Table A.1.
K corrections as a function of stellar parameters, redshift, and reddening.
Teff | log g | [Fe/H] | z | E(B-V) | F555W | F814W | F160W | 2MASS J | 2MASS Ks | F115W | F150W | F200W | F277W | |||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Kext | Aapp | Kext | Aapp | Kext | Aapp | Kext | Aapp | Kext | Aapp | Kext | Aapp | Kext | Aapp | Kext | Aapp | Kext | Aapp | |||||
(K) | (cgs) | (mag) | (mag) | (mag) | (mag) | (mag) | (mag) | (mag) | (mag) | (mag) | (mag) | (mag) | (mag) | (mag) | (mag) | (mag) | (mag) | (mag) | (mag) | (mag) | ||
5400 | 1.5 | 0.00 | 0.005 | 0.00 | -0.010 | 0.000 | -0.001 | 0.000 | -0.001 | 0.000 | -0.002 | 0.000 | 0.005 | 0.000 | -0.002 | 0.000 | -0.001 | 0.000 | 0.005 | 0.000 | 0.004 | 0.000 |
5400 | 1.5 | 0.00 | 0.005 | 0.01 | 0.022 | 0.032 | 0.017 | 0.018 | 0.005 | 0.006 | 0.007 | 0.009 | 0.009 | 0.004 | 0.008 | 0.010 | 0.006 | 0.006 | 0.009 | 0.004 | 0.008 | 0.004 |
5400 | 1.5 | 0.00 | 0.005 | 0.03 | 0.086 | 0.095 | 0.054 | 0.054 | 0.018 | 0.018 | 0.024 | 0.026 | 0.016 | 0.011 | 0.028 | 0.029 | 0.019 | 0.019 | 0.018 | 0.013 | 0.015 | 0.011 |
5400 | 1.5 | 0.00 | 0.005 | 0.05 | 0.151 | 0.158 | 0.091 | 0.089 | 0.031 | 0.031 | 0.042 | 0.043 | 0.024 | 0.018 | 0.048 | 0.049 | 0.032 | 0.032 | 0.026 | 0.021 | 0.022 | 0.018 |
5400 | 1.5 | 0.00 | 0.005 | 0.10 | 0.311 | 0.315 | 0.183 | 0.179 | 0.062 | 0.061 | 0.087 | 0.085 | 0.042 | 0.035 | 0.099 | 0.097 | 0.066 | 0.064 | 0.048 | 0.042 | 0.039 | 0.035 |
5400 | 1.5 | 0.00 | 0.010 | 0.00 | -0.021 | 0.000 | -0.003 | 0.000 | -0.002 | 0.000 | -0.003 | 0.000 | 0.010 | 0.000 | -0.003 | 0.000 | -0.001 | 0.000 | 0.010 | 0.000 | 0.009 | 0.000 |
5400 | 1.5 | 0.00 | 0.010 | 0.01 | 0.011 | 0.032 | 0.015 | 0.018 | 0.004 | 0.006 | 0.006 | 0.009 | 0.014 | 0.004 | 0.007 | 0.010 | 0.005 | 0.006 | 0.014 | 0.004 | 0.012 | 0.004 |
5400 | 1.5 | 0.00 | 0.010 | 0.03 | 0.075 | 0.095 | 0.052 | 0.054 | 0.017 | 0.018 | 0.023 | 0.026 | 0.021 | 0.011 | 0.027 | 0.029 | 0.018 | 0.019 | 0.023 | 0.013 | 0.019 | 0.011 |
5400 | 1.5 | 0.00 | 0.010 | 0.05 | 0.139 | 0.157 | 0.089 | 0.089 | 0.030 | 0.031 | 0.041 | 0.043 | 0.029 | 0.018 | 0.047 | 0.049 | 0.032 | 0.032 | 0.031 | 0.021 | 0.026 | 0.018 |
5400 | 1.5 | 0.00 | 0.010 | 0.10 | 0.299 | 0.315 | 0.180 | 0.178 | 0.061 | 0.061 | 0.085 | 0.085 | 0.047 | 0.035 | 0.097 | 0.097 | 0.064 | 0.064 | 0.053 | 0.042 | 0.044 | 0.035 |
5400 | 1.5 | 0.00 | 0.015 | 0.00 | -0.031 | 0.000 | -0.004 | 0.000 | -0.002 | 0.000 | -0.004 | 0.000 | 0.016 | 0.000 | -0.005 | 0.000 | -0.003 | 0.000 | 0.015 | 0.000 | 0.013 | 0.000 |
5400 | 1.5 | 0.00 | 0.015 | 0.01 | 0.001 | 0.031 | 0.014 | 0.018 | 0.004 | 0.006 | 0.005 | 0.009 | 0.019 | 0.004 | 0.005 | 0.010 | 0.004 | 0.006 | 0.020 | 0.004 | 0.017 | 0.004 |
5400 | 1.5 | 0.00 | 0.015 | 0.03 | 0.065 | 0.094 | 0.050 | 0.053 | 0.016 | 0.018 | 0.023 | 0.026 | 0.027 | 0.010 | 0.025 | 0.029 | 0.017 | 0.019 | 0.028 | 0.013 | 0.024 | 0.011 |
5400 | 1.5 | 0.00 | 0.015 | 0.05 | 0.128 | 0.157 | 0.087 | 0.089 | 0.029 | 0.030 | 0.040 | 0.043 | 0.034 | 0.017 | 0.045 | 0.049 | 0.030 | 0.032 | 0.036 | 0.021 | 0.031 | 0.018 |
5400 | 1.5 | 0.00 | 0.015 | 0.10 | 0.287 | 0.314 | 0.177 | 0.178 | 0.060 | 0.061 | 0.084 | 0.085 | 0.052 | 0.035 | 0.094 | 0.097 | 0.063 | 0.064 | 0.058 | 0.042 | 0.048 | 0.035 |
5400 | 1.5 | 0.00 | 0.020 | 0.00 | -0.040 | 0.000 | -0.005 | 0.000 | -0.003 | 0.000 | -0.007 | 0.000 | 0.021 | 0.000 | -0.007 | 0.000 | -0.004 | 0.000 | 0.020 | 0.000 | 0.017 | 0.000 |
5400 | 1.5 | 0.00 | 0.020 | 0.01 | -0.009 | 0.031 | 0.013 | 0.018 | 0.003 | 0.006 | 0.002 | 0.009 | 0.024 | 0.003 | 0.003 | 0.010 | 0.002 | 0.006 | 0.024 | 0.004 | 0.021 | 0.004 |
5400 | 1.5 | 0.00 | 0.020 | 0.03 | 0.055 | 0.094 | 0.049 | 0.053 | 0.016 | 0.018 | 0.019 | 0.026 | 0.032 | 0.010 | 0.022 | 0.029 | 0.015 | 0.019 | 0.033 | 0.012 | 0.028 | 0.011 |
5400 | 1.5 | 0.00 | 0.020 | 0.05 | 0.118 | 0.157 | 0.085 | 0.089 | 0.028 | 0.030 | 0.037 | 0.042 | 0.039 | 0.017 | 0.042 | 0.048 | 0.028 | 0.032 | 0.041 | 0.021 | 0.035 | 0.018 |
5400 | 1.5 | 0.00 | 0.020 | 0.10 | 0.275 | 0.313 | 0.175 | 0.177 | 0.059 | 0.061 | 0.080 | 0.085 | 0.057 | 0.035 | 0.091 | 0.097 | 0.061 | 0.064 | 0.062 | 0.042 | 0.052 | 0.035 |
5400 | 1.5 | 0.00 | 0.025 | 0.00 | -0.049 | 0.000 | -0.006 | 0.000 | -0.004 | 0.000 | -0.009 | 0.000 | 0.025 | 0.000 | -0.010 | 0.000 | -0.005 | 0.000 | 0.024 | 0.000 | 0.021 | 0.000 |
5400 | 1.5 | 0.00 | 0.025 | 0.01 | -0.018 | 0.031 | 0.012 | 0.018 | 0.003 | 0.006 | -0.001 | 0.008 | 0.029 | 0.003 | 0.000 | 0.010 | 0.001 | 0.006 | 0.028 | 0.004 | 0.025 | 0.004 |
5400 | 1.5 | 0.00 | 0.025 | 0.03 | 0.045 | 0.094 | 0.048 | 0.053 | 0.015 | 0.018 | 0.016 | 0.025 | 0.036 | 0.010 | 0.020 | 0.029 | 0.014 | 0.019 | 0.037 | 0.012 | 0.032 | 0.010 |
5400 | 1.5 | 0.00 | 0.025 | 0.05 | 0.108 | 0.156 | 0.083 | 0.089 | 0.027 | 0.030 | 0.034 | 0.042 | 0.043 | 0.017 | 0.039 | 0.048 | 0.027 | 0.032 | 0.045 | 0.021 | 0.039 | 0.017 |
5400 | 1.5 | 0.00 | 0.025 | 0.10 | 0.264 | 0.312 | 0.172 | 0.177 | 0.058 | 0.061 | 0.077 | 0.085 | 0.062 | 0.035 | 0.088 | 0.097 | 0.059 | 0.064 | 0.066 | 0.041 | 0.056 | 0.035 |
5400 | 1.5 | 0.00 | 0.030 | 0.00 | -0.059 | 0.000 | -0.007 | 0.000 | -0.006 | 0.000 | -0.012 | 0.000 | 0.030 | 0.000 | -0.012 | 0.000 | -0.006 | 0.000 | 0.028 | 0.000 | 0.025 | 0.000 |
5400 | 1.5 | 0.00 | 0.030 | 0.01 | -0.027 | 0.031 | 0.011 | 0.018 | 0.001 | 0.006 | -0.003 | 0.008 | 0.034 | 0.003 | -0.002 | 0.010 | 0.000 | 0.006 | 0.032 | 0.004 | 0.029 | 0.003 |
5400 | 1.5 | 0.00 | 0.030 | 0.03 | 0.035 | 0.094 | 0.046 | 0.053 | 0.013 | 0.018 | 0.014 | 0.025 | 0.041 | 0.010 | 0.017 | 0.029 | 0.013 | 0.019 | 0.040 | 0.012 | 0.036 | 0.010 |
5400 | 1.5 | 0.00 | 0.030 | 0.05 | 0.097 | 0.156 | 0.081 | 0.088 | 0.025 | 0.030 | 0.031 | 0.042 | 0.048 | 0.017 | 0.036 | 0.048 | 0.026 | 0.032 | 0.048 | 0.021 | 0.043 | 0.017 |
5400 | 1.5 | 0.00 | 0.030 | 0.10 | 0.253 | 0.312 | 0.170 | 0.177 | 0.055 | 0.060 | 0.074 | 0.084 | 0.066 | 0.035 | 0.085 | 0.096 | 0.058 | 0.064 | 0.069 | 0.041 | 0.060 | 0.035 |
… |
Noes.
Extinction-dependent K corrections, Kext(Λ), for a wide parameter range covering Teff between 3500 and 6000 K; log g between 2.0 and 0.0; [Fe/H] between −2.0 and 0.5; redshift z between 0.005 and 0.030, and host reddening E(B − V)host between 0.0 and 0.5 mag in the HST/WFC3 filters F555W, F814W, and F160W, 2MASS J & Ks, and JWST/NIRCAM filters F115W, F150W, F200W, and F277W. Kext(Λ) is listed together with Aapp (extinction correction based on apparent color excess) for each filter; (Eq. 9). Extinction applicable to absolute calibration and the foreground is assumed to be corrected, that is, E(B − V)cal = E(B − V)fg = 0.00 mag. The subset of results shown highlight results for the fiducial 10 d Cepheid. The full version of the table is available in machine-readable format at the CDS.
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