We present new determinations of the stellar-to-halo mass relation (SHMR) at z= 0–10 that
match the evolution of the galaxy stellar mass function, the star formation rate (SFR)–M …

Calculating the galaxy merger rate requires both a census of galaxies identified as merger
candidates and a cosmologically averaged" observability" timescale< T obs (z)> for …

We perform a detailed analysis of the resolved colors and stellar populations of a complete
sample of 323 star-forming galaxies (SFGs) at 0.5< z< 1.5 and 326 SFGs at 1.5< z< 2.5 in …

We use a suite of semi-empirical models to predict the galaxy–galaxy merger rate and
relative contributions to bulge growth as a function of mass (both halo and stellar), redshift …

At fixed galaxy stellar mass, there is a clear observational connection between structural
asymmetry and offset from the star-forming main sequence, ΔSFMS. Herein, we use the …

We investigate the spatial structure and evolution of star formation and the interstellar
medium (ISM) in interacting galaxies. We use an extensive suite of parsec-scale galaxy …

A fundamental feature of galaxies is their structure, yet we are just now understanding the
evolution of structural properties in quantitative ways. As such, we explore the quantitative …

Different theoretical methodologies lead to order-of-magnitude variations in predicted galaxy–
galaxy merger rates. We examine how this arises and quantify the dominant uncertainties …

We use a large sample of∼ 350 000 galaxies constructed by combining the UKIDSS UDS,
VIDEO/CFHT-LS, UltraVISTA/COSMOS and GAMA survey regions to probe the major (1: 4 …

We measure the merger fraction of massive galaxies using the UltraVISTA/COSMOS
catalog, complemented with the deeper, higher resolution 3DHST+ CANDELS catalog …