arnett(time, redshift, f_nickel, mej, **kwargs)
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- param time:
time in days
|
arnett_bolometric(time, f_nickel, mej, **kwargs)
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- param time:
time in days
|
basic_magnetar_powered(time, redshift, p0, ...)
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- param time:
time in days in observer frame
|
basic_magnetar_powered_bolometric(time, p0, ...)
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- param time:
time in days in source frame
|
csm_interaction(time, redshift, mej, ...)
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- param time:
time in days in observer frame
|
csm_interaction_bolometric(time, mej, ...)
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- param time:
time in days in source frame
|
csm_nickel(time, redshift, mej, f_nickel, ...)
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Assumes csm and nickel engine with homologous expansion |
exponential_powerlaw_bolometric(time, ...)
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- param time:
rest frame time in days
|
general_magnetar_driven_supernova(time, ...)
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- param time:
time in observer frame in days
|
general_magnetar_driven_supernova_bolometric(...)
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- param time:
time in observer frame in days
|
general_magnetar_slsn(time, redshift, l0, ...)
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- param time:
time in days in observer frame
|
general_magnetar_slsn_bolometric(time, l0, ...)
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- param time:
time in days in source frame
|
homologous_expansion_supernova(time, ...)
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Assumes homologous expansion to transform kinetic energy to ejecta velocity |
homologous_expansion_supernova_model_bolometric(...)
|
Assumes homologous expansion to transform kinetic energy to ejecta velocity |
magnetar_nickel(time, redshift, f_nickel, ...)
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- param time:
time in days in observer frame
|
shock_cooling_and_arnett(time, redshift, ...)
|
- param time:
time in days
|
slsn(time, redshift, p0, bp, mass_ns, ...)
|
Same as basic magnetar_powered but with constraint on rotational_energy/kinetic_energy and nebula phase |
slsn_bolometric(time, p0, bp, mass_ns, ...)
|
Same as basic magnetar_powered but with constraint on rotational_energy/kinetic_energy and nebula phase |
sn_exponential_powerlaw(time, redshift, ...)
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- param time:
observer frame time in days
|
sncosmo_models(time, redshift[, model_kwargs])
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A wrapper to SNCosmo models |
thin_shell_supernova(time, redshift, mej, ...)
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Assumes thin shell ejecta to transform kinetic energy into ejecta velocity |
thin_shell_supernova_model_bolometric(time, ...)
|
Assumes thin shell ejecta to transform kinetic energy into ejecta velocity |
type_1a(time, redshift, f_nickel, mej, **kwargs)
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A nickel powered explosion with line absorption and cutoff blackbody SED for SNe 1A. |
type_1c(time, redshift, f_nickel, mej, pp, ...)
|
A nickel powered explosion with synchrotron and blackbody SED's for SNe 1C. |