SpectrumDatasetOnOff¶
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class
gammapy.spectrum.SpectrumDatasetOnOff(model=None, counts=None, counts_off=None, livetime=None, aeff=None, edisp=None, mask_safe=None, mask_fit=None, acceptance=None, acceptance_off=None, name='', gti=None)[source]¶ Bases:
gammapy.spectrum.SpectrumDatasetSpectrum dataset for on-off likelihood fitting.
The on-off spectrum dataset bundles reduced counts data, off counts data, with a spectral model, relative background efficiency and instrument response functions to compute the fit-statistic given the current model and data.
Parameters: - model :
SpectralModel Fit model
- counts :
CountsSpectrum ON Counts spectrum
- counts_off :
CountsSpectrum OFF Counts spectrum
- livetime :
Quantity Livetime
- aeff :
EffectiveAreaTable Effective area
- edisp :
EnergyDispersion Energy dispersion
- mask_safe :
array Mask defining the safe data range.
- mask_fit :
array Mask to apply to the likelihood for fitting.
- acceptance :
arrayor float Relative background efficiency in the on region.
- acceptance_off :
arrayor float Relative background efficiency in the off region.
- name : str
Name of the dataset.
- gti :
GTI GTI of the observation or union of GTI if it is a stacked observation
See also
SpectrumDataset,FluxPointsDataset,MapDataset
Attributes Summary
alphaExposure ratio between signal and background regions backgrounddata_shapeShape of the counts data energy_rangeEnergy range defined by the safe mask excessExcess (counts - alpha * counts_off) likelihood_typemaskCombined fit and safe mask mask_safemodelparametersMethods Summary
copy(self)A deep copy. create(e_reco[, e_true, reference_time])Create empty SpectrumDatasetOnOff. fake(self, background_model[, random_state])Simulate fake counts for the current model and reduced irfs. from_ogip_files(filename)Read SpectrumDatasetOnOfffrom OGIP files.likelihood(self)Total likelihood given the current model parameters. likelihood_per_bin(self)Likelihood per bin given the current model parameters npred(self)Return npred map (model + background) npred_sig(self)Predicted counts from source model ( CountsSpectrum).peek(self[, figsize])Quick-look summary plots. plot_counts(self[, ax])Plot predicted and detected counts. plot_fit(self)Plot counts and residuals in two panels. plot_residuals(self[, method, ax])Plot residuals. read(filename)Read from file residuals(self[, method])Compute the spectral residuals. stack(self, other)Stack this dataset with another one. to_ogip_files(self[, outdir, use_sherpa, …])Write OGIP files. Attributes Documentation
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alpha¶ Exposure ratio between signal and background regions
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background¶
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data_shape¶ Shape of the counts data
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energy_range¶ Energy range defined by the safe mask
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excess¶ Excess (counts - alpha * counts_off)
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likelihood_type= 'wstat'¶
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mask¶ Combined fit and safe mask
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mask_safe¶
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model¶
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parameters¶
Methods Documentation
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copy(self)¶ A deep copy.
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classmethod
create(e_reco, e_true=None, reference_time='2000-01-01')[source]¶ Create empty SpectrumDatasetOnOff.
Empty containers are created with the correct geometry. counts, counts_off and aeff are zero and edisp is diagonal.
The safe_mask is set to False in every bin.
Parameters:
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fake(self, background_model, random_state='random-seed')[source]¶ Simulate fake counts for the current model and reduced irfs.
This method overwrites the counts and off counts defined on the dataset object.
Parameters: - background_model :
CountsSpectrum BackgroundModel. In the future will be part of the SpectrumDataset Class. For the moment, a CountSpectrum.
- random_state : {int, ‘random-seed’, ‘global-rng’,
RandomState} Defines random number generator initialisation. Passed to
get_random_state.
- background_model :
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classmethod
from_ogip_files(filename)[source]¶ Read
SpectrumDatasetOnOfffrom OGIP files.BKG file, ARF, and RMF must be set in the PHA header and be present in the same folder.
Parameters: - filename : str
OGIP PHA file to read
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likelihood(self)¶ Total likelihood given the current model parameters.
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npred(self)¶ Return npred map (model + background)
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npred_sig(self)[source]¶ Predicted counts from source model (
CountsSpectrum).
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plot_counts(self, ax=None)¶ Plot predicted and detected counts.
Parameters: - ax :
Axes Axes object.
Returns: - ax :
Axes Axes object.
- ax :
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plot_fit(self)¶ Plot counts and residuals in two panels.
Calls
plot_countsandplot_residuals.
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plot_residuals(self, method='diff', ax=None, **kwargs)¶ Plot residuals.
Parameters: - ax :
Axes Axes object.
- method : {“diff”, “diff/model”, “diff/sqrt(model)”}
Normalization used to compute the residuals, see
SpectrumDataset.residuals()- **kwargs : dict
Keywords passed to
CountsSpectrum.plot()
Returns: - ax :
Axes Axes object.
- ax :
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classmethod
read(filename)[source]¶ Read from file
For now, filename is assumed to the name of a PHA file where BKG file, ARF, and RMF names must be set in the PHA header and be present in the same folder
Parameters: - filename : str
OGIP PHA file to read
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residuals(self, method='diff')¶ Compute the spectral residuals.
Parameters: - method : {“diff”, “diff/model”, “diff/sqrt(model)”}
- Method used to compute the residuals. Available options are:
diff(default): data - modeldiff/model: (data - model) / modeldiff/sqrt(model): (data - model) / sqrt(model)
Returns: - residuals :
CountsSpectrum Residual spectrum
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stack(self, other)[source]¶ Stack this dataset with another one.
Safe mask is applied to compute the stacked counts vector. Counts outside each dataset safe mask are lost.
Stacking is performed in-place.
The stacking of 2 datasets is implemented as follows. Here, \(k\) denotes a bin in reconstructed energy and \(j = {1,2}\) is the dataset number
The
mask_safeof each dataset is defined as:\[\begin{split}\epsilon_{jk} =\left\{\begin{array}{cl} 1, & \mbox{if k is inside the energy thresholds}\\ 0, & \mbox{otherwise} \end{array}\right.\end{split}\]Then the total
countsandcounts_offare computed according to:\[ \begin{align}\begin{aligned}\overline{\mathrm{n_{on}}}_k = \mathrm{n_{on}}_{1k} \cdot \epsilon_{1k} + \mathrm{n_{on}}_{2k} \cdot \epsilon_{2k}\\\overline{\mathrm{n_{off}}}_k = \mathrm{n_{off}}_{1k} \cdot \epsilon_{1k} + \mathrm{n_{off}}_{2k} \cdot \epsilon_{2k}\end{aligned}\end{align} \]The stacked
safe_maskis then:\[\overline{\epsilon_k} = \epsilon_{1k} OR \epsilon_{2k}\]In each energy bin \(k\), the count excess is computed taking into account the ON
acceptance, \(a_{on}_k\) and the OFF one:acceptance_off, \(a_{off}_k\). They define the \(\alpha_k=a_{on}_k/a_{off}_k\) factors such that \(n_{ex}_k = n_{on}_k - \alpha_k n_{off}_k\). We define the stacked value of \(\overline{{a}_{on}}_k = 1\) so that:\[\overline{{a}_{off}}_k = \frac{\overline{\mathrm {n_{off}}}}{\alpha_{1k} \cdot \mathrm{n_{off}}_{1k} \cdot \epsilon_{1k} + \alpha_{2k} \cdot \mathrm{n_{off}}_{2k} \cdot \epsilon_{2k}}\]Please refer to the
IRFStackerfor the description of how the IRFs are stacked.Parameters: - other :
SpectrumDatasetOnOff the dataset to stack to the current one
Examples
>>> from gammapy.spectrum import SpectrumDatasetOnOff >>> obs_ids = [23523, 23526, 23559, 23592] >>> datasets = [] >>> for obs in obs_ids: >>> filename = "$GAMMAPY_DATA/joint-crab/spectra/hess/pha_obs{}.fits" >>> ds = SpectrumDatasetOnOff.from_ogip_files(filename.format(obs)) >>> datasets.append(ds) >>> stacked = datasets[0] >>> for ds in datasets[1:]: >>> stacked.stack(ds) >>> print(stacked.livetime) 6313.8116406202325 s
- other :
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to_ogip_files(self, outdir=None, use_sherpa=False, overwrite=False)[source]¶ Write OGIP files.
If you want to use the written files with Sherpa you have to set the
use_sherpaflag. Then all files will be written in units ‘keV’ and ‘cm2’.Parameters: - outdir :
pathlib.Path output directory, default: pwd
- use_sherpa : bool, optional
Write Sherpa compliant files, default: False
- overwrite : bool
Overwrite existing files?
- outdir :
- model :