Table 1
Spectral types and effective temperatures of the stars used in our SED sample.
Star | Spectral type | Effective temperature (K) |
---|---|---|
_(1) | A0 | 10 000 |
_(2) | A7 | 7500 |
WASP-17 | F4 | 6548 |
HD 149026 | G0 | 6084 |
WASP-127 | G5 | 5828 |
Sun | G2 | 5800 |
WASP-77 A | G8 | 5605 |
TOI-193 | G7 | 5443 |
HD 97658 | K1 | 5110 |
HD 40307 | K2.5 | 4880 |
HAT-P-12 | K5 | 4653 |
HD 85512 | K6 | 4200 |
WASP-43 | K7 | 4124 |
GJ 15 A | M1 | 3700 |
GJ 176 | M2 | 3600 |
GJ 436 | M3 | 3500 |
GJ 849 | M3.5 | 3450 |
GJ 876 | M4 | 3400 |
LHS-2686 | M5 | 3200 |
LP-791-18 | M6 | 2949 |
TRAPPIST-1 | M7.5 | 2800 |
Notes. For the stars from the MUSCLES Extension (Behr et al. 2023), we adopted the spectral types and effective temperatures as listed in the paper. For the other stars, we first adopted the spectral type from Simbad3, using an intermediate value when there are multiple measurements. We then adopted an effective temperature based on a conversion table from the spectral type, assuming main-sequence stars4. (1)Synthetic spectrum from Fossati et al. (2018). (2)Synthetic spectrum from Fossati et al. (2018), with 3× solar XUV flux.
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