J/A+A/629/A100      MUSE library of stellar spectra              (Ivanov+, 2019)

MUSE library of stellar spectra. Ivanov V.D., Coccato L., Neeser M.J., Selman F., Pizzella A., Dalla Bont E., Corsini E.M., Morelli L. <Astron. Astrophys. 629, A100 (2019)> =2019A&A...629A.100I 2019A&A...629A.100I (SIMBAD/NED BibCode)
ADC_Keywords: Atlases ; Stars, nearby ; Spectra, optical Keywords: standards - atlases - stars: atmospheres - stars: general Abstract: Empirical stellar spectral libraries have applications in both extragalactic and stellar studies, and they confer an advantage over theoretical libraries because they naturally include all relevant chemical species and physical processes. In recent years we have seen a stream of new sets of high-quality spectra, but increasing the spectral resolution and widening the wavelength coverage means resorting to multi-order echelle spectrographs. Assembling the spectra from many pieces results in lower fidelity of their shapes. We aim to offer the community a library of high-signal-to-noise spectra with reliable continuum shapes. Furthermore, the use of an integral field unit (IFU) alleviates the issue of slit losses. Our library was built with the MUSE (Multi-Unit Spectroscopic Explorer) IFU instrument. We obtained spectra over nearly the entire visual band (λ∼4800-9300Å). We assembled a library of 35 high-quality MUSE spectra for a subset of the stars from the X-shooter Spectral Library. We verified the continuum shape of these spectra with synthetic broadband colors derived from the spectra. We also report some spectral indices from the Lick system, derived from the new observations. We offer a high-fidelity set of stellar spectra covering the Hertzsprung-Russell diagram. These can be used for both extragalactic and stellar studies and demonstrate that the IFUs are excellent tools for building reliable spectral libraries. Description: The data set contains 35 files, each with a MUSE spectrum of one target star. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file stars.dat 62 35 List of stars with spectrum sp/* . 35 Individual spectra -------------------------------------------------------------------------------- Byte-by-byte Description of file: stars.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 15 A15 --- Name Star name 17- 18 I2 h RAh Simbad right ascension (J2000) 20- 21 I2 min RAm Simbad right ascension (J2000) 23- 27 F5.2 s RAs Simbad right ascension (J2000) 29 A1 --- DE- Simbad declination sign (J2000) 30- 31 I2 deg DEd Simbad declination (J2000) 33- 34 I2 arcmin DEm Simbad declination (J2000) 36- 39 F4.1 arcsec DEs Simbad declination (J2000) 41- 62 A22 --- FileName Name of the spectrum table in subdirectory sp -------------------------------------------------------------------------------- Byte-by-byte Description of file: sp/* -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 F9.4 0.1nm lambda Wavelength (Å) 11- 20 E10.5 10-2W/m2/nm Flux Flux (in erg/cm^2/s/Å) 22- 31 E10.5 10-2W/m2/nm e_Flux Flux error (in erg/cm^2/s/Å) -------------------------------------------------------------------------------- Acknowledgements: Valentin Ivanov, vivanov(at)eso.org
(End) Patricia Vannier [CDS] 06-Aug-2019
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