In TNG and EAGLE simulations, central and high-mass satellite galaxies are best predicted to quench by black hole mass while low-mass satellites by halo mass, yielding opposite predictions for detecting environmental quenching with MOONRISE.
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Environmental vs. intrinsic quenching at cosmic noon: Predictions from cosmological hydrodynamical simulations for VLT-MOONRISE
In TNG and EAGLE simulations, central and high-mass satellite galaxies are best predicted to quench by black hole mass while low-mass satellites by halo mass, yielding opposite predictions for detecting environmental quenching with MOONRISE.