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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
2 766
Nos notices
3 269
Nos thématiques
Ultraviolet galaxies
Galaxies interactions
Galaxies dwarf
Galaxies stellar content
Galaxies evolution
Telescopes
Infrared galaxies
Protoplanetary disks
H II regions
Galaxies haloes
Galaxies statistics
ISM clouds
Cosmological parameters
Astrophysics - Cosmology and Nongalactic Astrophysics
Comets
Dark matter
Galaxies starburst
Instrumentation adaptive optics
Neutrino detector
Planets and satellites detection
Gravitational lensing strong
Planets and satellites composition
Methods numerical
Galaxies structure
Galaxy evolution
Exoplanets
Galaxies
Galaxies formation
Gravitational lensing
Submillimeter ISM
ANTARES
Data analysis
Techniques polarimetric
Planets and satellites fundamental parameters
Planets and satellites atmospheres
Galaxies clusters general
Star formation
Galaxies luminosity function
Astrophysics - Astrophysics of Galaxies
Mass function
Submillimeter galaxies
Astrophysics
Quasars absorption lines
Methods statistical
X-rays galaxies clusters
Methods observational
Astrophysics - Solar and Stellar Astrophysics
Gravitational lensing weak
Galaxies high-redshift
Photometry
Comets general
Minor planets
Astrophysics - Instrumentation and Methods for Astrophysics
Galaxies clusters individual Virgo
Galaxies groups general
Intergalactic medium
OPTIQUE ADAPTATIVE
Adaptive optics
Galaxies kinematics and dynamics
Galaxies photometry
Galaxies active
Quasars general
Supernovae general
Techniques high angular resolution
Galaxies ISM
Catalogs
Galaxy formation
Methods data analysis
Planetary systems
Galaxies spiral
Adaptive Optics
Infrared ISM
Surveys
Techniques photometric
ISM molecules
Galaxies abundances
Radiative transfer
Extinction
Dark energy
Spectroscopy
Galaxies distances and redshifts
Galaxies fundamental parameters
Cosmology
Galaxies star formation
High-redshift galaxies
Instrumentation high angular resolution
Galaxies Evolution
Techniques spectroscopic
Cosmic background radiation
Stars fundamental parameters
Techniques radial velocities
Dust
Stars formation
67P/Churyumov-Gerasimenko
Techniques image processing
Galaxies general
Astrophysics - Earth and Planetary Astrophysics
Large-scale structure of Universe
Cosmology observations
CD
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