Table C.1.
Comparison between PWJK relations in the LMC based on different extinction laws.
| Mode |
 |
α | σα | β | σβ | RMS | n.stars | Ext. law |
|---|---|---|---|---|---|---|---|---|
| mag | mag | mag/dex | mag/dex | mag | ||||
| F | 0.52 | 16.564 | 0.024 | −3.20 | 0.13 | 0.146 | 76 | Wang & Chen (2023) |
| F | 0.69 | 16.504 | 0.025 | −3.21 | 0.13 | 0.152 | 76 | Cardelli et al. (1989) |
| F | 0.74 | 16.492 | 0.025 | −3.21 | 0.13 | 0.152 | 76 | Fitzpatrick (1999) |
| F+1O | 0.52 | 16.542 | 0.015 | −3.19 | 0.11 | 0.156 | 111 | Wang & Chen (2023) |
| F+1O | 0.69 | 16.494 | 0.022 | −3.25 | 0.11 | 0.148 | 109 | Cardelli et al. (1989) |
| F+1O | 0.74 | 16.482 | 0.015 | −3.25 | 0.11 | 0.148 | 109 | Fitzpatrick (1999) |
Notes. The different columns report: (1) the pulsating mode; (2) the coefficient of the color term in the PWJK; (3)–(4) the α coefficient (relative intercept) and relative uncertainty; (5)–(6) the β coefficient (slope) and relative uncertainty; (7) the Root Mean Square (RMS) of the relation; (8) the number of stars used in the fit; (9) the corresponding extinction law.
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