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GALAXY STELLAR MASS ASSEMBLY BETWEEN 0.2 < z < 2 FROM THE S-COSMOS SURVEYBased on observations with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, which is operated by AURA Inc., under NASA contract NAS 5-26555. Also based on observations made with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under NASA contract 1407. Also based on data collected at: the Subaru Telescope, which is operated by the National Astronomical Observatory of Japan; the XMM-Newton, an ESA science mission with instruments and contributions directly funded by ESA Member States and NASA; the European Southern Observatory under Large Program 175.A-0839, Chile; Kitt Peak National Observatory, Cerro Tololo Inter-American Observatory, and the National Optical Astronomy Observatory, which are operated by the Association of Universities for Research in Astronomy, Inc. (AURA) under cooperative agreement with the National Science Foun
Online Contents | 2010| -
Accurate photometric redshifts for the CFHT legacy survey calibrated using the VIMOS VLT deep survey
Online Contents | 2006| -
Stellar mass and velocity functions of galaxies
Free accessBackward evolution and the fate of Milky Way siblingsEDP Sciences | 2010| -
Stellar mass and velocity functions of galaxies. Backward evolution and the fate of Milky Way siblings
British Library Online Contents | 2010| -
Photometric redshifts for the CFHTLS T0004 deep and wide fields
British Library Online Contents | 2009| -
The cosmic star formation rate evolution from z = 5 to z = 0 from the VIMOS VLT deep survey
British Library Online Contents | 2007| -
ASPIC and GAZPAR : National Resources for Observations in Astronomy-Astrophysics at CeSAM
British Library Conference Proceedings | 2019| -
Rest-frame far-ultraviolet to far-infrared view of Lyman break galaxies at z = 3: Templates and dust attenuation⋆
Free accessEDP Sciences | 2019| -
Rest-frame FUV-to-FIR view of Lyman break galaxies at $z\sim3$: Templates and dust attenuation
Free accessArXiv | 2019| -
The VIMOS-VLT deep survey. Evolution of the galaxy luminosity function up to z = 2 in first epoch data
British Library Online Contents | 2005| -
The VIMOS-VLT Deep Survey. Galaxy luminosity function per morphological type up to z = 1.2
British Library Online Contents | 2006|
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