about
A test of the nature of cosmic acceleration using galaxy redshift distortions.The dust morphology of the elliptical Galaxy M 86 with SPIREThe star formation histories of galaxies in the Sloan Digital Sky SurveyThe abundance of star-forming galaxies in the redshift range 8.5-12: new results from the 2012 Hubble ultra deep field campaignThe Origin of the Mass‐Metallicity Relation: Insights from 53,000 Star‐forming Galaxies in the Sloan Digital Sky SurveyFaint galaxy evolution via interactionsScience case and requirements for the MOSAIC concept for a multi-object spectrograph for the European Extremely Large TelescopeA deep ALMA image of theHubble Ultra Deep FieldHerschel★-ATLAS: rapid evolution of dust in galaxies over the last 5 billion yearsFIR colours and SEDs of nearby galaxies observed with HerschelGOODS–Herschel: an infrared main sequence for star-forming galaxiesOptical signatures of high-redshift galaxy clustersThe evolving star formation rate: M⋆relation and sSFR since z ≃ 5 from the VUDS spectroscopic surveyStellar mass to halo mass relation from galaxy clustering in VUDS: a high star formation efficiency at z ≃ 3The 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~ 3.3Discovery of a rich proto-cluster atz= 2.9 and associated diffuse cold gas in the VIMOS Ultra-Deep Survey (VUDS)Discovering extremely compact and metal-poor, star-forming dwarf galaxies out toz~ 0.9 in the VIMOS Ultra-Deep SurveyEvidence for major mergers of galaxies at 2 ≲z< 4 in the VVDS and VUDS surveysThe VIMOS VLT Deep Survey final data release: a spectroscopic sample of 35 016 galaxies and AGN out to z ~ 6.7 selected with 17.5 ≤ iAB ≤ 24.75He II emitters in the VIMOS VLT Deep Survey: Population III star formation or peculiar stellar populations in galaxies at 2 <z< 4.6?Comparison of the VIMOS-VLT Deep Survey with the Munich semi-analytical modelThe VIMOS-VLT deep survey: the group catalogueThe VIMOS-VLT Deep Survey: evolution in the halo occupation number since z∼ 1★The Vimos VLT deep survey. Stellar mass segregation and large-scale galaxy environment in the redshift range 0.2 < z < 1.4The VIMOS VLT Deep Survey. Evolution of the major merger rate since z ~ 1 from spectroscopically confirmed galaxy pairsPhysical properties of galaxies and their evolution in the VIMOS VLT Deep SurveyPhysical properties of galaxies and their evolution in the VIMOS VLT Deep SurveyThe VVDS-VLA deep field. IV. Radio-optical propertiesEddington ratios of faint AGN at intermediate redshift: evidence for a population of half-starved black holesThe VVDS-SWIRE-GALEX-CFHTLS surveys: physical properties of galaxies at z below 1.2 from photometric dataThe VIMOS VLT Deep SurveyThe VIMOS VLT Deep Survey. Tracing the galaxy stellar mass assembly history over the last 8 GyrThe Vimos VLT deep surveyThe VIMOS VLT deep survey. The K-band follow-up in the 0226-04 fieldThe VIMOS-VLT Deep Survey (VVDS). The dependence of clustering on galaxy stellar mass at z ~ 1The SWIRE-VVDS-CFHTLS surveys: stellar mass assembly over the last 10 Gyr. Evidence for a major build up of the red sequence between z = 2 and z = 1The VIMOS VLT Deep SurveyVVDS-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
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description
Frans onderzoeker
@nl
French astrophysicist
@en
astrofísico francés
@es
astrophysicien français
@fr
investigador francés
@ast
name
Stéphane Charlot
@ast
Stéphane Charlot
@en
Stéphane Charlot
@es
Stéphane Charlot
@fr
Stéphane Charlot
@nl
Stéphane Charlot
@sl
type
label
Stéphane Charlot
@ast
Stéphane Charlot
@en
Stéphane Charlot
@es
Stéphane Charlot
@fr
Stéphane Charlot
@nl
Stéphane Charlot
@sl
prefLabel
Stéphane Charlot
@ast
Stéphane Charlot
@en
Stéphane Charlot
@es
Stéphane Charlot
@fr
Stéphane Charlot
@nl
Stéphane Charlot
@sl
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P106
P1412
P21
P214
P27
P31
P3762
P496
0000-0003-3458-2275
P734
P735
P7859
lccn-no99011360