Vertaisarvioitu alkuperäisartikkeli tai data-artikkeli tieteellisessä aikakauslehdessä (A1)
Event Horizon and Environs (ETHER): A Curated Database for EHT and ngEHT Targets and Science
Julkaisun tekijät: Ramakrishnan Venkatessh, Nagar Neil, Arratia Vicente, Hernandez-Yevenes Joaquín, Pesce Dominic W, Nair Dhanya G, Bandyopadhyay Bidisha, Medina-Porcile Catalina, Krichbaum Thomas P, Doeleman Sheperd, Ricarte Angelo, Fish Vincent L, Blackburn Lindy, Falcke Heino, Bower Geoffrey, Natarajan Priyamvada
Kustantaja: MDPI
Julkaisuvuosi: 2023
Journal: Galaxies
Tietokannassa oleva lehden nimi: GALAXIES
Lehden akronyymi: GALAXIES
Volyymi: 11
Julkaisunumero: 11
Sivujen määrä: 18
eISSN: 2075-4434
DOI: http://dx.doi.org/10.3390/galaxies11010015
Verkko-osoite: https://www.mdpi.com/2075-4434/11/1/15
Rinnakkaistallenteen osoite: https://research.utu.fi/converis/portal/detail/Publication/179084739
The next generation Event Horizon Telescope (ngEHT) will observe multiple supermassive black hole (SMBH) candidates down to a few tens of mJy, and profoundly transform our understanding of the local SMBH population. Given the impossibility of large-area high-resolution millimeter surveys, multi-frequency spectral energy densities (SEDs), and models are required to both identify source samples tailored to specific science goals, and to predict the feasibility of detection of individual interesting sources. Here, we present the Event Horizon and Environs (ETHER) source and SED model database whose primary use is to enable the selection and optimization of targets for EHT and ngEHT science. The living ETHER database currently consolidates 1.6 million black hole mass estimates, similar to 15,500 milliarcsec-scale radio fluxes, similar to 14,000 hard X-ray fluxes (expected to grow by factor greater than or similar to 40 with the eROSITA data release) and SED information as obtained from catalogs and database queries, the literature, and our own new observations. Jet and accretion flow models are fit to individual SEDs in an automated way in order to predict the ngEHT observable fluxes from the jet base and accretion inflow. The database can be filtered by parameters or cross matched to a user source list, with the automated SED fitting models optionally fine tuned by the user. We have identified an initial ngEHT 'gold sample' for jet base studies and potentially black hole shadows; this sample will grow significantly in the coming years. While the ngEHT requires and will best exploit the ETHER database, six (eleven) ETHER sources have already been observed (scheduled) with the EHT in 2022 (2023), and the database has wide ranging applications in galaxy and black hole mass evolution studies.
Ladattava julkaisu This is an electronic reprint of the original article. |  |
