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Possible Evidence of the Radio AGN Quenching of Neighboring Galaxies at z 1
Lu Shen, Adam R. Tomczak, Brian C. Lemaux +9
Using 57 Radio Active Galactic nuclei (RAGN) at 0.55 z 1.3 drawn from five fields of the Observations of Redshift Evolution in Large Scale Environments (ORELSE) surve…
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…
The progeny of a Cosmic Titan: a massive multi-component proto-supercluster in formation at z=2.45 in VUDS
O. Cucciati, B. C. Lemaux, G. Zamorani +22
[Abridged] We unveil the complex shape of a proto-supercluster at z~2.45 in the COSMOS field using the spectroscopic redshifts of the VIMOS Ultra-Deep Survey (VUDS), complemented b…
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…