The VIMOS-VLT deep survey Evolution of the galaxy luminosity function up to z = 2 in first epoch data - Wikidata - awgldk - TriplyDB

The VIMOS-VLT deep survey Evolution of the galaxy luminosity function up to z = 2 in first epoch data

The VIMOS-VLT deep survey Evolution of the galaxy luminosity function up to z = 2 in first epoch data

http://www.wikidata.org/entity/Q58908105

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Caught in the act: discovery of a physical quasar triplet Geometrical tests of cosmological models I. Probing dark energy using the kinematics of high redshift galaxies FMOS near-IR spectroscopy of Herschel-selected galaxies: star formation rates, metallicity and dust attenuation at z ∼ 1 MASSIV: Mass Assemby Survey with SINFONI in VVDS The VIMOS Public Extragalactic Redshift Survey. Reconstruction of the redshift-space galaxy density field The VIMOS Public Extragalactic Redshift Survey (VIPERS)Discovery of a rich proto-cluster atz= 2.9 and associated diffuse cold gas in the VIMOS Ultra-Deep Survey (VUDS)The VIMOS Public Extragalactic Redshift Survey. Searching for cosmic voids The zCOSMOS redshift survey: evolution of the light in bulges and discs since z ~ 0.8 The VIMOS Public Extragalactic Redshift Survey (VIPERS): A quiescent formation of massive red-sequence galaxies over the past 9 Gyr The VIMOS Public Extragalactic Redshift Survey (VIPERS)The VIMOS Public Extragalactic Redshift Survey (VIPERS)He II emitters in the VIMOS VLT Deep Survey: Population III star formation or peculiar stellar populations in galaxies at 2 <z< 4.6?Mass assembly in quiescent and star-forming galaxies since z ≃ 4 from UltraVISTA Obscured AGN at z ~ 1 from the zCOSMOS-Bright Survey Comparison of the VIMOS-VLT Deep Survey with the Munich semi-analytical model The star formation rate density and dust attenuation evolution over 12 Gyr with the VVDS surveys The VIMOS VLT Deep Survey Comparison of the VIMOS-VLT Deep Survey with the Munich semi-analytical model The zCOSMOS 10k-sample: the role of galaxy stellar mass in the colour-density relation up toz ~ 1 Tracking the impact of environment on the galaxy stellar mass function up toz ~ 1 in the 10 k zCOSMOS sample The zCOSMOS survey: the role of the environment in the evolution of the luminosity function of different galaxy types The zCOSMOS survey. The dependence of clustering on luminosity and stellar mass at $z=0.2$–1 The zCOSMOS redshift survey: the role of environment and stellar mass in shaping the rise of the morphology-density relation from z ~ 1 The VIMOS VLT Deep Survey. Evolution of the major merger rate since z ~ 1 from spectroscopically confirmed galaxy pairs Physical properties of galaxies and their evolution in the VIMOS VLT Deep Survey The VVDS-VLA deep field. IV. Radio-optical properties The zCOSMOS redshift survey: the three-dimensional classification cube and bimodality in galaxy physical properties The VVDS-SWIRE-GALEX-CFHTLS surveys: physical properties of galaxies at z below 1.2 from photometric data The VIMOS VLT Deep Survey The VIMOS VLT Deep Survey. Tracing the galaxy stellar mass assembly history over the last 8 Gyr The VIMOS VLT Deep Survey VVDS-SWIRE. Clustering evolution from a spectroscopic sample of galaxies with redshift 0.2 < z < 2.1 selected from Spitzer IRAC 3.6 {mu}m and 4.5 {mu}m photometry The VVDS type-1 AGN sample: the faint end of the luminosity function The VIMOS-VLT deep survey. Color bimodality and the mix of galaxy populations up to z~2 The VIMOS VLT deep survey Accurate photometric redshifts for the CFHT legacy survey calibrated using the VIMOS VLT deep survey The VIMOS VLT Deep Survey: the build-up of the colour–density relation The VIMOS VLT Deep Survey: the faint type-1 AGN sample Geometrical tests of cosmological models III. The Cosmology-evolution diagram at z = 1

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The VIMOS-VLT deep survey Evolution of the galaxy luminosity function up to z = 2 in first epoch data

http://www.wikidata.org/entity/Q58908105

description

article publié dans la revue scientifique Astronomy and Astrophysics

@fr

im August 2005 veröffentlichter wissenschaftlicher Artikel

@de

wetenschappelijk artikel

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наукова стаття, опублікована в серпні 2005

@uk

name

The VIMOS-VLT deep survey Evol ...... p to z = 2 in first epoch data

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The VIMOS-VLT deep survey Evol ...... p to z = 2 in first epoch data

@nl

type

label

The VIMOS-VLT deep survey Evol ...... p to z = 2 in first epoch data

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The VIMOS-VLT deep survey Evol ...... p to z = 2 in first epoch data

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prefLabel

The VIMOS-VLT deep survey Evol ...... p to z = 2 in first epoch data

@en

The VIMOS-VLT deep survey Evol ...... p to z = 2 in first epoch data

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0004-6361:20041961

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Astronomy and Astrophysics

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The VIMOS-VLT deep survey Evol ...... p to z = 2 in first epoch data

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A. Mazure

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A. Pollo

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B. Marano

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B. Meneux

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C. Adami

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C. Marinoni

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D. Bottini

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D. Maccagni

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D. Rizzo

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F. Lamareille

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P2860

The Galaxy Luminosity Function and Luminosity Density at Redshiftz= 0.1

The evolution of the luminosity functions in the FORS Deep Field from low to high redshift

The GALEXVIMOS-VLT Deep Survey Measurement of the Evolution of the 1500 Å Luminosity Function

The Evolution of the Galaxy Luminosity Function in the Rest-Frame Blue Band up toz=3.5

Measuring the redshift evolution of clustering: the Hubble Deep Field South

The VIMOS VLT deep survey. First epoch VVDS-deep survey: 11564 spectra with 17.5<=I_AB_<=24, and the redshift distribution over 0<=z<=5

The VIMOS VLT Deep Survey

The CNOC2 Field Galaxy Luminosity Function. I. A Description of Luminosity Function Evolution

Bias in the estimation of global luminosity functions

The VIRMOS deep imaging survey

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863–876

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scholarly article

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10.1051/0004-6361:20041961

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3

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439

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Magda Arnaboldi

Marco Scodeggio

Paolo Franzetti

Giovanni Zamorani

Roberto Scaramella

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2005-08-12T00:00:00Z

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astro-ph/0409134

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2005A&A...439..863I

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