check_boundaries(val, val_min, val_max, val_name) |
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check_gamma_tansp(jet, beaming_val, …) |
retrun tau_gamma_gamma for a given IC frequency |
check_t_var(R, beaming, z) |
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constr_B_from_nu_peaks(jet, nu_p_S, nu_p_IC, …) |
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constr_R_from_CD(jet, nuFnu_p_S, nuFnu_p_IC, …) |
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find_B_from_nu_p_S(nu_p_S, gamma_3p, …) |
returns B according to Ep_S and gamma_3p |
find_gamma0(r, s, gamma_3p) |
returns the value of gamma_0 for |
find_gamma_3p_SSC(nu_p_S, nu_p_IC, …[, …]) |
returns the value of gamma_3p from nu_p_S/nu_p_IC |
find_gamma_Synch(nu_S, rest_frame, B, beaming, z) |
returns the value of gamma corresponding to the Synch freq |
find_HE_cut_off(distr_e, nu_S_max, …) |
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find_s(class_obj, nu_p_S_obs, S_LE_slope, …) |
Find the index of the low-energy PL branch of n(gamma), from PL fit over various instrument bands |
find_s1(class_obj, indices) |
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find_turn_over(jet, distr_e, gamma_3p) |
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get_Comp_factor(gamma, nu_p_S_blob) |
returns the compton factor = nu_blob_seed_Synch*hplanck/(mec2) |
get_R_tvar(beaming, t_var_sec, z) |
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get_U_Sync_from_Ph(jet[, re_eval_sync]) |
returns U_synch by integrating Synch photon spectrum |
rescale_Ne(jet, Lp_S, rest_frame) |
Rescales N.blob to get the wanted Lp_S_blob |
set_gmin_from_nu_cut_IR(nu_cut_IR, …) |
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