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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
2 703
Nos notices
3 294
Nos thématiques
Astrophysics
Cosmological parameters
Quasars absorption lines
Techniques high angular resolution
Techniques image processing
Ultraviolet galaxies
Galaxies clusters general
High-redshift galaxies
Galaxies abundances
Intergalactic medium
X-rays galaxies clusters
Galaxies Evolution
Infrared galaxies
Gravitational lensing weak
Planets and satellites detection
Large-scale structure of Universe
Neutrino detector
Galaxies active
Adaptive optics
Dark energy
Extinction
Catalogs
Dark matter
Quasars general
Astrophysics - Astrophysics of Galaxies
Infrared ISM
Galaxies kinematics and dynamics
Astrophysics - Cosmology and Nongalactic Astrophysics
Protoplanetary disks
Galaxies evolution
Galaxy evolution
Galaxies general
Planets and satellites fundamental parameters
Comets
H II regions
Galaxies fundamental parameters
ISM clouds
Instrumentation adaptive optics
Galaxies groups general
Methods observational
Gravitational lensing strong
Galaxies spiral
Planets and satellites composition
Galaxies high-redshift
Spectroscopy
Planetary systems
Cosmology observations
Galaxies structure
Radiative transfer
Supernovae general
Gravitational lensing
Cosmic background radiation
Exoplanets
Techniques spectroscopic
Galaxies star formation
Galaxies formation
Individual
Galaxy formation
Astrophysics - Solar and Stellar Astrophysics
Methods data analysis
Galaxies stellar content
Telescopes
Galaxies haloes
Galaxies ISM
Mass function
Galaxies starburst
Galaxies
Planets and satellites atmospheres
Stars formation
Dust
Methods statistical
Comets general
Submillimeter ISM
67P/Churyumov-Gerasimenko
CD
Surveys
Galaxies clusters individual Virgo
OPTIQUE ADAPTATIVE
Galaxies luminosity function
Photometry
Techniques photometric
Methods numerical
Stars fundamental parameters
Data analysis
Submillimeter galaxies
Galaxies photometry
ISM molecules
Galaxies statistics
Adaptive Optics
Techniques radial velocities
Galaxies dwarf
Techniques polarimetric
Instrumentation high angular resolution
Galaxies distances and redshifts
ANTARES
Cosmology
Astrophysics - Instrumentation and Methods for Astrophysics
Astrophysics - Earth and Planetary Astrophysics
Star formation
Galaxies interactions
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Nos collaborations internationales