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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| Main Authors: | , , , , , , , , , , |
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| Format: | Article (Journal) |
| Language: | English |
| Published: |
28 May 2024
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| In: |
Universe
Year: 2024, Volume: 10, Issue: 6, Pages: 1-20 |
| ISSN: | 2218-1997 |
| DOI: | 10.3390/universe10060237 |
| Online Access: | Verlag, kostenfrei, Volltext: https://doi.org/10.3390/universe10060237 Verlag, kostenfrei, Volltext: https://www.mdpi.com/2218-1997/10/6/237 |
| Author Notes: | Adi Foord, Nico Cappelluti, Tingting Liu, Marta Volonteri, Melanie Habouzit, Fabio Pacucci, Stefano Marchesi, Nianyi Chen, Tiziana Di Matteo, Labani Mallick and Michael Koss |
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| 520 | |a 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 | ||
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