activity
19962023
most citedFinal Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant

3.3k citations · 18.5k across the 133 of their papers we have counts for

collaborators

133 papers

astro-ph.GA2023★ 2 cited

LATIS: The Stellar Mass-Metallicity Relation of Star-forming Galaxies at

Nima Chartab, Andrew B. Newman, Gwen C. Rudie +2

We present the stellar mass - stellar metallicity relation for 3491 star-forming galaxies at using rest-frame far-ultraviolet (FUV) spectra from the Ly…

astro-ph.GA2023

Confirmation of a Substantial Discrepancy between Radio and UV--IR Measures of the Star Formation Rate Density at 0.2 < z < 1.3

A. M Matthews, D. D. Kelson, A. B. Newman +6

We present the initial sample of redshifts for 3,839 galaxies in the MeerKAT DEEP2 field -- the deepest 1.4\,GHz radio field yet observed. Using a spectrophotometric techniqu…

astro-ph.GA2023★ 26 cited

Fraction of Clumpy Star-Forming Galaxies at in UVCANDELS: Dependence on Stellar Mass and Environment

Zahra Sattari, Bahram Mobasher, Nima Chartab +25

High-resolution imaging of galaxies in rest-frame UV has revealed the existence of giant star-forming clumps prevalent in high redshift galaxies. Studying these sub-structures prov…

astro-ph.GA2023★ 10 cited

Constraints on Fluctuating Star Formation Rates for Intermediate-mass Galaxies with H and UV Luminosities

Shannon G. Patel, Daniel D. Kelson, Louis E. Abramson +2

We study the recent star formation histories (SFHs) of 575 intermediate-mass galaxies (IMGs, ) in COSMOS at by comparing their H$α…

astro-ph.GA2022

UV Slopes At All Redshifts Are Consistent with H=1 Stochastic Star Formation Histories

Daniel D. Kelson, Louis E. Abramson

Multiple investigations support describing galaxy growth as a stochastic process with correlations over a range of timescales governed by a parameter, , empirically and theoreti…

astro-ph.GA2022★ 24 cited

A population of ultraviolet-dim protoclusters detected in absorption

Andrew B. Newman, Gwen C. Rudie, Guillermo A. Blanc +8

Galaxy protoclusters, which will eventually grow into the massive clusters we see in the local universe, are usually traced by locating overdensities of galaxies. Large spectroscop…