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Table 1

Binary stellar parameters for known CBP hosts taken from Georgakarakos et al. (2021).

System M1 (M) M2 (M) R1 (R) R2 (R) T1 (K) T2 (K) L (L) L at 1 Myr (L) Fin (L AU−2)
Kepler-16* 0.69 0.20 0.65 0.23 4450 3311 0.15 1.2 25
Kepler-34 1.05 1.02 1.16 1.09 5913 5867 2.5 4.3 82
Kepler-35* 0.89 0.81 1.03 0.79 5606 5202 1.3 3.1 100
Kepler-38 0.95 0.25 1.76 0.27 5640 3325 2.1 2.8 98
Kepler-47* 1.04 0.25 1.76 0.27 5640 3325 0.8 2.5 400
Kepler-64 1.53 0.38 1.73 0.41 6407 3561 4.5 4.5 145
Kepler-413 0.82 0.54 0.77 0.48 4700 3463 0.3 2.2 213
Kepler-453 0.94 0.19 0.83 0.21 5527 3226 0.6 1.9 55
Kepler-1647* 1.21 0.97 1.79 0.97 6210 5777 5.1 5.1 290
Kepler-1661 0.84 0.26 0.76 0.28 5100 3585 0.36 1.8 52
TOI-1338* 1.04 0.3 1.3 0.3 5990 3316 1.96 2.8 167

Notes. Systems considered in this work indicated by asterisks. Left to right, the columns correspond to the mass of the primary, M1, the mass of the secondary, M2, the radius of the primary, R1, the radius of the secondary, R2, the temperature of the primary, T1, the temperature of the secondary, T2, the binary luminosity, L, the binary luminosity at 1 Myr, and irradiation flux at the disc edge, Fin.

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