about
Is 3C324 the first gravitationally lensed giant galaxy?Peculiar morphology of the high-redshift radio galaxies 3C 13 and 3C 256 in subarcsecond seeingGeometrical tests of cosmological models I. Probing dark energy using the kinematics of high redshift galaxiesALMA spectroscopic survey in the Hubble Ultra Deep Field: survey descriptionSPACE: the spectroscopic all-sky cosmic explorerzCOSMOS: A Large VLT/VIMOS Redshift Survey Covering 0 <z< 3 in the COSMOS FieldProto-groups at 1.8 < z < 3 in the zCOSMOS-deep sampleScience case and requirements for the MOSAIC concept for a multi-object spectrograph for the European Extremely Large TelescopeFirst Data Release of the COSMOS Lyα Mapping and Tomography Observations: 3D Lyα Forest Tomography at 2.05 < z < 2.55Detection of z ∼ 2.3 Cosmic Voids from 3D Lyα Forest Tomography in the COSMOS FieldShadow of a colossus: a z = 2.44 galaxy protocluster detected in 3D Ly{alpha}Forest tomographic mapping of the COSMOS fieldLYα FOREST TOMOGRAPHY FROM BACKGROUND GALAXIES: THE FIRST MEGAPARSEC-RESOLUTION LARGE-SCALE STRUCTURE MAP ATz> 2The galaxy–halo connection from a joint lensing, clustering and abundance analysis in the CFHTLenS/VIPERS fieldAutomated reliability assessment for spectroscopic redshift measurementsMirage simulations of the massiv sampleMASSIV: Mass Assembly Survey with SINFONI in VVDS. VI. Metallicity-related fundamental relations in star-forming galaxies at 1<z<2The 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 VVDSProbing the Mass Assembly and Chemical Evolution of high-z Galaxies with MASSIVIntegral field spectroscopy with SINFONI of VVDS galaxiesMass and kinematics of late-type galaxies (1.3 < z < 3.3) from the VVDSThe VLT‐VIRMOS Mask Manufacturing UnitThe VIMOS Public Extragalactic Redshift Survey. Reconstruction of the redshift-space galaxy density fieldThe evolving star formation rate: M⋆relation and sSFR since z ≃ 5 from the VUDS spectroscopic surveyThe VIMOS Public Extragalactic Redshift Survey (VIPERS)Extreme emission-line galaxies out toz~ 1 in zCOSMOSStellar 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)The dependence of galactic outflows on the properties and orientation of zCOSMOS galaxies at z ~ 1The VIMOS Public Extragalactic Redshift Survey. Searching for cosmic voidsDiscovering extremely compact and metal-poor, star-forming dwarf galaxies out toz~ 0.9 in the VIMOS Ultra-Deep SurveyThe VIMOS Public Extragalactic Redshift Survey (VIPERS)Evidence for major mergers of galaxies at 2 ≲z< 4 in the VVDS and VUDS surveys
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description
Frans astrofysicus
@nl
French astrophysicist
@en
astrofísico francés
@es
astrophysicien français
@fr
name
Olivier Le Fèvre
@ast
Olivier Le Fèvre
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Olivier Le Fèvre
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Olivier Le Fèvre
@fr
Olivier Le Fèvre
@nl
Olivier Le Fèvre
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Olivier Le Fèvre
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Olivier Le Fèvre
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Olivier Le Fèvre
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Olivier Le Fèvre
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Olivier Le Fèvre
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Olivier Le Fèvre
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O. Le Fevre
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O. Le Fèvre
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Olivier Le Fevre
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Olivier Le Fèvre
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Olivier Le Fèvre
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Olivier Le Fèvre
@es
Olivier Le Fèvre
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Olivier Le Fèvre
@nl
Olivier Le Fèvre
@sl
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P496
0000-0001-5891-2596