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Table B.1

Observed and synthetic photometry.

Magnitude Observation Model
or color Single Binary

(mag)

Johnson-Cousins: (1), (2)
UB −0.568 ± 0.013 −0.584 −0.580
BV −0.120 ± 0.014 −0.099 −0.099
V 5.995 ± 0.008 5.994 5.994

Strömgren: (3), (4), (5)
by −0.035 ± 0.000 −0.008 −0.009
m 1 0.081 ± 0.003 0.058 0.060
c 1 0.411 ± 0.002 0.425 0.427
Hβ 2.660 ± 0.003 2.665 2.671

Geneva: (6), (7)
UB 0.729 ± ... 0.742 0.745
VB 1.098 ± ... 1.098 1.097
B1 − B 0.808 ± ... 0.813 0.814
B2 − B 1.575 ± ... 1.600 1.599
V1 − B 1.786 ± ... 1.799 1.798
GB 2.306 ± ... 2.319 2.318

Hipparcos: (8), (2)
H p 5.9625 ± 0.0010 5.9629 5.9625

Tycho: (9), (2)
B T 5.838 ± 0.014 5.860 5.860
V T 5.973 ± 0.010 5.975 5.975

2MASS: (10), (11)
J 6.189 ± 0.021 6.179 6.180
H 6.212 ± 0.040 6.194 6.195
K 6.238 ± 0.024 6.250 6.251

WISE: (12), (13)
W1 6.282 ± 0.045 6.276 6.278
W2 6.295 ± 0.022 6.289 6.291

Artificial box filter: normalized to Vega
13001800 Å 4.281 ± ... 4.218 4.217
20002500 Å 4.769 ± ... 4.727 4.727
25003000 Å 4.758 ± ... 4.754 4.757

Notes. The quoted uncertainties are taken from literature and are interpreted as 1σ-confidence intervals. Measurements without given uncertainty are assigned the largest of the listed uncertainties of its type, i.e., 0.045 mag for magnitudes and 0.014 mag for colors. A systematic error of 0.012 mag is later added in quadrature to all observations to achieve a reduced χ2 of about 1 at the best fit. For each system, the first reference is with respect to the measurements while the following ones are the sources for synthetic photometry, i.e., for the system response functions and the reference magnitudes of Vega, for which the flux-calibrated spectrum alpha_lyr_stis_008.fits from the CALSPEC database (http://www.stsci.edu/hst/observatory/crds/calspec.html) is used.

Reference. (1) Mermilliod (1991); (2) Bessell & Murphy (2012); (3) Hauck & Mermilliod (1998); (4) Bessell (2011); (5) Castelli & Kurucz (2006); (6) Mermilliod et al. (1997); (7) Rufener & Nicolet (1988); (8) van Leeuwen (2007); (9) Høg et al. (2000); (10) Skrutskie et al. (2006); (11) Cohen et al. (2003); (12) Cutri & et al. (2012); (13) Wright et al. (2010).

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