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.
Kinematic extracting Firstly, we used the V oronoi binning method to merge adjacent pixels and achieve a signal-to-noise ratio 𝑆/𝑁 ≳ 20 for each bin using the vorbin package [73]
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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.