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Table 8
Period-luminosity relations for the Milky Way Cepheids of the form M = a × (log (P) − 1.0) + b.
| Band | a | b | σ |
|
|
|||
| MB | −2.13 ± 0.13 | −3.28 ± 0.05 | 0.39 |
| MV | −2.67 ± 0.10 | −3.96 ± 0.03 | 0.26 |
| MI | −2.81 ± 0.10 | −4.76 ± 0.03 | 0.23 |
| WVI | −3.26 ± 0.11 | −5.96 ± 0.04 | 0.26 |
| MJ | −3.18 ± 0.09 | −5.22 ± 0.03 | 0.22 |
| MH | −3.30 ± 0.08 | −5.59 ± 0.03 | 0.22 |
| MK | −3.33 ± 0.09 | −5.66 ± 0.03 | 0.22 |
| WJK | −3.44 ± 0.09 | −5.96 ± 0.03 | 0.23 |
Notes. The dispersion around the fit is also tabulated as well as the formal uncertainties on the coefficients as returned from the linear regression.
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