Table A.1
Targets and their basic properties (see text for details), ordered by increasing RA.
| Name | Sp. Type | d (pc) | E (B - V) | log(LBOL/L⊙) |  (K) |
log(g−1) | v1 sin(i) (km s−1) |  |
 |
Age (Myr) | Known EB? | Sectors |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| LS I +61 145 | B1V | 2625±79 | 0.46 | 3.97±0.06 | 26000 (fixed) | 109.5±1.3 | 11.2±0.7 | 5.0±0.5 | 4.9±3.6 | g,i,j,p | 17,18,58*,78*,85* | |
| LSI+61 275 | B1.5V | 2142±85 | 0.62 | 3.74±0.08 | 24630±388 | 160±12 | 9.6±0.6 | 4.1±0.4 | 3.3±3.0 | a,h,j,p | 18,58,85,86 | |
| AN Dor | B2V | 950±38 | 0.02 | 3.65±0.08 | 21529±65 | 4.02±0.01 | 162.1±1.1 | 8.2±0.3 | 4.7±0.1 | 17.6±1.7 | c,f,g,i,j,k,n,p,r,s,t,u | t |
| TYC 1881-933-1 | B2V | 1928±96 | 0.33 | 3.40±0.10 | 18700±428 | 4.11 ±0.12 | 143.3±20.7 | 6.6±0.4 | 4.1±0.5 | 29.3±6.7 | b,m,p | K+ 43,44,45,71,72 |
| HD 254346 | B1.5V | 1730±82 | 0.45 | 4.02±0.09 | 24757±145 | 3.80±0.02 | 201.2±1.9 | 11.0±0.5 | 5.9±0.5 | 11.6±1.2 | g,l | 43*,44*,45*,71*,72* |
| TYC 741-1565-1 | B2V | 3030±154 | 0.50 | 3.49±0.10 | 23634±391 | 3.95±0.05 | 148.9±5.8 | 8.8±0.3 | 3.8±0.3 | 3.9±3.4 | h,s,t | 6*, 33, 71*,72* |
| HD 309317 | B2V | 2197±95 | 0.21 | 3.80±0.09 | 22978±167 | 4.14±0.02 | 203.1±2.6 | 9.0±0.5 | 4.5±0.5 | 11.8±3.5 | i,j,v | 10,11,37,38,64* |
| HD 112485 | B1.5V | 1749±67 | 0.37 | 4.07±0.08 | 26096±659 | 4.06±0.07 | 184.0±8.4 | 11.6±0.6 | 5.2±0.4 | 7.2±1.9 | g,i,j | 11,38,64*,65* |
| V1061 Cen | B2V | 1374±39 | 0.33 | 3.57±0.06 | c,g,p,q | 11,38,65* | ||||||
| V1208Sco | B0.5V | 1504±32 | 0.49 | 4.14±0.04 | 29600±100 | 4.25±0.02 | 87±8 | 13.6±0.2 | 4.6±0.1 | 0.6±0.4 | d,e,o | 12,39 |
| HD 154407C | B1V | 1298±70 | 0.45 | 4.13±0.11 | 25696±467 | 4.32±0.06 | 144.8±7.3 | 11.0±0.6 | 4.6±0.4 | 4.8±2.7 | g,i,j | 12,66* |
| HD 350685 | B1.5V | 1974±82 | 0.37 | 3.98±0.08 | 25832±142 | 4.09±0.02 | 247.7±2.0 | 11.2±0.6 | 5.0±0.2 | 6.2±1.0 | h,i,j,v | 14,41,54 |
Notes. Error on the bolometric luminosity is derived from the error on distance. The effective temperature of LS I +61 145 could not be evaluated from spectra hence is assumed to be that corresponding to its spectral type. For LS I +61 275, the effective temperature comes from Huang & Gies (2006b) and the projected rotational velocity from Huang & Gies (2006a). For TYC 1881933-1, the effective temperature, gravity, and projected rotation rates are averages from values reported for the star in Xiang et al. (2022) and errors correspond to dispersions. For V1208 Sco, the effective temperature, gravity, and projected rotation rates come from McSwain et al. (2009). For the best-fit evolutionary parameters, the largest error is used if asymmetric. References for the eclipsing binary (EB) status are: (a) Antipin (2008), (b) Armstrong et al. (2015), (c) Avvakumova et al. (2013), (d) Balona & Engelbrecht (1985), (e) Banyard et al. (2023), (f) Dubath et al. (2011), (g) Eze & Handler (2024), (h) Green et al. (2023), (i) IJspeert et al. (2021), (j) IJspeert et al. (2024), (k) Kazarovets et al. (1999), (l) Labadie-Bartz et al. (2020), (m) LaCourse et al. (2015), (n) Malkov et al. (2006), (o) Martín-Ravelo et al. (2024), (p) Mowlavi et al. (2023), (q) Otero (2003), (r) Percy & Au-Yong (2000), (s) Prsa et al. (2022), (t) Shi et al. (2022), (u) Southworth & Bowman (2022), and (v) Tkachenko et al. (2024). For the last column, K indicates Kepler data, the asterisk * identifies 2-min light curves, bold shows which Sectors were averaged and combined to get the binned light curve which was analyzed, and the † symbol corresponds to Sectors 2*,3*,4*,5*,6*,9,12,13,29*,30*,31*,32*,33*,36*,39*,63*,64*,65*, 66*,67*,69*.
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