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Table 2

VEGA angular diameter measurements for the 18 early-type stars (see Sect. 3 for a detailed description of the method used to derive the angular diameter of stars).

Name Sp. Type V AV K-ref uR
[mag] [mag] [mag] [mas]
HD 11415 B2V 3.35 0.050 − 0.484±0.012 Ducati (2002) 0.281 0.471±0.007 1.097
HD 114330 A1IV 4.38 0.012 − 0.022±0.04 Cutri et al. (2003) 0.413 0.443±0.023 1.107
HD 145389 B9V 4.23(*) 0.028 − 0.115±0.017 Cutri et al. (2003) 0.358 0.452±0.007 0.089
HD 145570 A1V 4.93 0.003 0.297±0.02 Cutri et al. (2003) 0.512 0.431±0.008 0.114
HD 148112 A2V 4.57(*) 0.016 0.036±0.022 Ducati (2002) 0.410 0.423±0.010 0.089
HD 149438 B0V 2.82 0.214 − 0.939±0.032 Ducati (2002) 0.235 0.338±0.011 0.528
HD 152107 A1V 4.82(*) 0.022 0.229±0.022 Cutri et al. (2003) 0.434 0.432±0.009 0.134
HD 192640 A2V 4.95(*) 0.009 0.520±0.02 Cutri et al. (2003) 0.447 0.489±0.011 0.244
HD 195810 B6IV 4.03(*) 0.053 − 0.398±0.038 Cutri et al. (2003) 0.319 0.394±0.003 0.038
HD 27819 A2V 4.80 0.003 0.347±0.014 Ducati (2002) 0.468 0.489±0.007 1.592
HD 27962 A2IV 4.30(*) 0.003 0.199±0.033 Cutri et al. (2003) 0.350 0.538±0.013 0.587
HD 3360 B2IV 3.67(*) 0.090 − 0.618±0.038 Cutri et al. (2003) 0.278 0.350±0.004 0.299
HD 33959 A9V 5.00(*) 0.006 0.610±0.026 Cutri et al. (2003) 0.476 0.515±0.004 0.472
HD 35468 B2V 1.64(*) 0.003 − 0.686±0.038 Ducati (2002) 0.267 0.785±0.007 1.162
HD 58142 A0.5V 4.61 0.006 0.033±0.018 Cutri et al. (2003) 0.410 0.419±0.008 0.303
HD 886 B2IV 2.83(*) 0.034 − 0.756±0.032 Ducati (2002) 0.277 0.435±0.004 0.478
HD 89021 A1IV 3.43 0.006 0.045±0.094 Ducati (2002) 0.453 0.757±0.007 0.389
HD 97633 A2IV 3.32 0.003 0.017±0.094 Cutri et al. (2003) 0.431 0.769±0.010 1.443

Notes. From left toright: the name of the star, its spectral type taken from the SIMBAD Astronomical Database, the V magnitude (Kharchenko & Roeser 2009), the visual interstellar extinction (Lallement et al. 2014; Capitanio et al. 2017), the color corrected from the extinction, the reference used for the infrared K photometry,the limb-darkening coefficient, the limb-darkened angular diameter, and the reduced chi-squared. (*) Variable stars.

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