469 citations · 1.8k across the 20 of their papers we have counts for
20 papers
Conditional Quenching: A detailed look at the SFR-Density Relation at z ~ 0.9 from ORELSE
Adam R. Tomczak, Brian C. Lemaux, Lori M. Lubin +10
We present a study of the star-formation rate (SFR)-density relation at z ~ 0.9 using data drawn from the Observations of Redshift Evolution in Large Scale Environments (ORELSE) su…
Persistence of the Color-Density Relation and Efficient Environmental Quenching to
Brian C. Lemaux, Adam R. Tomczak, Lori M. Lubin +10
Using ~5000 spectroscopically-confirmed galaxies drawn from the Observations of Redshift Evolution in Large Scale Environments (ORELSE) survey we investigate the relationship betwe…
Searching for Environmental Effects on Galaxy Kinematics in Groups and Clusters at z~1 from the ORELSE Survey
Debora Pelliccia, Brian C. Lemaux, Adam R. Tomczak +9
We present an investigation of the dependence of galaxy kinematics on the environment for a sample of 94 star-forming galaxies at from the ORELSE survey. ORELSE is a lar…
Evaluating Tests of Virialization and Substructure Using Galaxy Clusters in the ORELSE Survey
N. Rumbaugh, B. C. Lemaux, A. R. Tomczak +9
We evaluated the effectiveness of different indicators of cluster virialization using 12 large-scale structures in the ORELSE survey spanning from . We located diffuse X…
Glimpsing the Imprint of Local Environment on the Galaxy Stellar Mass Function
Adam R. Tomczak, Brian C. Lemaux, Lori M. Lubin +8
We investigate the impact of local environment on the galaxy stellar mass function (SMF) spanning a wide range of galaxy densities from the field up to dense cores of massive galax…
The Properties of Radio Galaxies and the Effect of Environment in Large Scale Structures at
Lu Shen, Neal A. Miller, Brian C. Lemaux +8
In this study we investigate 89 radio galaxies that are spectroscopically-confirmed to be members of five large scale structures in the redshift range of . Bas…
Suppressed Star Formation by a Merging Cluster System
Alison S. Mansheim, Brian C. Lemaux, Adam R. Tomczak +7
We examine the effects of an impending cluster merger on galaxies in the large scale structure (LSS) RX J0910 at . Using multi-wavelength data, including 102 spectral mem…
X-Ray Emitting Active Galactic Nuclei from z = 0.6-1.3 in the Intermediate and High-Density Environments of the ORELSE Survey
N. Rumbaugh, B. Lemaux, A. Tomczak +8
We studied AGN activity in twelve LSSs in the ORELSE survey, at 0.65<z<1.28, using a combination of Chandra observations, optical and NIR imaging and spectroscopy. We located a tot…
Chronos and Kairos: Mosfire Observations of Post-Starburst Galaxies in z~1 Clusters and Groups
Brian C. Lemaux, Adam R. Tomczak, Lori M. Lubin +5
In this study we present the exploration of 500 spectroscopically confirmed galaxies in and around two large scale structures at drawn from the ORELSE survey. A sub-…
H0LiCOW V. New COSMOGRAIL time delays of HE0435-1223: to 3.8% precision from strong lensing in a flat CDM model
V. Bonvin, F. Courbin, S. H. Suyu +15
We present a new measurement of the Hubble Constant H0 and other cosmological parameters based on the joint analysis of three multiply-imaged quasar systems with measured gravitati…
H0LiCOW IV. Lens mass model of HE 0435-1223 and blind measurement of its time-delay distance for cosmology
Kenneth C. Wong, Sherry H. Suyu, Matthew W. Auger +13
Strong gravitational lenses with measured time delays between the multiple images allow a direct measurement of the time-delay distance to the lens, and thus a measure of cosmologi…
H0LiCOW II. Spectroscopic survey and galaxy-group identification of the strong gravitational lens system HE0435-1223
D. Sluse, A. Sonnenfeld, N. Rumbaugh +15
Galaxies located in the environment or on the line of sight towards gravitational lenses can significantly affect lensing observables, and can lead to systematic errors on the meas…
H0LiCOW I. Lenses in COSMOGRAIL's Wellspring: Program Overview
S. H. Suyu, V. Bonvin, F. Courbin +21
Strong gravitational lens systems with time delays between the multiple images allow measurements of time-delay distances, which are primarily sensitive to the Hubble constant that…
Radio Monitoring Campaigns of Six Strongly Lensed Quasars
N. Rumbaugh, C. D. Fassnacht, J. P. McKean +3
We observed six strongly lensed, radio-loud quasars (MG 0414+0534, CLASS B0712+472, JVAS B1030+074, CLASS B1127+385, CLASS B1152+199, and JVAS B1938+666) in order to identify syste…
Strong Lens Time Delay Challenge: II. Results of TDC1
Kai Liao, Tommaso Treu, Phil Marshall +23
We present the results of the first strong lens time delay challenge. The motivation, experimental design, and entry level challenge are described in a companion paper. This paper…
Star Formation Quenching in High-redshift Large-scale Structure: Post-starburst Galaxies in the Cl1604 Supercluster at
Po-Feng Wu, Roy R. Gal, Brian C. Lemaux +4
The Cl1604 supercluster at is one of the most extensively studied high redshift large scale structures, with more than 500 spectroscopically confirmed members. It cons…
Strong Lens Time Delay Challenge: I. Experimental Design
Gregory Dobler, Christopher Fassnacht, Tommaso Treu +5
The time delays between point-like images in gravitational lens systems can be used to measure cosmological parameters. The number of lenses with measured time delays is growing ra…
The Violent Youth of Bright and Massive Cluster Galaxies and their Maturation over 7 Billion Years
Begoña Ascaso, Brian C. Lemaux, Lori M. Lubin +4
In this study we investigate the formation and evolution mechanisms of the brightest cluster galaxies (BCGs) over cosmic time. At high redshift (), we selected BCGs and m…
The X-ray-Optical Relations for Nine Clusters at z = 0.7-1.1
Nick Rumbaugh, Dale D. Kocevski, Roy R. Gal +4
We use Chandra observations of nine optically and X-ray selected clusters in five different structures at z ~ 0.7-1.1 from the Observations of Redshift Evolution in Large-Scale Env…
The Evolution and Environments of X-ray Emitting Active Galactic Nuclei in High-Redshift Large-Scale Structures
Nick A. Rumbaugh, Dale D. Kocevski, Roy R. Gal +5
We use deep Chandra imaging and an extensive optical spectroscopy campaign on the Keck 10-m telescopes to study the properties of X-ray point sources in five large-scale structures…