J/A+A/634/A133      X-Shooter Spectral Library (XSL). DR2       (Gonneau+, 2020)

The X-Shooter Spectral Library (XSL): Data Release 2. Gonneau A., Lyubenova M., Lancon A., Trager S.C., Peletier R.F., Arentsen A., Chen Y.-P., Coelho P.R.T., Dries M., Falcon-Barroso J., Prugniel P., Sanchez-Blazquez P., Vazdekis A., Verro K. <Astron. Astrophys. 634, A133 (2020)> =2020A&A...634A.133G 2020A&A...634A.133G (SIMBAD/NED BibCode)
ADC_Keywords: Fundamental catalog ; Stars, standard ; Spectroscopy Keywords: Hertzsprung-Russell and C-M diagrams - catalogs Abstract: We present the second data release (DR2) of the X-Shooter Spectral Library (XSL), which contains all the spectra obtained over the six semesters of that program. This release supersedes our first data release from 2014, with a larger number of spectra (813 observations of 666 stars) and with a more extended wavelength coverage as the data from the near-infrared arm of the X-Shooter spectrograph are now included. The DR2 spectra then consist of three segments that were observed simultaneously and, if combined, cover the range between 300nm and 2.45um at a spectral resolving power close to R=10000. The spectra were corrected for instrument transmission and telluric absorption, and they were also corrected for wavelength-dependent flux-losses in 85% of the cases. On average, synthesized broad-band colors agree with those of the MILES library and of the combined IRTF and Extended IRTF libraries to within 1%. The scatter in these comparisons indicates typical errors on individual colors in the XSL of 2-4%. The comparison with 2MASS point source photometry shows systematics of up to 5% in some colors, which we attribute mostly to zero-point or transmission curve errors and a scatter that is consistent with the above uncertainty estimates. The final spectra were corrected for radial velocity and are provided in the rest-frame (with wavelengths in air). The spectra cover a large range of spectral types and chemical compositions (with an emphasis on the red giant branch), which makes this library an asset when creating stellar population synthesis models or for the validation of near-ultraviolet to near-infrared theoretical stellar spectra across the Hertzsprung-Russell diagram. Description: The X-shooter spectra cover three wavelength ranges, referred to as arms: ultraviolet-blue (UVB), visible (VIS) and near-infrared (NIR). The final data products released as DR2 consist of single-arms spectra, with linearly sampled wavelengths in the rest-frame. Therefore, each arm has its own resolution: 9100 for the UVB, 11000 for the VIS and 7700 for the NIR. The spectra are provided as FITS binary tables, each containing three columns: the wavelength (in nm), the flux spectrum (in erg/s/cm2/Å), and an error spectrum (in the same units). A set of keywords in the headers of the FITS files keep track of various steps of the data-reduction and calibration processes, and of results of the quality assessments. A (non-exhaustive) list of these keywords is given in Table 8 of the paper. The DR2 spectra are made available as two separate sets: 1. All the spectra for which a correction for slit-losses across the spectrograph slit was possible (85% of the observations). 2. Remaining 15% of the spectra, without slit-loss correction. They are identified via header keyword LOSS_COR, which is then set to F. The table provided is a merged version of several tables from our paper. It contains the list of our stars some observational properties as described in Table C1 (coordinates, XSL_ID, MJD, arm missing or deprecated from this data release). The comments about individual objects from Table B1 are also included in this table. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table.dat 401 813 Properties of our sample of XSL stars fits/* . 2043 Individual Fits spectra corrected for slit-loss fits_nlc/* . 345 Individual Fits spectra NOT corrected for slit-loss -------------------------------------------------------------------------------- See also: J/A+A/565/A117 : X-Shooter Spectral Library (XSL). DR1 (Chen+, 2014) Byte-by-byte Description of file: table.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 25 A25 --- Star Name of the star (from table C1) 26 A1 --- n_Star [?] Uncertainty flag on Star name (see Comments) 28- 29 I2 h RAh Right ascension (J2000) (from table C1) 31- 32 I2 min RAm Right ascension (J2000) (from table C1) 34- 39 F6.3 s RAs Right ascension (J2000) (from table C1) 41 A1 --- DE- Declination sign (J2000) (from table C1) 42- 43 I2 deg DEd Declination (J2000) (from table C1) 45- 46 I2 arcmin DEm Declination (J2000) (from table C1) 48- 51 F4.1 arcsec DEs Declination (J2000) (from table C1) 54- 58 A5 --- XSLID XSL unique identifier (from table C1) 60- 69 F10.4 d MJD Modified Julian Date (from table C1) 71- 77 A7 --- ArmMissing Arm missing or deprecated (from table C1) 79-118 A40 --- FileUVB Name of UVB FITS file (with sub-directory name) 120-159 A40 --- FileVIS Name of VIS FITS file (with sub-directory name) 161-200 A40 --- FileNIR Name of NIR FITS file (with sub-directory name) 202-401 A200 --- Comments Comments on individual stars (table B1) -------------------------------------------------------------------------------- Acknowledgements: Anais Gonneau, agonneau(at)ast.cam.ac.uk
(End) Patricia Vannier [CDS] 21-Jan-2020
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line