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Abstract:

This paper presents a self-consistent analysis combining 2D stellar dynamics and strong gravitational lensing to precisely measure the supermassive black hole (SMBH) at the center of the Cosmic Horseshoe gravitational lens system (at redshift z=0.44).

Using integral-field spectroscopy from MUSE and high-resolution Hubble Space Telescope imaging, the study simultaneously models the galaxy's central mass distribution, including a central point mass, and its stellar kinematics. Bayesian model comparison decisively (5-sigma) detects an ultramassive black hole (UMBH) with a mass of log10(MBH/M☉) = 10.56+0.07−0.08, a result robust across various systematic tests.

This finding places the Cosmic Horseshoe's SMBH approximately 1.5 standard deviations above the established M-sigma (SMBH mass vs. host galaxy velocity dispersion) relation. This supports an emerging trend observed in other massive galaxies and brightest cluster galaxies, suggesting a steeper M-sigma relationship at the highest mass end, potentially indicating different co-evolutionary pathways for these systems. The study highlights the power of combining lensing and dynamics for SMBH detection in the distant Universe and anticipates future discoveries that will refine our understanding of galaxy and SMBH co-evolution.

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