First M87 Event Horizon Telescope Results. III. Data Processing and Calibration
Woodwell Climate Research Center · Harvard University · +74 more institutions
Abstract
Abstract We present the calibration and reduction of Event Horizon Telescope (EHT) 1.3 mm radio wavelength observations of the supermassive black hole candidate at the center of the radio galaxy M87 and the quasar 3C 279, taken during the 2017 April 5–11 observing campaign. These global very long baseline interferometric observations include for the first time the highly sensitive Atacama Large Millimeter/submillimeter Array (ALMA); reaching an angular resolution of 25 μ as, with characteristic sensitivity limits of ∼1 mJy on baselines to ALMA and ∼10 mJy on other baselines. The observations present challenges for existing data processing tools, arising from the rapid atmospheric phase fluctuations, wide…
Citation impact
- FWCI
- 68.14
- Percentile
- 100%
- References
- 78
Authors
217- KAKazunori AkiyamaCorresponding
Woodwell Climate Research Center, Harvard University, National Radio Astronomy Observatory, National Astronomical Observatory of Japan, Massachusetts Institute of Technology
- AAA. Alberdi
Instituto de Astrofísica de Andalucía
- WAW. Alef
Max Planck Institute for Radio Astronomy
- KAKeiichi Asada
Institute of Astronomy and Astrophysics, Academia Sinica
- RARebecca Azulay
Universitat de València, Parc Científic de la Universitat de València, Max Planck Institute for Radio Astronomy
Topics & keywords
- Physics
- Supermassive black hole
- Millimeter
- Amplitude
- Astrophysics
- Telescope
- Calibration
- Angular resolution (graph drawing)