Note:
Dust mean SEDs here are derived by broad band SED fitting or interpolation, which may cause model dependance.
Dust mean SED derived by X-Cigale fitting is relatively lower than others. It’s because X-Cigale considers a cooler disk component which contibutes more at IR bands.
Catalog Description
| Column Name | Description |
|---|---|
wavelength |
Rest-frame wavelength (\(\mu m\)) |
polar_frac_a |
Polar dust fraction (Case A) |
polar_frac_b |
Polar dust fraction (Case B) |
polar_frac_a_10 |
Polar dust fraction assuming 10% contribution at 2.1 \(\mu m\) (Case A) |
polar_frac_b_10 |
Polar dust fraction assuming 10% contribution at 2.1 \(\mu m\) (Case B) |
mean_sed_hc |
Dust mean SED derived from hot + cold dust model SED fitting |
mean_sed_xc |
Dust mean SED derived from X-Cigale SED fitting |
mean_sed_l |
Dust mean SED derived from linear interpolation |
mean_sed_s |
Dust mean SED derived from spline interpolation |
polar_mean_sed_hc_a |
Polar dust mean SED derived from hot + cold dust model SED fitting (Case A) |
polar_mean_sed_xc_a |
Polar dust mean SED derived from X-Cigale SED fitting (Case A) |
polar_mean_sed_l_a |
Polar dust mean SED derived from linear interpolation (Case A) |
polar_mean_sed_s_a |
Polar dust mean SED derived from spline interpolation (Case A) |
polar_mean_sed_hc_b |
Polar dust mean SED derived from hot + cold dust model SED fitting (Case B) |
polar_mean_sed_xc_b |
Polar dust mean SED derived from X-Cigale SED fitting (Case B) |
polar_mean_sed_l_b |
Polar dust mean SED derived from linear interpolation (Case B) |
polar_mean_sed_s_b |
Polar dust mean SED derived from spline interpolation (Case B) |