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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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Lindsey A Kwok, Matthew R Siebert, Joel Johansson, Saurabh W Jha, Stephane Blondin, et al.. Ground-based and JWST Observations of SN 2022pul: II. Evidence from Nebular Spectroscopy for a Violent Merger in a Peculiar Type-Ia Supernova. Astrophys.J., 2024, 966 (1), pp.135. ⟨10.3847/1538-4357/ad2c0d⟩. ⟨hal-04201936⟩
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K Tanidis, V.F Cardone, M Martinelli, I Tutusaus, S Camera, et al.. Euclid preparation. TBD. The effect of linear redshift-space distortions in photometric galaxy clustering and its cross-correlation with cosmic shear. Astron.Astrophys., 2024, 683, pp.A17. ⟨10.1051/0004-6361/202347870⟩. ⟨hal-04205044⟩
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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
2 764
Nos notices
3 270
Nos thématiques
Galaxies evolution
Galaxies
X-rays galaxies clusters
Techniques photometric
Quasars general
Galaxies luminosity function
Galaxies groups general
H II regions
Adaptive Optics
Cosmic background radiation
Stars formation
Star formation
Galaxies photometry
Comets general
Dust
Techniques spectroscopic
ISM clouds
Astrophysics - Earth and Planetary Astrophysics
Techniques radial velocities
Minor planets
Galaxies general
Radiative transfer
Astrophysics - Instrumentation and Methods for Astrophysics
Supernovae general
Comets
Instrumentation adaptive optics
Galaxies ISM
ISM molecules
Galaxies haloes
Large-scale structure of Universe
Methods statistical
Galaxies dwarf
Galaxies abundances
Ultraviolet galaxies
Photometry
High-redshift galaxies
Techniques polarimetric
OPTIQUE ADAPTATIVE
Astrophysics - Solar and Stellar Astrophysics
Methods observational
Techniques high angular resolution
Mass function
Techniques image processing
Data analysis
Galaxies spiral
CD
Galaxy formation
Surveys
Infrared galaxies
Galaxies star formation
Methods numerical
Spectroscopy
Stars fundamental parameters
Cosmology
Gravitational lensing
Planets and satellites composition
Infrared ISM
Gravitational lensing weak
Gravitational lensing strong
67P/Churyumov-Gerasimenko
Astrophysics
Extinction
Cosmological parameters
Submillimeter galaxies
Galaxies stellar content
Adaptive optics
Cosmology observations
Planets and satellites atmospheres
Dark energy
Galaxies distances and redshifts
Planets and satellites detection
Submillimeter ISM
Galaxy evolution
Astrophysics - Cosmology and Nongalactic Astrophysics
Galaxies active
Galaxies interactions
Dark matter
Instrumentation high angular resolution
ANTARES
Planets and satellites fundamental parameters
Quasars absorption lines
Galaxies clusters general
Telescopes
Neutrino detector
Galaxies clusters individual Virgo
Galaxies high-redshift
Methods data analysis
Intergalactic medium
Galaxies structure
Protoplanetary disks
Galaxies statistics
Galaxies formation
Exoplanets
Planetary systems
Galaxies starburst
Astrophysics - Astrophysics of Galaxies
Catalogs
Galaxies Evolution
Galaxies kinematics and dynamics
Galaxies fundamental parameters
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Nos collaborations internationales