The Observations of Redshift Evolution in Large Scale Environments

The ORELSE survey is a wide-field survey dedicated to studying galaxy evolution across the full range of local environments with extensive photometric and spectroscopic observations of multiple well-known galaxy overdensities at z ~ 1. Recently, we move to higher redshift universe. The goal is to study the cluster evolution by linking these proto-Large Scale Structures (LSSs) to LSSs at z~1. To be continued.

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The ORELSE survey

-- the sacred one

  • Map Out Large Scale Structure at z~1
  • Galaxy evolution across all environments
  • Relationship between color, star formation, stellar mass, morphology, and density
  • Developing new methods to detect and characterize structure
  • The triggering and co-evolution of Active Galactic Nuclei (AGN) activity
  • Characterizing the virialization state of clusters
  • Galaxy dynamics
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The C3VO survey

-- the golden one

Charting Cluster Construction with VUDS and ORELSE

  • Mapping the growth of structure from z~0.5 to z~5
  • Probing the evolution of galaxies in LSSs across cosmic time
  • Develop detection methods to find forming clusters (protoclusters)
  • Detection biases for proto-clusters using different galaxy types
  • Relationship between, color, star-formation, stellar mass, AGN activity, and density
  • Characterizing the virialization state of protoclusters
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Lori Lubin1, Brian Lemaux1, Roy Gal2, Lu Shen1,3, Denise Hung2, Olga Cucciati4, Ben Forrest1, Ekta Shah1, Debora Pelliccia5, Olivier Le Fèvre6, Christopher D. Fassnacht1, Adam Tomczak1, Po-Feng Wu7, Dale Kocevski8, Gordon Squires9

1University of California, Davis, 2University of Hawai’i, 3University of Science and Technology of China, 4INAF - Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, 5University of California, Santa Crus, 6Aix-Marseille Univ, 7National Astronomical Observatory of Japan, 8Colby College, 9California Institute of Technology.

Dogs in the ORELSE family

Luna, Fitz


Hoku, Naia, and Akira