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Tracking supermassive black hole mergers from kpc to sub-pc scales with AXIS

We present an analysis showcasing how the Advanced X-ray Imaging Satellite (AXIS), a proposed NASA Probe-class mission, will significantly increase our understanding of supermassive black holes undergoing mergers—from kpc to sub-pc scales. In particular, the AXIS point spread function, field of view...

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Autori principali: Foord, Adi (Autore) , Cappelluti, Nico (Autore) , Liu, Tingting (Autore) , Volonteri, Marta (Autore) , Habouzit, Mélanie (Autore) , Pacucci, Fabio (Autore) , Marchesi, Stefano (Autore) , Chen, Nianyi (Autore) , Di Matteo, Tiziana (Autore) , Mallick, Labani (Autore) , Koss, Michael (Autore)
Natura: Article (Journal)
Lingua:inglese
Pubblicazione: 28 May 2024
In: Universe
Year: 2024, Volume: 10, Fascicolo: 6, Pages: 1-20
ISSN:2218-1997
DOI:10.3390/universe10060237
Accesso online:Verlag, kostenfrei, Volltext: https://doi.org/10.3390/universe10060237
Verlag, kostenfrei, Volltext: https://www.mdpi.com/2218-1997/10/6/237
Testo
Note sull'autore:Adi Foord, Nico Cappelluti, Tingting Liu, Marta Volonteri, Melanie Habouzit, Fabio Pacucci, Stefano Marchesi, Nianyi Chen, Tiziana Di Matteo, Labani Mallick and Michael Koss
Descrizione
Riassunto:We present an analysis showcasing how the Advanced X-ray Imaging Satellite (AXIS), a proposed NASA Probe-class mission, will significantly increase our understanding of supermassive black holes undergoing mergers—from kpc to sub-pc scales. In particular, the AXIS point spread function, field of view, and effective area are expected to result in (1) the detection of hundreds to thousands of new dual AGNs across the redshift range 0
Descrizione del documento:Gesehen am 28.02.2025
Descrizione fisica:Online Resource
ISSN:2218-1997
DOI:10.3390/universe10060237

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