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Table 11.
Combined fits to cluster Cepheids and (field) MW Cepheids.
| Filter | α | β | ΔϖCep | ⟨[Fe/H]⟩ | NCep | Ncl |
|---|---|---|---|---|---|---|
| (mag/log P) | (mag) | (μas) | ||||
 |
−3.412 ± 0.053 | −6.003 ± 0.020 | −19 ± 5 | 0.086 | 67 | 15 |
| WG | −3.303 ± 0.049 | −6.051 ± 0.020 | −22 ± 3 | 0.069 | 225 | 26 |
| Bp | −2.513 ± 0.080 | −4.225 ± 0.036 | −21 ± 6 | 0.069 | 243 | 23 |
| V | −2.553 ± 0.071 | −4.377 ± 0.033 | −22 ± 5 | 0.069 | 246 | 22 |
| G | −2.751 ± 0.077 | −4.612 ± 0.035 | −22 ± 5 | 0.068 | 238 | 23 |
| Rp | −2.804 ± 0.058 | −4.984 ± 0.025 | −19 ± 4 | 0.068 | 234 | 23 |
| F160W(a) | −3.353 ± 0.060 | −5.729 ± 0.023 | −23 ± 6 | 0.088 | 67 | 15 |
| WH(b) | −3.406 ± 0.052 | −5.953 ± 0.020 | −18 ± 5 | 0.086 | 67 | 15 |
| F160W(b) | −3.346 ± 0.060 | −5.679 ± 0.023 | −22 ± 6 | 0.088 | 67 | 15 |
Notes.
(b)
Includes the CRNL correction (mean 0.010 mag) to facilitate comparison with extragalactic Cepheid samples (Riess et al. 2022a).
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