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The DESI Experiment Part II: Instrument Design
DESI Collaboration, Amir Aghamousa, Jessica Aguilar +290
DESI (Dark Energy Spectropic Instrument) is a Stage IV ground-based dark energy experiment that will study baryon acoustic oscillations and the growth of structure through redshift…
The DESI Experiment Part I: Science,Targeting, and Survey Design
DESI Collaboration, Amir Aghamousa, Jessica Aguilar +290
DESI (Dark Energy Spectroscopic Instrument) is a Stage IV ground-based dark energy experiment that will study baryon acoustic oscillations (BAO) and the growth of structure through…
The SDSS-IV eBOSS: emission line galaxy catalogues at z=0.8 and study of systematic errors in the angular clustering
T. Delubac, A. Raichoor, J. Comparat +17
We present two wide-field catalogs of photometrically-selected emission line galaxies (ELGs) at z=0.8 covering about 2800 deg^2 over the south galactic cap. The catalogs were obtai…
The evolution of the [OII], Hβ and [OIII] emission-line luminosity functions over the last nine billions years
Johan Comparat, Guangtun Zhu, Violeta Gonzalez-Perez +12
Emission line galaxies are one of the main tracers of the large-scale structure to be targeted by the next-generation dark energy surveys. To provide a better understanding of the…
Size growth of red-sequence early-type galaxies in clusters in the last 10 Gyr
S. Andreon, Hui Dong, A. Raichoor
We carried out a photometric and structural analysis in the rest-frame band of a mass-selected () sample of red-sequence galaxies in 14 galaxy clusters, 6…