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*...
Using a sample of ~410,000 galaxies to a depth of IAB=24 over 8.26 deg2 in the Boötes field (~10 tim...
Using galaxy sample observed by the BATC large-field multi-color sky survey and galaxy data of SDSS ...
Using a sample of ~410,000 galaxies to a depth of ${I}_{\mathrm{AB}}=24$ over 8.26 deg2 in the Boöte...
We present the B-band luminosity function and comoving space and luminosity densities for a sample ...
We examine the evolution of the galaxy luminosity function (LF) using a sample of over 2000 galaxies...
We present a detailed empirical assessment of how the galaxy luminosity function and stellar lumino...
We present a detailed empirical assessment of how the galaxy luminosity function and stellar lu...
We present results from the Las Campanas Infrared Survey, designed to identify a statistically signi...
We measure the redshift-dependent luminosity function and the comoving radial density of galaxies in...
In this thesis I investigate galaxy evolution by measuring the luminosity functions of galaxies acro...
In this thesis I investigate galaxy evolution by measuring the luminosity functions of galaxies acro...
Aims. An unbiased and detailed characterization of the galaxy luminosity function (LF) is a basic re...
The cosmic evolution of the field galaxy population has been studied out to a redshift of z ∼ 1 usin...
Using a sample of ~410,000 galaxies to a depth of IAB=24 over 8.26 deg2 in the Boötes field (~10 tim...
Using a sample of ~410,000 galaxies to a depth of IAB=24 over 8.26 deg2 in the Boötes field (~10 tim...
Using a sample of ~410,000 galaxies to a depth of IAB=24 over 8.26 deg2 in the Boötes field (~10 tim...
Using galaxy sample observed by the BATC large-field multi-color sky survey and galaxy data of SDSS ...
Using a sample of ~410,000 galaxies to a depth of ${I}_{\mathrm{AB}}=24$ over 8.26 deg2 in the Boöte...
We present the B-band luminosity function and comoving space and luminosity densities for a sample ...
We examine the evolution of the galaxy luminosity function (LF) using a sample of over 2000 galaxies...
We present a detailed empirical assessment of how the galaxy luminosity function and stellar lumino...
We present a detailed empirical assessment of how the galaxy luminosity function and stellar lu...
We present results from the Las Campanas Infrared Survey, designed to identify a statistically signi...
We measure the redshift-dependent luminosity function and the comoving radial density of galaxies in...
In this thesis I investigate galaxy evolution by measuring the luminosity functions of galaxies acro...
In this thesis I investigate galaxy evolution by measuring the luminosity functions of galaxies acro...
Aims. An unbiased and detailed characterization of the galaxy luminosity function (LF) is a basic re...
The cosmic evolution of the field galaxy population has been studied out to a redshift of z ∼ 1 usin...
Using a sample of ~410,000 galaxies to a depth of IAB=24 over 8.26 deg2 in the Boötes field (~10 tim...
Using a sample of ~410,000 galaxies to a depth of IAB=24 over 8.26 deg2 in the Boötes field (~10 tim...
Using a sample of ~410,000 galaxies to a depth of IAB=24 over 8.26 deg2 in the Boötes field (~10 tim...
Using galaxy sample observed by the BATC large-field multi-color sky survey and galaxy data of SDSS ...
Using a sample of ~410,000 galaxies to a depth of ${I}_{\mathrm{AB}}=24$ over 8.26 deg2 in the Boöte...