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
2 692
Nos notices
3 297
Nos thématiques
Telescopes
High-redshift galaxies
Planetary systems
ISM clouds
Astrophysics - Astrophysics of Galaxies
Cosmological parameters
Planets and satellites detection
Techniques spectroscopic
Extinction
Large-scale structure of Universe
Galaxies kinematics and dynamics
Galaxies general
Galaxies dwarf
Stars fundamental parameters
Dark matter
Methods data analysis
Intergalactic medium
CD
Ultraviolet galaxies
Planets and satellites fundamental parameters
X-rays galaxies clusters
Astrophysics - Cosmology and Nongalactic Astrophysics
H II regions
Infrared ISM
Surveys
Radiative transfer
Adaptive optics
Galaxies ISM
Cosmology
Gravitational lensing weak
Galaxies clusters individual Virgo
Gravitational lensing strong
Astrophysics
Galaxies haloes
Cosmic background radiation
Catalogs
Galaxies groups general
Galaxy formation
Photometry
Galaxies photometry
Galaxies structure
Galaxies luminosity function
Galaxies active
Exoplanets
Neutrino detector
OPTIQUE ADAPTATIVE
Methods numerical
Methods statistical
Dust
67P/Churyumov-Gerasimenko
Star formation
Mass function
Planets and satellites composition
Galaxies evolution
Techniques polarimetric
Galaxies fundamental parameters
Instrumentation adaptive optics
Galaxies statistics
Dark energy
Galaxies Evolution
Astrophysics - Earth and Planetary Astrophysics
Spectroscopy
Quasars general
Supernovae general
Galaxies spiral
Comets general
Techniques image processing
ISM molecules
Techniques radial velocities
Techniques high angular resolution
Galaxies interactions
Galaxies formation
Galaxies
Protoplanetary disks
Stars formation
Data analysis
Gravitational lensing
Galaxies star formation
Galaxy evolution
Galaxies stellar content
Galaxies clusters general
Galaxies abundances
Instrumentation high angular resolution
Galaxies high-redshift
Galaxies distances and redshifts
Quasars absorption lines
Adaptive Optics
Planets and satellites atmospheres
ANTARES
Interstellar medium
Methods observational
Cosmology observations
Submillimeter ISM
Galaxies starburst
Comets
Astrophysics - Solar and Stellar Astrophysics
Astrophysics - Instrumentation and Methods for Astrophysics
Infrared galaxies
Techniques photometric
Submillimeter galaxies
Nous suivre !
Nos collaborations internationales