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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
2 766
Nos notices
3 269
Nos thématiques
Techniques polarimetric
Adaptive Optics
ANTARES
Comets
Large-scale structure of Universe
Catalogs
Surveys
Ultraviolet galaxies
Gravitational lensing
Neutrino detector
Galaxies active
Galaxies starburst
Galaxies general
Radiative transfer
Comets general
X-rays galaxies clusters
Galaxies abundances
Gravitational lensing strong
Infrared ISM
Techniques radial velocities
Planets and satellites fundamental parameters
Galaxy evolution
Submillimeter galaxies
Galaxies clusters general
Techniques high angular resolution
Planets and satellites atmospheres
Instrumentation adaptive optics
Planets and satellites composition
Galaxies haloes
ISM clouds
Astrophysics - Instrumentation and Methods for Astrophysics
Infrared galaxies
Star formation
Galaxies Evolution
Galaxies luminosity function
Astrophysics - Solar and Stellar Astrophysics
Dark energy
Astrophysics
Galaxies distances and redshifts
Supernovae general
Techniques image processing
OPTIQUE ADAPTATIVE
Dark matter
Astrophysics - Astrophysics of Galaxies
Galaxies star formation
Astrophysics - Earth and Planetary Astrophysics
67P/Churyumov-Gerasimenko
Gravitational lensing weak
Spectroscopy
Planets and satellites detection
Instrumentation high angular resolution
Methods numerical
Galaxies evolution
Galaxies ISM
ISM molecules
Cosmic background radiation
High-redshift galaxies
Methods statistical
Galaxies formation
Astrophysics - Cosmology and Nongalactic Astrophysics
Galaxies clusters individual Virgo
Galaxies dwarf
Galaxies structure
Data analysis
Exoplanets
Galaxies kinematics and dynamics
Photometry
Methods observational
Mass function
Galaxies
Methods data analysis
Adaptive optics
Protoplanetary disks
Quasars general
Extinction
Cosmology observations
Galaxies stellar content
H II regions
Techniques photometric
Planetary systems
Galaxies high-redshift
Galaxies fundamental parameters
Galaxies interactions
Submillimeter ISM
Intergalactic medium
Galaxies spiral
Techniques spectroscopic
Telescopes
Galaxies statistics
Stars formation
Galaxy formation
Stars fundamental parameters
Quasars absorption lines
Cosmology
Cosmological parameters
Minor planets
CD
Galaxies photometry
Dust
Galaxies groups general
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Nos collaborations internationales