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
about
Cosmic voids and void lensing in the Dark Energy Survey Science Verification dataRedshift distributions of galaxies in the Dark Energy Survey Science Verification shear catalogue and implications for weak lensingGeometrical tests of cosmological models I. Probing dark energy using the kinematics of high redshift galaxiesA mature cluster with X-ray emission atz= 2.07The KMOS Redshift One Spectroscopic Survey (KROSS): dynamical properties, gas and dark matter fractions of typicalz∼ 1 star-forming galaxiesA relationship between specific star formation rate and metallicity gradient within z ∼ 1 galaxies from KMOS-HiZELSJKCS 041: a colour-detected galaxy cluster at $z_{\mathrm{phot}}$ ~ 1.9 with deep potential well as confirmed by X-ray dataEvidence against a supervoid causing the CMB Cold SpotGalaxy And Mass Assembly (GAMA): stellar mass estimatesGalaxy and Mass Assembly (GAMA): the red fraction and radial distribution of satellite galaxiesNew spectroscopic redshifts from the CDFS and a test of the cosmological relevance of the GOODS-South fieldOTELO survey: deep BVRI broad-band photometry of the Groth strip. I. Number counts and two-point correlation functionsOn using angular cross-correlations to determine source redshift distributionsFMOS near-IR spectroscopy of Herschel-selected galaxies: star formation rates, metallicity and dust attenuation at z ∼ 1The galaxy–halo connection from a joint lensing, clustering and abundance analysis in the CFHTLenS/VIPERS fieldCFHTLenS: the relation between galaxy dark matter haloes and baryons from weak gravitational lensingCFHTLenS: the Canada–France–Hawaii Telescope Lensing Survey – imaging data and catalogue productsCFHTLenS tomographic weak lensing: quantifying accurate redshift distributionsVery weak lensing in the CFHTLS wide: cosmology from cosmic shear in the linear regimeCosmic shear analysis with CFHTLS deep dataPhotometric redshift analysis in the Dark Energy Survey Science Verification dataCombining Dark Energy Survey Science Verification data with near-infrared data from the ESO VISTA Hemisphere SurveyThe WiggleZ Dark Energy Survey: Final data release and cosmological resultsThe intriguing life of star-forming galaxies in the redshift range 1 ≤ z ≤ 2 using MASSIVMASSIV: Mass Assembly Survey with SINFONI in VVDSMASSIV: Mass Assembly Survey with SINFONI in VVDSMASSIV: Mass Assembly Survey with SINFONI in VVDSMASSIV: Mass Assembly Survey with SINFONI in VVDSMASSIV: Mass Assemby Survey with SINFONI in VVDSIntegral field spectroscopy with SINFONI of VVDS galaxiesThe VIMOS Ultra-Deep Survey: ~10 000 galaxies with spectroscopic redshifts to study galaxy assembly at early epochs 2 < z ≃ 6The VIMOS Ultra-Deep Survey (VUDS): fast increase in the fraction of strong Lyman-α emitters from z = 2 to z = 6VIMOS Ultra-Deep Survey (VUDS): Witnessing the assembly of a massive cluster atz~ 3.3Evidence for major mergers of galaxies at 2 ≲z< 4 in the VVDS and VUDS surveysThe VIMOS Public Extragalactic Redshift Survey (VIPERS) - from the galaxy clustering ratio measured at z ~1The VIMOS Public Extragalactic Redshift Survey (VIPERS): A quiescent formation of massive red-sequence galaxies over the past 9 GyrSpot the differenceThe 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?
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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
description
article publié dans la revue scientifique Astronomy and Astrophysics
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im August 2005 veröffentlichter wissenschaftlicher Artikel
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wetenschappelijk artikel
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наукова стаття, опублікована в серпні 2005
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The VIMOS VLT deep survey. Fir ...... hift distribution over 0<=z<=5
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The VIMOS VLT deep survey. Fir ...... hift distribution over 0<=z<=5
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The VIMOS VLT deep survey. Fir ...... hift distribution over 0<=z<=5
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The VIMOS VLT deep survey. Fir ...... hift distribution over 0<=z<=5
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prefLabel
The VIMOS VLT deep survey. Fir ...... hift distribution over 0<=z<=5
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The VIMOS VLT deep survey. Fir ...... hift distribution over 0<=z<=5
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The VIMOS VLT deep survey. Fir ...... hift distribution over 0<=z<=5
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C. Marinoni
D. Bottini
D. Maccagni
F. Lamareille
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10.1051/0004-6361:20041960
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2005-08-12T00:00:00Z
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astro-ph/0409133
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2005A&A...439..845L