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Table 1.
Parameters of the 
relation for each method.
| Slope | Y-intercept | σ | r | Pu | Nin(b) | Nout(b) | |
|---|---|---|---|---|---|---|---|
| Method(a) | (K/μHz) | (K) | (%) | (%) | (%) | (%) | |
| LFIT(1) | 2.94 ± 0.24 | 6980 ± 50 | 5.82 | 0.424 | 7 × 10−30 | 99.3 | 0.7 |
| LFIT(2) | 2.50 ± 0.10 | 7050 ± 30 | 5.62 | 0.551 | 6 × 10−116 | 99.4 | 0.6 |
| MFIT | 3.34 ± 0.17 | 6890 ± 40 | 0.81 | 0.972 | 13 × 10−19 | 99.4 | 0.6 |
| KFIT | 2.50 ± 0.55 | 7090 ± 120 | 1.59 | 0.882 | 4 × 10−3 | 99.4 | 0.6 |
Notes.
(a)
See Sect. 3.1.
(b)
Number of stars in and out of the expected departure of temperature limits taking into account Ω ∼ ΩC (see text).
(1)
Values taken from Barceló Forteza et al. (2018).
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