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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.
Nos derniers dépôts
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B. Hernández-Martín, T. Schrabback, H. Hoekstra, N. Martinet, J. Hlavacek-Larrondo, et al.. Constraining the masses of high-redshift clusters with weak lensing: Revised shape calibration testing for the impact of stronger shears and increased blending. Astronomy and Astrophysics - A&A, 2020, 640, pp.A117. ⟨10.1051/0004-6361/202037844⟩. ⟨hal-02905288⟩
Nos dépôts
2 754
Nos notices
3 273
Nos thématiques
Techniques radial velocities
Galaxies general
Galaxies clusters individual Virgo
Dark energy
Galaxy formation
Catalogs
Galaxies interactions
Instrumentation high angular resolution
Galaxies Evolution
ANTARES
Techniques polarimetric
Galaxies active
Gravitational lensing
Planetary systems
Planets and satellites fundamental parameters
Cosmology
Star formation
Methods data analysis
Galaxies luminosity function
Radiative transfer
Surveys
Adaptive Optics
Minor planets
H II regions
Techniques image processing
Galaxies ISM
Submillimeter ISM
Neutrino detector
Galaxies star formation
Methods numerical
Galaxies photometry
Astrophysics - Cosmology and Nongalactic Astrophysics
Astrophysics - Astrophysics of Galaxies
Protoplanetary disks
Quasars absorption lines
Galaxies distances and redshifts
Adaptive optics
Dark matter
Galaxies kinematics and dynamics
Quasars general
Astrophysics - Instrumentation and Methods for Astrophysics
Cosmological parameters
Infrared galaxies
Techniques high angular resolution
Comets general
Galaxies
Photometry
Galaxies structure
Galaxies dwarf
Ultraviolet galaxies
ISM clouds
67P/Churyumov-Gerasimenko
Cosmology observations
Spectroscopy
Planets and satellites atmospheres
Astrophysics
Instrumentation adaptive optics
Astrophysics - Solar and Stellar Astrophysics
Galaxies clusters general
Methods observational
Submillimeter galaxies
Galaxies statistics
Gravitational lensing weak
Galaxies spiral
Data analysis
Techniques photometric
Dust
Infrared ISM
Large-scale structure of Universe
Galaxies high-redshift
Galaxies groups general
Extinction
Methods statistical
Stars formation
Planets and satellites composition
Galaxies abundances
Supernovae general
OPTIQUE ADAPTATIVE
ISM molecules
Stars fundamental parameters
Galaxies fundamental parameters
Gravitational lensing strong
X-rays galaxies clusters
Cosmic background radiation
CD
Comets
Astrophysics - Earth and Planetary Astrophysics
Planets and satellites detection
Galaxies stellar content
Galaxy evolution
Galaxies starburst
Galaxies formation
Mass function
High-redshift galaxies
Exoplanets
Techniques spectroscopic
Galaxies haloes
Telescopes
Intergalactic medium
Galaxies evolution
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Nos collaborations internationales