redback.transient_models.spectral_models
Functions
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Band function (Band et al. 1993) spectrum. |
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Blackbody spectrum for high-energy transients. |
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A blackbody spectrum at a given redshift, properly accounting for redshift effects. |
A blackbody spectrum with one absorption line and one emission line. |
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Blackbody spectrum with multiple P-Cygni line profiles |
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Comptonized (cutoff power-law with peak energy) spectrum converted to flux density. |
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Cutoff power-law photon spectrum converted to flux density. |
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Elementary P-Cygni profile with simple parameterization |
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Pure Gaussian line profile |
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Pure Lorentzian (Cauchy) line profile |
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Full spectrum with multiple P-Cygni profiles |
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P-Cygni line profile using Sobolev approximation |
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Power-law photon spectrum converted to flux density. |
A powerlaw + blackbody spectrum at a given redshift and time, properly accounting for redshift effects. |
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A power law spectrum with one absorption line and one emission line. |
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Add multiple Voigt absorption lines to a continuum |
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SYNOW-style parameterized line profile |
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TBabs-absorbed power-law spectrum converted to flux density. |
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Voigt profile: convolution of Gaussian and Lorentzian line profiles |