New release of the ELODIE library: Version 3.1
arXiv:astro-ph/0703658
Abstract
We present ELODIE.3.1, an updated release of the library published in Prugniel & Soubiran (2001, 2004). The library includes 1962 spectra of 1388 stars obtained with the ELODIE spectrograph at the Observatoire de Haute-Provence 193cm telescope in the wavelength range 390 to 680 nm. It provides a wide coverage of atmospheric parameters : T_eff from 3100 K to 50000 K, log g from -0.25 to 4.9 and [Fe/H] from -3 to +1. The library is given at two resolutions: R~42000, with the flux normalized to the pseudo-continuum, FWHM=0.55Å(R~10000) calibrated in physical flux (reduced above earth atmosphere) with a broad-band photometric precision of 2.5% and narrow-band precision of 0.5%. In this new release the data-reduction (flux calibration, reconnection of the echelle orders) has been improved, and in particular the blue region, between 390 and 400 nm has been added. The FITS files for each spectra, and the measured atmospheric parameters are publicly available. See the ELODIE.3.1 page for more details: http://www.obs.u-bordeaux1.fr/m2a/soubiran/elodie_library.html
v2 removed unused figures
Cited by in corpus (26)
- Modeling the color evolution of luminous red galaxies - improvements with empirical stellar spectra
- The LAMOST Stellar Parameter Pipeline at Peking University --- LSP3
- Spectral and atmospheric characterization of 51 Eridani b using VLT/SPHERE
- Age and metallicity gradients in early-type galaxies: A dwarf to giant sequence
- LAMOST Spectroscopic Survey of the Galactic Anti-centre (LSS-GAC): target selection and the first release of value-added catalogues
- Formation and Evolution of Dwarf Elliptical Galaxies - II. Spatially resolved star-formation histories
- Atmospheric Parameters of 169 F, G, K and M-type Stars in the Kepler Field
- Empirical metallicity-dependent calibrations of effective temperature against colours for dwarfs and giants based on interferometric data
- X-ray eruptions every 22 days from the nucleus of a nearby galaxy
- What Drives Galaxy Quenching? Resolving Molecular Gas and Star Formation in the Green Valley
- The Nearest High-Velocity Stars Revealed by LAMOST Data Release 1
- The Diversity of Thick Galactic Discs
- Inversion of stellar fundamental parameters from Espadons and Narval high-resolution spectra
- Towards a Solution for the Ca II Triplet Puzzle : Results from Dwarf Elliptical Galaxies
- Star formation history of KDG 61 and KDG 64 from spectroscopy and colour-magnitude diagrams
- The discrepancy between dynamical and stellar masses in massive compact galaxies traces non-homology
- Principal component analysis-based inversion of effective temperatures for late-type stars
- Star formation histories and evolution of 35 brightest E+A galaxies from SDSS DR5
- Automatic stellar spectral parameterization pipeline for LAMOST survey
- Properties of Stellar Populations in Isolated Lenticular Galaxies
- Kinematics and stellar population of NGC 4486A
- Comparisons of Different Fitting Methods for the Physical Parameters of A Star Cluster Sample of M33 with Spectroscopy and Photometry
- Identification of metal-poor stars using the artificial neural network
- Physical Parameters of Stars in NGC 6397 Using ANN-Based Interpolation and Full Spectrum Fitting
- Homogenized effective temperatures from stellar libraries
- Kinematics And Stellar Population In Isolated Lenticular Galaxies