================================================================================
* evaluating spectral indices for data *
================================================================================
================================================================================
* Log-Polynomial fitting of the synchrotron component *
---> first blind fit run, fit range: [10, 21]
---> class: HSP
---> class: HSP
================================================================================
* Log-Polynomial fitting of the IC component *
---> fit range: [21, 29]
---> LogCubic fit
-------------------------------------------------------------------------
Fit report
Model: IC-shape-fit
Table length=4
model name
name
par type
units
val
phys. bound. min
phys. bound. max
log
frozen
LogCubic
b
curvature
-1.547080e-01
-1.000000e+01
0.000000e+00
False
False
LogCubic
c
third-degree
-3.773118e-02
-1.000000e+01
1.000000e+01
False
False
LogCubic
Ep
peak freq
Hz
2.526637e+01
0.000000e+00
3.000000e+01
True
False
LogCubic
Sp
peak flux
erg / (cm2 s)
-1.057499e+01
-3.000000e+01
0.000000e+00
True
False
converged=Truecalls=8mesg=
'Both actual and predicted relative reductions in the sum of squaresn are at most 0.000000 and the relative error between two consecutive iterates is at n most 0.000000'
================================================================================
* constrains parameters from observable *
================================================================================
---> * 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 =3.576347e-01
---> setting par type curvature, corresponding to par r
---> s_radio_mm -0.47152657988709734 1.9430531597741947
---> s_X 3.269798782130266
---> s_Fermi 1.742749327549109
---> s_UV_X 2.745697034461969
---> s_Opt_UV -1.6299328389425476 4.259865677885095
---> 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 2.244223
---> setting par type LE_spectral_slope, corresponding to par s
---> task completed True
---> setting gamma_3p_Sync= 1.738772e+05, assuming B=5.500000e-02
---> task completed True
---> gamma_max=2.858471e+06 from nu_max_Sync= 2.413075e+19, using B=5.500000e-02
---> task completed True
---> setting par type high-energy-cut-off, corresponding to par gmax=6.456134e+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=4.183610e+00
---> task completed True
---> using gamma_3p_Sync= 173877.18803029598
---> nu_p_seed_blob=6.152472e+15
---> COMPTON FACTOR=8.658007e+00 19174.739458022297
---> determine gamma_3p_SSCc= 2.532431e+05
---> task completed True
---> setting par type turn-over energy, corresponding to par gamma0_log_parab=4.346905e+00
---> task completed True
---> using gamma_3p_SSC=2.532431e+05
---> setting par type emitters_density, corresponding to par N
---> to N=3.270101e+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=3.372112e-02
---> setting par type magnetic_field, corresponding to par B
---> task completed True
---> best B found: 3.372112e-02
---> update pars for new B
---> setting par type low-energy-cut-off, corresponding to par gmin
---> task completed True
---> set to 2.220564e+00
---> setting par type low-energy-cut-off, corresponding to par gamma0_log_parab
---> task completed True
---> task completed True
---> using gamma_3p_Sync= 222061.35198046843
---> to 4.289841e+00
---> gamma_max=3.650600e+06 from nu_max_Sync= 2.413075e+19, using B=3.372112e-02
---> task completed True
---> setting par type high-energy-cut-off, corresponding to par gmax
---> set to 6.562364e+00
---> setting par type emitters_density, corresponding to par N
---> to N=6.992430e+00
---> task completed (None, True)
---> setting R from Compton Dominance (CD)
Best R=3.938998e+16
---> setting par type region_size, corresponding to par R
---> set to 3.938998e+16
---> task completed True
---> updating setting par type emitters_density, corresponding to par N
---> set to 6.077016e+00
---> task completed (None, True)
---> t_var (days) 1.0478825116048178
show pars