Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование
First M87 Event Horizon Telescope Results. IV. Imaging the Central Supermassive Black Hole. / Event Horizon Telescope Collaborat ; Эрштадт, Светлана Георгиевна.
в: Astrophysical Journal Letters, Том 875, № 1, L4, 10.04.2019.Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование
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TY - JOUR
T1 - First M87 Event Horizon Telescope Results. IV. Imaging the Central Supermassive Black Hole
AU - Event Horizon Telescope Collaborat
AU - Akiyama, Kazunori
AU - Alberdi, Antxon
AU - Alef, Walter
AU - Asada, Keiichi
AU - Azulay, Rebecca
AU - Baczko, Anne-Kathrin
AU - Ball, David
AU - Balokovic, 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 - Broderick, Avery E.
AU - Broguiere, Dominique
AU - Bronzwaer, Thomas
AU - Byun, Do-Young
AU - Carlstrom, John E.
AU - Chael, Andrew
AU - Chan, Chi-Kwan
AU - Chatterjee, Shami
AU - Chatterjee, Koushik
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 - Davelaar, Jordy
AU - De Laurentis, Mariafelicia
AU - Deane, Roger
AU - Dempsey, Jessica
AU - Desvignes, Gregory
AU - Dexter, Jason
AU - Doeleman, Sheperd S.
AU - Eatough, Ralph P.
AU - Falcke, Heino
AU - Fish, Vincent L.
AU - Fomalont, Ed
AU - Fraga-Encinas, Raquel
AU - Freeman, William T.
AU - Friberg, Per
AU - Fromm, Christian M.
AU - Эрштадт, Светлана Георгиевна
PY - 2019/4/10
Y1 - 2019/4/10
N2 - We present the first Event Horizon Telescope (EHT) images of M87, using observations from April 2017 at 1.3 mm wavelength. These images show a prominent ring with a diameter of ∼40 μas, consistent with the size and shape of the lensed photon orbit encircling the "shadow" of a supermassive black hole. The ring is persistent across four observing nights and shows enhanced brightness in the south. To assess the reliability of these results, we implemented a two-stage imaging procedure. In the first stage, four teams, each blind to the others' work, produced images of M87 using both an established method (CLEAN) and a newer technique (regularized maximum likelihood). This stage allowed us to avoid shared human bias and to assess common features among independent reconstructions. In the second stage, we reconstructed synthetic data from a large survey of imaging parameters and then compared the results with the corresponding ground truth images. This stage allowed us to select parameters objectively to use when reconstructing images of M87. Across all tests in both stages, the ring diameter and asymmetry remained stable, insensitive to the choice of imaging technique. We describe the EHT imaging procedures, the primary image features in M87, and the dependence of these features on imaging assumptions.
AB - We present the first Event Horizon Telescope (EHT) images of M87, using observations from April 2017 at 1.3 mm wavelength. These images show a prominent ring with a diameter of ∼40 μas, consistent with the size and shape of the lensed photon orbit encircling the "shadow" of a supermassive black hole. The ring is persistent across four observing nights and shows enhanced brightness in the south. To assess the reliability of these results, we implemented a two-stage imaging procedure. In the first stage, four teams, each blind to the others' work, produced images of M87 using both an established method (CLEAN) and a newer technique (regularized maximum likelihood). This stage allowed us to avoid shared human bias and to assess common features among independent reconstructions. In the second stage, we reconstructed synthetic data from a large survey of imaging parameters and then compared the results with the corresponding ground truth images. This stage allowed us to select parameters objectively to use when reconstructing images of M87. Across all tests in both stages, the ring diameter and asymmetry remained stable, insensitive to the choice of imaging technique. We describe the EHT imaging procedures, the primary image features in M87, and the dependence of these features on imaging assumptions.
KW - black hole physics
KW - galaxies: individual (M87)
KW - galaxies: jets
KW - techniques: high angular resolution
KW - techniques: image processing
KW - techniques: interferometric
KW - SELF-CALIBRATION
KW - HIGH-RESOLUTION
KW - JET
KW - INTERFEROMETRY
KW - RECONSTRUCTION
KW - IMPLEMENTATION
KW - DECONVOLUTION
KW - PRINCIPLES
KW - MOTION
UR - http://www.scopus.com/inward/record.url?scp=85064456798&partnerID=8YFLogxK
UR - http://stacks.iop.org/2041-8205/875/i=1/a=L4?key=crossref.f93f0b1565bb46b48cb890351d9fef13
UR - http://www.mendeley.com/research/first-m87-event-horizon-telescope-results-iv-imaging-central-supermassive-black-hole
U2 - 10.3847/2041-8213/ab0e85
DO - 10.3847/2041-8213/ab0e85
M3 - статья
VL - 875
JO - Astrophysical Journal Letters
JF - Astrophysical Journal Letters
SN - 2041-8205
IS - 1
M1 - L4
ER -
ID: 41191567