redback.sed
Functions
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A general blackbody_to_flux_density formula |
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Create a blackbody spectrum directly from physical parameters. |
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Compute the boosted bolometric luminosity for a blackbody with temperature T (K) and radius R (cm) to account for missing blue flux. |
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Convert flux density in observer frame to spectrum in erg/cm^2/s/Angstrom. |
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Use SNcosmo to get the bandpass flux or magnitude in AB from spectra at given times. |
Classes
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A class that modifies an input SED by incorporating a time‐dependent absorption line feature. |
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SED class for power law + blackbody combination with time-evolving power law |
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