Photographing Black Holes with the Event Horizon Telescope - Past, Present and Future
Photographing Black Holes with the Event Horizon Telescope - Past, Present and Future - Kazu Akiyama MIT Haystack Observatory The Shadow of a Black Hole BH ~5.2 Rs Rs = 2GMBH/c2 (Hilbert 1916) Credit: Hung-Yi Pu Kazu Akiyama, NEROC Symposium 2020, Online, 2020/11/17 (Tue) Event Horizon Telescope Kazu Akiyama, NEROC Symposium 2020, Online, 2020/11/17 (Tue) Event Horizon Telescope Sgr A* EHT 50μas Credit: Hotaka Shiokawa M87 EHT 40μas Credit: Monika Moscibrodzka Kazu Akiyama, NEROC Symposium 2020, Online, 2020/11/17 (Tue) Units of the Angular Size Protractor:1 ticks = 1 degree x 1/60 = 1 arcmin x 1/60 = 1 arcsec x 1/1000 = 1 mas x 1/1000 = 1 μas 0.5 deg 30 arcmin 40 - 50 μas Kazu Akiyama, NEROC Symposium 2020, Online, 2020/11/17 (Tue) Event Horizon Telescope Collaboration >300 members, >59 institutes, >18 countries in North & South America, Europe, Asia, and Africa. Kazu Akiyama, NEROC Symposium 2020, Online, 2020/11/17 (Tue) Meet the Telescope SMT, Arizona LMT, Mexico IRAM 30m Spain APEX, Chile JCMT, Hawaii Photos: ALMA, Sven Dornbusch, Junhan Kim, Helge Rottmann, David Sanchez, Daniel Michalik, Jonathan Weintroub, William Montgomerie Meet the Telescope Photos: ALMA, Sven ALMA, Chile Dornbusch, Junhan Kim, Helge Rottmann, David Sanchez, Daniel Michalik, Jonathan Weintroub, William Montgomerie SPT, South Pole SMA, Hawaii From Observations to Images Kazu Akiyama, NEROC Symposium 2020, Online, 2020/11/17 (Tue) Credit: Lindy Blackburn EHT Hardware EHT Backend (R2DBE, Mark 6) Recording Rate: - VLBA, GMVA: 2-4 Gbps - EHT: 32 Gbps (2017), 64 Gbps (2018-) Kazu Akiyama, NEROC Symposium 2020, Online, 2020/11/17 (Tue) From Observations to Images MIT Haystack Observatory 8 TB x 8 HDD (x 92 modules) Credit: Bryce Vickmark Credit: Lindy Blackburn Kazu Akiyama, NEROC Symposium 2020, Online, 2020/11/17 (Tue) Data Calibration HOPS Pipeline (EHT-HOPS) CASA Pipeline (rPICARD) EHT AIPS Pipeline Blackburn et al.
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