44 citations · 118 across the 4 of their papers we have counts for
9 papers
Resolved Multi-element Stellar Chemical Abundances in the Brightest Quiescent Galaxy at z 2
Marziye Jafariyazani, Andrew B. Newman, Bahram Mobasher +3
Measuring the chemical composition of galaxies is crucial to our understanding of galaxy formation and evolution models. However, such measurements are extremely challenging for qu…
Gravity and the Nonlinear Growth of Structure in the Carnegie-Spitzer-IMACS Redshift Survey
Daniel D. Kelson, Louis E. Abramson, Andrew J. Benson +6
A key obstacle to developing a satisfying theory of galaxy evolution is the difficulty in extending analytic descriptions of early structure formation into full nonlinearity, the r…
Wide-Field Optical Spectroscopy of Abell 133: A Search for Filaments Reported in X-ray Observations
Thomas Connor, Daniel D. Kelson, John Mulchaey +7
Filaments of the cosmic web have long been associated with the threadlike structures seen in galaxy redshift surveys. However, despite their baryon content being dominated by hot g…
Testing the Breathing Mode in Intermediate Mass Galaxies and its Predicted Star Formation Rate-Size Anti-Correlation
Shannon G. Patel, Daniel D. Kelson, Nicholas Diao +2
Recent hydrodynamical simulations predict that stellar feedback in intermediate mass galaxies (IMGs) can drive strong fluctuations in structure (e.g., half-light radius, ). Th…
Resolving Quiescent Galaxies at : II. Direct Measures of Rotational Support
Andrew B. Newman, Sirio Belli, Richard S. Ellis +1
Stellar kinematics provide insights into the masses and formation histories of galaxies. At high redshifts, spatially resolving the stellar kinematics of quiescent galaxies is chal…
Resolving Quiescent Galaxies at : I. Search for Gravitationally Lensed Sources and Characterization of their Structure, Stellar Populations, and Line Emission
Andrew B. Newman, Sirio Belli, Richard S. Ellis +1
Quiescent galaxies at are compact and have weak or absent emission lines, making it difficult to spatially resolve their kinematics and stellar populations using grou…