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First M87 Event Horizon Telescope Results. III. Data Processing and Calibration

2019

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 μas, 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, …

010504 meteorology & atmospheric sciencesgalaxies: jetRadio galaxyAstronomyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesgalaxies: individualGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic Astrophysicsgalaxies: individual: M8701 natural sciencesSubmillimeter ArrayGeneral Relativity and Quantum CosmologyTechniques: high angular resolutionindividual (M87 3C279) [Galaxies]0103 physical sciencesInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysics0105 earth and related environmental sciencesRemote sensingPhysicsEvent Horizon TelescopeSupermassive black hole3C279Astrophysics::Instrumentation and Methods for AstrophysicsAstronomy and AstrophysicsQuasarBlack hole physicsblack hole physicAstrophysics - Astrophysics of Galaxies3. Good healthhigh angular resolution [Techniques]InterferometryAmplitudeSpace and Planetary ScienceGalaxies: jetsAstrophysics of Galaxies (astro-ph.GA)Techniques: interferometricinterferometric [Techniques]jets [Galaxies]Astrophysics - Instrumentation and Methods for Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Galaxies: individual (M87 3C279)Radio wave
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