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arXiv: 1906.11239
handle: 10261/179919 , https://repository.ubn.ru.nl/handle/2066/202541 , 11588/765060 , 11245.1/947b10a6-89a8-46ed-bbaa-27daace890ad , 11370/6fdf5182-be2d-4e49-8edf-3dc08895e859 , 2066/202541 , 21.11116/0000-0003-811B-D , 21.11116/0000-0003-811D-B , 11584/327401 , 20.500.12386/29341 , 2144/40692 , 2263/77167
arXiv: 1906.11239
handle: 10261/179919 , https://repository.ubn.ru.nl/handle/2066/202541 , 11588/765060 , 11245.1/947b10a6-89a8-46ed-bbaa-27daace890ad , 11370/6fdf5182-be2d-4e49-8edf-3dc08895e859 , 2066/202541 , 21.11116/0000-0003-811B-D , 21.11116/0000-0003-811D-B , 11584/327401 , 20.500.12386/29341 , 2144/40692 , 2263/77167
Abstract The Event Horizon Telescope (EHT) is a very long baseline interferometry (VLBI) array that comprises millimeter- and submillimeter-wavelength telescopes separated by distances comparable to the diameter of the Earth. At a nominal operating wavelength of ∼1.3 mm, EHT angular resolution (λ/D) is ∼25 μas, which is sufficient to resolve nearby supermassive black hole candidates on spatial and temporal scales that correspond to their event horizons. With this capability, the EHT scientific goals are to probe general relativistic effects in the strong-field regime and to study accretion and relativistic jet formation near the black hole boundary. In this Letter we describe the system design of the EHT, detail the technology and instrumentation that enable observations, and provide measures of its performance. Meeting the EHT science objectives has required several key developments that have facilitated the robust extension of the VLBI technique to EHT observing wavelengths and the production of instrumentation that can be deployed on a heterogeneous array of existing telescopes and facilities. To meet sensitivity requirements, high-bandwidth digital systems were developed that process data at rates of 64 gigabit s−1, exceeding those of currently operating cm-wavelength VLBI arrays by more than an order of magnitude. Associated improvements include the development of phasing systems at array facilities, new receiver installation at several sites, and the deployment of hydrogen maser frequency standards to ensure coherent data capture across the array. These efforts led to the coordination and execution of the first Global EHT observations in 2017 April, and to event-horizon-scale imaging of the supermassive black hole candidate in M87.
Gravitational lensing: strong, Astronomy, black hole physics, galaxies: individual, Astrophysics, strong [Gravitational lensing], General Relativity and Quantum Cosmology, black hole physics – galaxies: individual (M87) – Galaxy: center – gravitational lensing: strong – instrumentation: interferometers – techniques: high angular resolution, Galaxies: individual (M87), Very long baseline interferometry (VLBI), instrumentation: interferometers, High Energy Astrophysical Phenomena (astro-ph.HE), Galaxy: center, black hole physics; galaxies: individual (M87); Galaxy: center; gravitational lensing: strong; instrumentation: interferometers; techniques: high angular resolution, gravitational lensing: strong, center [Galaxy], 520, QB460-466, Astronomy & astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, 330, FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), galaxies: individual: M87, 530, galaxies: individual (M87), Event Horizon Telescope (EHT), Techniques: high angular resolution, FIS/05 - ASTRONOMIA E ASTROFISICA, Instrumentation and Methods for Astrophysics (astro-ph.IM), Astronomical and space sciences, techniques: high angular resolution, interferometers [Instrumentation], Black hole physics, black hole physics – galaxies: individual (M87) – Galaxy: center – gravitational lensing: strong – instrumentation: interferometers – techniques: high angular resolution, individual (M87) [Galaxies], Astrophysics - Astrophysics of Galaxies, echniques: high angular resolution, high angular resolution [Techniques], Black hole physics; Galaxies: individual (M87); Galaxy: center; Gravitational lensing: strong; Instrumentation: interferometers; Techniques: high angular resolution, Instrumentation: interferometers, Astrophysics of Galaxies (astro-ph.GA), [PHYS.ASTR] Physics [physics]/Astrophysics [astro-ph]
Gravitational lensing: strong, Astronomy, black hole physics, galaxies: individual, Astrophysics, strong [Gravitational lensing], General Relativity and Quantum Cosmology, black hole physics – galaxies: individual (M87) – Galaxy: center – gravitational lensing: strong – instrumentation: interferometers – techniques: high angular resolution, Galaxies: individual (M87), Very long baseline interferometry (VLBI), instrumentation: interferometers, High Energy Astrophysical Phenomena (astro-ph.HE), Galaxy: center, black hole physics; galaxies: individual (M87); Galaxy: center; gravitational lensing: strong; instrumentation: interferometers; techniques: high angular resolution, gravitational lensing: strong, center [Galaxy], 520, QB460-466, Astronomy & astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, 330, FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), galaxies: individual: M87, 530, galaxies: individual (M87), Event Horizon Telescope (EHT), Techniques: high angular resolution, FIS/05 - ASTRONOMIA E ASTROFISICA, Instrumentation and Methods for Astrophysics (astro-ph.IM), Astronomical and space sciences, techniques: high angular resolution, interferometers [Instrumentation], Black hole physics, black hole physics – galaxies: individual (M87) – Galaxy: center – gravitational lensing: strong – instrumentation: interferometers – techniques: high angular resolution, individual (M87) [Galaxies], Astrophysics - Astrophysics of Galaxies, echniques: high angular resolution, high angular resolution [Techniques], Black hole physics; Galaxies: individual (M87); Galaxy: center; Gravitational lensing: strong; Instrumentation: interferometers; Techniques: high angular resolution, Instrumentation: interferometers, Astrophysics of Galaxies (astro-ph.GA), [PHYS.ASTR] Physics [physics]/Astrophysics [astro-ph]
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