Bibcode
Arentsen, Anke; Prugniel, Philippe; Gonneau, Anais; Lançon, Ariane; Trager, Scott; Peletier, Reynier; Lyubenova, Mariya; Chen, Yan-Ping; Falcón Barroso, Jesús; Sánchez Blázquez, Patricia; Vazdekis, Alejandro
Bibliographical reference
Astronomy and Astrophysics, Volume 627, id.A138, 14 pp.
Advertised on:
7
2019
Journal
Citations
51
Refereed citations
51
Description
Context. The X-shooter Spectral Library (XSL) is an empirical stellar
library at medium spectral resolution covering the wavelength range from
3000 Å to 24 800 Å. This library aims to provide a benchmark
for stellar population studies. Aims: In this work, we present a
uniform set of stellar atmospheric parameters, effective temperatures,
surface gravities, and iron abundances for 754 spectra of 616 XSL stars.
Methods: We used the full-spectrum fitting package ULySS with the
empirical MILES library as reference to fit the ultraviolet-blue (UVB)
and visible (VIS) spectra. We tested the internal consistency and we
compared our results with compilations from the literature.
Results: The stars cover a range of effective temperature 2900 <
Teff < 38 000 K, surface gravity 0 < logg < 5.7, and
iron abundance -2.5 < [Fe/H] < +1.0, with a couple of stars
extending down to [Fe/H] = -3.9. The precisions of the measurements for
the G- and K-type stars are 0.9%, 0.14, and 0.06 in Teff,
logg, and [Fe/H], respectively. For the cool giants with logg < 1,
the precisions are 2.1%, 0.21, and 0.22, and for the other cool stars
these values are 1%, 0.14, and 0.10. For the hotter stars
(Teff > 6500 K), these values are 2.6%, 0.20, and 0.10 for
the three parameters.
Full Tables A.1-A.3 are only available at the CDS via anonymous ftp to
http://cdsarc.u-strasbg.fr
(ftp://130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/627/A138Based
on ESO observations from run IDs 084.B-0869(A/B), 085.B-0751(A/B) and
189.B-0925(A/B/C/D).
Related projects
Traces of Galaxy Formation: Stellar populations, Dynamics and Morphology
We are a large, diverse, and very active research group aiming to provide a comprehensive picture for the formation of galaxies in the Universe. Rooted in detailed stellar population analysis, we are constantly exploring and developing new tools and ideas to understand how galaxies came to be what we now observe.
Ignacio
Martín Navarro