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Table 3.
Same as in Table 2, but for All Sky Cepheids.
| Type | Mode | α | β | σABL | Band | N |
|---|---|---|---|---|---|---|
| All sky | ||||||
| DCEP | F | −2.744 ± 0.045 | −3.391 ± 0.052 | 0.015 | W(G, GBP − GRP) | 898 |
| DCEP | 1O | −3.224 ± 0.028 | −3.588 ± 0.065 | 0.021 | W(G, GBP − GRP) | 416 |
| ACEP | F | −1.717 ± 0.025 | −3.080 fixed | 0.010 | W(G, GBP − GRP) | 4 |
| ACEP | 1O | −2.220 ± 0.061 | −3.500 fixed | 0.013 | W(G, GBP − GRP) | 4 |
| T2CEP | – | −1.224 ± 0.039 | −2.542 ± 0.088 | 0.041 | W(G, GBP − GRP) | 264 |
Notes. The reported values of the scatter refer to the residuals around the fit in the ABL formalism. For the ACEPs the slopes are fixed to those of the LMC.
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