Estimating black hole spin from AGN SED fitting: the impact of general-relativistic ray tracing
(2023)
Journal Article
Hagen, S., & Done, C. (2023). Estimating black hole spin from AGN SED fitting: the impact of general-relativistic ray tracing. Monthly Notices of the Royal Astronomical Society, 525(3), 3455-3467. https://doi.org/10.1093/mnras/stad2499
Accretion disc model fitting to optical/UV quasar spectra requires that the highest mass black holes have the highest spin, with implications on the hierarchical growth of supermassive black holes and their host galaxies over cosmic time. However, th... Read More about Estimating black hole spin from AGN SED fitting: the impact of general-relativistic ray tracing.