Simulated ELT/HARMONI observations of VCC 1861 show that a 2.5e5 solar mass IMBH (5% of the nuclear cluster mass) can be recovered from stellar kinematics at Virgo distance.
We generated the mock IFS data cube s with the HARMONI Simulation (HSIM a) program [52]
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Extending the simulations of intermediate-mass black hole mass measurements to Virgo Cluster using ELT/HARMONI high resolution integral-field stellar kinematics
Simulated ELT/HARMONI observations of VCC 1861 show that a 2.5e5 solar mass IMBH (5% of the nuclear cluster mass) can be recovered from stellar kinematics at Virgo distance.