Laurence Tresse
Tresse, Laurence, 19..-...., astronome
![Sudoc [ABES], France](/viaf/images/flags/SUDOC.png "Sudoc [ABES], France")
VIAF ID: 211201943 (Personal)
Permalink: http://viaf.org/viaf/211201943
Preferred Forms
4xx's: Alternate Name Forms (3)
Works
| Title | Sources |
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| Catalog-free modeling of galaxy types in deep survey images : massive dimensional reduction with neural networks |
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| Clustering redshift : une nouvelle fenêtre sur l'univers |
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| Clustering redshifts : a new window through the Universe. |
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| The colors of central and satellite galaxies in zCOSMOS out to z =~ 0.8 and implications for quenching |
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| COSMOS photometric redshifts with 30-Bands for 2-deg^2^ |
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| DEEP SPECTROCOPIC SURVEY IN I OF FIELD GALAXIES: LUMINOSITY FUNCTION AT Z LESS THAN 1.3, NATURE OF GALAXIES AT Z LESS THAN 0.3. |
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| THE DEPENDENCE OF GALACTIC OUTFLOWS ON THE PROPERTIES AND ORIENTATION OF zCOSMOS GALAXIES ATz∼ 1 |
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| DISSECTING PHOTOMETRIC REDSHIFT FOR ACTIVE GALACTIC NUCLEUS USINGXMM- ANDCHANDRA-COSMOS SAMPLES |
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| Etude de la cinématique des galaxies sur une période de 8 milliards d'années. |
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| Etude de la morphologie de galaxies lointaines à partir de grands relevés en imagerie infrarouge depuis le sol |
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| Étude des sources de la réionisation dans la simulation SPHINX |
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| Formation and evolution of galaxy populations up to high redshift. |
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| Formation et évolution de populations de galaxies à grand décalage spectral : fonctions de luminosité du relevé VVDS |
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| From dark halos to light : proceedings of the XLIst Rencontres de Moriond : La Thuile, Aosta Valley Italy, March 11-18, 2006 |
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| Les galaxies de faible masse vues par MUSE et l'amplification gravitationnelle |
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| Galaxy evolution in dense environments observed by the IFS MUSE, a kinematic approach |
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| Inférence de l'évolution photométrique et en taille des galaxies au moyen d'images simulées. |
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| Inferring the photometric and size evolution of galaxies from image simulations |
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| Kinematics of COSMOS star-forming galaxies over the last eight billion years |
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| Low mass galaxies seen by MUSE and gravitational lensing. |
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| Lyman alpha haloes of distant galaxies revealed by MUSE : analysis of the circum-galactic medium. |
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| LYα FOREST TOMOGRAPHY FROM BACKGROUND GALAXIES: THE FIRST MEGAPARSEC-RESOLUTION LARGE-SCALE STRUCTURE MAP ATz> 2 |
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| Morphologies of distant galaxies from large cosmological surveys using ground based NIR imaging. |
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| AN OPTICAL GROUP CATALOG TOz= 1 FROM THE zCOSMOS 10 k SAMPLE |
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| Precise modeling of massive galaxies clusters observed by Hubble and MUSE. |
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| Properties and environment of radio-emitting galaxies in the VLA-zCOSMOS survey |
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| Propriétés Résolues des Galaxies Fortement Lentillées |
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| Proto-groups at 1.8 < z < 3 in the zCOSMOS-deep sample |
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| Pseudo-bulge formation in intermediate-mass local spiral galaxies via gas-rich major mergers. |
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| The radial and azimuthal profiles of Mg II absorption around 0.5 < z < 0.9 zCOSMOS galaxies of different colors, masses, and environments |
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| Recent stellar mass assembly of low-mass star-forming galaxies at redshifts 0.3 < z < 0.9 |
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| RELEVE SPECTROSCOPIQUE PROFOND EN I DE GALAXIES DE CHAMP : FONCTION DE LUMINOSITE A Z INFERIEUR A 1.3, NATURE DES GALAXIES A Z INFERIEUR A 0.3 |
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| Resolved properties of high redshift lensed galaxies. |
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| Searching for environmental effects on galaxy kinematics in groups and clusters at z ∼ 1 from the ORELSE survey |
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| SHARDS: a global view of the star formation activity at z ~ 0.84 and z ~ 1.23 |
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| SHARDS: an optical spectro-photometric survey of distant galaxies |
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| SHARDS: stellar populations and star formation histories of a mass-selected sample of 0.65 < z < 1.1 galaxies |
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| A simultaneous search for high-z LAEs and LBGs in the SHARDS survey |
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| The spatial clustering of X-ray selected AGN in the XMM-COSMOS field |
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| Spot the difference |
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| Star formation, metallicity and dust properties derived from the StromloAPM galaxy survey spectra |
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| Teenage galaxies |
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| TheGALEX-VVDS Measurement of the Evolution of the Far-Ultraviolet Luminosity Density and the Cosmic Star Formation Rate |
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| TheXMM‐NewtonWide‐Field Survey in the COSMOS Field. I. Survey Description |
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| Tracking the impact of environment on the galaxy stellar mass function up toz ~ 1 in the 10 k zCOSMOS sample |
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| Transfert radiatif dans les galaxies à Grand Redshift |
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| Ultraluminous X-ray sources out to z ~ 0.3 in the COSMOS field |
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| Understanding the shape of the galaxy two-point correlation function at z ≃ 1 in the COSMOS field |
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| Unveiling the hidden side of the first 3 billion years of galaxy formation |
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| The Very Large Telescope Visible Multi‐Object Spectrograph Mask Preparation Software |
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| The VIMOS Ultra Deep Survey first data release: Spectra and spectroscopic redshifts of 698 objects up to zspec ~ 6 in CANDELS |
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| The VIMOS Ultra-Deep Survey (VUDS): fast increase in the fraction of strong Lyman-α emitters from z = 2 to z = 6 |
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| VIMOS Ultra-Deep Survey (VUDS): IGM transmission towards galaxies with 2.5 <z< 5.5 and the colour selection of high-redshift galaxies |
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| VIMOS Ultra-Deep Survey (VUDS): Witnessing the assembly of a massive cluster atz~ 3.3 |
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| The VIRMOS-VLT Deep Survey |
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| The VVDS Data‐Reduction Pipeline: Introducing VIPGI, the VIMOS Interactive Pipeline and Graphical Interface |
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| VVDS-SWIRE |
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| 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 |
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| The VVDS-VLA deep field. IV. Radio-optical properties |
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| Where's the matter : tracing dark and bright matter with the new generation of large-scale surveys |
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| The XMM-LSS survey: optical assessment and properties of different X-ray selected cluster classes |
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| THE zCOSMOS 10k-BRIGHT SPECTROSCOPIC SAMPLE |
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| zCOSMOS 20k: satellite galaxies are the main drivers of environmental effects in the galaxy population at least to z ∼ 0.7 |
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| zCOSMOS: A Large VLT/VIMOS Redshift Survey Covering 0 <z< 3 in the COSMOS Field |
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| The zCOSMOS-Bright survey: the clustering of early and late galaxy morphological types since z≃ 1 |
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| The zCOSMOS redshift survey: evolution of the light in bulges and discs since z ~ 0.8 |
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| The zCOSMOS redshift survey: how group environment alters global downsizing trends |
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| The zCOSMOS redshift survey: the role of environment and stellar mass in shaping the rise of the morphology-density relation from z ~ 1 |
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| The zCOSMOS redshift survey: the three-dimensional classification cube and bimodality in galaxy physical properties |
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| The zCOSMOS survey. The dependence of clustering on luminosity and stellar mass at $z=0.2$–1 |
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| The zCOSMOS survey: the role of the environment in the evolution of the luminosity function of different galaxy types |
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