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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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Natália V.N. Rodrigues, L. Raul Abramo, Carolina Queiroz, Ginés Martínez-Solaeche, Ignasi Pérez Ràfols, et al.. The miniJPAS survey quasar selection II: Machine learning classification with photometric measurements and uncertainties. Monthly Notices of the Royal Astronomical Society, 2023, 520 (3), pp.3494-3509. ⟨10.1093/mnras/stac2836⟩. ⟨hal-04012294⟩
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A Niemiec, M Jauzac, D Eckert, D Lagattuta, K Sharon, et al.. Beyond the Ultra-deep Frontier Fields And Legacy Observations (BUFFALO): a high-resolution strong + weak-lensing view of Abell 370. Monthly Notices of the Royal Astronomical Society, 2023, 524 (2), pp.2883-2910. ⟨10.1093/mnras/stad1999⟩. ⟨hal-04158369⟩
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Jianhang Chen, R.J. Ivison, Martin A. Zwaan, Ian Smail, Anne Klitsch, et al.. ALMACAL IX: multi-band ALMA survey for dusty star-forming galaxies and the resolved fractions of the cosmic infrared background. Monthly Notices of the Royal Astronomical Society, 2023, 518 (1), pp.1378-1397. ⟨10.1093/mnras/stac2989⟩. ⟨hal-03839770⟩
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César Ramírez-Pérez, Ignasi Pérez-Ràfols, Andreu Font-Ribera, M Abdul Karim, E Armengaud, et al.. The Lyman-$\alpha$ forest catalog from the Dark Energy Spectroscopic Instrument Early Data Release. Monthly Notices of the Royal Astronomical Society, 2024, 528 (4), pp.6666-6679. ⟨10.1093/mnras/stad3781⟩. ⟨hal-04143306⟩
Nos dépôts
2 733
Nos notices
3 284
Nos thématiques
ISM clouds
H II regions
Instrumentation adaptive optics
Catalogs
Astrophysics - Instrumentation and Methods for Astrophysics
Astrophysics - Earth and Planetary Astrophysics
Galaxies luminosity function
Methods numerical
Galaxies fundamental parameters
Galaxy evolution
Galaxies clusters individual Virgo
Spectroscopy
Astrophysics
Galaxies
Quasars general
Large-scale structure of Universe
Techniques photometric
Techniques high angular resolution
Submillimeter galaxies
Adaptive optics
Methods data analysis
Galaxies starburst
Infrared galaxies
Adaptive Optics
Comets
Telescopes
Cosmic background radiation
Comets general
Galaxies interactions
X-rays galaxies clusters
Planets and satellites atmospheres
Techniques radial velocities
Exoplanets
Infrared ISM
Galaxies statistics
Techniques spectroscopic
ISM molecules
Radiative transfer
Techniques image processing
Galaxies distances and redshifts
Astrophysics - Solar and Stellar Astrophysics
Galaxies haloes
Methods statistical
Surveys
Quasars absorption lines
Planets and satellites fundamental parameters
Galaxies dwarf
Neutrino detector
Cosmological parameters
Galaxies general
Intergalactic medium
Astrophysics - Astrophysics of Galaxies
Mass function
Stars fundamental parameters
Instrumentation high angular resolution
Protoplanetary disks
Cosmology
Gravitational lensing strong
Galaxies formation
Individual
Data analysis
Galaxies high-redshift
Galaxies stellar content
Techniques polarimetric
Galaxies spiral
Star formation
Galaxies structure
Galaxies groups general
Galaxies photometry
Galaxies ISM
ANTARES
Supernovae general
Ultraviolet galaxies
Submillimeter ISM
Photometry
Galaxies star formation
Galaxies kinematics and dynamics
Galaxies Evolution
Dark energy
Gravitational lensing
Planets and satellites composition
Cosmology observations
CD
Stars formation
Methods observational
67P/Churyumov-Gerasimenko
High-redshift galaxies
Galaxy formation
Galaxies evolution
Planets and satellites detection
Planetary systems
Gravitational lensing weak
Extinction
Astrophysics - Cosmology and Nongalactic Astrophysics
Galaxies abundances
Dust
Galaxies active
Galaxies clusters general
Dark matter
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Nos collaborations internationales