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arXiv · 1605.02225

Metallicity Calibration and Photometric Parallax Estimation: I. UBV photometry

S. Tuncel Guctekin·S. Bilir·S. Karaali·S. Ak·T. Ak·Z. F. Bostanci
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Abstract

We present metallicity and photometric parallax calibrations for the F and G type dwarfs with photometric, astrometric and spectroscopic data. The sample consists of 168 dwarf stars covering the colour, iron abundance and absolute magnitude intervals $0.30<(B-V)_0<0.68$ mag, $-2.0<[Fe/H]<0.4$ dex and $3.4<M_V<6.0$ mag, respectively. The means and standard deviations of the metallicity and absolute magnitude residuals are small, i.e. $\langle\Delta[Fe/H]_{res}\rangle=0$ and $\sigma=0.134$ dex, and $\langle\Delta (M_V)_{res}\rangle=0$ and $\sigma=0.174$ mag, respectively, which indicate accurate metallicity and photometric parallax estimations.

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S. Tuncel Guctekin, S. Bilir, S. Karaali, S. Ak, T. Ak, Z. F. Bostanci. 2016-05-07. Metallicity Calibration and Photometric Parallax Estimation: I. UBV photometry. https://doi.org/10.1007/s10509-016-2776-2

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