B/pastel     The PASTEL catalogue                            (Soubiran+, 2016-)

The PASTEL catalogue : 2020 version. Soubiran C., Le Campion J.-F., Brouillet N., Chemin L. <Astron. Astrophys., 591, A118 (2016)> =2016A&A...591A.118S 2016A&A...591A.118S
ADC_Keywords: Abundances ; Abundances, [Fe/H] ; Effective temperatures Keywords: catalogues - stars: abundances - stars: atmospheres - stars: fundamental parameters Description: PASTEL is a bibliographical catalogue compiling determinations of stellar atmospheric parameters. It provides (Teff, logg, [Fe/H]) determinations obtained from detailed analyses of high resolution, high signal to noise spectra, carried out with the help of model atmospheres. It also provides effective temperatures Teff from various methods. PASTEL is regularly updated. The catalogue supersedes the two previous versions of the [Fe/H] catalogue (Cayrel de Strobel et al., 1997 [Cat. III/200], 2001 [Cat. III/221]). PASTEL is regularly updated. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file pastel.dat 223 81362 The catalogue of stellar atmospheric parameters (Version 2020-01-30) -------------------------------------------------------------------------------- See also: III/200 : Catalogue of [Fe/H] (Cayrel de Strobel+, 1997) III/221 : Catalogue of [Fe/H] of F, G, K stars (Cayrel de Strobel+, 2001) Byte-by-byte Description of file: pastel.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 33 A33 --- ID Designation 35- 49 F15.11 deg RAdeg ? Right Ascension (J2000) from Simbad or 2MASS 51- 65 F15.11 deg DEdeg ? Declination (J2000) from Simbad or 2MASS 67 A1 --- o_coo [ST?] Origin of coordinates (1) 69- 74 F6.3 mag Bmag ? Johnson B magnitude from Simbad 76- 80 F5.3 mag e_Bmag ? Standard error on Bmag 83- 88 F6.3 mag Vmag ? Johnson V magnitude from Simbad 90- 94 F5.3 mag e_Vmag ? Standard error on Vmag 97-102 F6.3 mag Jmag ? 2MASS J apparent magnitude 103-108 F6.3 mag e_Jmag ? 2MASS J total magnitude uncertainty 111-116 F6.3 mag Hmag ? 2MASS H apparent magnitude 118-123 F6.3 mag e_Hmag ? 2MASS H total magnitude uncertainty 126-131 F6.3 mag Ksmag ? 2MASS Ks apparent magnitude 132-137 F6.3 mag e_Ksmag ? 2MASS Ks total magnitude uncertainty 141-145 I5 K Teff ? Effective temperature 147-151 I5 K e_Teff ? Standard error on effective temperature 153-158 F6.3 [cm/s2] logg ? Logarithm of gravity 161-165 F5.3 [cm/s2] e_logg ? Standard error on the logarithm of gravity 167-172 F6.3 [Sun] [Fe/H] ? Iron abundance relative to the Sun 175-179 F5.3 [Sun] e_[Fe/H] ? Standard error on iron abundance 181 A1 --- n_[Fe/H] ? [2M] Metal abundance, Fe2 (2) 182 A1 --- f_[Fe/H] ? [N] NLTE analysis (3) 184-203 A20 --- Author First author of the analysis 205-223 A19 --- bibcode Bibcode of publication -------------------------------------------------------------------------------- Note (1): Origin of coordinates as follows: S = coordinates come from SIMBAD T = coordinates are from 2MASS ? = coordinates not available Note (2): Metal abundance, ionised iron, flag as follows: M = [M/H] is given instead of [Fe/H] 2 = [FeII/H] is given Note (3): N = NLTE analysis of iron -------------------------------------------------------------------------------- Acknowledgements: Caroline Soubiran, caroline.soubiran(at)u-bordeaux.fr Philippe Prugniel (Observatoire de Lyon) is thanked for his contribution to the 2020 version of PASTEL References: SIMBAD at http://simbad.u-strasbg.fr History: * 08-Apr-2010: Version 30151 records. * 20-Apr-2011: Version 31724 records. * 02-May-2013: Version 52045 records. * 18-Mar-2016: Version 64083 records. * 02-May-2016: Version 64082 records, some IDs corrected in multiple systems * 13-Jan-2020: Version 80230 records * 30-Jan-2020: Version 81362 records, 1 reference added
(End) C. Soubiran [Laboratoire d'Astrophysique de Bordeaux] 30-Jan-2020
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