pith. sign in

arxiv: astro-ph/0503110 · v1 · submitted 2005-03-04 · 🌌 astro-ph

The effective temperature scale of FGK stars. II. Teff : color : [Fe/H] calibrations

classification 🌌 astro-ph
keywords calibrationsrangestarsteffbeencolorcolorsfits
0
0 comments X
read the original abstract

We present up-to-date metallicity-dependent temperature vs. color calibrations for main sequence and giant stars based on temperatures derived with the infrared flux method (IRFM). Seventeen colors in the following photometric systems: UBV, uvby, Vilnius, Geneva, RI(Cousins), DDO, Hipparcos-Tycho, and 2MASS, have been calibrated. The spectral types covered range from F0 to K5 (7000 K<Teff<4000 K) with some relations extending below 4000 K or up to 8000 K. Most of the calibrations are valid in the metallicity range -3.5<[Fe/H]<0.4, although some of them extend to as low as [Fe/H]=-4.0. All fits to the data have been performed with more than 100 stars; standard deviations range from 30 K to 120 K. Fits were carefully performed and corrected to eliminate the small systematic errors introduced by the calibration formulae. Tables of colors as a function of Teff and [Fe/H] are provided. (Abridged)

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Recalibration of SDSS photometric zero-points based on the InfraRed Flux Method temperature scale

    astro-ph.IM 2026-06 conditional novelty 5.0

    Revised SDSS ugriz zero-points obtained by inverting IRFM on 6000+ FGK stars to match an adopted temperature scale, with largest offset in u band depending on filter curves.

  2. Empirical colour--effective temperature relations in the SDSS system from IRFM temperatures of GALAH and APOGEE stars

    astro-ph.SR 2026-06 unverdicted novelty 4.0

    New empirical color-Teff calibrations in the SDSS system from IRFM temperatures of 3902 GALAH and 2535 APOGEE stars, with 30-50 K precision for long-baseline colors.