The DEEP2 Galaxy Redshift Survey: The Galaxy Luminosity Function to z ~ 1
arXiv:astro-ph/0506041 · doi:10.1086/505455
Abstract
The evolution of the B-band galaxy luminosity function is measured using a sample of more than 11,000 galaxies with spectroscopic redshifts from the DEEP2 Redshift Survey. The rest-frame M_B versus U-B color-magnitude diagram of DEEP2 galaxies shows that the color-magnitude bi-modality seen in galaxies locally is still present at redshifts z > 1. Dividing the sample at the trough of this color bimodality into predominantly red and blue galaxies, we find that the luminosity function of each galaxy color type evolves differently. Blue counts tend to shift to brighter magnitudes at constant number density, while the red counts remain largely constant at a fixed absolute magnitude. Using Schechter functions with fixed faint-end slopes we find that M*_B for blue galaxies brightens by ~ 1.3 magnitudes per unit redshift, with no significant evolution in number density. For red galaxies M*_B brightens somewhat less with redshift, while the formal value of phi* declines. When the population of blue galaxies is subdivided into two halves using the rest-frame color as the criterion, the measured evolution of both blue subpopulations is very similar.
Accepted by ApJ, emulateapj format, 24 pages, 17 figures, 4 in JPEG, includes referee's comments
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- Stellar populations of galaxies in the ALHAMBRA survey up to . III. The stellar content of the quiescent galaxy population during the last Gyr
- Tracing Recent Star Formation of Red Early-type Galaxies out to 1
- Stellar populations of a sample of far-IR AGN and non-AGN green valley galaxies
- Spectroscopy of Luminous Compact Blue Galaxies in Distant Clusters II. Physical Properties of dE Progenitor Candidates
- Direct determination of oxygen abundances in line emitting star-forming galaxies at intermediate redshift
- The WiggleZ Dark Energy Survey: Galaxy Evolution at 0.25 < z < 0.75 Using The Second Red-Sequence Cluster Survey (RCS-2)
- HST Hα grism spectroscopy of ROLES: a flatter low-mass slope for the z~1 SSFR--mass relation
- Joint Modelling of Astrophysical Systematics for Cosmology with LSST Cosmic Shear
- Searching for low-redshift faint galaxies with MMT/Hectospec
- A study on the multicolour evolution of Red Sequence galaxy populations: insights from hydrodynamical simulations and semi-analytical models
- Unravelling the orbits of cluster galaxy populations according to their dominant gas ionization source
- Active Galactic Nuclei in the Green Valley at z0.7
- CATS: Optical to Near-Infrared Colors of the Bulge and Disk of Two z=0.7 Galaxies Using HST and Keck Laser Adaptive Optics Imaging
- Empirically-Driven Multiwavelength K-corrections At Low Redshift
- Completeness III: identifying characteristic systematics and evolution in galaxy redshift surveys
- Optical Observations and Modeling of the Superluminous Supernova 2018lfe
- The galaxy luminosity function in the LAMOST Complete Spectroscopic Survey of Pointing Area at the Southern Galactic Cap
- The Evolution of the Luminosity Function for Luminous Compact Blue Galaxies to z=1
- Oxford SWIFT IFS and multi-wavelength observations of the Eagle galaxy at z=0.77
- Past, present and Future of the Scaling Relations of Galaxies and Active Galactic Nuclei
- Evidence for merging or disruption of red galaxies from the evolution of their clustering
- On the quenching of star formation in observed and simulated central galaxies: Evidence for the role of integrated AGN feedback
- Galaxy Environments in DEEP2: The Birth of the Red Sequence
- The Star Formation History and Stellar Assembly of High Redshift Galaxies
- Quantifying the Poor Purity and Completeness of Morphological Samples Selected by Galaxy Colour
- The satellite population around luminous red galaxies in the 25 square degree DESI Legacy Imaging Surveys Early Data Release
- A z1 galactic-scale outflow transversally mapped to 50 kpc through gravitational-arc tomography
- Photometric Selection of a Massive Galaxy Catalog with