Gas-rich galaxies follow a single Schechter stellar mass function; abundance matching the HI and stellar mass functions yields a selection-corrected M_HI-M_star relation.
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Nonparametric conditional density estimation packages and diagnostics are released for Python and R, with applications to photometric redshifts and likelihood-free cosmology.
Composite cluster stellar mass functions show marginal M* evolution at high z and a factor of 2.5 growth in stellar mass fraction from z=0.8 to 0.2 after accounting for halo mass growth.
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The Stellar Mass Function of Gas-Rich Galaxies and the Underlying $M_{\rm HI}-M_{\rm star}$ Scaling Relation in the Local Universe
Gas-rich galaxies follow a single Schechter stellar mass function; abundance matching the HI and stellar mass functions yields a selection-corrected M_HI-M_star relation.
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Conditional Density Estimation Tools in Python and R with Applications to Photometric Redshifts and Likelihood-Free Cosmological Inference
Nonparametric conditional density estimation packages and diagnostics are released for Python and R, with applications to photometric redshifts and likelihood-free cosmology.
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The Atacama Cosmology Telescope: stellar mass growth in massive galaxy clusters from DR5 over the past 7 billion years
Composite cluster stellar mass functions show marginal M* evolution at high z and a factor of 2.5 growth in stellar mass fraction from z=0.8 to 0.2 after accounting for halo mass growth.