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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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C. Moutou, M. Ould-Elhkim, J.-F. Donati, P. Charpentier, C. Cadieux, et al.. Characterizing planetary systems with SPIRou: a temperate sub-Neptune exoplanet orbiting the nearby fully-convective star GJ 1289 and a candidate around GJ 3378 ⋆. Astronomy and Astrophysics - A&A, 2024, 688, pp.A196. ⟨10.1051/0004-6361/202450466⟩. ⟨hal-04752284⟩
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J. Fowler, Sebastiaan Y. Haffert, Maaike A. M. van Kooten, Rico Landman, Alexis Bidot, et al.. Visible extreme adaptive optics on extremely large telescopes: towards detecting oxygen in Proxima Centauri b and analogs. SPIE OPTICAL ENGINEERING + APPLICATIONS. Techniques and Instrumentation for Detection of Exoplanets XI, SPIE, Aug 2023, San Diego, California, United States. ⟨10.1117/12.2677503⟩. ⟨insu-04479042⟩
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Niyati Desai, Lorenzo König, Emiel Por, Roser Juanola-Parramon, Ruslan Belikov, et al.. Integrated photonic-based coronagraphic systems for future space telescopes. SPIE OPTICAL ENGINEERING + APPLICATIONS. Techniques and Instrumentation for Detection of Exoplanets XI, SPIE, Aug 2023, San Diego, California, United States. ⟨10.1117/12.2677210⟩. ⟨insu-04479043⟩
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Adrien Hours, Alexis Carlotti, David Mouillet, Alain Delboulbé, Sylvain Guieu, et al.. HARMONI at ELT: A Zernike wavefront sensor for the high-contrast module: testbed results with realistic observation conditions. Adaptive Optics Systems VIII, Jul 2022, Montréal, Canada. pp.86, ⟨10.1117/12.2627291⟩. ⟨hal-03868056⟩
Nos dépôts
3 085
Nos notices
3 230
Nos thématiques
Galaxies kinematics and dynamics
Large-scale structure of Universe
Comets
Astrophysics - Solar and Stellar Astrophysics
Protoplanetary disks
Extinction
Techniques polarimetric
Galaxies distances and redshifts
Surveys
Submillimeter ISM
Galaxies luminosity function
Galaxies stellar content
Techniques radial velocities
Planets and satellites atmospheres
Submillimeter galaxies
Dark matter
Galaxies general
Dust
Reionization
Cosmology
High-redshift galaxies
Telescopes
H II regions
Exoplanets
Supernovae general
Methods statistical
Planets and satellites composition
Galaxies Evolution
Galaxies ISM
Gravitational lensing weak
Techniques high angular resolution
Galaxies high-redshift
Galaxies interactions
Galaxies starburst
Galaxy formation
Galaxies clusters individual Virgo
Astrophysics
ISM molecules
Minor planets
Catalogs
Cosmology observations
Ultraviolet galaxies
X-rays galaxies clusters
Infrared ISM
Star formation
Planetary systems
Methods numerical
Astrophysics - Instrumentation and Methods for Astrophysics
Techniques image processing
Methods data analysis
Galaxies star formation
Galaxies active
Spectroscopy
Galaxies evolution
Galaxies haloes
Gravitational lensing strong
ANTARES
Galaxies structure
Galaxies dwarf
Astrophysics - Astrophysics of Galaxies
Galaxies formation
Dark energy
Planets and satellites fundamental parameters
Adaptive Optics
Galaxies clusters general
Instrumentation adaptive optics
67P/Churyumov-Gerasimenko
Infrared galaxies
Methods observational
Quasars general
Gravitational lensing
Galaxies fundamental parameters
Techniques photometric
Galaxies photometry
Planets and satellites detection
Radiative transfer
Neutrino detector
Stars fundamental parameters
Adaptive optics
Galaxies
Astrophysics - Earth and Planetary Astrophysics
Astrophysics - Cosmology and Nongalactic Astrophysics
Intergalactic medium
Galaxy evolution
Cosmic background radiation
Instrumentation high angular resolution
Galaxies statistics
Comets general
Quasars absorption lines
Mass function
Data analysis
OPTIQUE ADAPTATIVE
Galaxies spiral
Techniques spectroscopic
Galaxies groups general
Stars formation
Cosmological parameters
ISM clouds
Galaxies abundances
Photometry
Nous suivre !
Nos collaborations internationales