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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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Marco Scodeggio, D. Vergani, O. Cucciati, Angela Iovino, P. Franzetti, et al.. The Vimos VLT Deep Survey. Stellar mass segregation and large-scale galaxy environment in the redshift range 0.2 < z < 1.4. Astronomy & Astrophysics - A&A, 2009, 501, pp.21-27. ⟨10.1051/0004-6361/200810511⟩. ⟨hal-03730777⟩
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Élodie M. Hebrard, Jean-François Donati, Xavier Delfosse, Julien Morin, Isabelle Boisse, et al.. Detecting planets around active stars: impact of magnetic fields on radial velocities and line bisectors. Monthly Notices of the Royal Astronomical Society, 2014, 443 (3), pp.2599--2611. ⟨10.1093/mnras/stu1285⟩. ⟨hal-01440971⟩
Nos dépôts
3 230
Nos notices
3 221
Nos thématiques
Dark energy
Galaxies kinematics and dynamics
Data analysis
Radiative transfer
Galaxies haloes
Infrared galaxies
Planets and satellites gaseous planets
Techniques photometric
High-redshift galaxies
Dark matter
Galaxy formation
Planets and satellites fundamental parameters
Astrophysics - Astrophysics of Galaxies
Techniques image processing
Cosmic background radiation
Neutrino detector
H II regions
Galaxies distances and redshifts
Comets general
Astrophysics
Stars formation
Methods numerical
Cosmology
Gravitational lensing strong
Star formation
Cosmology observations
Techniques polarimetric
Galaxies starburst
X-rays galaxies clusters
ISM clouds
Galaxies luminosity function
Astrophysics - Earth and Planetary Astrophysics
Instrumentation high angular resolution
ISM molecules
Dust
Spectroscopy
Galaxies fundamental parameters
Galaxies high-redshift
Galaxies structure
Planets and satellites atmospheres
Galaxies
Techniques spectroscopic
Galaxy evolution
Mass function
Cosmological parameters
Gravitational lensing
Planetary systems
Galaxies star formation
Surveys
Stars fundamental parameters
Galaxies statistics
Submillimeter galaxies
Extinction
Submillimeter ISM
Galaxies active
Ultraviolet galaxies
Methods statistical
Galaxies clusters general
Galaxies formation
Methods data analysis
Galaxies interactions
Galaxies general
Planets and satellites detection
Galaxies evolution
Galaxies photometry
Techniques high angular resolution
Methods observational
Telescopes
OPTIQUE ADAPTATIVE
Galaxies dwarf
Infrared ISM
Adaptive optics
Gravitational lensing weak
ANTARES
Techniques radial velocities
Galaxies clusters individual Virgo
Quasars absorption lines
Supernovae general
Photometry
Astrophysics - Cosmology and Nongalactic Astrophysics
Instrumentation adaptive optics
Galaxies groups general
Astrophysics - Instrumentation and Methods for Astrophysics
Exoplanets
67P/Churyumov-Gerasimenko
Intergalactic medium
Planets and satellites composition
Galaxies stellar content
Large-scale structure of Universe
Adaptive Optics
Astrophysics - Solar and Stellar Astrophysics
Protoplanetary disks
Catalogs
Galaxies ISM
Galaxies spiral
Galaxies Evolution
Galaxies abundances
Comets
Minor planets
Quasars general
Nous suivre !
Nos collaborations internationales
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