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