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240202 ||| eng |
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|a 9783036593548
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|a books978-3-0365-9355-5
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|a 9783036593555
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|a Johnson, Michael D.
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|a From Vision to Instrument: Creating a Next-Generation Event Horizon Telescope for a New Era of Black Hole Science
|h Elektronische Ressource
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260 |
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|a Basel
|b MDPI - Multidisciplinary Digital Publishing Institute
|c 2023
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300 |
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|a 1 electronic resource (470 p.)
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653 |
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|a Radio Astronomy
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|a submillimeter astronomy (1647)
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|a accretion inflows
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|a active galaxies
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|a AGN
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|a scientific collaborations
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|a accretion disk
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|a very long baseline interferometry
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|a astronomical instrumentation
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|a event horizon telescope
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|a interferometry
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|a quasars
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|a photon rings
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|a imaging
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|a next-generation event horizon telescope
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|a VLBI
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|a SFPR
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|a millimeter astronomy
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|a interferometric techniques
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|a radio astronomy
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|a telescopes
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|a history
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|a StarWarps
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|a radio telescopes (1360)
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|a philosophy
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|a astrometry
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|a multi-wavelength studies
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|a Tensor Core
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|a precipitable water vapor
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|a astronomical instrumentation (799)
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|a Research & information: general / bicssc
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|a Very Long Baseline Interferometry
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|a Physics / bicssc
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|a Sagittarius A*
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|a visualization
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|a hot spot
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|a very-long-baseline interferometry
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|a high angular resolution (2167)
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|a social sciences
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|a radiative transfer
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|a magnetohydrodynamics
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|a EHT
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|a plasma composition
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|a relativistic jet
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|a high angular resolution
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|a general relativity
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|a M87*
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|a no hair theorems
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|a algorithms
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|a polarimetry
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|a radio instrumentation
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|a radio telescopes
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|a n/a
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|a data analysis
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|a very long baseline interferometry (VLBI)
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|a SMA
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|a radio astronomy (1338)
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|a governance
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|a millimeter astronomy (1061)
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|a GRMHD
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|a Sgr A*
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|a active galactic nuclei
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|a black hole
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|a time-variability
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|a neutrinos
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|a instrument design
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|a correlation
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|a jet launching
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|a very long baseline interferometry (1769)
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|a radio interferometry
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|a Messier 87
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|a astronomical techniques
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|a signal processing
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|a black holes
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|a relativistic Jet
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|a GPU
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|a SMBHs
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|a galaxy jets
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|a radio continuum
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|a robustness
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|a Astronomy, space & time / bicssc
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|a ngEHT
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|a relativistic jets
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|a supermassive black holes
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|a accretion
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|a dynamical image reconstruction
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|a Doeleman, Shep
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|a Gómez, Jose L.
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|a Johnson, Michael D.
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|a eng
|2 ISO 639-2
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|b DOAB
|a Directory of Open Access Books
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|a Creative Commons (cc), https://creativecommons.org/licenses/by/4.0/
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|a 10.3390/books978-3-0365-9355-5
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|u https://www.mdpi.com/books/pdfview/book/8277
|7 0
|x Verlag
|3 Volltext
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|u https://directory.doabooks.org/handle/20.500.12854/128810
|z DOAB: description of the publication
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|a 000
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|a 100
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|a 530
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|a 900
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|a 320
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|a 300
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|a In April 2019, the Event Horizon Telescope Collaboration successfully imaged the first supermassive black hole (M87*), opening a new era in detailed study of these exotic objects. By sharply enhancing the capabilities of black hole imaging, the next-generation EHT (ngEHT) is poised to again revolutionize our view of horizon-scale physics. The ngEHT will enable the first movies of black hole accretion, produce high-dynamic-range images that connect black holes directly to their galactic-scale relativistic jets, and bring into range a larger population of black holes and explosive transients to explore. This Special Issue develops the key science drivers and architecture of the ngEHT. The contributions sharpen the ngEHT scientific vision and implementation by illuminating and proposing new possibilities in the following areas: Fundamental physics; Black holes and their cosmic context; Accretion; Jet launching; Transients and impulsive phenomena; Algorithms and inference; History, philosophy, and cultural implications of building new instruments in the current era; Advances in submillimeter VLBI instrumentation; VLBI array design and optimization
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