León, Gisela N.; Oyama, Tomoaki; zel, Feryal; Palumbo, Daniel C.M.; Park, Jongho; Patel, Nimesh; Pen, Ue Li; Pesce, Dominic W.; Plambeck, Richard; Piétu, Vincent; Popstefanija, Aleksandar; Porth, Oliver; Preciado-López, Jorge A.; Psaltis, Dimitrios; Ramakrishnan, Venkatessh; Rao, Ramprasad; Rawlings, Mark G.; Raymond, Alexander W.; Rezzolla, Luciano; Roelofs, Freek; Rogers, Alan; Ros, Eduardo; Rose, Mel; Roshanineshat, Arash; Rottmann, Helge; Roy, Alan L.; Ruszczyk, Chet; Rygl, Kazi L.J.; Sánchez, Salvador; Sánchez-Arguelles, David; Sasada, Mahito; Savolainen, Tuomas; Schuster, Karl Friedrich; Schloerb, F. Peter; Shao, Lijing; Shen, Zhiqiang; Small, Des; Sohn, Bong Won; Soohoo, Jason; Tiede, Paul; Tazaki, Fumie; Tilanus, Remo P.J.; Titus, Michael; Toma, Kenji; Torne, Pablo; Trent, Tyler; Traianou, Thalia; Trippe, Sascha; Tsuda, Shuichiro; Van Langevelde, Huib Jan; Bemmel, Ilse Van; Van Rossum, Daniel R.; Wagner, Jan; Wardle, John; Wex, Norbert; Weintroub, Jonathan; Wharton, Robert; Wielgus, Maciek; Wong, George N.; Wu, Qingwen; Yoon, Doosoo; Young, Ken; Young, André; Yuan, Feng; Yuan, Ye Fei; Zensus, J. Anton; Zhao, Guangyao; Zhao, Shan Shan; Zhu, Ziyan.
In: Astrophysical Journal, Vol. 897, No. 2, 148, 10.07.2020.Research output: Contribution to journal › Article › peer-review
}
TY - JOUR
T1 - Verification of Radiative Transfer Schemes for the EHT
AU - Eatough, Ralphp
AU - Gold, Roman
AU - Broderick, Avery E.
AU - Younsi, Ziri
AU - Fromm, Christian M.
AU - Gammie, Charles F.
AU - Mościbrodzka, Monika
AU - Pu, Hung Yi
AU - Bronzwaer, Thomas
AU - Davelaar, Jordy
AU - Dexter, Jason
AU - Ball, David
AU - Chan, Chi Kwan
AU - Kawashima, Tomohisa
AU - Mizuno, Yosuke
AU - Ripperda, Bart
AU - Akiyama, Kazunori
AU - Alberdi, Antxon
AU - Alef, Walter
AU - Asada, Keiichi
AU - Azulay, Rebecca
AU - Baczko, Anne Kathrin
AU - Baloković, Mislav
AU - Barrett, John
AU - Bintley, Dan
AU - Blackburn, Lindy
AU - Boland, Wilfred
AU - Bouman, Katherine L.
AU - Bower, Geoffrey C.
AU - Bremer, Michael
AU - Brinkerink, Christiaan D.
AU - Brissenden, Roger
AU - Britzen, Silke
AU - Broguiere, Dominique
AU - Byun, Do Young
AU - Carlstrom, John E.
AU - Chael, Andrew
AU - Chatterjee, Koushik
AU - Chatterjee, Shami
AU - Chen, Ming Tang
AU - Chen, Yongjun
AU - Cho, Ilje
AU - Christian, Pierre
AU - Conway, John E.
AU - Cordes, James M.
AU - Crew, Geoffrey B.
AU - Cui, Yuzhu
AU - Laurentis, Mariafelicia De
AU - Deane, Roger
AU - Dempsey, Jessica
AU - Desvignes, Gregory
AU - Doeleman, Sheperd S.
AU - Eatough, Ralphp
AU - Falcke, Heino
AU - Fish, Vincent L.
AU - Fomalont, Ed
AU - Fraga-Encinas, Raquel
AU - Freeman, Bill
AU - Friberg, Per
AU - Gómez, José L.
AU - Galison, Peter
AU - García, Roberto
AU - Gentaz, Olivier
AU - Georgiev, Boris
AU - Goddi, Ciriaco
AU - Gu, Minfeng
AU - Gurwell, Mark
AU - Hada, Kazuhiro
AU - Hecht, Michael H.
AU - Hesper, Ronald
AU - Ho, Luis C.
AU - Ho, Paul
AU - Honma, Mareki
AU - Huang, Chih Wei L.
AU - Huang, Lei
AU - Hughes, David H.
AU - Inoue, Makoto
AU - Issaoun, Sara
AU - James, David J.
AU - Jannuzi, Buell T.
AU - Janssen, Michael
AU - Jeter, Britton
AU - Jiang, Wu
AU - Jimenez-Rosales, Alejandra
AU - Johnson, Michael D.
AU - Jorstad, Svetlana
AU - Jung, Taehyun
AU - Karami, Mansour
AU - Karuppusamy, Ramesh
AU - Keating, Garrett K.
AU - Kettenis, Mark
AU - Kim, Jae Young
AU - Kim, Junhan
AU - Kim, Jongsoo
AU - Kino, Motoki
AU - Koay, Jun Yi
AU - Koch, Patrick M.
AU - Koyama, Shoko
AU - Kramer, Michael
AU - Kramer, Carsten
AU - Krichbaum, Thomas P.
AU - Kuo, Cheng Yu
AU - Lauer, Tod R.
AU - Lee, Sang Sung
AU - Li, Yan Rong
AU - Li, Zhiyuan
AU - Lico, Rocco
AU - Lindqvist, Michael
AU - Liu, Kuo
AU - Liuzzo, Elisabetta
AU - Lo, Wen Ping
AU - Lobanov, Andrei P.
AU - Loinard, Laurent
AU - Lonsdale, Colin
AU - Lu, Ru Sen
AU - Macdonald, Nicholas R.
AU - Markoff, Sera
AU - Mao, Jirong
AU - Marrone, Daniel P.
AU - Marscher, Alan P.
AU - Martí-Vidal, Iván
AU - Matsushita, Satoki
AU - Matthews, Lynn D.
AU - Medeiros, Lia
AU - Menten, Karl M.
AU - Mizuno, Izumi
AU - Moran, James M.
AU - Moriyama, Kotaro
AU - Müller, Cornelia
AU - Nagai, Hiroshi
AU - Nakamura, Masanori
AU - Nagar, Neil M.
AU - Narayan, Ramesh
AU - Narayanan, Gopal
AU - Natarajan, Iniyan
AU - Neri, Roberto
AU - Ni, Chunchong
AU - Noutsos, Aristeidis
AU - Okino, Hiroki
AU - Ortiz-León, Gisela N.
AU - Oyama, Tomoaki
AU - zel, Feryal
AU - Palumbo, Daniel C.M.
AU - Park, Jongho
AU - Patel, Nimesh
AU - Pen, Ue Li
AU - Pesce, Dominic W.
AU - Plambeck, Richard
AU - Piétu, Vincent
AU - Popstefanija, Aleksandar
AU - Porth, Oliver
AU - Preciado-López, Jorge A.
AU - Psaltis, Dimitrios
AU - Ramakrishnan, Venkatessh
AU - Rao, Ramprasad
AU - Rawlings, Mark G.
AU - Raymond, Alexander W.
AU - Rezzolla, Luciano
AU - Roelofs, Freek
AU - Rogers, Alan
AU - Ros, Eduardo
AU - Rose, Mel
AU - Roshanineshat, Arash
AU - Rottmann, Helge
AU - Roy, Alan L.
AU - Ruszczyk, Chet
AU - Rygl, Kazi L.J.
AU - Sánchez, Salvador
AU - Sánchez-Arguelles, David
AU - Sasada, Mahito
AU - Savolainen, Tuomas
AU - Schuster, Karl Friedrich
AU - Schloerb, F. Peter
AU - Shao, Lijing
AU - Shen, Zhiqiang
AU - Small, Des
AU - Sohn, Bong Won
AU - Soohoo, Jason
AU - Tiede, Paul
AU - Tazaki, Fumie
AU - Tilanus, Remo P.J.
AU - Titus, Michael
AU - Toma, Kenji
AU - Torne, Pablo
AU - Trent, Tyler
AU - Traianou, Thalia
AU - Trippe, Sascha
AU - Tsuda, Shuichiro
AU - Van Langevelde, Huib Jan
AU - Bemmel, Ilse Van
AU - Van Rossum, Daniel R.
AU - Wagner, Jan
AU - Wardle, John
AU - Wex, Norbert
AU - Weintroub, Jonathan
AU - Wharton, Robert
AU - Wielgus, Maciek
AU - Wong, George N.
AU - Wu, Qingwen
AU - Yoon, Doosoo
AU - Young, Ken
AU - Young, André
AU - Yuan, Feng
AU - Yuan, Ye Fei
AU - Zensus, J. Anton
AU - Zhao, Guangyao
AU - Zhao, Shan Shan
AU - Zhu, Ziyan
N1 - Publisher Copyright: © 2020. The American Astronomical Society. All rights reserved.. Copyright: Copyright 2020 Elsevier B.V., All rights reserved.
PY - 2020/7/10
Y1 - 2020/7/10
N2 - The Event Horizon Telescope (EHT) Collaboration has recently produced the first resolved images of the central supermassive black hole in the giant elliptical galaxy M87. Here we report on tests of the consistency and accuracy of the general relativistic radiative transfer codes used within the collaboration to model M87∗ and Sgr A∗. We compare and evaluate (1) deflection angles for equatorial null geodesics in a Kerr spacetime; (2) images calculated from a series of simple, parameterized matter distributions in the Kerr metric using simplified emissivities and absorptivities; (3) for a subset of codes, images calculated from general relativistic magnetohydrodynamics simulations using different realistic synchrotron emissivities and absorptivities; (4) observables for the 2017 configuration of EHT, including visibility amplitudes and closure phases. The error in total flux is of order 1% when the codes are run with production numerical parameters. The dominant source of discrepancies for small camera distances is the location and detailed setup of the software "camera"that each code uses to produce synthetic images. We find that when numerical parameters are suitably chosen and the camera is sufficiently far away the images converge and that for given transfer coefficients, numerical uncertainties are unlikely to limit parameter estimation for the current generation of EHT observations. The purpose of this paper is to describe a verification and comparison of EHT radiative transfer codes. It is not to verify EHT models more generally.
AB - The Event Horizon Telescope (EHT) Collaboration has recently produced the first resolved images of the central supermassive black hole in the giant elliptical galaxy M87. Here we report on tests of the consistency and accuracy of the general relativistic radiative transfer codes used within the collaboration to model M87∗ and Sgr A∗. We compare and evaluate (1) deflection angles for equatorial null geodesics in a Kerr spacetime; (2) images calculated from a series of simple, parameterized matter distributions in the Kerr metric using simplified emissivities and absorptivities; (3) for a subset of codes, images calculated from general relativistic magnetohydrodynamics simulations using different realistic synchrotron emissivities and absorptivities; (4) observables for the 2017 configuration of EHT, including visibility amplitudes and closure phases. The error in total flux is of order 1% when the codes are run with production numerical parameters. The dominant source of discrepancies for small camera distances is the location and detailed setup of the software "camera"that each code uses to produce synthetic images. We find that when numerical parameters are suitably chosen and the camera is sufficiently far away the images converge and that for given transfer coefficients, numerical uncertainties are unlikely to limit parameter estimation for the current generation of EHT observations. The purpose of this paper is to describe a verification and comparison of EHT radiative transfer codes. It is not to verify EHT models more generally.
UR - http://www.scopus.com/inward/record.url?scp=85088029004&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=85088029004&partnerID=8YFLogxK
U2 - 10.3847/1538-4357/ab96c6
DO - 10.3847/1538-4357/ab96c6
M3 - Article
AN - SCOPUS:85088029004
VL - 897
JO - Astrophysical Journal
JF - Astrophysical Journal
SN - 0004-637X
IS - 2
M1 - 148
ER -