20.14.6 gold_sample_spss
A table of the best parameters for spectrophotometric standard stars.
Recommended parameters for the Gaia Spectro-Photometric Standard stars (Pancino et al. 2021), selected as described in Gaia Collaboration et al. (2022c), from the available parameters produced by CU8 (Creevey et al. 2022) and CU6 (Katz et al. 2022).
Columns description:
A unique single numerical identifier of the source obtained from gaia_source (for a detailed description see gaia_source.source_id).
Identifier defined by the SPSS team (Pancino et al. 2021).
Preferred star name adopted by the SPSS team.
Recommended spectral type based on estimates by the CU8-Apsis pipeline (Creevey et al. 2022).
Flag indicating whether the star is a known binary () or not ().
Flag indicating whether the star is a known variable () or not ().
Recommended effective temperature based on estimates by the CU8-Apsis pipeline (Creevey et al. 2022).
Uncertainty on the recommended effective temperature based on estimates by the CU8-Apsis pipeline (Creevey et al. 2022).
Recommended surface gravity (logarithmic) based on estimates by the CU8-Apsis pipeline (Creevey et al. 2022).
Uncertainty on the recommended surface gravity based on estimates by the CU8-Apsis pipeline (Creevey et al. 2022).
Recommended iron abundance (logarithmic) based on estimates by the CU8-Apsis pipeline (Creevey et al. 2022).
Uncertainty on the recommended iron abundance based on estimates by the CU8-Apsis pipeline (Creevey et al. 2022).
Recommended alpha enhancement based on estimates by GSP-Spec (Creevey et al. 2022).
Uncertainty on the recommended alpha enhancement based on estimates by GSP-Spec (Creevey et al. 2022).
Recommended radius based on estimates by the CU8-Apsis pipeline (Creevey et al. 2022).
Uncertainty on the recommended radius based on estimates by the CU8-Apsis pipeline (Creevey et al. 2022).
Recommended luminosity based on estimates by the CU8-Apsis pipeline (Creevey et al. 2022).
Uncertainty on the recommended luminosity based on estimates by the CU8-Apsis pipeline (Creevey et al. 2022).
Recommended mass based on estimates by FLAME (Creevey et al. 2022).
Uncertainty on the recommended mass based on estimates by FLAME (Creevey et al. 2022).
Recommended age based on estimates by FLAME (Creevey et al. 2022).
Uncertainty on the recommended age based on estimates by FLAME (Creevey et al. 2022).
Recommended extinction at 541.4 nm based on estimates by the CU8-Apsis pipeline (Creevey et al. 2022).
Uncertainty on the recommended extinction at 541.4 nm based on estimates by the CU8-Apsis pipeline (Creevey et al. 2022).
Recommended extinction in the G band based on estimates by the CU8-Apsis pipeline (Creevey et al. 2022).
Uncertainty on the recommended extinction in the G band based on estimates by the CU8-Apsis pipeline (Creevey et al. 2022).
Recommended reddening in BP-RP based on estimates by GSP-Phot (Creevey et al. 2022).
Uncertainty on the recommended reddening in BP-RP based on estimates by GSP-Phot (Creevey et al. 2022).
Recommended distance based on estimates by GSP-Phot (Creevey et al. 2022).
Uncertainty on recommended distance based on estimates by GSP-Phot (Creevey et al. 2022).
Radial velocity measurement from CU6 and RVS spectra (Katz et al. 2022).
Uncertainty on the radial velocity from CU6 and RVS spectra (Katz et al. 2022).
Recommended projected rotational velocity from CU6 and CU8 estimates.
Uncertainty on recommended projected rotation from CU6 and CU8 estimates.
Various annotations on the star, including considerations on the parameters quality.