A database of high and medium-resolution stellar spectra ?;??

By P. Prugniel, C. Lyon, O. Bordeaux. 2001

364 citations recorded by the source corpus.

We present a database of 908 spectra of 709 stars obtained with the ELODIE spectrograph at the Observatoire de Haute-Provence. 52 orders of the echelle spectra have been carefully tted together to provide continuous, high-resolution spectra in the wavelength range = 410 680 nm. The archive provides a large coverage of the space of atmospheric parameters: Te from 3700 K to 13 600 K, log g from 0.03 to 5.86 and (Fe/H) from 2:8 to +0.7. At the nominal resolution, R = 42 000, the mean signal-to-noise ratio is 150 per pixel. The spectra given at this resolution are normalized to their pseudo-continuum and are intended to serve for abundance studies, spectral classication and tests of stellar atmosphere models. A lower resolution version of the archive, at R = 10 000, is calibrated in physical flux with a broad-band photometric precision of 2.5% and narrow-band precision of 0.5%. It is well suited to stellar population synthesis of galaxies and clusters, and to kinematical investigations of stellar systems. The archive is distributed in FITS format through the HYPERCAT and CDS databases.

Subfields: Astronomy and Astrophysics, Computational Mechanics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/e010227a5170a3f3e0c53365aca3f1848be759a3

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Citations in the corpus

Modeling the Panchromatic Spectral Energy Distributions of Galaxies (2013, background): “Later optical/NIR libraries included Pickles (1998), Jones (1999), ELODIE (Prugniel & Soubiran 2001), STELIB (Le Borgne et al. 2003), Indo-US (Valdes et al. 2004), NGSL (Gregg et al. 2006, Heap & Lindler 2011), MILES (Sánchez-Blázquez et al. 2006), IRTF (Rayner, Cushing & Vacca 2009), and the…”
Modelling and interpreting spectral energy distributions of galaxies with BEAGLE (2016, background): “Many spectral evolution models available in the literature (e.g. Pégase, Fioc & Rocca-Volmerange 1997; Le Borgne et al. 2004; GALAXEV, Bruzual & Charlot 2003; FSPS, Conroy et al. 2009; ; Vazdekis et al. 2010; MaStro, Maraston & Strömbäck 2011; Conroy & van Dokkum 2012a) rely on libraries of obser”
SPECTRAL CLASSIFICATION AND REDSHIFT MEASUREMENT FOR THE SDSS-III BARYON OSCILLATION SPECTROSCOPIC SURVEY (2012, methodology): “Stellar velocity dispersions σv of galaxies are measured using a stellar template basis derived from the ELODIE library (Prugniel & Soubiran 2001), covering the restframe spectral range 4100 Å–6800 Å.”
A Spectroscopic Study of the Ancient Milky Way: F- and G-Type Stars in the Third Data Release of the Sloan Digital Sky Survey (2005, methodology): “…for checking our analysis procedure: the Indo-US library of Coudé feed stellar spectra (Valdes et al. 2004, hereafter CFLIB), the ELODIE library (Prugniel & Soubiran 2001, hereafter ELODIE), and the Spectroscopic Survey of Stars in the Solar Neighborhood (Allende Prieto et al. 2004a, hereafter…”
Spectroscopic ages and metallicities of stellar populations : validation of full spectrum fitting (2008, methodology): “The ELODIE library is constructed from the spectroscopic archive of Observatoire de Haute-Provence3 (Moultaka et al. 2004) and the principle of the data-reduction, flux calibration and determination of the atmospheric parameters are described in Prugniel & Soubiran (2001).”
Evolutionary synthesis of galaxies at high spectral resolution with the code PEGASE-HR. Metallicity and age tracers (2004, methodology): “We also briefly describe the main features of the updated stellar library ÉLODIE (Prugniel & Soubiran 2001a) as well as the “interpolator”, the method used to convert the set of ÉLODIE stellar spectra to a grid of spectra with the regularly spaced stellar parameters of the BaSeL library.”
The Gaia-ESO Survey: the analysis of high-resolution UVES spectra of FGK-type stars (2014, methodology): “A reference library composed of 270 high-resolution (R = 42 000) spectra of slowly-rotating FGKM-type stars available in the ELODIE archive (Prugniel & Soubiran 2001) was used.”
Coudé-feed stellar spectral library – atmospheric parameters (2010, background): “(Prugniel & Soubiran 2001), the star was on the dwarf sequence: log g = 5.27 dex.”
THE SEVENTH DATA RELEASE OF THE SLOAN DIGITAL SKY SURVEY (2008, methodology): “The stellar spectral template library which gives the best radial velocity estimates is based on the ELODIE library (Prugniel & Soubiran 2001).”
Improving the full spectrum fitting method: accurate convolution with Gauss-Hermite functions (2016, background): “…high resolution empirical stellar libraries spanning large ranges of atmospheric parameters over a wide wavelength range (e.g. Cenarro et al. 2001; Prugniel & Soubiran 2001; Valdes et al. 2004; Sánchez-Blázquez et al. 2006), libraries of synthetic stellar spectra (e.g. Coelho et al. 2005; Munari…”
STELIB: A library of stellar spectra at R 2000 ?;?? (2003, background): “Several stars with unknown atmospheric parameters were also part of the ELODIE database (Prugniel & Soubiran 2001).”
COUNTING LOW-MASS STARS IN INTEGRATED LIGHT (2011, methodology): “We have found parameters for 35 of the stars (38% of the sample) in one or more of the MILES, ELODIE (Prugniel & Soubiran 2001), SPOCS (Valenti & Fischer 2005), and Indo-US (Valdes et al. 2004; Wu et al. 2011) libraries.”
Evolutionary stellar population synthesis with MILES – II. Scaled-solar and α-enhanced models (2015, neutral): “Among the most widely employed stellar libraries in the optical range are those of Jones (1999), ELODIE (Prugniel & Soubiran 2001), STELIB (Le Borgne et al. 2003), Indo-US (Valdes et al. 2004) and MILES (Sánchez-Blázquez et al. 2006a) and more recently XSL (Chen et al. 2014).”
An updated MILES stellar library and stellar population models (2011, background): “Details of the library can be found in Prugniel & Soubiran (2001).”
Vertical distribution of Galactic disk stars , IV. AMR and AVR from clump giants (2007, methodology): “About 177 local giants have been observed for this project (Mishenina et al. 2006); radial velocities of other stars were retrieved from the ELODIE library (Prugniel & Soubiran 2001, 2004) and the ELODIE archive (Moultaka et al. 2004).”
Fitting the integrated spectral energy distributions of galaxies (2010, background): “As with the evolutionary tracks, stellar libraries have improved significantly in recent years, with both fully theoretical (e.g. Kurucz 1992; Westera et al. 2002; Smith et al. 2002; Coelho et al. 2005; Martins et al. 2005; Lançon et al. 2007) and empirical, e.g. STELIB (Le Borgne et al. 2003), MILE”
UV-extended E-MILES stellar population models: young components in massive early-type galaxies (2016, methodology): “This has been possible by employing extensive empirical stellar spectral libraries, mostly in the optical range (e.g. Jones 1999; Prugniel & Soubiran 2001; Le Borgne et al. 2003; Valdes et al. 2004; Sánchez-Blázquez et al. 2006), but also theoretical libraries (e.g. Coelho et al. 2005).”
Selection and Photometric Properties of K+A Galaxies (2003, background): “The eigenspectra are constructed over the rest-frame wavelength range 4100 Å k 6800 Å from a high-resolution spectroscopic library (Prugniel & Soubiran 2001).”