Loading...
Le LAM constitue l’un des plus importants instituts de recherche publique en France dans le domaine de l’Astrophysique et associe la recherche fondamentale et le développement d’instrumentation pour les grands télescopes au sol et dans l’espace. Il fait partie de l'Institut OSU Pythéas. Le LAM est une Unité Mixte de Recherche (n°7326) avec comme tutelles le CNRS-INSU, l’Université Aix-Marseille (AMU) et le CNES.
Nos derniers dépôts
Nos dépôts
2 807
Nos notices
3 236
Nos thématiques
Adaptive Optics
Methods observational
Submillimeter ISM
Techniques image processing
Galaxies haloes
Astrophysics - Cosmology and Nongalactic Astrophysics
Gravitational lensing
Photometry
Galaxies kinematics and dynamics
Cosmic background radiation
Dust
Astrophysics - Solar and Stellar Astrophysics
67P/Churyumov-Gerasimenko
Astrophysics
Cosmology
Planets and satellites atmospheres
Techniques spectroscopic
Protoplanetary disks
Galaxies structure
Exoplanets
Methods numerical
Telescopes
High-redshift galaxies
Techniques polarimetric
Ultraviolet galaxies
Data analysis
Galaxy formation
Spectroscopy
Gravitational lensing weak
Stars fundamental parameters
Mass function
Instrumentation high angular resolution
Galaxies formation
Surveys
Astrophysics - Instrumentation and Methods for Astrophysics
Galaxies interactions
Minor planets
Extinction
CD
Neutrino detector
Infrared galaxies
Galaxies stellar content
Galaxies spiral
Galaxies dwarf
Astrophysics - Astrophysics of Galaxies
Infrared ISM
Galaxies starburst
Astrophysics - Earth and Planetary Astrophysics
Galaxies Evolution
Galaxies abundances
Galaxies photometry
Instrumentation adaptive optics
Galaxies clusters individual Virgo
Galaxies fundamental parameters
X-rays galaxies clusters
Galaxies distances and redshifts
Intergalactic medium
Quasars absorption lines
OPTIQUE ADAPTATIVE
H II regions
Planetary systems
Galaxies statistics
Planets and satellites composition
Galaxies general
Adaptive optics
Galaxies active
Galaxy evolution
Gravitational lensing strong
Cosmology observations
Galaxies
Galaxies ISM
Cosmological parameters
Methods statistical
Techniques photometric
Methods data analysis
Planets and satellites fundamental parameters
Star formation
Galaxies star formation
Submillimeter galaxies
Galaxies luminosity function
Comets general
Radiative transfer
Techniques radial velocities
Comets
ANTARES
Supernovae general
Galaxies clusters general
Galaxies evolution
Techniques high angular resolution
Dark matter
Quasars general
Dark energy
Planets and satellites detection
ISM molecules
Large-scale structure of Universe
Galaxies groups general
Stars formation
Galaxies high-redshift
ISM clouds
Catalogs
Nous suivre !
Nos collaborations internationales