The Luminosity Function Of Field Galaxies And Its Evolution Since z=1
arXiv:astro-ph/0012343 · doi:10.1051/0004-6361:20000466
Abstract
We present the B-band luminosity function and comoving space and luminosity densities for a sample of 2779 I-band selected field galaxies based on multi-color data from the CADIS survey. The sample is complete down to I_815 = 22 without correction and with completeness correction extends to I_815=23.0. By means of a new multi-color analysis the objects are classified according to their spectral energy distributions (SEDs) and their redshifts are determined with typical errors of delta z <= 0.03. We have split our sample into four redshift bins between z=0.1 and z=1.04 and into three SED bins E-Sa,Sa-Sc and starbursting (emission line) galaxies. The evolution of the luminosity function is clearly differential with SED. The normalization phi* of luminosity function for the E-Sa galaxies decreases towards higher redshift, and we find evidence that the comoving galaxy space density decreases with redshift as well. In contrast, we find phi* and the comoving space density increasing with redshift for the Sa-Sc galaxies. For the starburst galaxies we find a steepening of the luminosity function at the faint end and their comoving space density increases with redshift.
15 pages, 14 figures, accepted by Astronomy&Astrophysics
References in corpus (13)
- The Evolution of Early-Type Galaxies in Distant Clusters
- The CANADA-FRANCE REDSHIFT SURVEY VI: Evolution of the galaxy luminosity function to z ~ 1
- Evolution of the Hubble Sequence in Hierarchical Models for Galaxy Formation
- Hubble Space Telescope imaging of the CFRS and LDSS redshift surveys - IV. Influence of mergers in the evolution of faint field galaxies from z~1
- Autofib Redshift Survey - I. Evolution of the Galaxy Luminosity Function
- The 2dF Galaxy Redshift Survey: Spectral Types and Luminosity Functions
- Hubble Space Telescope imaging of the CFRS and LDSS redshift surveys II: Structural parameter and the evolution of disk galaxies to z=1
- The CNOC2 Field Galaxy Luminosity Function I: A Description of Luminosity Function Evolution
- HST imaging of CFRS and LDSS galaxies - I: Morphological Properties
- Detection of Strong Evolution in the Population of Early-Type Galaxies
- Hubble Space Telescope Imaging of the CFRS and LDSS Redshift Surveys---III. Field elliptical galaxies at 0.2 < z < 1.0
- The CANADA-FRANCE REDSHIFT SURVEY XI: Morphology of high-redshift field galaxies from high-resolution ground-based imaging
- The local space density of dwarf galaxies
Cited by in corpus (34)
- Galaxy Luminosity Functions to z~1: DEEP2 vs. COMBO-17 and Implications for Red Galaxy Formation
- The COMBO-17 Survey: Evolution of the Galaxy Luminosity Function from 25,000 Galaxies with 0.2<z<1.2
- GEMS: Galaxy Evolution from Morphologies and SEDs
- The Rest-Frame Optical Luminosity Density, Color, and Stellar Mass Density of the Universe from z=0 to z=3
- Cosmological Aspects of Gamma-Ray Bursts: Luminosity Evolution and an Estimate of the Star Formation Rate at High Redshifts
- The evolution of the luminosity functions in the FORS Deep Field from low to high redshift: I. The blue bands
- Improved Cosmological Constraints from Gravitational Lens Statistics
- The Cosmic Lens All-Sky Survey: statistical strong lensing, cosmological parameters, and global properties of galaxy populations
- MAGIICAT I. The MgII Absorber-Galaxy Catalog
- Star forming rates between z=0.25 and z=1.2 from the CADIS emission line survey
- The Las Campanas Infrared Survey. IV. The Photometric Redshift Survey and the Rest-frame R-band Galaxy Luminosity Function at 0.5 <= z <= 1.5
- Shedding Light on the Galaxy Luminosity Function
- Host Galaxies of Gamma-ray Bursts: Spectral Energy Distributions and Internal Extinction
- The ESO-Sculptor Survey: Luminosity functions of galaxies per spectral type at redshifts 0.1-0.5
- Near-IR Galaxy Counts and Evolution from the Wide-Field ALHAMBRA survey
- Evolution of the Luminosity Function and Colors of Galaxies in a Lambda-CDM Universe
- The Galaxy Luminosity Function at z~1 in the HUDF: Probing the Dwarf Population
- Measurement of the expansion rate of the Universe from γ-ray attenuation
- Finding structures in photometric redshift galaxy surveys: An extended friends-of-friends algorithm
- The Luminosity Function of Early-Type Galaxies at z~0.75
- Critical analysis of the luminosity functions per galaxy type measured from redshift surveys
- Limits on the evolution of galaxies from the statistics of gravitational lenses
- GOYA Survey: U and B Number Counts in the Groth-Westphal Strip
- Strong lensing constraints on the velocity dispersion and density profile of elliptical galaxies
- Relative clustering and the joint halo occupation distribution of red-sequence and blue-cloud galaxies in COMBO-17
- Starburst Galaxies and the X-Ray Background
- Exploring the Luminosity Evolution and Stellar Mass Assembly of 2SLAQ Luminous Red Galaxies Between Redshift 0.4 and 0.8
- Restrictions to the galaxy evolutionary models from the Hawaiian Deep Fields SSA13 and SSA22
- Galactic structure from the Calar Alto Deep Imaging Survey (CADIS)
- Introducing the Photometric Maximum Likelihood Method: Galaxy Luminosity Functions at z<1.2 in MUSYC-ECDFS
- The evolution of galaxy clustering since z=1 from the Calar Alto Deep Imaging Survey
- The ESO-Sculptor Survey: Evolution of late-type galaxies at redshifts 0.1-0.5
- Relativistic Cosmology Number Densities and the Luminosity Function
- Discovery of faint double-peak Halpha emission in the halo of low redshift galaxies