Table A.1.
Different reddening values (first entries only).
Name | E(B − V) | σ | E(B − V) | σ | E(B − V) | E(B − V) | σ | E(B − V) | σ | Remarks |
---|---|---|---|---|---|---|---|---|---|---|
AA Gem | 0.340 | 0.040 | − | − | 0.327 | 0.461 | 0.054 | 0.272 | 0.057 | |
AA Mon | 0.770 | 0.020 | − | − | 0.628 | 0.972 | 0.093 | 0.679 | 0.087 | |
AB Cam | 0.620 | 0.040 | − | − | 0.800 | 0.951 | 0.105 | 0.575 | 0.204 | |
AC Mon | 0.510 | 0.030 | − | − | 0.464 | 0.464 | 0.144 | 0.560 | 0.314 | |
AD Cam | 0.870 | 0.010 | − | − | 0.830 | 0.973 | 0.058 | 0.875 | 0.110 | |
AD Cru | 0.640 | 0.010 | − | − | 0.426 | 0.568 | 0.081 | − | − | |
AD Gem | 0.210 | 0.050 | − | − | 0.141 | 0.172 | 0.028 | 0.055 | 0.044 | |
AD Pup | 0.360 | 0.020 | − | − | 0.257 | 0.498 | 0.084 | 0.240 | 0.078 | |
AE Tau | 0.570 | 0.060 | − | − | 0.526 | 0.832 | 0.070 | 0.455 | 0.018 | |
AE Vel | 0.690 | 0.060 | − | − | 0.338 | 0.368 | 0.136 | − | − | |
AG Cru | 0.240 | 0.020 | − | − | 0.243 | 0.243 | 0.146 | − | − | |
AH Vel | 0.040 | 0.020 | − | − | 0.057 | 0.057 | 0.056 | − | − | |
α UMi | 0.020 | 0.010 | − | − | 0.007 | 0.007 | 0.015 | − | − | |
AN Aur | 0.540 | 0.040 | − | − | 0.346 | 0.514 | 0.070 | 0.436 | 0.050 | |
AO Aur | 0.440 | 0.040 | − | − | 0.393 | 0.620 | 0.122 | 0.388 | 0.072 | |
AO CMa | 0.690 | 0.070 | − | − | 0.157 | 0.279 | 0.112 | 0.525 | 0.071 | |
AP Pup | 0.250 | 0.030 | − | − | 0.354 | 0.354 | 0.082 | − | − | |
AP Sgr | 0.180 | 0.010 | − | − | 0.236 | 0.236 | 0.109 | 0.230 | 0.075 | |
AQ Car | 0.170 | 0.010 | − | − | 0.197 | 0.296 | 0.085 | − | − | |
AQ Pup | 0.530 | 0.020 | 0.486 | 0.023 | 0.186 | 0.249 | 0.130 | 0.302 | 0.059 | |
AS Per | 0.680 | 0.040 | − | − | 0.670 | 0.670 | 0.123 | 0.621 | 0.162 | |
AT Pup | 0.170 | 0.010 | − | − | 0.185 | 0.185 | 0.008 | − | − | |
AV Cir | 0.370 | 0.010 | − | − | 0.176 | 0.176 | 0.047 | − | − | |
AV Sgr | 1.240 | 0.030 | − | − | 1.421 | 1.440 | 0.150 | 1.099 | 0.398 | |
AW Per | 0.480 | 0.020 | 0.520 | 0.017 | 0.588 | 0.588 | 0.087 | 0.488 | 0.055 | |
AX Cir | 0.270 | 0.120 | 0.313 | 0.017 | 0.128 | 0.128 | 0.042 | − | − | |
AX Vel | 0.260 | 0.040 | − | − | 0.114 | 0.114 | 0.073 | − | − | |
AY Cen | 0.360 | 0.070 | − | − | 0.211 | 0.211 | 0.054 | − | − | |
AZ Cen | 0.170 | 0.010 | − | − | 0.296 | 0.296 | 0.056 | − | − | |
BB Cen | 0.380 | 0.040 | − | − | 0.338 | 0.527 | 0.065 | − | − | |
BB Gem | 0.430 | 0.040 | − | − | 0.474 | 0.612 | 0.102 | 0.452 | 0.092 | |
BB Her | 0.390 | 0.040 | − | − | 0.366 | 0.460 | 0.025 | 0.359 | 0.055 | |
BB Sgr | 0.280 | 0.010 | 0.290 | 0.017 | 0.235 | 0.235 | 0.089 | 0.304 | 0.071 | |
BC Pup | 0.800 | 0.080 | − | − | 0.236 | 0.780 | 0.051 | 0.708 | 0.081 | |
BD Cas | 1.010 | 0.100 | − | − | 0.529 | 0.582 | 0.081 | 0.850 | 0.148 | HRD |
β Dor | 0.070 | 0.010 | −.007 | 0.017 | 0.014 | 0.014 | 0.016 | − | − | |
BF Oph | 0.260 | 0.020 | 0.219 | 0.017 | 0.281 | 0.281 | 0.071 | 0.235 | 0.031 | |
BG Cru | 0.100 | 0.020 | − | − | 0.148 | 0.148 | 0.036 | − | − | |
BG Lac | 0.340 | 0.020 | 0.282 | 0.017 | 0.187 | 0.187 | 0.040 | 0.286 | 0.032 | |
BG Vel | 0.430 | 0.010 | − | − | 0.073 | 0.073 | 0.161 | − | − | |
BK Aur | 0.390 | 0.030 | − | − | 0.396 | 0.418 | 0.052 | 0.375 | 0.025 | |
BM Per | 0.920 | 0.060 | − | − | 0.966 | 1.023 | 0.117 | 0.951 | 0.475 | |
BN Pup | 0.420 | 0.020 | 0.485 | 0.020 | 0.163 | 0.358 | 0.165 | 0.490 | 0.095 | |
BP Cir | 0.260 | 0.040 | − | − | 0.166 | 0.166 | 0.049 | − | − | |
BQ Ser | 0.780 | 0.010 | − | − | 0.766 | 0.766 | 0.114 | 0.706 | 0.080 | |
BZ Cyg | 0.830 | 0.020 | − | − | 0.665 | 0.665 | 0.073 | 0.987 | 0.157 | |
CD Cyg | 0.510 | 0.020 | 0.593 | 0.016 | 0.641 | 0.704 | 0.071 | 0.458 | 0.154 |
Notes. Columns 2–3 are the adopted reddening and error, repeated from Table 1, Cols. 4–5 are the reddening and error from Trahin (2019), Cols. 6–8 are the results from the 3D model by Lallement et al. (2018). The E(B − V) value in Col. 6 is the one in the available grid at the distance closest to distance of the object. The value in Col. 7 is the E(B − V) value at the distance of the object, based on the extrapolation explained in the main text. Column 8 lists the error. Cols. 9–10 are the results from the 3D model by Green et al. (2019), The last column indicates if a star is an outlier in the HRD (Fig. 2, labelled as HRD) or in the comparison with the spectroscopic temperature determinations (Fig. 4, labelled as TEF). The full table is available at the CDS.
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