Cavendish Astrophysics
REACH uses advanced Bayesian tools (eg. PolyChord nested sampling) in combination with state of the art physics rooted instrument, foreground and cosmological models for the data analysis.
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The dynamics of parsec-scale eccentric stellar disks around SMBHs in galactic nuclei: disk disruption mechanisms, tidal disruption events and milliparsec stars
Exploring the atmospheric structure of water-rich sub-Neptunes
Hierarchical star cluster assembly boosts intermediate-mass black hole formation