The processes that rapidly quench massive galaxies and maintain their quiescence remain poorly understood. Substantial molecular gas reservoirs can survive this shutdown in post-starburst galaxies, raising the question of what prevents the remaining gas from efficiently forming stars. We present deep, subarcsecond VLA...
V. D'Onofrio, J. Spilker, K. Smith et al.· 0 citations
The discovery of a population of massive, ancient quiescent galaxies within the first 2 Gyr of the Universe’s history has led to significant tensions with models of galaxy formation. However, these analyses are often based on slit spectroscopy, which typically captures only the centermost region of these galaxies and,...
S. Cutler, Luke Robbins, D. Marchesini et al.· Astrophysical Journal Letter...· 1 citation
One of the fundamental uncertainties in the study of galaxies at the interface between star formation and quiescence--post-starburst galaxies--is their instantaneous star formation rate. While these galaxies appear quiescent in the rest UV-optical, many of the youngest systems are highly CO luminous, implying dense mol...
D. Setton, J. Greene, R. Bezanson et al.· 0 citations
We present spectrally resolved structural parameter measurements of 28,274 sources from the legacy lensing field of A2744, quantifying global structures from the observed 0.7−4.8 μm and spanning rest-frame UV to near-infrared (NIR) at R ∼ 15. These measurements are made on imaging mosaics mainly from the UNCOVER/MegaSc...
Yunchong Zhang, T. Miller, S. Price et al.· Astrophysical Journal Supple...· 0 citations
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