Multi-Wavelength and Multi-Messenger Studies Using the Next-Generation Event Horizon Telescope

Multi-Wavelength and Multi-Messenger Studies Using the Next-Generation Event Horizon Telescope

The next-generation Event Horizon Telescope (ngEHT) will provide us with the best opportunity to investigate supermassive black holes (SMBHs) at the highest possible resolution and sensitivity. With respect to the existing Event Horizon Telescope (EHT) array, the ngEHT will provide increased sensiti...

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Veröffentlicht in:Galaxies 2023-01, Vol.11 (1), p.17
Hauptverfasser: Lico, Rocco, Jorstad, Svetlana G., Marscher, Alan P., Gómez, Jose L., Liodakis, Ioannis, Dahale, Rohan, Alberdi, Antxon, Gold, Roman, Traianou, Efthalia, Toscano, Teresa, Foschi, Marianna
Format: Artikel
Sprache:eng
Schlagworte:
Accretion disks
active galactic nuclei
Astronomical research
Black holes
Black holes (Astronomy)
Event horizon
Magnetic fields
multi-wavelength studies
Neutrinos
Radio astronomy
relativistic jets
Sensitivity
Supermassive black holes
Telescopes
very long baseline interferometry (VLBI)
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Zusammenfassung:The next-generation Event Horizon Telescope (ngEHT) will provide us with the best opportunity to investigate supermassive black holes (SMBHs) at the highest possible resolution and sensitivity. With respect to the existing Event Horizon Telescope (EHT) array, the ngEHT will provide increased sensitivity and uv-coverage (with the addition of new stations), wider frequency coverage (from 86 GHz to 345 GHz and higher), finer resolution (
ISSN:2075-4434
2075-4434
DOI:10.3390/galaxies11010017