Table 3
Broad-band photometry for Gaia FGK benchmark stars used for indirect determinations of θLD and/or Fbol.
| Name | V | σ(V) | BCV | (B−V) | J | K |
|
|
||||||
| HD 84937 | 8.324 | 0.021 | 0.389 | 7.359 | 7.062 | |
| ϵ For | 5.883 | 0.005 | –0.25 | 0.790 | 4.364 | 3.824 |
| HD 22879 | 6.689 | 0.009 | 0.540 | 5.588 | 5.179 | |
| μ Ara | 5.131 | 0.012 | 0.700 | 4.158 | 3.683 | |
| HD 122563 | 6.200 | 0.009 | –0.47 | |||
| μ Leo | 3.880 | 0.005 | –0.51 | |||
| HD 107328 | 4.970 | 0.012 | –0.49 | |||
| HD 220009 | 5.047 | 0.008 | –0.64 | |||
| β Ara | 2.842 | 0.004 | –0.75 | |||
Notes. The V magnitudes and B−V colour indices are mean values and σ(V) the standard deviation extracted from the GCPD (Mermilliod et al. 1997). The bolometric corrections BCV were calculated as described in the text, Sect. 3.3. The J and K magnitudes are taken from the 2MASS catalogue (Cutri et al. 2003).
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