Spectral fitting of The Cliff LRD with Bagpipes yields a BH*-like solution with a low-mass metal-poor host, moderate dust, smooth star formation history, and high BH-to-stellar mass ratio.
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Two z~6.6 galaxies host overmassive black holes and show remnant ionized bubbles from recent quasar episodes, with BH-to-stellar mass ratios 400-800 times above the local relation.
JWST broad-line AGN lack X-ray and high-ionization signatures, consistent with super-Eddington accretion that suppresses those emissions without heavy dust.
A large collaboration compiles and compares merger rate predictions for massive black holes across multiple galaxy formation models to forecast LISA detections and quantify uncertainties.
Clustered dark matter may enable small seed black holes to grow to over 10^7 solar masses by redshift 10 in dense nuclear star clusters, with special behavior for ultralight dark matter due to its de Broglie wavelength.
citing papers explorer
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Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff
Spectral fitting of The Cliff LRD with Bagpipes yields a BH*-like solution with a low-mass metal-poor host, moderate dust, smooth star formation history, and high BH-to-stellar mass ratio.
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Life After the Quasar: Overmassive Black Holes and Remnant Ionised Bubbles in and Around Two z~6.6 Galaxies
Two z~6.6 galaxies host overmassive black holes and show remnant ionized bubbles from recent quasar episodes, with BH-to-stellar mass ratios 400-800 times above the local relation.
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The case for super-Eddington accretion in JWST broad-line AGN during the first billion years
JWST broad-line AGN lack X-ray and high-ionization signatures, consistent with super-Eddington accretion that suppresses those emissions without heavy dust.
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The LISA Astrophysics MBHcatalogues Project: A comparison of predictions of simulated massive black hole binaries
A large collaboration compiles and compares merger rate predictions for massive black holes across multiple galaxy formation models to forecast LISA detections and quantify uncertainties.
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Dark Matter and the Early Formation of Supermassive Black Holes
Clustered dark matter may enable small seed black holes to grow to over 10^7 solar masses by redshift 10 in dense nuclear star clusters, with special behavior for ultralight dark matter due to its de Broglie wavelength.