Table 1.
Coefficients for K corrections as a function of redshift for 10 d Cepheids.
Λ | a | b | c |
---|---|---|---|
HST/WFC3 | |||
F555W | 0.0130 | −2.3909 | |
F814W | 0.0137 | −0.6839 | |
F160W | 0.0044 | −0.1708 | −3.7457 |
WH, VI | 0.0038 | 0.1416 | |
2MASS | |||
J | 0.0065 | −0.1980 | −11.1874 |
Ks | 0.0037 | 1.0587 | −3.1459 |
JWST/NIRCAM | |||
F115W | 0.0084 | −0.6372 | |
F150W | 0.0051 | −0.3688 | |
F200W | 0.0013 | 1.1349 | −8.6439 |
F277W | −0.0003 | 0.8735 |
Notes. K corrections for 10 d Cepheids are computed using mag. Coefficients are limited to z < 0.03 for linear relations and to 0.005 < z < 0.03 for quadratic ones. Quadratic relations were adopted if nonlinear behavior is readily apparent from inspecting the computed values of
, which include host reddening equivalent to E(B − V)host = 0.20 mag that is corrected using apparent color excess.
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