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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.
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Nos dépôts
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Nos notices
3 277
Nos thématiques
Planets and satellites composition
Neutrino detector
Mass function
Submillimeter galaxies
Quasars general
Spectroscopy
Surveys
Supernovae general
Galaxies distances and redshifts
Planets and satellites detection
Stars formation
Galaxies haloes
Astrophysics - Solar and Stellar Astrophysics
Photometry
Instrumentation high angular resolution
Adaptive optics
Galaxies Evolution
Stars fundamental parameters
Methods statistical
Galaxies ISM
Radiative transfer
Astrophysics - Instrumentation and Methods for Astrophysics
Gravitational lensing
Instrumentation adaptive optics
Telescopes
Galaxies structure
CD
Galaxies star formation
Galaxies spiral
Astrophysics - Astrophysics of Galaxies
Methods observational
Galaxies stellar content
Planets and satellites fundamental parameters
Ultraviolet galaxies
ISM molecules
Galaxies dwarf
Dark energy
Techniques image processing
ISM clouds
Astrophysics - Earth and Planetary Astrophysics
Dust
Gravitational lensing weak
Galaxies starburst
Extinction
Galaxies
Galaxies interactions
Galaxies kinematics and dynamics
67P/Churyumov-Gerasimenko
Galaxies fundamental parameters
Galaxies clusters general
Exoplanets
Techniques spectroscopic
Galaxies groups general
Intergalactic medium
Infrared galaxies
Galaxies statistics
Techniques high angular resolution
Astrophysics - Cosmology and Nongalactic Astrophysics
X-rays galaxies clusters
Submillimeter ISM
Comets
Techniques radial velocities
Galaxies high-redshift
Galaxy evolution
Planets and satellites atmospheres
Protoplanetary disks
Catalogs
Galaxy formation
Cosmology
Astrophysics
Galaxies luminosity function
Cosmology observations
Star formation
Galaxies clusters individual Virgo
Comets general
Adaptive Optics
Galaxies general
Dark matter
Planetary systems
Galaxies abundances
Methods data analysis
Techniques photometric
Galaxies formation
Quasars absorption lines
H II regions
Cosmological parameters
Infrared ISM
Large-scale structure of Universe
Galaxies photometry
Galaxies active
Cosmic background radiation
ANTARES
Minor planets
Methods numerical
High-redshift galaxies
Data analysis
OPTIQUE ADAPTATIVE
Techniques polarimetric
Gravitational lensing strong
Galaxies evolution
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Nos collaborations internationales