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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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Hauptverfasser: Foord, Adi (VerfasserIn) , Cappelluti, Nico (VerfasserIn) , Liu, Tingting (VerfasserIn) , Volonteri, Marta (VerfasserIn) , Habouzit, Mélanie (VerfasserIn) , Pacucci, Fabio (VerfasserIn) , Marchesi, Stefano (VerfasserIn) , Chen, Nianyi (VerfasserIn) , Di Matteo, Tiziana (VerfasserIn) , Mallick, Labani (VerfasserIn) , Koss, Michael (VerfasserIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: 28 May 2024
In: Universe
Year: 2024, Jahrgang: 10, Heft: 6, Pages: 1-20
ISSN:2218-1997
DOI:10.3390/universe10060237
Online-Zugang:Verlag, kostenfrei, Volltext: https://doi.org/10.3390/universe10060237
Verlag, kostenfrei, Volltext: https://www.mdpi.com/2218-1997/10/6/237
Volltext
Verfasserangaben:Adi Foord, Nico Cappelluti, Tingting Liu, Marta Volonteri, Melanie Habouzit, Fabio Pacucci, Stefano Marchesi, Nianyi Chen, Tiziana Di Matteo, Labani Mallick and Michael Koss
Beschreibung
Zusammenfassung: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
Beschreibung:Gesehen am 28.02.2025
Beschreibung:Online Resource
ISSN:2218-1997
DOI:10.3390/universe10060237

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