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Table 2

Photometry and parallax of metal-poor benchmark candidates.

Star B σB V σV N J2MASS σJ K2MASS σK π σπ E(BV)
(mag) (mag) (mag) (mag) (mag) (mag) (mag) (mag) (mas) (mas) (mag)

Selected

BD+264251 10.52 0.03 10.05 0.03 2 8.98 0.02 8.64 0.02 9.03 1.68 0.007
HD 102200 9.21 0.01 8.76 0.00 2 7.69 0.02 7.38 0.02 13.00 0.98 0.005
HD 106038 10.63 0.01 10.16 0.01 9 9.11 0.03 8.76 0.02 9.98 1.57 0.003
HD 126681 9.90 0.01 9.31 0.01 4 8.04 0.02 7.63 0.02 21.04 1.12 0.000
HD 175305 7.93 0.02 7.17 0.01 6 5.61 0.02 5.06 0.02 6.39 0.36 0.000
HD 196892 8.73 0.02 8.23 0.02 5 7.18 0.03 6.82 0.02 16.15 0.93 0.000
HD 201891 7.89 0.01 7.38 0.02 10 6.25 0.02 5.93 0.02 29.10 0.64 0.000
HD 218857 9.60 0.11 8.88 0.11 3 7.40 0.02 6.87 0.02 3.21 1.09 0.019
HD 241253 10.24 0.00 9.72 0.00 2 8.64 0.03 8.29 0.02 8.66 1.77 0.001
HD 298986 10.46 0.03 10.03 0.03 4 9.04 0.02 8.74 0.02 6.61 1.41 0.004

Not selected

BD+053640 11.16 ... 10.43 ... 0 8.85 0.04 8.34 0.04 15.58 1.82 ...
HD 021581 9.54 0.01 8.71 0.00 2 6.98 0.02 6.41 0.02 4.03 1.00 ...
HD 023439A 8.93 0.01 8.18 0.02 4 6.62 0.02 6.12 0.02 46.65 2.63 ...
HD 023439B 9.26 0.03 8.77 0.01 4 6.95 0.02 6.35 0.02 50.72 1.02 ...
HD 063791 8.81 0.02 7.90 0.01 0 6.05 0.04 5.43 0.02 1.07 0.73 ...
HD 083212 9.39 0.04 8.32 0.03 3 6.31 0.02 5.61 0.02 0.96 0.77 ...
HD 103095 7.19 0.02 6.44 0.02 2 4.94 0.20 4.37 0.03 109.99 0.41 ...
HD 134440 10.22 0.02 9.43 0.01 1 ... ... ... ... 35.14 1.48 ...
HD 199289 8.82 ... 8.30 ... 1 7.18 0.02 6.84 0.02 18.95 0.76 ...
HD 204543 9.17 0.02 8.30 0.01 0 6.46 0.02 5.78 0.02 –0.13 1.08 ...
HD 206739 9.45 0.03 8.60 0.02 0 6.70 0.02 6.03 0.02 1.93 1.17 ...

Notes. The B and V magnitudes were sourced from the GCPD catalogue (Mermilliod et al. 1997) with N number of references. In cases where the B and V were not found in the GCPD catalogue, they were taken from the Simbad database. The J2MASS and K2MASS magnitudes are sourced from 2MASS (Cutri et al. 2003). All parallaxes were taken from a reanalysis of the Hipparcos catalogue (van Leeuwen 2007). The adopted reddening values were taken from Meléndez et al. (2010), Casagrande et al. (2010, 2011).

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