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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
2 757
Nos notices
3 275
Nos thématiques
67P/Churyumov-Gerasimenko
Galaxy evolution
Cosmic background radiation
Submillimeter galaxies
X-rays galaxies clusters
Comets general
Galaxies interactions
Techniques image processing
Astrophysics - Solar and Stellar Astrophysics
Planetary systems
Infrared ISM
Galaxies high-redshift
Cosmological parameters
High-redshift galaxies
Galaxies dwarf
Supernovae general
ANTARES
Catalogs
Surveys
Dark matter
Galaxies star formation
Astrophysics - Astrophysics of Galaxies
Cosmology
Techniques polarimetric
Gravitational lensing strong
Galaxies fundamental parameters
Galaxies ISM
Gravitational lensing weak
Astrophysics
Spectroscopy
Methods numerical
Planets and satellites fundamental parameters
Instrumentation adaptive optics
Galaxies Evolution
Astrophysics - Cosmology and Nongalactic Astrophysics
Planets and satellites composition
Techniques spectroscopic
Methods data analysis
Galaxies stellar content
Mass function
Techniques photometric
Dust
Galaxies general
Infrared galaxies
Dark energy
Galaxies haloes
OPTIQUE ADAPTATIVE
Planets and satellites atmospheres
Neutrino detector
Galaxies abundances
Galaxy formation
Galaxies groups general
Gravitational lensing
Telescopes
Minor planets
Galaxies starburst
ISM molecules
Ultraviolet galaxies
Methods statistical
Galaxies formation
Submillimeter ISM
Star formation
Large-scale structure of Universe
Methods observational
Galaxies active
Techniques high angular resolution
Galaxies evolution
Instrumentation high angular resolution
Quasars absorption lines
Galaxies spiral
Cosmology observations
Intergalactic medium
ISM clouds
Galaxies
Astrophysics - Instrumentation and Methods for Astrophysics
Exoplanets
Adaptive Optics
CD
Extinction
Data analysis
Photometry
Astrophysics - Earth and Planetary Astrophysics
Stars formation
Galaxies photometry
Comets
Galaxies structure
Quasars general
Radiative transfer
Galaxies clusters general
Galaxies kinematics and dynamics
Galaxies statistics
Galaxies luminosity function
Protoplanetary disks
Galaxies distances and redshifts
Techniques radial velocities
Galaxies clusters individual Virgo
Planets and satellites detection
Stars fundamental parameters
H II regions
Adaptive optics
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Nos collaborations internationales