activity
20172019
most citedSimba: Cosmological Simulations with Black Hole Growth and Feedback

1.1k citations · 1.1k across the 2 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2019

Classifying galaxies according to their HI content

Sambatra Andrianomena, Mika Rafieferantsoa, Romeel Davé

We use machine learning to classify galaxies according to their HI content, based on both their optical photometry and environmental properties. The data used for our analyses are…

astro-ph.GA20191.1k cited

Simba: Cosmological Simulations with Black Hole Growth and Feedback

Romeel Davé, Daniel Anglés-Alcázar, Desika Narayanan +3

We introduce the Simba simulations, the next generation of the Mufasa cosmological galaxy formation simulations run with Gizmo's meshless finite mass hydrodynamics. Simba includes…

astro-ph.GA2018

Timescales for Hi consumption and SFR depletion of satellite galaxies in groups

Mika Rafieferantsoa, Romeel Davé, Thorsten Naab

We investigate the connection between the HI~content, SFR and environment of galaxies using a hydrodynamic simulation that incorporates scaling relations for galactic wind and a he…

astro-ph.GA2018

IQ-Collaboratory 1.1: the Star-Forming Sequence of Simulated Central Galaxies

ChangHoon Hahn, Tjitske K. Starkenburg, Ena Choi +12

A tightly correlated star formation rate-stellar mass relation of star forming galaxies, or star-forming sequence (SFS), is a key feature in galaxy property-space that is predicted…

astro-ph.GA2018

Predicting the Neutral Hydrogen Content of Galaxies From Optical Data Using Machine Learning

Mika Rafieferantsoa, Sambatra Andrianomena, Romeel Davé

We develop a machine learning-based framework to predict the HI content of galaxies using more straightforwardly observable quantities such as optical photometry and environmental…

astro-ph.GA201717 cited

Mufasa:The strength and evolution of galaxy conformity in various tracers

Mika Rafieferantsoa, Romeel Davé

We investigate galaxy conformity using the Mufasa cosmological hydrodynamical simulation. We show a bimodal distribution in galaxy colour with radius, albeit with too many low-mass…