Example to use the Sherpa minimizer plugin with a JeSeT model#
In this tutorial we show how to import a jetset model into sherpa, and finally we perform a model fitting. To run this plugin you have to install Sherpa: https://sherpa.readthedocs.io/en/latest/install.html
import jetset
print('tested with',jetset.__version__)
tested with 1.4.0rc3
import warnings
warnings.filterwarnings('ignore')
import matplotlib.pylab as plt
import jetset
from jetset.test_data_helper import test_SEDs
from jetset.data_loader import ObsData,Data
from jetset.plot_sedfit import PlotSED
from jetset.test_data_helper import test_SEDs
test_SEDs
['/Users/orion/miniforge3/envs/jetset/lib/python3.12/site-packages/jetset/test_data/SEDs_data/SED_3C345.ecsv',
'/Users/orion/miniforge3/envs/jetset/lib/python3.12/site-packages/jetset/test_data/SEDs_data/SED_MW_Mrk421_EBL_DEABS.ecsv',
'/Users/orion/miniforge3/envs/jetset/lib/python3.12/site-packages/jetset/test_data/SEDs_data/SED_MW_Mrk501_EBL_ABS.ecsv',
'/Users/orion/miniforge3/envs/jetset/lib/python3.12/site-packages/jetset/test_data/SEDs_data/SED_MW_Mrk501_EBL_DEABS.ecsv']
Loading data#
see the Data format and SED data user guide for further information about loading data
print(test_SEDs[2])
data=Data.from_file(test_SEDs[2])
/Users/orion/miniforge3/envs/jetset/lib/python3.12/site-packages/jetset/test_data/SEDs_data/SED_MW_Mrk501_EBL_ABS.ecsv
%matplotlib inline
sed_data=ObsData(data_table=data)
sed_data.group_data(bin_width=0.2)
sed_data.add_systematics(0.1,[10.**6,10.**29])
p=sed_data.plot_sed()
================================================================================ * binning data * ---> N bins= 88 ---> bin_width= 0.2 ================================================================================
sed_data.save('Mrk_501.pkl')
phenomenological model constraining#
see the Phenomenological model constraining: application user guide for further information about phenomenological constraining
spectral indices#
from jetset.sed_shaper import SEDShape
my_shape=SEDShape(sed_data)
my_shape.eval_indices(minimizer='lsb',silent=True)
p=my_shape.plot_indices()
p.setlim(y_min=1E-15,y_max=1E-6)
================================================================================ * evaluating spectral indices for data * ================================================================================
sed shaper#
mm,best_fit=my_shape.sync_fit(check_host_gal_template=True,
Ep_start=None,
minimizer='lsb',
silent=True,
fit_range=[10.,21.])
================================================================================ * Log-Polynomial fitting of the synchrotron component * ---> first blind fit run, fit range: [10.0, 21.0] ---> class: HSP ---> class: HSPTable length=6
| model name | name | val | bestfit val | err + | err - | start val | fit range min | fit range max | frozen |
|---|---|---|---|---|---|---|---|---|---|
| LogCubic | b | -5.589204e-02 | -5.589204e-02 | 6.234641e-03 | -- | -5.237376e-02 | -1.000000e+01 | 0.000000e+00 | False |
| LogCubic | c | -3.292704e-04 | -3.292704e-04 | 8.968206e-04 | -- | 7.639964e-03 | -1.000000e+01 | 1.000000e+01 | False |
| LogCubic | Ep | 1.698160e+01 | 1.698160e+01 | 8.583094e-02 | -- | 1.556163e+01 | 0.000000e+00 | 3.000000e+01 | False |
| LogCubic | Sp | -1.030620e+01 | -1.030620e+01 | 1.607997e-02 | -- | -1.019011e+01 | -3.000000e+01 | 0.000000e+00 | False |
| host_galaxy | nuFnu_p_host | -9.972939e+00 | -9.972939e+00 | 3.177593e-02 | -- | -1.019011e+01 | -1.219011e+01 | -8.190114e+00 | False |
| host_galaxy | nu_scale | -2.290459e-03 | -2.290459e-03 | 1.811408e-03 | -- | 0.000000e+00 | -2.908697e-03 | 2.908697e-03 | False |
---> sync nu_p=+1.698160e+01 (err=+8.583094e-02) nuFnu_p=-1.030620e+01 (err=+1.607997e-02) curv.=-5.589204e-02 (err=+6.234641e-03)
================================================================================
my_shape.IC_fit(fit_range=[23.,29.],minimizer='minuit',silent=True)
p=my_shape.plot_shape_fit()
p.setlim(y_min=1E-15)
================================================================================ * Log-Polynomial fitting of the IC component * ---> fit range: [23.0, 29.0] ---> LogCubic fitTable length=4
| model name | name | val | bestfit val | err + | err - | start val | fit range min | fit range max | frozen |
|---|---|---|---|---|---|---|---|---|---|
| LogCubic | b | -1.627265e-01 | -1.627265e-01 | 2.483991e-02 | -- | -1.000000e+00 | -1.000000e+01 | 0.000000e+00 | False |
| LogCubic | c | -4.569970e-02 | -4.569970e-02 | 1.984551e-02 | -- | -1.000000e+00 | -1.000000e+01 | 1.000000e+01 | False |
| LogCubic | Ep | 2.526444e+01 | 2.526444e+01 | 1.736457e-01 | -- | 2.531190e+01 | 0.000000e+00 | 3.000000e+01 | False |
| LogCubic | Sp | -1.057790e+01 | -1.057790e+01 | 4.914805e-02 | -- | -1.000000e+01 | -3.000000e+01 | 0.000000e+00 | False |
---> IC nu_p=+2.526444e+01 (err=+1.736457e-01) nuFnu_p=-1.057790e+01 (err=+4.914805e-02) curv.=-1.627265e-01 (err=+2.483991e-02)
================================================================================
Model constraining#
In this step we are not fitting the model, we are just obtaining the
phenomenological pre_fit model, that will be fitted in using minuit
ore least-square bound, as shown below
from jetset.obs_constrain import ObsConstrain
from jetset.model_manager import FitModel
sed_obspar=ObsConstrain(beaming=25,
B_range=[0.001,0.1],
distr_e='lppl',
t_var_sec=3*86400,
nu_cut_IR=1E12,
SEDShape=my_shape)
prefit_jet=sed_obspar.constrain_SSC_model(electron_distribution_log_values=False,silent=True)
prefit_jet.save_model('prefit_jet.pkl')
================================================================================ * constrains parameters from observable *
/Users/orion/miniforge3/envs/jetset/lib/python3.12/site-packages/jetset/obs_constrain.py:1514: RankWarning: Polyfit may be poorly conditioned
p=polyfit(nu_p_IC_model_log,B_grid_log,2)
| model name | name | par type | units | val | phys. bound. min | phys. bound. max | log | frozen |
|---|---|---|---|---|---|---|---|---|
| jet_leptonic | R | region_size | cm | 1.216622e+16 | 1.000000e+03 | 1.000000e+30 | False | False |
| jet_leptonic | R_H | region_position | cm | 1.000000e+17 | 0.000000e+00 | -- | False | True |
| jet_leptonic | B | magnetic_field | gauss | 5.050000e-02 | 0.000000e+00 | -- | False | False |
| jet_leptonic | NH_cold_to_rel_e | cold_p_to_rel_e_ratio | 1.000000e+00 | 0.000000e+00 | -- | False | True | |
| jet_leptonic | beam_obj | beaming | 2.500000e+01 | 1.000000e-04 | -- | False | False | |
| jet_leptonic | z_cosm | redshift | 3.360000e-02 | 0.000000e+00 | -- | False | False | |
| jet_leptonic | gmin | low-energy-cut-off | lorentz-factor* | 4.703917e+02 | 1.000000e+00 | 1.000000e+09 | False | False |
| jet_leptonic | gmax | high-energy-cut-off | lorentz-factor* | 2.121873e+06 | 1.000000e+00 | 1.000000e+15 | False | False |
| jet_leptonic | N | emitters_density | 1 / cm3 | 5.583991e+00 | 0.000000e+00 | -- | False | False |
| jet_leptonic | gamma0_log_parab | turn-over-energy | lorentz-factor* | 6.673207e+03 | 1.000000e+00 | 1.000000e+09 | False | False |
| jet_leptonic | s | LE_spectral_slope | 2.251647e+00 | -1.000000e+01 | 1.000000e+01 | False | False | |
| jet_leptonic | r | spectral_curvature | 2.794602e-01 | -1.500000e+01 | 1.500000e+01 | False | False |
================================================================================
pl=prefit_jet.plot_model(sed_data=sed_data)
pl.add_model_residual_plot(prefit_jet,sed_data)
pl.setlim(y_min=1E-15,x_min=1E7,x_max=1E29)
Model fitting with Sherpa#
from jetset.template_2Dmodel import EBLAbsorptionTemplate
ebl_franceschini=EBLAbsorptionTemplate.from_name('Franceschini_2008')
from jetset.jet_model import Jet
prefit_jet=Jet.load_model('prefit_jet.pkl')
composite_model=FitModel(nu_size=500,name='EBL corrected',template=my_shape.host_gal)
composite_model.add_component(prefit_jet)
composite_model.add_component(ebl_franceschini)
composite_model.link_par(par_name='z_cosm', from_model='Franceschini_2008', to_model='jet_leptonic')
composite_model.composite_expr='(jet_leptonic+host_galaxy)*Franceschini_2008'
composite_model.eval()
composite_model.plot_model()
<jetset.plot_sedfit.PlotSED at 0x1632253d0>
composite_model.freeze('jet_leptonic','z_cosm')
composite_model.freeze('jet_leptonic','R_H')
composite_model.jet_leptonic.parameters.beam_obj.fit_range=[5., 50.]
composite_model.jet_leptonic.parameters.R.fit_range=[10**15.5,10**17.5]
composite_model.jet_leptonic.parameters.gmax.fit_range=[1E5,1E7]
composite_model.host_galaxy.parameters.nuFnu_p_host.frozen=False
composite_model.host_galaxy.parameters.nu_scale.frozen=True
from jetset.minimizer import ModelMinimizer
composite_model.jet_leptonic.parameters.z_cosm.frozen=True
model_minimizer_lsb=ModelMinimizer('sherpa')
best_fit=model_minimizer_lsb.fit(composite_model,sed_data,1E11,1E29,fitname='SSC-best-fit-sherpa',repeat=1)
filtering data in fit range = [1.000000e+11,1.000000e+29] data length 31 ================================================================================ * start fit process * -----
0it [00:00, ?it/s]
jetset model name R renamed to R_sh due to sherpa internal naming convention
- best chisq=1.39839e+01
-------------------------------------------------------------------------
Fit report
Model: SSC-best-fit-sherpa
| model name | name | par type | units | val | phys. bound. min | phys. bound. max | log | frozen |
|---|---|---|---|---|---|---|---|---|
| host_galaxy | nuFnu_p_host | nuFnu-scale | erg / (s cm2) | -9.967888e+00 | -2.000000e+01 | 2.000000e+01 | False | False |
| host_galaxy | nu_scale | nu-scale | Hz | -2.290459e-03 | -2.000000e+00 | 2.000000e+00 | False | True |
| jet_leptonic | gmin | low-energy-cut-off | lorentz-factor* | 2.794248e+02 | 1.000000e+00 | 1.000000e+09 | False | False |
| jet_leptonic | gmax | high-energy-cut-off | lorentz-factor* | 1.941690e+06 | 1.000000e+00 | 1.000000e+15 | False | False |
| jet_leptonic | N | emitters_density | 1 / cm3 | 6.214331e+00 | 0.000000e+00 | -- | False | False |
| jet_leptonic | gamma0_log_parab | turn-over-energy | lorentz-factor* | 2.340413e+03 | 1.000000e+00 | 1.000000e+09 | False | False |
| jet_leptonic | s | LE_spectral_slope | 2.182704e+00 | -1.000000e+01 | 1.000000e+01 | False | False | |
| jet_leptonic | r | spectral_curvature | 1.770089e-01 | -1.500000e+01 | 1.500000e+01 | False | False | |
| jet_leptonic | R | region_size | cm | 1.665370e+16 | 1.000000e+03 | 1.000000e+30 | False | False |
| jet_leptonic | R_H | region_position | cm | 1.000000e+17 | 0.000000e+00 | -- | False | True |
| jet_leptonic | B | magnetic_field | gauss | 1.161425e-02 | 0.000000e+00 | -- | False | False |
| jet_leptonic | NH_cold_to_rel_e | cold_p_to_rel_e_ratio | 1.000000e+00 | 0.000000e+00 | -- | False | True | |
| jet_leptonic | beam_obj | beaming | 4.364947e+01 | 1.000000e-04 | -- | False | False | |
| jet_leptonic | z_cosm(M) | redshift | 3.360000e-02 | 0.000000e+00 | -- | False | True | |
| Franceschini_2008 | scale_factor | scale_factor | 1.000000e+00 | 0.000000e+00 | -- | False | True | |
| Franceschini_2008 | z_cosm(L,jet_leptonic) | redshift | -- | -- | -- | False | True |
converged=True
calls=374
mesg=
<Fit results instance>
Fit parameters
| Parameter | Best-fit value | Approximate error |
|---|---|---|
| EBL corrected.nuFnu_p_host | -9.96789 | ± 0.0315974 |
| EBL corrected.gmin | 279.425 | ± 214.103 |
| EBL corrected.gmax | 1.94169e+06 | ± 0 |
| EBL corrected.N | 6.21433 | ± 3.78388 |
| EBL corrected.gamma0_log_parab | 2340.41 | ± 0 |
| EBL corrected.s | 2.1827 | ± 0.159093 |
| EBL corrected.r | 0.177009 | ± 0.048761 |
| EBL corrected.R_sh | 1.66537e+16 | ± 0 |
| EBL corrected.B | 0.0116143 | ± 0.00482729 |
| EBL corrected.beam_obj | 43.6495 | ± 10.6151 |
Summary (10)
Method
levmar
Statistic
chi2
Final statistic
13.9839
Number of evaluations
370
Reduced statistic
0.665899
Probability (Q-value)
0.870291
Initial statistic
147.741
Δ statistic
133.757
Number of data points
31
Degrees of freedom
21
dof=21
chisq=13.983884, chisq/red=0.665899 null hypothesis sig=0.870291
best fit pars
| model name | name | val | bestfit val | err + | err - | start val | fit range min | fit range max | frozen |
|---|---|---|---|---|---|---|---|---|---|
| host_galaxy | nuFnu_p_host | -9.967888e+00 | -9.967888e+00 | 3.159744e-02 | -- | -9.972939e+00 | -1.219011e+01 | -8.190114e+00 | False |
| host_galaxy | nu_scale | -2.290459e-03 | -- | -- | -- | -2.290459e-03 | -2.908697e-03 | 2.908697e-03 | True |
| jet_leptonic | gmin | 2.794248e+02 | 2.794248e+02 | 2.141028e+02 | -- | 4.703917e+02 | 1.000000e+00 | 1.000000e+09 | False |
| jet_leptonic | gmax | 1.941690e+06 | 1.941690e+06 | 0.000000e+00 | -- | 2.121873e+06 | 1.000000e+05 | 1.000000e+07 | False |
| jet_leptonic | N | 6.214331e+00 | 6.214331e+00 | 3.783882e+00 | -- | 5.583991e+00 | 0.000000e+00 | -- | False |
| jet_leptonic | gamma0_log_parab | 2.340413e+03 | 2.340413e+03 | 0.000000e+00 | -- | 6.673207e+03 | 1.000000e+00 | 1.000000e+09 | False |
| jet_leptonic | s | 2.182704e+00 | 2.182704e+00 | 1.590927e-01 | -- | 2.251647e+00 | -1.000000e+01 | 1.000000e+01 | False |
| jet_leptonic | r | 1.770089e-01 | 1.770089e-01 | 4.876099e-02 | -- | 2.794602e-01 | -1.500000e+01 | 1.500000e+01 | False |
| jet_leptonic | R | 1.665370e+16 | 1.665370e+16 | 0.000000e+00 | -- | 1.216622e+16 | 3.162278e+15 | 3.162278e+17 | False |
| jet_leptonic | R_H | 1.000000e+17 | -- | -- | -- | 1.000000e+17 | 0.000000e+00 | -- | True |
| jet_leptonic | B | 1.161425e-02 | 1.161425e-02 | 4.827287e-03 | -- | 5.050000e-02 | 0.000000e+00 | -- | False |
| jet_leptonic | NH_cold_to_rel_e | 1.000000e+00 | -- | -- | -- | 1.000000e+00 | 0.000000e+00 | -- | True |
| jet_leptonic | beam_obj | 4.364947e+01 | 4.364947e+01 | 1.061505e+01 | -- | 2.500000e+01 | 5.000000e+00 | 5.000000e+01 | False |
| jet_leptonic | z_cosm(M) | 3.360000e-02 | -- | -- | -- | 3.360000e-02 | 0.000000e+00 | -- | True |
| Franceschini_2008 | scale_factor | 1.000000e+00 | -- | -- | -- | 1.000000e+00 | 0.000000e+00 | -- | True |
| Franceschini_2008 | z_cosm(L,jet_leptonic) | 3.360000e-02 | -- | -- | -- | -- | 0.000000e+00 | -- | True |
-------------------------------------------------------------------------
================================================================================
composite_model.set_nu_grid(1E6,1E30,200)
composite_model.eval()
p=composite_model.plot_model(sed_data=sed_data)
Using the sherpa_fitter you can access all the sherpa fetarues
https://sherpa.readthedocs.io/en/latest/fit/index.html
model_minimizer_lsb.minimizer.sherpa_fitter.est_errors()
<covariance results instance>
covariance 1σ (68.2689%) bounds
| Parameter | Best-fit value | Lower Bound | Upper Bound |
|---|---|---|---|
| EBL corrected.nuFnu_p_host | -9.96789 | -0.0305658 | 0.0305658 |
| EBL corrected.gmin | 279.425 | -30.8224 | 30.8224 |
| EBL corrected.gmax | 1.94169e+06 | -3747.88 | 3747.88 |
| EBL corrected.N | 6.21433 | -2.45689 | 2.45689 |
| EBL corrected.gamma0_log_parab | 2340.41 | -540.898 | 540.898 |
| EBL corrected.s | 2.1827 | -0.0301012 | 0.0301012 |
| EBL corrected.r | 0.177009 | -0.0181166 | 0.0181166 |
| EBL corrected.R_sh | 1.66537e+16 | -5.48328e+15 | 5.48328e+15 |
| EBL corrected.B | 0.0116143 | -0.000915756 | 0.000915756 |
| EBL corrected.beam_obj | 43.6495 | -8.7653 | 8.7653 |
Summary (2)
Fitting Method
levmar
Statistic
chi2
from sherpa.plot import IntervalProjection
iproj = IntervalProjection()
iproj.prepare(fac=5, nloop=15)
iproj.calc(model_minimizer_lsb.minimizer.sherpa_fitter, model_minimizer_lsb.minimizer._sherpa_model.s)
iproj.plot()