J/A+A/566/A98       The Gaia Benchmark Stars - Library  (Blanco-Cuaresma+, 2014)

The Gaia FGK benchmark stars. High resolution spectral library. Blanco-Cuaresma S., Soubiran C., Jofre P., Heiter U. <Astron. Astrophys. 566, A98 (2014)> =2014A&A...566A..98B 2014A&A...566A..98B
ADC_Keywords: Atlases ; Spectroscopy ; Stars, normal Keywords: stars: atmospheres - stars: abundances - Galaxy: general - galaxies: stellar content Abstract: An increasing number of high-resolution stellar spectra is available today thanks to many past and ongoing spectroscopic surveys. Consequently, numerous methods have been developed to perform an automatic spectral analysis on a massive amount of data. When reviewing published results, biases arise and they need to be addressed and minimized. We are providing a homogeneous library with a common set of calibration stars (known as the Gaia FGK benchmark stars) that will allow us to assess stellar analysis methods and calibrate spectroscopic surveys. High-resolution and signal-to-noise spectra were compiled from different instruments. We developed an automatic process to homogenize the observed data and assess the quality of the resulting library. Description: We built a high-quality library that will facilitate the assessment of spectral analyses and the calibration of present and future spectroscopic surveys. The automation of the process minimizes the human subjectivity and ensures reproducibility. Additionally, it allows us to quickly adapt the library to specific needs that can arise from future spectroscopic analyses. * Please, make sure you are using the latest version of the library by checking the author's website: http://www.blancocuaresma.com/s/ File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file list.dat 83 78 List of FITS spectra for 33 stars + the Sun fits/* . 4 Subdirectories with individual FITS spectra -------------------------------------------------------------------------------- See also: III/281 : Gaia FGK benchmark stars v2.1 (Jofre+, 2018) J/A+A/564/A133 : Gaia FGK benchmark stars: metallicity (Jofre+, 2014) J/A+A/582/A81 : Gaia FGK benchmark stars: abundances (Jofre+, 2015) J/A+A/592/A70 : Gaia FGK stars: low-metallicities candidates (Hawkins+, 2016) Byte-by-byte Description of file: list.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 13 A13 --- FileName Name for data files (1) 15- 25 A11 --- Star Star name 27- 34 A8 --- Origin Spectra's origins 36- 45 A10 "Y-M-D" ObsDate Observation date 47- 63 A17 --- SpType MK spectral type (2) 65- 83 A19 --- r_SpType Reference bibcode for SpType -------------------------------------------------------------------------------- Note (1): The fits files are stored in the fits directory, which contains four subdirectories: orig = Original resolution and not continuum normalized orig70000 = Homogeneous resolution of 70000 and not continuum normalized norm = Original resolution and continuum normalized norm70000 = Homogeneous resolution of 70000 and continuum normalized Note (2): Spectral types kindly supplied by Eric Mamajek, Rochester University -------------------------------------------------------------------------------- Acknowledgements: Sergi Blanco-Cuaresma, blanco(at)obs.u-bordeaux1.fr References: Heiter et al., Paper I 2015A&A...582A..49H 2015A&A...582A..49H Blanco-Cuaresma et al., Paper II 2014A&A...566A..98B 2014A&A...566A..98B, Cat. J/A+A/566/A98 Jofre et al., Paper III 2014A&A...564A.133J 2014A&A...564A.133J, Cat. J/A+A/564/A133 Jofre et al., Paper IV 2015A&A...582A..81J 2015A&A...582A..81J, Cat. J/A+A/582/A81 Hawkins et al., Paper V 2016A&A...592A..70H 2016A&A...592A..70H, Cat. J/A+A/592/A70 Jofre et al., 2017A&A...601A..38J 2017A&A...601A..38J
(End) Patricia Vannier [CDS] 07-May-2014
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