about
A test of the nature of cosmic acceleration using galaxy redshift distortions.SPACE: 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 sampleThe molecular hydrogen explorer H2EXLYα FOREST TOMOGRAPHY FROM BACKGROUND GALAXIES: THE FIRST MEGAPARSEC-RESOLUTION LARGE-SCALE STRUCTURE MAP ATz> 2The MUSE Hubble Ultra Deep Field Survey. II. Spectroscopic redshifts and comparisons to color selections of high-redshift galaxiesMirage 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 galaxiesCommissioning and performances of the VLT-VIMOSThe evolving star formation rate: M⋆relation and sSFR since z ≃ 5 from the VUDS spectroscopic surveyExtreme 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 ~ 1Discovering 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 zCOSMOS redshift survey: evolution of the light in bulges and discs since z ~ 0.8zCOSMOS 20k: satellite galaxies are the main drivers of environmental effects in the galaxy population at least to z ∼ 0.7The 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 ≤ 24.75Spot the differenceHe II emitters in the VIMOS VLT Deep Survey: Population III star formation or peculiar stellar populations in galaxies at 2 <z< 4.6?Investigating the relationship between AGN activity and stellar mass in zCOSMOS galaxies at 0 < z < 1 using emission-line diagnostic diagramsMass assembly in quiescent and star-forming galaxies since z ≃ 4 from UltraVISTAObscured AGN at z ~ 1 from the zCOSMOS-Bright SurveyThe colors of central and satellite galaxies in zCOSMOS out to z =~ 0.8 and implications for quenchingEnvironmental effects in the interaction and merging of galaxies in zCOSMOSThe cosmic evolution of oxygen and nitrogen abundances in star-forming galaxies over the past 10 GyrComparison of the VIMOS-VLT Deep Survey with the Munich semi-analytical model
P50
Q34743650-1E64AC40-6EDA-41AC-9409-AE13AF795DCFQ56555882-2C4E8B27-F8CA-4955-8CCA-B248B552780FQ56556487-60EEEDF7-0099-44F0-96F9-84DC45F36710Q56659278-50738A70-C223-4133-BACD-E4015D1DE8E7Q56915486-FED99893-2F24-4CF3-A9FB-D337FC907DFDQ57630642-D341CE57-42BE-469E-8377-5C52D81D1135Q57712676-CAA0AE62-D93F-4AC8-9225-9E48DA2A2994Q57854129-B6D63472-E2A9-40B4-A39A-731106FD65DDQ57854172-50BA2630-EA13-4A41-B340-9652C4BBDB99Q57854278-2010C47B-B375-44F3-9919-55ED00DFBC0BQ57854319-D2F75446-4633-4E0B-9AA2-3C9A785E73CFQ57854385-C9DF646F-CDB5-4D5E-8A54-A92AF43F6A9EQ57854508-7C8E43C2-46AE-4436-AFA4-6A1387846539Q57854525-8EA5AB09-DA6E-4394-984A-D0D7F0D5C062Q57854544-529C8845-FCF2-4446-9A61-0A43B198FCF0Q57854593-0CE392AC-746C-4ECC-9864-D1DBC407FB3DQ57854861-422D9D0A-0520-4694-817D-E1DBF4B149B6Q57855856-71833114-76E2-41AE-BAA6-5FD0EB9B6227Q58035331-689D4C5D-1494-4C7A-9945-BB2B47405D74Q58035338-D384BB8A-DB3B-4F63-A1FB-8158E1C74802Q58035342-D0A235DC-8219-49C3-9772-DF70FD3E93B3Q58035346-41F6FAD2-5D37-4177-B441-FC7D224BA174Q58035356-6B83DB57-322B-46E1-8854-1EBFD70F6766Q58035359-84CD7226-E0A0-4B8A-AEE0-2E2D12930BEFQ58035364-BB3D8B37-D08A-4FFC-955F-591E6EDF5102Q58035367-30567792-3497-477C-99CA-E0C843424DFBQ58035377-0F7ED7DD-CBCC-49A3-8459-5DE94A750857Q58035384-C0FFAEF8-631A-4D16-AAFE-E7817CAFD708Q58035406-F0A06555-C929-4F55-92B6-224E912A1995Q58035425-A640D7B7-438A-4889-A03A-E91BE568A227Q58035436-2A5A3589-1086-4D61-9E62-7B25203E3312Q58035439-A5586ACD-FC4B-46CE-B484-1DCFC8163110Q58035453-3637DE91-D9A7-4795-834A-DE480D522601Q58035458-26628E0E-B34F-42DC-B14A-ABE6CBB85B98Q58035460-F9C9D0AC-66C5-4BF9-88BC-81AC95553326Q58035465-22B672E9-BEC2-4CC2-AE75-9E5430C10DC8Q58035470-5C63D219-D183-47B1-A42D-311A3817719CQ58035474-AA3094D6-AEBB-4EB6-A8E7-758C9C67F95CQ58035484-74539066-D58A-4185-B775-B70E1022527DQ58035486-0A6E1D53-BCBB-4097-8CC4-AE7F70DE9BF2
P50
description
French astrophysicist
@en
astrofisica francese
@it
astrofisikari frantziarra
@eu
astrofísica francesa
@ast
astrofísica francesa
@ca
astrofísica francesa
@es
astrofísica francesa
@gl
astrofísica francesa
@pt
astrophysicienne française
@fr
name
Laurence Tresse
@ast
Laurence Tresse
@de
Laurence Tresse
@en
Laurence Tresse
@es
Laurence Tresse
@fr
Laurence Tresse
@nl
Laurence Tresse
@sl
type
label
Laurence Tresse
@ast
Laurence Tresse
@de
Laurence Tresse
@en
Laurence Tresse
@es
Laurence Tresse
@fr
Laurence Tresse
@nl
Laurence Tresse
@sl
prefLabel
Laurence Tresse
@ast
Laurence Tresse
@de
Laurence Tresse
@en
Laurence Tresse
@es
Laurence Tresse
@fr
Laurence Tresse
@nl
Laurence Tresse
@sl
P106
P1412
P1559
Laurence Tresse
@fr