bulla_bns_kilonova(time, redshift, mej_dyn, ...)
|
Kilonovanet model based on Bulla BNS merger simulations |
bulla_nsbh_kilonova(time, redshift, mej_dyn, ...)
|
Kilonovanet model based on Bulla NSBH merger simulations |
gwem_BaKa2016_bolometric(times, **parameters)
|
|
gwem_BaKa2016_magnitudes(times, **parameters)
|
|
gwem_Bu2019_bolometric(times, **parameters)
|
|
gwem_Bu2019_magnitudes(times, **parameters)
|
|
gwem_Bu2019bc_bolometric(times, **parameters)
|
|
gwem_Bu2019bc_magnitudes(times, **parameters)
|
|
gwem_Bu2019inc_bolometric(times, **parameters)
|
|
gwem_Bu2019inc_magnitudes(times, **parameters)
|
|
gwem_Bu2019lf_bolometric(times, **parameters)
|
|
gwem_Bu2019lf_magnitudes(times, **parameters)
|
|
gwem_Bu2019lm_bolometric(times, **parameters)
|
|
gwem_Bu2019lm_magnitudes(times, **parameters)
|
|
gwem_Bu2019lr_bolometric(times, **parameters)
|
|
gwem_Bu2019lr_magnitudes(times, **parameters)
|
|
gwem_Bu2019lw_bolometric(times, **parameters)
|
|
gwem_Bu2019lw_magnitudes(times, **parameters)
|
|
gwem_Bu2019nsbh_bolometric(times, **parameters)
|
|
gwem_Bu2019nsbh_magnitudes(times, **parameters)
|
|
gwem_Bu2019op_bolometric(times, **parameters)
|
|
gwem_Bu2019op_magnitudes(times, **parameters)
|
|
gwem_Bu2019ops_bolometric(times, **parameters)
|
|
gwem_Bu2019ops_magnitudes(times, **parameters)
|
|
gwem_Bu2019re_bolometric(times, **parameters)
|
|
gwem_Bu2019re_magnitudes(times, **parameters)
|
|
gwem_Bu2019rp_bolometric(times, **parameters)
|
|
gwem_Bu2019rp_magnitudes(times, **parameters)
|
|
gwem_Bu2019rps_bolometric(times, **parameters)
|
|
gwem_Bu2019rps_magnitudes(times, **parameters)
|
|
gwem_DiUj2017_bolometric(times, **parameters)
|
|
gwem_DiUj2017_magnitudes(times, **parameters)
|
|
gwem_Ka2017_bolometric(times, **parameters)
|
|
gwem_Ka2017_magnitudes(times, **parameters)
|
|
gwem_Ka2017inc_bolometric(times, **parameters)
|
|
gwem_Ka2017inc_magnitudes(times, **parameters)
|
|
gwem_Ka2017x2_bolometric(times, **parameters)
|
|
gwem_Ka2017x2_magnitudes(times, **parameters)
|
|
gwem_Ka2017x2inc_bolometric(times, **parameters)
|
|
gwem_Ka2017x2inc_magnitudes(times, **parameters)
|
|
gwem_KaKy2016_bolometric(times, **parameters)
|
|
gwem_KaKy2016_magnitudes(times, **parameters)
|
|
gwem_Me2017_bolometric(times, **parameters)
|
|
gwem_Me2017_magnitudes(times, **parameters)
|
|
gwem_RoFe2017_bolometric(times, **parameters)
|
|
gwem_RoFe2017_magnitudes(times, **parameters)
|
|
gwem_SmCh2017_bolometric(times, **parameters)
|
|
gwem_SmCh2017_magnitudes(times, **parameters)
|
|
gwem_Wo2020dw_bolometric(times, **parameters)
|
|
gwem_Wo2020dw_magnitudes(times, **parameters)
|
|
gwem_Wo2020dyn_bolometric(times, **parameters)
|
|
gwem_Wo2020dyn_magnitudes(times, **parameters)
|
|
gwem_WoKo2017_bolometric(times, **parameters)
|
|
gwem_WoKo2017_magnitudes(times, **parameters)
|
|
kasen_bns_kilonova(time, redshift, mej, vej, ...)
|
Kilonovanet model based on Kasen BNS simulations |
metzger_kilonova_model(time, redshift, mej, ...)
|
|
mosfit_kilonova(time, redshift, mej_1, ...)
|
A three component kilonova model that should be exactly the same as mosfit's kilonova model or Villar et al. 2017. |
mosfit_rprocess(time, redshift, mej, vej, ...)
|
A single component kilonova model that should be exactly the same as mosfit's r-process model. |
nicholl_bns(time, redshift, mass_1, mass_2, ...)
|
Kilonova model from Nicholl et al. 2021, inclides three kilonova components + shock heating from cocoon + disk winds from remnant. |
one_comp_kne_rosswog_heatingrate(time, ...)
|
|
one_component_ejecta_relation(time, ...)
|
Assumes no velocity projection in the ejecta velocity ejecta relation |
one_component_ejecta_relation_projection(...)
|
Assumes a velocity projection between the orthogonal and orbital plane |
one_component_kilonova_model(time, redshift, ...)
|
|
one_component_nsbh_ejecta_relation(time, ...)
|
One component NSBH model |
polytrope_eos_two_component_bns(time, ...)
|
Assumes two kilonova components corresponding to dynamical and disk wind ejecta with properties derived using ejecta relation specified by keyword argument and lambda set by polytropic EOS. |
power_law_stratified_kilonova(time, ...)
|
Assumes a power law distribution of ejecta velocities and a power law distribution of kappa corresponding to the ejecta velocity layers for a total of 10 "shells" and calculates the kilonova light curve, using kilonova heating rate. |
three_component_kilonova_model(time, ...)
|
|
two_comp_kne_rosswog_heatingrate(time, ...)
|
|
two_component_bns_ejecta_relation(time, ...)
|
Assumes two kilonova components corresponding to dynamical and disk wind ejecta with properties derived using ejecta relation specified by keyword argument. |
two_component_kilonova_model(time, redshift, ...)
|
|
two_component_kilonova_with_cocoon(time, ...)
|
|
two_component_nsbh_ejecta_relation(time, ...)
|
Two component NSBH model with dynamical and disk wind ejecta |
two_layer_stratified_kilonova(time, ...)
|
Uses kilonova_heating_rate module to model a two layer stratified kilonova |