The X-shooter Spectral Library (XSL). I. DR1: Near-ultraviolet through optical spectra from the first year of the survey

Bibcode
2014A&A...565A.117C
DOI
10.1051/0004-6361/201322505
Chen, Y.-P.; Trager, S. C.; Peletier, R. F.; Lançon, A.; Vazdekis, A.; Prugniel, Ph.; Silva, D. R.; Gonneau, A.
Bibliographical reference

Astronomy and Astrophysics, Volume 565, id.A117, 32 pp.

Advertised on:
5
2014
Journal
Astronomy and Astrophysics
Number of authors
8
IAC number of authors
1
Citations
105
Refereed citations
94
Description
We present the first release of the X-shooter Spectral Library (XSL). This release contains 237 stars. The spectra in this release span a wavelength range of 3000-10 200 Å and have been observed at a resolving power of R ≡ λ/ Δλ ~ 10 000. The spectra were obtained at ESO's 8-m Very Large Telescope (VLT). The sample contains O-M, long-period variable, C and S stars. The spectra are flux-calibrated and telluric-corrected. We describe a new technique for the telluric correction. The wavelength coverage, spectral resolution, and spectral type of this library make it well suited to stellar population synthesis of galaxies and clusters, kinematical investigation of stellar systems, and the study of the physics of cool stars. Full Table 3 and Table A.1 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/565/A117
Related projects
Group members
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.
Anna
Ferré Mateu
In progress
Type
Refereed
Galaxies

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