Table F.1.
IRFM measurements, photometry, and reddening of the stellar components in KIC 10001167, including magnitude corrections to account for the companion in the photometry.
IRFMa | ||
---|---|---|
Angular diameter, RG (mas) | 0.1376 ± 0.0017 (stat) ±0.0003 (syst) | |
Angular diameter, MS (mas) | 0.01055 ± 0.00022 (stat) ±0.0003 (syst) | |
Teff, RG (K) | 4625 ± 29 (stat) ±30 (syst) | |
Teff, MS (K) | 6031 ± 108 (stat) ±30 (syst) | |
Radius RRG (R⊙) | 12.82 ± 0.30 (stat) ±0.24 (syst) | |
Radius RMS (R⊙) | 0.983 ± 0.47 | |
SB-luminosityb, RG (L⊙) | 67.7 ± 6.1 | |
SB-luminosityb, MS (L⊙) | 1.15 ± 0.14 | |
Companion correction, photometry | RG (dex) | MS (dex) |
Gaia DR3 BP | 0.0259(12) | 4.022(54) |
Gaia DR3 G | 0.0206(8) | 4.275(45) |
Gaia DR3 RP | 0.0166(6) | 4.516(43) |
2MASS J | 0.0117(3) | 4.903(32) |
2MASS H | 0.0089(2) | 5.204(24) |
2MASS Ks | 0.0085(2) | 5.256(23) |
Photometry | RG (mag) | MS (mag) |
Gaia DR3 BP | 10.6213(14) | 14.617(54) |
Gaia DR3 G | 10.06685(82) | 14.321(45) |
Gaia DR3 RP | 9.36093(72) | 13.860(43) |
Gaia DR3 (BP-RP) | 1.2604(16) | 0.757(69) |
2MASS J | 8.407(23) | 13.298(39) |
2MASS H | 7.858(36) | 13.053(43) |
2MASS Ks | 7.756(23) | 13.003(33) |
Reddening & extinction, RG | dex | |
Assumed E(B-V) | 0.0350 (105) | |
(BP-RP)0 | 1.223 (11) | |
ABP | 0.094 (28) | |
AG | 0.074 (22) | |
ARP | 0.057 (17) | |
AJ | 0.0252 (75) | |
AH | 0.0159 (48) | |
AKs | 0.0107 (32) | |
Bolometric corrections, RG | dex | |
BCBP | -0.651 (18) | |
BCG | -0.128 (10) | |
BCRP | 0.5498 (39) | |
BCJ | 1.4461 (79) | |
BCH | 2.019 (18) | |
BCKs | 2.145 (20) | |
Bolometric luminosityc | SB-radiusb, RG | L⊙ | R⊙ |
Lbolo, BP | RBP | 66.1 (57) | 12.66 (60) |
Lbolo, G | RG | 66.8 (56) | 12.73 (58) |
Lbolo, RP | RRP | 67.5 (56) | 12.80 (56) |
Lbolo, J | RJ | 69.2 (58) | 12.95 (56) |
Lbolo, H | RH | 67.1 (60) | 12.76 (56) |
Lbolo, Ks | RKs | 65.3 (56) | 12.59 (53) |
Notes. The IRFM used the temperature ratio TMS/ TRG = 1.2973 ± 0.0076 and radius ratio RMS / RRG = 0.07642 ± 0.00069 from the eclipsing binary analysis. A reddening estimate of E(B−V) = 0.0350 ± 0.0105 is used, a conservative value that puts all three reddening maps discussed in the text within 1σ. The distance used is 866 ± 35pc.
To obtain the single-passband estimates of luminosity and radius of the RG, the following parameters are also used for bolometric corrections: [Fe/H] = −0.68 ± 0.1 dex, Teff, RG = 4625 ± 29 (normal) ± 30 (uniform) K, with Gaia DR3 FSF extinction coefficients from Casagrande et al. (2021) ([Table B1]).
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