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Star Formation on the scales of galaxies
Star Formation is at the very core of the evolution of galaxies. From their gas reservoir (filled by infall or fusions), stars form at the "Star Formation Rate" (SFR),... -
Study of the physical properties of nearby galaxies seen by Herschel
The Herschel Reference Survey (Boselli et al. 2010b) is a guaranteed time key project aimed at studying the physical properties of the interstellar medium (ISM) of 323... -
The anisotropies of the cosmic infrared backgrounda new tool to probe the evo...
The Cosmic Infrared Background is the contribution of all infrared galaxies integrated on the history of the Universe. It emits between 8 and 1000 um with a peak... -
GRB091127/SN2009nz and the VLT/X-shooter spectroscopy of its host galaxy: pro...
10 pages, 6 figures, accepted for publication in A&A. Major revision on the host metallicity -
Observing GRB host galaxies with the integral field unit of X-shooter
International audience -
Galaxy Counterparts of metal-rich Damped Lyman-alpha Absorbers - I: The case ...
9 pages, 7 figures. Accepted for publication in MNRAS -
Galaxy counterparts of metal-rich damped Lyman-alpha absorbers - II. A solar-...
8 pages, 6 figures, Accepted for publication in MNRAS. 2nd paper in a series for which the first paper is Fynbo et al. (2010), MNRAS, 408, 2128 -
Time resolved spectroscopy of GRB 100418A and its host galaxy with X-shooter
International audience -
Metallicities of high redshift GRB hosts: The case of GRB 100219A
International audience -
VLT/X-shooter spectroscopy of the GRB 090926A afterglow
12 pages, 8 .ps figures, accepted for publication in A&A. Abstract reduced due to space constraints -
Quantum WDM fermions and gravitation determine the observed galaxy structures
14 pages, 2 figures. -
Understanding the star formation modes in the distant universe
The goal of my PhD study consists at attempt to understand what are the main processes at the origin of the star formation in the galaxies over the last 10 billions... -
Evolution of galaxies:<br />interactions, mergers, and gas accretion
Studying present day properties of galaxies can give information both on their past evolution and on the matter content of the Universe. Morphological and kinematical... -
Modelling of the Lyman-alpha emission in high redshift galaxies and cosmologi...
Many galaxies have been detected at high redshift since the late nineties thanks to their strong Lyman-alpha emission line. These objects, knows as Lyman-alpha... -
Relative merits of different types of observations to constrain galaxy physic...
The spectral energy distribution of the light emitted from galaxies across the electromagnetic spectrum contains a myriad of details about the stellar, nebular and... -
Laboratory Studies of Polycyclic Aromatic Hydrocarbons: the Search for Inters...
International audience -
S5 0716+714 : GeV variability study
The GeV observations by Fermi-LAT give us the opportunity to characterize the high-energy emission (100 MeV - 300 GeV) variability properties of the BL Lac object S5... -
The M33 CO(2-1) survey - Star formation and molecular clouds formation
International audience -
Cosmography of the local universe : data processed for the Tully-Fisher relation
This phD thesis is part of the COSFLOS’project. Its goal is to understand the galaxy structure evolution in the local universe. For this purpose, we make use of the... -
The Nearby Supernova Factory
The Nearby Supernova Factory (SNfactory) is an ambitious project to find and study in detail approximately 300 nearby Type Ia supernovae (SNe Ia) at redshifts 0.03<...
