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