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20152025
most citedAssessing Colour-dependent Occupation Statistics Inferred from Galaxy Group Catalogues

101 citations · 168 across the 8 of their papers we have counts for

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Showing 2019Show all

7 papers · 1 filter

astro-ph.CO2019

Generating Synthetic Cosmological Data with GalSampler

Andrew Hearin, Danila Korytov, Eve Kovacs +4

As part of the effort to meet the needs of the Large Synoptic Survey Telescope Dark Energy Science Collaboration (LSST DESC) for accurate, realistically complex mock galaxy catalog…

astro-ph.CO2019

Cosmological Evidence Modelling: a new simulation-based approach to constrain cosmology on non-linear scales

Johannes U. Lange, Frank C. van den Bosch, Andrew R. Zentner +3

Extracting accurate cosmological information from galaxy-galaxy and galaxy-matter correlation functions on non-linear scales () requires cosmologic…

astro-ph.CO2019

CosmoDC2: A Synthetic Sky Catalog for Dark Energy Science with LSST

Danila Korytov, Andrew Hearin, Eve Kovacs +27

This paper introduces cosmoDC2, a large synthetic galaxy catalog designed to support precision dark energy science with the Large Synoptic Survey Telescope (LSST). CosmoDC2 is the…

astro-ph.CO2019

Physical Correlations of the Scatter between Galaxy Mass, Stellar Content, and Halo Mass

Christopher Bradshaw, Alexie Leauthaud, Andrew Hearin +2

We use the UniverseMachine to analyze the source of scatter between the central galaxy mass, the total stellar mass in the halo, and the dark matter halo mass. We also propose a ne…

astro-ph.GA20191 cited

Astro2020: Empirically Constraining Galaxy Evolution

Peter Behroozi, Matthew R. Becker, Frank C. van den Bosch +22

Over the past decade, empirical constraints on the galaxy-dark matter halo connection have significantly advanced our understanding of galaxy evolution. Past techniques have focuse…

astro-ph.GA2019

PRIMUS: Clustering of Star-forming and Quiescent Central Galaxies at

Angela M. Berti, Alison L. Coil, Andrew P. Hearin +1

Previous work has demonstrated that at a given stellar mass, quiescent galaxies are more strongly clustered than star-forming galaxies. The contribution to this signal from central…