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The black hole occupation fraction of local dwarf galaxies with AXIS

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arxiv 2311.09161 v1 pith:KM5YGLOA submitted 2023-11-15 astro-ph.HE astro-ph.GA

Elena Gallo , Edmund Hodges-Kluck , Tommaso Treu , Vivienne Baldassare , Anil Seth , Jenny Greene , Fabio Pacucci , Richard Plotkin
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Amy Reines Belinda Wilkes
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keywords blackgalaxiesaxisdwarffractionholeslocalachieved
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The fraction of local dwarf galaxies that hosts massive black holes is arguably the cleanest diagnostic of the dominant seed formation mechanism of today's supermassive black holes. A 5 per cent constraint on this quantity can be achieved with AXIS observations of 3300 galaxies across the mass spectrum through a combination of serendipitous extra-galactic fields plus a dedicated 1 Msec GO program.

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  1. Probability of gravitational-wave lensing by intermediate-mass black holes and globular clusters

    astro-ph.CO 2026-08 conditional novelty 6.0 of 10

    The rate of compound gravitational-wave lensing by intermediate-mass black holes in globular clusters is at most about 10^-3 of galaxy-scale lensed events, disfavoring GW231123 as such an event.

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