A1 Vertaisarvioitu alkuperäisartikkeli tieteellisessä lehdessä
Multi-Wavelength and Multi-Messenger Studies Using the Next-Generation Event Horizon Telescope
Tekijät: Lico Rocco, Jorstad Svetlana G, Marscher Alan P, Gomez Jose L, Liodakis Ioannis, Dahale Rohan, Alberdi Antxon, Gold Roman, Traianou Efthalia, Toscano Teresa, Foschi Marianna
Julkaisuvuosi: 2023
Lehti: Galaxies
Tietokannassa oleva lehden nimi: GALAXIES
Lehden akronyymi: GALAXIES
Artikkelin numero: 17
Vuosikerta: 11
Numero: 1
Sivujen määrä: 9
eISSN: 2075-4434
DOI: https://doi.org/10.3390/galaxies11010017
Julkaisun avoimuus kirjaamishetkellä: Avoimesti saatavilla
Julkaisukanavan avoimuus : Kokonaan avoin julkaisukanava
Verkko-osoite: https://www.mdpi.com/2075-4434/11/1/17
Rinnakkaistallenteen osoite: https://research.utu.fi/converis/portal/detail/Publication/179085471
Rinnakkaistallenteen lisenssi: CC BY
Rinnakkaistallennetun julkaisun versio: Kustantajan versio
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 (<15 micro-arcseconds), and better monitoring capabilities. The ngEHT will offer a unique opportunity to deeply investigate the physics around SMBHs, such as the disk-jet connection, the mechanisms responsible for high-energy photon and neutrino events, and the role of magnetic fields in shaping relativistic jets, as well as the nature of binary SMBH systems. In this white paper we describe some ngEHT science cases in the context of multi-wavelength studies and synergies.
Ladattava julkaisu This is an electronic reprint of the original article. |  |
