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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
2 758
Nos notices
3 275
Nos thématiques
Galaxies photometry
Galaxies groups general
Stars fundamental parameters
Methods data analysis
67P/Churyumov-Gerasimenko
Quasars absorption lines
Galaxies general
Comets
Astrophysics
Galaxies clusters individual Virgo
Adaptive optics
Exoplanets
Techniques radial velocities
Protoplanetary disks
Planets and satellites detection
Planets and satellites atmospheres
ISM molecules
X-rays galaxies clusters
Galaxies star formation
Gravitational lensing weak
Star formation
Neutrino detector
Instrumentation adaptive optics
Galaxies
Techniques high angular resolution
High-redshift galaxies
Techniques spectroscopic
Astrophysics - Earth and Planetary Astrophysics
Galaxies Evolution
Cosmology
Methods observational
Planets and satellites fundamental parameters
Astrophysics - Instrumentation and Methods for Astrophysics
Techniques image processing
Photometry
Intergalactic medium
Galaxies structure
Spectroscopy
Galaxies spiral
Mass function
Instrumentation high angular resolution
Galaxies kinematics and dynamics
Large-scale structure of Universe
Galaxies high-redshift
Catalogs
Submillimeter galaxies
Cosmology observations
Galaxies stellar content
Techniques photometric
ISM clouds
OPTIQUE ADAPTATIVE
Galaxy evolution
Submillimeter ISM
H II regions
Gravitational lensing
Planetary systems
Quasars general
ANTARES
Adaptive Optics
Galaxies ISM
Galaxies abundances
CD
Galaxies luminosity function
Galaxy formation
Supernovae general
Techniques polarimetric
Galaxies formation
Dark matter
Infrared ISM
Radiative transfer
Galaxies starburst
Planets and satellites composition
Galaxies interactions
Astrophysics - Solar and Stellar Astrophysics
Ultraviolet galaxies
Data analysis
Galaxies haloes
Methods numerical
Surveys
Infrared galaxies
Galaxies evolution
Telescopes
Stars formation
Astrophysics - Cosmology and Nongalactic Astrophysics
Extinction
Galaxies distances and redshifts
Dust
Gravitational lensing strong
Comets general
Galaxies statistics
Cosmological parameters
Galaxies active
Astrophysics - Astrophysics of Galaxies
Dark energy
Minor planets
Cosmic background radiation
Methods statistical
Galaxies dwarf
Galaxies fundamental parameters
Galaxies clusters general
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Nos collaborations internationales