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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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