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* evaluating spectral indices for data *
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================================================================================
* Log-Polynomial fitting of the synchrotron component *
---> first blind fit run, fit range: [10, 21]
---> class: HSP
---> class: HSP
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* Log-Polynomial fitting of the IC component *
---> fit range: [21, 29]
---> LogCubic fit
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Fit report
Model: IC-shape-fit
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* constrains parameters from observable *
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---> * emitting region parameters *
---> setting par type redshift, corresponding to par z_cosm
---> setting par type magnetic_field, corresponding to par B=5.500000e-02
---> setting par type region_size, corresponding to par R=3.759008e+16
---> completed True
---> * electron distribution parameters *
---> emitters distribution spectral type lp
---> emitters distribution name lppl
---> r elec. spec. curvature =3.164664e-01
---> setting par type curvature, corresponding to par r
---> s_radio_mm -0.30143740557836884 1.6028748111567377
---> s_X 3.260509876361173
---> s_Fermi 1.7437546345348394
---> s_UV_X 2.751533577945437
---> s_Opt_UV -1.4757840746130748 3.9515681492261496
---> s from synch log-log fit -1.0
---> s from (s_Fermi + s_UV)/2
---> power-law index s, class obj=HSP s chosen is 2.247644
---> setting par type LE_spectral_slope, corresponding to par s
---> task completed True
---> setting gamma_3p_Sync= 1.640668e+05, assuming B=5.500000e-02
---> task completed True
---> gamma_max=2.624871e+06 from nu_max_Sync= 2.034788e+19, using B=5.500000e-02
---> task completed True
---> setting par type high-energy-cut-off, corresponding to par gmax=6.419108e+00
---> setting par type low-energy-cut-off, corresponding to par gmin=2.114333e+00
---> task completed True
---> setting par type turn-over energy, corresponding to par gamma0_log_parab=4.026339e+00
---> task completed True
---> using gamma_3p_Sync= 164066.75635246406
---> nu_p_seed_blob=5.477793e+15
---> COMPTON FACTOR=7.273642e+00 19280.86710976314
---> determine gamma_3p_SSCc= 2.354425e+05
---> task completed True
---> setting par type turn-over energy, corresponding to par gamma0_log_parab=4.183203e+00
---> task completed True
---> using gamma_3p_SSC=2.354425e+05
---> setting par type emitters_density, corresponding to par N
---> to N=3.847571e+00
---> task completed (None, True)
---> setting B from nu_p_S to B=1.000000e+00
---> to B=1.000000e+00
---> setting B from best matching of nu_p_IC
Best B=3.381593e-02
---> setting par type magnetic_field, corresponding to par B
---> task completed True
---> best B found: 3.381593e-02
---> update pars for new B
---> setting par type low-energy-cut-off, corresponding to par gmin
---> task completed True
---> set to 2.219954e+00
---> setting par type low-energy-cut-off, corresponding to par gamma0_log_parab
---> task completed True
---> task completed True
---> using gamma_3p_Sync= 209238.34842644221
---> to 4.131959e+00
---> gamma_max=3.347563e+06 from nu_max_Sync= 2.034788e+19, using B=3.381593e-02
---> task completed True
---> setting par type high-energy-cut-off, corresponding to par gmax
---> set to 6.524729e+00
---> setting par type emitters_density, corresponding to par N
---> to N=8.124667e+00
---> task completed (None, True)
---> setting R from Compton Dominance (CD)
Best R=4.529214e+16
---> setting par type region_size, corresponding to par R
---> set to 4.529214e+16
---> task completed True
---> updating setting par type emitters_density, corresponding to par N
---> set to 4.644690e+00
---> task completed (None, True)
---> t_var (days) 1.2048961072957096
show pars