136 citations · 405 across the 6 of their papers we have counts for
10 papers
CLEAR II: Evidence for Early Formation of the Most Compact Quiescent Galaxies at High Redshift
Vicente Estrada-Carpenter, Casey Papovich, Ivelina Momcheva +11
The origin of the correlations between mass, morphology, quenched fraction, and formation history in galaxies is difficult to define, primarily due to the uncertainties in galaxy s…
Figuring Out Gas & Galaxies in Enzo (FOGGIE). III. The Mocky Way: Investigating Biases in Observing the Milky Way's Circumgalactic Medium
Yong Zheng, Molly S. Peeples, Brian W. O'Shea +6
The circumgalactic medium (CGM) of the Milky Way is mostly obscured by nearby gas in position-velocity space because we reside inside the Galaxy. Substantial biases exist in most s…
HST Imaging of the Ionizing Radiation from a Star-forming Galaxy at z = 3.794
Zhiyuan Ji, Mauro Giavalisco, Eros Vanzella +17
We report on the HST detection of the Lyman-continuum (LyC) radiation emitted by a galaxy at redshift z=3.794, dubbed Ion1 (Vanzella et al. 2012). The LyC from Ion1 is detected at…
Studying the Physical Properties of Tidal Features I. Extracting Morphological Substructure in CANDELS Observations and VELA Simulations
Kameswara Bharadwaj Mantha, Daniel H. McIntosh, Cody P. Ciaschi +17
The role of major mergers in galaxy evolution remains a key open question. Existing empirical merger identification methods use non-parametric and subjective visual classifications…
Understanding the circumgalactic medium is critical for understanding galaxy evolution
Molly S. Peeples, Peter Behroozi, Rongmon Bordoloi +69
Galaxies evolve under the influence of gas flows between their interstellar medium and their surrounding gaseous halos known as the circumgalactic medium (CGM). The CGM is a major…
Distinguishing Mergers and Disks in High Redshift Observations of Galaxy Kinematics
Raymond C. Simons, Susan A. Kassin, Gregory F. Snyder +9
The majority of massive star-forming galaxies at have velocity gradients suggestive of rotation, in addition to large amounts of disordered motions. In this paper, we demo…