no code implementations • 10 Dec 2020 • Ben Moews, Romeel Davé, Sourav Mitra, Sultan Hassan, Weiguang Cui
In doing so, we are able to recover more properties than the analytic formalism alone can provide, creating a high-speed hydrodynamic simulation emulator that populates galactic dark matter haloes in N-body simulations with baryonic properties.
2 code implementations • 29 Jul 2019 • Francisco Rodríguez Montero, Romeel Davé, Vivienne Wild, Daniel Anglés-Alcázar, Desika Narayanan
We use the Simba cosmological galaxy formation simulation to investigate the relationship between major mergers ($\leq$ 4:1), starbursts, and galaxy quenching.
Astrophysics of Galaxies
no code implementations • 22 Mar 2018 • Mika Rafieferantsoa, Sambatra Andrianomena, Romeel Davé
When we train on mock data from Mufasa and test on RESOLVE, this increases to {\sc rmse}$\sim0. 45$.
Astrophysics of Galaxies
no code implementations • 8 Dec 2017 • Shankar Agarwal, Romeel Davé, Bruce A. Bassett
Our ML framework takes input halo properties including halo mass, environment, spin, and recent growth history, and outputs central galaxy and halo baryonic properties including stellar mass ($M_*$), star formation rate (SFR), metallicity ($Z$), neutral ($\rm HI$) and molecular ($\rm H_2$) hydrogen mass.
Astrophysics of Galaxies