def fit_point(self, model, energy_group, energy_ref):
from gammapy.spectrum import SpectrumFit
sherpa_model = model.to_sherpa()
sherpa_model.gamma.freeze()
fit = SpectrumFit(self.obs, sherpa_model)
erange = energy_group.energy_range
# TODO: Notice channels contained in energy_group
fit.fit_range = erange.min, 0.9999 * erange.max
log.debug(
'Calling Sherpa fit for flux point '
' in energy range:\n{}'.format(fit)
)
fit.fit()
res = fit.global_result
energy_err_hi = energy_group.energy_range.max - energy_ref
energy_err_lo = energy_ref - energy_group.energy_range.min
diff_flux = res.model(energy_ref).to('m-2 s-1 TeV-1')
err = res.model_with_uncertainties(energy_ref.to('TeV').value)
diff_flux_err = err.s * Unit('m-2 s-1 TeV-1')
return OrderedDict(
energy=energy_ref,
energy_err_hi=energy_err_hi,
energy_err_lo=energy_err_lo,
diff_flux=diff_flux,
diff_flux_err_hi=diff_flux_err,
diff_flux_err_lo=diff_flux_err,
)
def fit_point(self, model, energy_group, energy_ref):
from gammapy.spectrum import SpectrumFit
sherpa_model = model.to_sherpa()
sherpa_model.gamma.freeze()
fit = SpectrumFit(self.obs, sherpa_model)
erange = energy_group.energy_range
# TODO: Notice channels contained in energy_group
fit.fit_range = erange.min, 0.9999 * erange.max
log.debug("Calling Sherpa fit for flux point " " in energy range:\n{}".format(fit))
fit.fit()
res = fit.global_result
energy_err_hi = energy_group.energy_range.max - energy_ref
energy_err_lo = energy_ref - energy_group.energy_range.min
diff_flux = res.model(energy_ref).to("m-2 s-1 TeV-1")
err = res.model_with_uncertainties(energy_ref.to("TeV").value)
diff_flux_err = err.s * u.Unit("m-2 s-1 TeV-1")
return OrderedDict(
energy=energy_ref,
energy_err_hi=energy_err_hi,
energy_err_lo=energy_err_lo,
diff_flux=diff_flux,
diff_flux_err_hi=diff_flux_err,
diff_flux_err_lo=diff_flux_err,
)
def fit_point(self, model, energy_group, energy_ref):
from gammapy.spectrum import SpectrumFit
fit = SpectrumFit(self.obs, model)
erange = energy_group.energy_range
# TODO: Notice channels contained in energy_group
fit.fit_range = erange.min, erange.max
log.debug('Calling Sherpa fit for flux point '
' in energy range:\n{}'.format(fit))
fit.fit()
fit.est_errors()
# First result contain correct model
res = fit.result[0]
e_max = energy_group.energy_range.max
e_min = energy_group.energy_range.min
diff_flux, diff_flux_err = res.model.evaluate_error(energy_ref)
return OrderedDict(
e_ref=energy_ref,
e_min=e_min,
e_max=e_max,
dnde=diff_flux.to('m-2 s-1 TeV-1'),
dnde_err=diff_flux_err.to('m-2 s-1 TeV-1'),
)
def fit_point(self, model, energy_group, energy_ref):
from gammapy.spectrum import SpectrumFit
# TODO: The code below won't work because SpectrumFit only accepts
# gammapy models. Add Parameter class to freeze index
# sherpa_model = model.to_sherpa()
# sherpa_model.gamma.freeze()
#fit = SpectrumFit(self.obs, sherpa_model)
fit = SpectrumFit(self.obs, model)
erange = energy_group.energy_range
# TODO: Notice channels contained in energy_group
fit.fit_range = erange.min, 0.9999 * erange.max
log.debug('Calling Sherpa fit for flux point '
' in energy range:\n{}'.format(fit))
fit.fit()
fit.est_errors()
# First result contain correct model
res = fit.result[0]
e_max = energy_group.energy_range.max
e_min = energy_group.energy_range.min
diff_flux, diff_flux_err = res.model.evaluate_error(energy_ref)
return OrderedDict(
e_ref=energy_ref,
e_min=e_min,
e_max=e_max,
dnde=diff_flux.to('m-2 s-1 TeV-1'),
dnde_err=diff_flux_err.to('m-2 s-1 TeV-1'),
)
def fit_gammapy():
"""
Current results
Parameters:
name value error unit min max frozen
--------- --------- --------- --------------- --- --- ------
index 2.602e+00 1.555e-01 nan nan False
amplitude 2.441e-11 3.452e-12 1 / (cm2 s TeV) nan nan False
reference 1.000e+00 0.000e+00 TeV nan nan True
Covariance:
name/name index amplitude
--------- -------- ---------
index 0.0242 3.79e-13
amplitude 3.79e-13 1.19e-23
Statistic: -157.719 (cash)
Fit Range: [1.0000000e+09 2.7825594e+10] keV
"""
obs = SpectrumObservation.read(obs_path)
# obs.peek()
# plt.show()
model = PowerLaw(
amplitude=1.23 * 1e-11 * u.Unit("cm-2 s-1 TeV-1"),
reference=1 * u.Unit("TeV"),
index=2.14 * u.Unit(""),
)
fit = SpectrumFit(obs_list=obs, model=model, fit_range=energy_range, stat="cash")
fit.run()
print(fit.result[0])
pprint(fit.__dict__)
obs = fit.obs_list[0]
print(obs)
print("This is fit_gammapy")
obs.peek()
import matplotlib.pyplot as plt
plt.savefig("fit_gammapy.png")
def test_spectral_model_absorbed_by_ebl():
# Observation parameters
obs_param = ObservationParameters(alpha=0.2 * u.Unit(''),
livetime=5. * u.h,
emin=0.08 * u.TeV,
emax=12 * u.TeV)
# Target, PKS 2155-304 from 3FHL
name = 'test'
absorption = Absorption.read('$GAMMAPY_EXTRA/datasets/ebl/ebl_dominguez11.fits.gz')
pwl = PowerLaw(index=3. * u.Unit(''),
amplitude=1.e-12 * u.Unit('1/(cm2 s TeV)'),
reference=1. * u.TeV)
input_model = AbsorbedSpectralModel(spectral_model=pwl,
absorption=absorption,
parameter=0.2)
target = Target(name=name, model=input_model)
# Performance
filename = '$GAMMAPY_EXTRA/datasets/cta/perf_prod2/point_like_non_smoothed/South_5h.fits.gz'
cta_perf = CTAPerf.read(filename)
# Simulation
simu = CTAObservationSimulation.simulate_obs(perf=cta_perf,
target=target,
obs_param=obs_param)
# Model we want to fit
pwl_model = PowerLaw(index=2.5 * u.Unit(''),
amplitude=1.e-12 * u.Unit('1/(cm2 s TeV)'),
reference=1. * u.TeV)
model = AbsorbedSpectralModel(spectral_model=pwl_model,
absorption=absorption,
parameter=0.2)
# fit
fit = SpectrumFit(obs_list=SpectrumObservationList([simu]),
model=model,
stat='wstat')
fit.fit()
fit.est_errors()
result = fit.result[0]
def run_analysis(which):
log.info(f"Fitting dataset: {which}")
dataset = config.datasets[which]
obs_list = dataset.get_SpectrumObservationList()
fit_range = dataset.energy_range
log.info(f"obs_list: {obs_list}")
model = Log10Parabola(
amplitude="3.8e-11 cm-2 s-1 TeV-1", reference="1 TeV", alpha=2.47, beta=0.24
)
fit = SpectrumFit(obs_list=obs_list, model=model, fit_range=fit_range)
log.info("Running fit")
fit.run()
fit_results = make_results_dict(fit)
utils.write_yaml(fit_results, f"results/fit/fit_{which}.yaml")
contour_results = compute_contours(fit)
utils.write_yaml(contour_results, f"results/fit/contours_{which}.yaml")
def test_spectral_model_absorbed_by_ebl():
# Observation parameters
obs_param = ObservationParameters(alpha=0.2 * u.Unit(''),
livetime=5. * u.h,
emin=0.08 * u.TeV,
emax=12 * u.TeV)
# Target, PKS 2155-304 from 3FHL
name = 'test'
absorption = Absorption.read(
'$GAMMAPY_EXTRA/datasets/ebl/ebl_dominguez11.fits.gz')
pwl = PowerLaw(index=3. * u.Unit(''),
amplitude=1.e-12 * u.Unit('1/(cm2 s TeV)'),
reference=1. * u.TeV)
input_model = AbsorbedSpectralModel(spectral_model=pwl,
absorption=absorption,
parameter=0.2)
target = Target(name=name, model=input_model)
# Performance
filename = '$GAMMAPY_EXTRA/datasets/cta/perf_prod2/point_like_non_smoothed/South_5h.fits.gz'
cta_perf = CTAPerf.read(filename)
# Simulation
simu = CTAObservationSimulation.simulate_obs(perf=cta_perf,
target=target,
obs_param=obs_param)
# Model we want to fit
pwl_model = PowerLaw(index=2.5 * u.Unit(''),
amplitude=1.e-12 * u.Unit('1/(cm2 s TeV)'),
reference=1. * u.TeV)
model = AbsorbedSpectralModel(spectral_model=pwl_model,
absorption=absorption,
parameter=0.2)
# fit
fit = SpectrumFit(obs_list=SpectrumObservationList([simu]),
model=model,
stat='wstat')
fit.fit()
fit.est_errors()
result = fit.result[0]
SpectrumObservation,
SpectrumFit,
DifferentialFluxPoints,
SpectrumFitResult,
SpectrumResult
)
import astropy.units as u
import numpy as np
import copy
import matplotlib.pyplot as plt
plt.style.use('ggplot')
obs = SpectrumObservation.read('$GAMMAPY_EXTRA/datasets/hess-crab4_pha/pha_obs23523.fits')
fit = SpectrumFit(obs)
fit.run()
best_fit = copy.deepcopy(fit.result[0].fit)
# Define Flux points binning
emin = np.log10(obs.lo_threshold.to('TeV').value)
emax = np.log10(40)
binning = np.logspace(emin, emax, 8) * u.TeV
# Fix index
fit.model.gamma.freeze()
# Fit norm in bands
diff_flux = list()
diff_flux_err = list()
e_err_hi = list()
model2fit1.parameters['beta'].parmin = 0.0
model2fit1.parameters['beta'].parmax = 10.0
model2fit1.parameters['amplitude'].parmin = 1e-14
model2fit1.parameters['amplitude'].parmax = 1e-5
model2fit2.parameters['index'].parmin = 0.1
model2fit2.parameters['index'].parmax = 5.0
model2fit2.parameters['lambda_'].parmin = 0.001
model2fit2.parameters['lambda_'].parmax = 100
model2fit2.parameters['amplitude'].parmin = 1.0e-14
model2fit2.parameters['amplitude'].parmax = 1.0e-3
model2fit3.parameters['index'].parmin = 1.0
model2fit3.parameters['index'].parmax = 7.0
model2fit3.parameters['amplitude'].parmin = 1.0e-14
model2fit3.parameters['amplitude'].parmax = 1.0e-4
models2fit = [model2fit3] #,model2fit2,model2fit3]
for k in range(len(models2fit)):
fit_crab = SpectrumFit(obs_list=simu,
model=models2fit[k],
fit_range=(1.0 * u.TeV, 55 * u.TeV),
stat="cash")
fit_crab.fit()
fit_crab.est_errors()
results = fit_crab.result
#ax0, ax1 = results[0].plot(figsize=(8,8))
#plt.show()
print(results[0])
# Define spectral model
index = 3.0 * u.Unit('')
amplitude = 2.5 * 1e-11 * u.Unit('cm-2 s-1 TeV-1')
reference = 1 * u.TeV
model = PowerLaw(index=index, amplitude=amplitude, reference=reference)
# for one obs only
mylist = datastore.obs_list((obsid[0], ))
n_obs = 1
seeds = np.arange(n_obs)
sim = SimulationRealBkg(source_model=model, obsrun=mylist[0], obspos=src)
sim.run(seeds)
obs = sim.result[0]
fit = SpectrumFit(obs, model=model, stat='wstat')
fit.model.parameters['index'].value = 2
fit.run()
fit.est_errors()
print fit.result[0]
#now run in a loop
n_obs = 200
mylist = datastore.obs_list(obsid[0:n_obs])
seeds = np.arange(n_obs)
sims = []
for i in range(n_obs):
sim = SimulationRealBkg(source_model=model, obsrun=mylist[i], obspos=src)
livetime=livetime) sim.simulate_obs(seed=42, obs_id=0) # In[ ]: sim.obs.peek() print(sim.obs) # ## Spectral analysis # # Now that we have some simulated CTA counts spectrum, let's analyse it. # In[ ]: # Fit data fit = SpectrumFit(obs_list=sim.obs, model=model, stat="cash") fit.run() result = fit.result[0] # In[ ]: print(result) # In[ ]: energy_range = [0.1, 100] * u.TeV model.plot(energy_range=energy_range, energy_power=2) result.model.plot(energy_range=energy_range, energy_power=2) result.model.plot_error(energy_range=energy_range, energy_power=2) # ## Exercises
#aeff.plot(ax=axes[1])
#plt.show()
aeff.lo_threshold = lo_threshold
aeff.hi_threshold = hi_threshold
sim = SpectrumSimulation(aeff=aeff,
edisp=edisp,
source_model=model,
livetime=livetime)
sim.simulate_obs(seed=42, obs_id=0)
sim.obs.peek()
print sim.obs
plt.show()
fit = SpectrumFit(obs_list=sim.obs, model=model, stat='cash')
fit.run()
result = fit.result[0]
print result
energy_range = [0.1, 100] * u.TeV
model.plot(energy_range=energy_range, energy_power=2)
result.model.plot(energy_range=energy_range, energy_power=2)
result.model.plot_error(energy_range=energy_range, energy_power=2)
plt.show()
#now importing a background
#from a background model
bkg_index = 2.5 * u.Unit('')
#print(sim2.result)
sim2 = sim1
Indiv_best_fit_index = []
best_fit_index = []
i = 0
while i < n_obs:
sim_result = (sim1.result[i], sim2.result[i])
#FIT SPECTRA:
pwl.parameters['index'].parmax = 10
for obs in sim_result:
fit = SpectrumFit(obs, pwl.copy(), stat='wstat')
fit.model.parameters['index'].value = 2
fit.fit()
fit.est_errors()
Indiv_best_fit_index.append(
fit.result[0].model.parameters['index'].value)
#print(fit.result[0])
#print(' Indiv_best_fit_index = ', Indiv_best_fit_index)
#i+=1
#STACK SPECTRA 2 by 2
# Add the two spectra
obs_stacker = SpectrumObservationStacker(sim_result)
#print('sim_result is the list = ',sim_result)
obs_stacker.run()
extraction.spectrum_observations[0].peek()
# Now we'll fit a model to the spectrum with SpectrumFit. First we load a power law model with an initial value for the index and the amplitude and then wo do a likelihood fit. The fit results are printed below.
# In[ ]:
model = PowerLaw(index=4,
amplitude="1.3e-9 cm-2 s-1 TeV-1",
reference="0.02 TeV")
fit_range = (0.04 * u.TeV, 0.4 * u.TeV)
ebounds = EnergyBounds.equal_log_spacing(0.04, 0.4, 7, u.TeV)
joint_fit = SpectrumFit(obs_list=extraction.spectrum_observations,
model=model,
fit_range=fit_range)
joint_fit.run()
joint_result = joint_fit.result
print(joint_result[0])
# Now you might want to do the stacking here even if in our case there is only one observation which makes it superfluous.
# We can compute flux points by fitting the norm of the global model in energy bands.
# In[ ]:
stacked_obs = extraction.spectrum_observations.stack()
seg = SpectrumEnergyGroupMaker(obs=stacked_obs)
seg.compute_groups_fixed(ebounds=ebounds)
print(pwl)
livetime = 2 * u.h
# In[5]:
sim = SpectrumSimulation(aeff=aeff,
edisp=edisp,
source_model=pwl,
livetime=livetime)
sim.simulate_obs(seed=2309, obs_id=1)
print(sim.obs)
# In[6]:
fit = SpectrumFit(obs_list=sim.obs, model=pwl.copy(), stat='cash')
fit.fit_range = [1, 10] * u.TeV
fit.fit()
fit.est_errors()
print(fit.result[0])
# ## Include background
#
# In this section we will include a background component. Furthermore, we will also simulate more than one observation and fit each one individuallt in order to get average fit results.
# In[7]:
bkg_index = 2.5 * u.Unit('')
bkg_amplitude = 1e-11 * u.Unit('cm-2 s-1 TeV-1')
reference = 1 * u.TeV
from astropy.tests.helper import assert_quantity_allclose
from gammapy.data import ObservationTable
from gammapy.datasets import gammapy_extra
from gammapy.spectrum import SpectrumFit, SpectrumObservationGrouping, group_obs_table
obs_table_file = gammapy_extra.filename(
'datasets/hess-crab4_pha/observation_table.fits')
obs_table = ObservationTable.read(obs_table_file)
fit = SpectrumFit.from_observation_table(obs_table)
fit.model = 'PL'
fit.energy_threshold_low = '1 TeV'
fit.energy_threshold_high = '10 TeV'
fit.run(method='sherpa')
#Use each obs in one group
obs_table1 = group_obs_table(obs_table, eff_range=[90, 95], n_eff_bin=5)
obs_table1.write('grouped_table1_debug.fits', overwrite=True)
grouping = SpectrumObservationGrouping(obs_table1)
grouping.run()
fit_band2 = SpectrumFit.from_observation_table(grouping.stacked_obs_table)
fit_band2.model = 'PL'
fit_band2.energy_threshold_low = '1 TeV'
fit_band2.energy_threshold_high = '10 TeV'
fit_band2.run(method='sherpa')
assert_quantity_allclose(fit.result.parameters["index"],
# Requires IPython widgets
# _ = extraction.spectrum_observations.peek()
extraction.spectrum_observations[0].peek()
# ## Fit spectrum
#
# Now we'll fit a global model to the spectrum. First we do a joint likelihood fit to all observations. If you want to stack the observations see below. We will also produce a debug plot in order to show how the global fit matches one of the individual observations.
# In[ ]:
model = PowerLaw(index=2,
amplitude=2e-11 * u.Unit("cm-2 s-1 TeV-1"),
reference=1 * u.TeV)
joint_fit = SpectrumFit(obs_list=extraction.spectrum_observations, model=model)
joint_fit.run()
joint_result = joint_fit.result
# In[ ]:
ax0, ax1 = joint_result[0].plot(figsize=(8, 8))
ax0.set_ylim(0, 20)
print(joint_result[0])
# ## Compute Flux Points
#
# To round up our analysis we can compute flux points by fitting the norm of the global model in energy bands. We'll use a fixed energy binning for now.
# In[ ]:
model2fit3.parameters['amplitude'].parmin = 1e-12
model2fit3.parameters['amplitude'].parmax = 1e-10
model2fit3.parameters['index'].parmin = 2.0
model2fit3.parameters['index'].parmax = 4.0
#Models to fit the circular and annular observations
models_ann_fit = [model2fit1, model2fit2, model2fit3]
models_circ_fit = [model2fit1, model2fit2, model2fit3]
# Fit
if est_hi_lim = 'yes':
hi_fit_energ = cube_on.energies('edges')[int(np.sum(ann_stats))]
for k in range(len(models_ann_fit)):
fit_source = SpectrumFit(obs_list = ann_sed_table, model=models_ann_fit[k],forward_folded=True, fit_range=(lo_fit_energ,hi_fit_energ))
fit_source.fit()
fit_source.est_errors()
results = fit_source.result
ax0, ax1 = results[0].plot(figsize=(8,8))
print(results[0])
if est_hi_lim = 'yes':
hi_fit_energ = cube_on.energies('edges')[int(np.sum(circ_stats))]
for k in range(len(models_circ_fit)):
fit_source = SpectrumFit(obs_list = circ_sed_table, model=models_circ_fit[k],forward_folded=True, fit_range=(lo_fit_energ,hi_fit_energ))
fit_source.fit()
fit_source.est_errors()
results = fit_source.result
print(results[0])
print(extraction.observations[0])
extraction.run(obs_list=obs_list, bkg_estimate=background_estimator.result, outdir=ANALYSIS_DIR)
extraction.run(obs_list=crablist, bkg_estimate=background_estimator.result, outdir=ANALYSIS_DIR)
extraction.write(obs_list=crablist, bkg_estimate=background_estimator.result, outdir=ANALYSIS_DIR)
extraction.write(crablist)
extraction.write(crablist, bkg_estimate=background_estimator.result, outdir=ANALYSIS_DIR)
extraction.write(crablist, background_estimator.result, outdir=ANALYSIS_DIR)
get_ipython().magic(u'pinfo extraction.write')
extraction.observations[0].peek()
model = PowerLaw(
index=2 * u.Unit(''),
amplitude=2e-11 * u.Unit('cm-2 s-1 TeV-1'),
reference=1 * u.TeV,
)
joint_fit = SpectrumFit(obs_list=extraction.observations, model=model)
joint_fit.fit()
joint_fit.est_errors()
#fit.run(outdir = ANALYSIS_DIR)
joint_result = joint_fit.result
ax0, ax1 = joint_result[0].plot(figsize=(8,8))
ax0.set_ylim(0, 20)
print(joint_result[0])
plt.show()
ebounds = [0.3, 1.1, 3, 10.1, 30] * u.TeV
stacked_obs = extraction.observations.stack()
seg = SpectrumEnergyGroupMaker(obs=stacked_obs)
seg.compute_range_safe()
# In[44]:
extract.observations[0].peek()
# Now we’ll fit a global model to the spectrum. First we do a joint likelihood fit to all observations.
# In[45]:
model = models.PowerLaw(
index=2 * u.Unit(''),
amplitude=1e-11 * u.Unit('cm-2 s-1 TeV-1'),
reference=1 * u.TeV,
)
fit = SpectrumFit(extract.observations,
model,
fit_range=(1 * u.TeV, 10 * u.TeV))
#probably not working
fit.fit()
fit.est_errors()
print(fit.result[0])
# We will also produce a debug plot in order to show how the global fit matches one of the individual observations.
# In[46]:
fit.result[0].plot()
# we can compute flux points by fitting the norm of the global model in energy bands. We’ll use a fixed energy binning for now.
# In[47]:
def make_fit(self, name):
dataset = config.datasets[name]
observations = dataset.get_SpectrumObservationList()
model = Log10ParabolaEnergyScale()
fit_range = dataset.energy_range
return SpectrumFit(obs_list=observations, model=model, fit_range=fit_range)
)
extract.run()
# ### Model fit
#
# The next step is to fit a spectral model, using all data (i.e. a "global" fit, using all energies).
# In[26]:
model = models.PowerLaw(
index=2 * u.Unit(''),
amplitude=1e-11 * u.Unit('cm-2 s-1 TeV-1'),
reference=1 * u.TeV,
)
fit = SpectrumFit(extract.observations, model)
fit.fit()
fit.est_errors()
print(fit.result[0])
# ### Spectral points
#
# Finally, let's compute spectral points. The method used is to first choose an energy binning, and then to do a 1-dim likelihood fit / profile to compute the flux and flux error.
# In[27]:
# Flux points are computed on stacked observation
stacked_obs = extract.observations.stack()
print(stacked_obs)
ebounds = EnergyBounds.equal_log_spacing(1, 40, 4, unit=u.TeV)
def run_gammapy_fit(obs_list, fit_range, eval_contours=None):
"""Run fit with Gammapy, using iminiuit"""
model_lp = Log10Parabola(
amplitude=3.80 * 1e-11 * u.Unit("cm-2 s-1 TeV-1"),
reference=1 * u.Unit("TeV"),
alpha=2.47 * u.Unit(""),
beta=0.24 * u.Unit(""),
)
# note this step is very important to iminuit, to initialize the parameter error!
fit = SpectrumFit(obs_list=obs_list, model=model_lp, fit_range=fit_range)
log.info("Starting fit ...")
t = time()
fit.optimize(backend="minuit", pedantic=True)
fit.run()
t = time() - t
log.info(f"Finished fit in {t} seconds.")
results = extract_spectrum_results_gammapy(fit)
print(fit.result[0])
if eval_contours is not None:
log.info("storing likelihood contours ...")
# points along the contour
like_points = 80
sigma = 1.
log.info(f"computing amplitude vs alpha {sigma} sigma contour")
cont = fit.minuit.mncontour("par_000_amplitude",
"par_002_alpha",
numpoints=like_points,
sigma=sigma)
# the third element of mncontour's returned object is a list of tuples with the contour coordinates
# (x_1,y_1), ..., (x_n, y_n)]
cont = np.asarray(cont[2])
amplitude = cont.T[0] # transpose and take the first row
alpha = cont.T[1] # transpose and take the
# trick to make a close circle when plotting: just repeat the first coordinate
amplitude = np.append(amplitude, amplitude[0])
alpha = np.append(alpha, alpha[0])
contour_amplitude_alpha = {"amplitude": amplitude, "alpha": alpha}
log.info(f"computing amplitude vs beta {sigma} sigma contour")
cont = fit.minuit.mncontour("par_000_amplitude",
"par_003_beta",
numpoints=like_points,
sigma=sigma)
cont = np.asarray(cont[2])
amplitude = cont.T[0] # transpose and take the first row
beta = cont.T[1] # transpose and take the
# trick to make a close circle when plotting: just repeat the first coordinate
amplitude = np.append(amplitude, amplitude[0])
beta = np.append(beta, beta[0])
contour_amplitude_beta = {"amplitude": amplitude, "beta": beta}
log.info(f"computing alpha vs beta {sigma} sigma contour")
cont = fit.minuit.mncontour("par_002_alpha",
"par_003_beta",
numpoints=like_points,
sigma=sigma)
cont = np.asarray(cont[2])
alpha = cont.T[0] # transpose and take the first row
beta = cont.T[1] # transpose and take the
# trick to make a close circle when plotting: just repeat the first coordinate
alpha = np.append(alpha, alpha[0])
beta = np.append(beta, beta[0])
contour_alpha_beta = {"alpha": alpha, "beta": beta}
# define the general dictionary and dump it in a .npy object
contours = {
"contour_amplitude_alpha": contour_amplitude_alpha,
"contour_amplitude_beta": contour_amplitude_beta,
"contour_alpha_beta": contour_alpha_beta,
}
logging.info(f"storing .yaml with contours in {eval_contours}")
path = Path(eval_contours)
path.mkdir(parents=True, exist_ok=True)
np.save(f"{eval_contours}/fit_{sigma}_sigma_contours_logparabola.npy",
contours)
return results
sim.simulate_obs(seed=42, obs_id=0)
sim = SpectrumSimulation(aeff=aeff,
edisp=edisp,
source_model=model,
livetime=livetime,
background_model=none, alpha=alpha)
sim = SpectrumSimulation(aeff=aeff,
edisp=edisp,
source_model=model,
livetime=livetime,
background_model="none", alpha=alpha)
sim.simulate_obs(seed=42, obs_id=0)
sim = SpectrumSimulation(aeff=aeff, edisp=edisp, source_model=model, livetime=livetime)
sim.simulate_obs(seed=42, obs_id=0)
get_ipython().magic(u'pinfo SpectrumFit')
fit = SpectrumFit(obs_list=sim.obs, model=model, background_model=inbuiltbkg, stat='cash')
fit.run()
get_ipython().magic(u'pinfo SpectrumFit')
fit = SpectrumFit(obs_list=sim.obs, model=model, background_model=inbuiltbkg, stat='wstat')
bkg_model
fit = SpectrumFit(obs_list=sim.obs, model=model, background_model=bkg_model, stat='wstat')
fit = SpectrumFit(obs_list=sim.obs, model=model, background_model=background_estimator1, stat='wstat')
fit = SpectrumFit(obs_list=sim.obs, model=model, background_model=background_estimator, stat='wstat')
background_estimator1.run()
fit = SpectrumFit(obs_list=sim.obs, model=model, background_model=background_estimator1, stat='wstat')
background_estimator1.plot()
plt.show()
background_estimator.obs_list
print background_estimator.obs_list
print background_estimator1.obs_list
background_estimator.plot()
TODO: Refactor and add to FluxPointsComputation class or so
"""
from gammapy.spectrum import (SpectrumObservation, SpectrumFit, FluxPoints,
SpectrumResult)
import astropy.units as u
from astropy.table import Table
import numpy as np
import copy
import matplotlib.pyplot as plt
plt.style.use('ggplot')
obs = SpectrumObservation.read(
'$GAMMAPY_EXTRA/datasets/hess-crab4_pha/pha_obs23523.fits')
fit = SpectrumFit(obs)
fit.run()
best_fit = copy.deepcopy(fit.result[0].fit)
# Define Flux points binning
emin = np.log10(obs.lo_threshold.to('TeV').value)
emax = np.log10(40)
binning = np.logspace(emin, emax, 8) * u.TeV
# Fix index
fit.model.gamma.freeze()
# Fit norm in bands
diff_flux = list()
diff_flux_err = list()
e_err_hi = list()
from gammapy.spectrum import SpectrumFit, SpectrumObservation, SpectrumFitResult
import matplotlib.pyplot as plt
import astropy.units as u
obs = SpectrumObservation.read('pha_obs31415.fits')
fit = SpectrumFit(obs)
obs.peek()
plt.savefig('observation.png')
plt.cla()
fit.run()
fit.result[0].plot_fit()
plt.savefig('debug_fit.png')
# TODO: implement properly
plt.cla()
fig = plt.figure()
ax = fig.add_subplot(111)
fit.result[0].fit.plot_butterfly(ax=ax, label='Fit result')
input_parameters = dict(index = 2.3 * u.Unit(''),
norm = 2.5 * 1e-12 * u.Unit('cm-2 s-1 TeV-1'),
reference = 1 * u.TeV)
input_parameter_errors = dict(index = 0 * u.TeV,
norm = 0 * u.Unit('cm-2 s-1 TeV-1'),
reference = 0 * u.TeV)
input_model = SpectrumFitResult(spectral_model = 'PowerLaw',
parameters = input_parameters,
parameter_errors = input_parameter_errors)
reference=1 * u.TeV)
print(pwl)
# In[ ]:
livetime = 2 * u.h
sim = SpectrumSimulation(aeff=aeff,
edisp=edisp,
source_model=pwl,
livetime=livetime)
sim.simulate_obs(seed=2309, obs_id=1)
print(sim.obs)
# In[ ]:
fit = SpectrumFit(obs_list=sim.obs, model=pwl.copy(), stat="cash")
fit.fit_range = [1, 10] * u.TeV
fit.run()
print(fit.result[0])
# ## Include background
#
# In this section we will include a background component. Furthermore, we will also simulate more than one observation and fit each one individuallt in order to get average fit results.
# In[ ]:
bkg_model = PowerLaw(index=2.5,
amplitude=1e-11 * u.Unit("cm-2 s-1 TeV-1"),
reference=1 * u.TeV)
# In[ ]:
def check_energy_binning_effects():
"""Check how spectral fit results change with energy binnings.
Actually this is still using the default:
In [14]: print(analysis.extraction.observations[0].edisp)
EnergyDispersion
NDDataArray summary info
e_true : size = 108, min = 0.010 TeV, max = 301.416 TeV
e_reco : size = 72, min = 0.011 TeV, max = 93.804 TeV
Data : size = 7776, min = 0.000, max = 1.000
But now, the fit results from SpectrumAnalysisIACT, which is just
driving Fitspectrum, are different, almost the same as Sherpa.
Current results
Parameters:
name value error unit min max frozen
--------- --------- --------- --------------- --- --- ------
index 2.620e+00 1.540e-01 nan nan False
amplitude 3.849e-11 5.407e-12 1 / (cm2 s TeV) nan nan False
reference 1.000e+00 0.000e+00 TeV nan nan True
Covariance:
name/name index amplitude
--------- -------- ---------
index 0.0237 5.85e-13
amplitude 5.85e-13 2.92e-23
Statistic: -157.166 (cash)
Fit Range: [ 1. 27.82559402] TeV
???
"""
data_store = DataStore.from_dir("data/hess")
obs_list = data_store.obs_list([23523])
on_region = CircleSkyRegion(conf.crab_position, conf.on_radius["hess"])
fp_binning = [1, 10, 30] * u.TeV
exclusion_mask = get_exclusion_mask(conf.crab_position)
model = PowerLaw(
amplitude=1.23 * 1e-11 * u.Unit("cm-2 s-1 TeV-1"),
reference=1 * u.Unit("TeV"),
index=2.14 * u.Unit(""),
)
cfg = dict(
outdir=None,
background=dict(
on_region=on_region,
exclusion_mask=exclusion_mask,
# min_distance=0.1 * u.rad,
),
extraction=dict(containment_correction=True),
fit=dict(
model=model,
stat="cash",
# forward_folded=True,
fit_range=energy_range,
),
fp_binning=fp_binning,
)
analysis = SpectrumAnalysisIACT(obs_list, cfg)
analysis.run()
analysis.fit.est_errors()
print("BEFORE", analysis.fit.result[0])
# print(analysis.extraction.observations[0].edisp)
# pprint(analysis.fit.__dict__)
# obs = analysis.fit.obs_list[0]
# print(obs)
# # import IPython; IPython.embed()
# obs.peek()
# import matplotlib.pyplot as plt
# plt.savefig('check_energy_binning_effects.png')
# print('This is check_energy_binning_effects')
# Try to see if the I/O causes a change in results.
analysis.extraction.observations.write("temp123")
analysis.extraction.observations.write("temp123", use_sherpa=True)
obs = SpectrumObservation.read("temp123/pha_obs23523.fits")
model = PowerLaw(
amplitude=1.23 * 1e-11 * u.Unit("cm-2 s-1 TeV-1"),
reference=1 * u.Unit("TeV"),
index=2.14 * u.Unit(""),
)
fit = SpectrumFit(obs_list=obs, model=model, fit_range=energy_range, stat="cash")
fit.run()
print("AFTER", fit.result[0])
def compute(cls, model, obs_list, binning):
"""Compute differential fluxpoints
The norm of the global model is fit to the
`~gammapy.spectrum.SpectrumObservationList` in the provided energy
binning and the differential flux is evaluated at the log bin center.
TODO : Add upper limit calculation
Parameters
----------
model : `~gammapy.spectrum.models.SpectralModel`
Global model
obs_list : `~gammapy.spectrum.SpectrumObservationList`
Observations
binning : `~astropy.units.Quantity`
Energy binning, see
:func:`~gammapy.spectrum.utils.calculate_flux_point_binning` for a
method to get flux points with a minimum significance.
"""
from gammapy.spectrum import SpectrumFit
binning = EnergyBounds(binning)
low_bins = binning.lower_bounds
high_bins = binning.upper_bounds
diff_flux = list()
diff_flux_err = list()
e_err_hi = list()
e_err_lo = list()
energy = list()
from ..spectrum import models, powerlaw
from sherpa.models import PowLaw1D
if isinstance(model, models.PowerLaw):
temp = model.to_sherpa()
temp.gamma.freeze()
sherpa_models = [temp] * binning.nbins
else:
sherpa_models = [None] * binning.nbins
for low, high, sherpa_model in zip(low_bins, high_bins, sherpa_models):
log.info('Computing flux points in bin [{}, {}]'.format(low, high))
# Make PowerLaw approximation for higher order models
if sherpa_model is None:
flux_low = model(low)
flux_high = model(high)
index = powerlaw.power_law_g_from_points(e1=low,
e2=high,
f1=flux_low,
f2=flux_high)
log.debug('Approximated power law index: {}'.format(index))
sherpa_model = PowLaw1D('powlaw1d.default')
sherpa_model.gamma = index
sherpa_model.gamma.freeze()
sherpa_model.ref = model.parameters.reference.to('keV')
sherpa_model.ampl = 1e-20
fit = SpectrumFit(obs_list, sherpa_model)
# If 'low' or 'high' fall onto a bin edge of the
# SpectrumObservation binning, numerical fluctuations can lead to
# the inclusion of unwanted bins
correction = 1e-5
fit.fit_range = ((1 + correction) * low, (1 - correction) * high)
fit.fit()
res = fit.global_result
bin_center = np.sqrt(low * high)
energy.append(bin_center)
e_err_hi.append(high - bin_center)
e_err_lo.append(bin_center - low)
diff_flux.append(res.model(bin_center).to('m-2 s-1 TeV-1'))
err = res.model_with_uncertainties(bin_center.to('TeV').value)
diff_flux_err.append(err.s * Unit('m-2 s-1 TeV-1'))
return cls.from_arrays(energy=energy,
diff_flux=diff_flux,
diff_flux_err_hi=diff_flux_err,
diff_flux_err_lo=diff_flux_err,
energy_err_hi=e_err_hi,
energy_err_lo=e_err_lo)
from astropy.tests.helper import assert_quantity_allclose
from gammapy.data import ObservationTable
from gammapy.datasets import gammapy_extra
from gammapy.spectrum import SpectrumFit, SpectrumGrouping, group_obs_table
obs_table_file = gammapy_extra.filename(
'datasets/hess-crab4_pha/observation_table.fits')
obs_table = ObservationTable.read(obs_table_file)
fit = SpectrumFit.from_observation_table(obs_table)
fit.model = 'PL'
fit.energy_threshold_low = '1 TeV'
fit.energy_threshold_high = '10 TeV'
fit.run(method='sherpa')
#Use each obs in one group
obs_table1 = group_obs_table(obs_table, eff_range=[90, 95], n_eff_bin=5)
obs_table1.write('grouped_table1_debug.fits', overwrite=True)
grouping = SpectrumGrouping(obs_table1)
grouping.run()
fit_band2 = SpectrumFit.from_observation_table(grouping.stacked_obs_table)
fit_band2.model = 'PL'
fit_band2.energy_threshold_low = '1 TeV'
fit_band2.energy_threshold_high = '10 TeV'
fit_band2.run(method='sherpa')
assert_quantity_allclose(fit.result.parameters["index"],