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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
2 803
Nos notices
3 240
Nos thématiques
Methods numerical
Spectroscopy
Galaxies star formation
Galaxies dwarf
ISM molecules
ISM clouds
Surveys
Instrumentation high angular resolution
Data analysis
Galaxies clusters individual Virgo
Galaxies evolution
Planetary systems
Minor planets
Galaxies photometry
Galaxies spiral
Radiative transfer
Supernovae general
Galaxies high-redshift
Galaxies kinematics and dynamics
Submillimeter ISM
Ultraviolet galaxies
Techniques spectroscopic
Planets and satellites detection
Astrophysics - Astrophysics of Galaxies
Astrophysics - Earth and Planetary Astrophysics
Protoplanetary disks
Photometry
OPTIQUE ADAPTATIVE
Large-scale structure of Universe
Stars formation
Cosmology observations
Submillimeter galaxies
Methods statistical
Exoplanets
Cosmic background radiation
Gravitational lensing
Techniques high angular resolution
Intergalactic medium
Comets
Infrared ISM
Techniques radial velocities
High-redshift galaxies
Galaxies interactions
Telescopes
Galaxies abundances
Instrumentation adaptive optics
Neutrino detector
Adaptive Optics
Galaxy formation
Techniques polarimetric
Galaxies Evolution
Galaxies starburst
Astrophysics - Cosmology and Nongalactic Astrophysics
Galaxies general
Planets and satellites atmospheres
Catalogs
Galaxies distances and redshifts
Galaxies active
Planets and satellites composition
Galaxies stellar content
Extinction
Star formation
Cosmology
Cosmological parameters
Galaxies fundamental parameters
67P/Churyumov-Gerasimenko
Dark energy
X-rays galaxies clusters
Galaxies luminosity function
CD
Galaxies structure
Comets general
Adaptive optics
Gravitational lensing weak
Galaxies haloes
Quasars absorption lines
Infrared galaxies
Galaxies
Planets and satellites fundamental parameters
Gravitational lensing strong
Methods data analysis
Quasars general
Galaxies clusters general
Dust
H II regions
Astrophysics
Galaxy evolution
Galaxies statistics
Mass function
Methods observational
Galaxies formation
Stars fundamental parameters
Techniques photometric
ANTARES
Astrophysics - Instrumentation and Methods for Astrophysics
Astrophysics - Solar and Stellar Astrophysics
Techniques image processing
Galaxies groups general
Galaxies ISM
Dark matter
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Nos collaborations internationales