# Licensed under a 3-clause BSD style license - see LICENSE.rst
import logging
import numpy as np
from astropy import units as u
from gammapy.datasets import Datasets
from gammapy.maps import MapAxis
from gammapy.modeling import Fit
from gammapy.utils.pbar import progress_bar
from gammapy.utils.table import table_from_row_data
from ..flux import FluxEstimator
from .core import FluxPoints
log = logging.getLogger(__name__)
__all__ = ["FluxPointsEstimator"]
[docs]class FluxPointsEstimator(FluxEstimator):
"""Flux points estimator.
Estimates flux points for a given list of datasets, energies and spectral model.
To estimate the flux point the amplitude of the reference spectral model is
fitted within the energy range defined by the energy group. This is done for
each group independently. The amplitude is re-normalized using the "norm" parameter,
which specifies the deviation of the flux from the reference model in this
energy group. See https://gamma-astro-data-formats.readthedocs.io/en/latest/spectra/binned_likelihoods/index.html
for details.
The method is also described in the Fermi-LAT catalog paper
https://ui.adsabs.harvard.edu/#abs/2015ApJS..218...23A
or the HESS Galactic Plane Survey paper
https://ui.adsabs.harvard.edu/#abs/2018A%26A...612A...1H
Parameters
----------
energy_edges : `~astropy.units.Quantity`
Energy edges of the flux point bins.
source : str or int
For which source in the model to compute the flux points.
norm_min : float
Minimum value for the norm used for the fit statistic profile evaluation.
norm_max : float
Maximum value for the norm used for the fit statistic profile evaluation.
norm_n_values : int
Number of norm values used for the fit statistic profile.
norm_values : `numpy.ndarray`
Array of norm values to be used for the fit statistic profile.
n_sigma : int
Number of sigma to use for asymmetric error computation. Default is 1.
n_sigma_ul : int
Number of sigma to use for upper limit computation. Default is 2.
selection_optional : list of str
Which additional quantities to estimate. Available options are:
* "all": all the optional steps are executed
* "errn-errp": estimate asymmetric errors on flux.
* "ul": estimate upper limits.
* "scan": estimate fit statistic profiles.
Default is None so the optional steps are not executed.
fit : `Fit`
Fit instance specifying the backend and fit options.
reoptimize : bool
Re-optimize other free model parameters. Default is True.
sum_over_energy_groups : bool
Whether to sum over the energy groups or fit the norm on the full energy
grid.
"""
tag = "FluxPointsEstimator"
def __init__(
self, energy_edges=[1, 10] * u.TeV, sum_over_energy_groups=False, **kwargs
):
self.energy_edges = energy_edges
self.sum_over_energy_groups = sum_over_energy_groups
fit = Fit(confidence_opts={"backend": "scipy"})
kwargs.setdefault("fit", fit)
super().__init__(**kwargs)
[docs] def run(self, datasets):
"""Run the flux point estimator for all energy groups.
Parameters
----------
datasets : `~gammapy.datasets.Datasets`
Datasets
Returns
-------
flux_points : `FluxPoints`
Estimated flux points.
"""
datasets = Datasets(datasets=datasets)
rows = []
for energy_min, energy_max in progress_bar(
zip(self.energy_edges[:-1], self.energy_edges[1:]), desc="Energy bins"
):
row = self.estimate_flux_point(
datasets,
energy_min=energy_min,
energy_max=energy_max,
)
rows.append(row)
meta = {
"n_sigma": self.n_sigma,
"n_sigma_ul": self.n_sigma_ul,
"sed_type_init": "likelihood",
}
table = table_from_row_data(rows=rows, meta=meta)
model = datasets.models[self.source]
return FluxPoints.from_table(
table=table,
reference_model=model.copy(),
gti=datasets.gti,
format="gadf-sed",
)
[docs] def estimate_flux_point(self, datasets, energy_min, energy_max):
"""Estimate flux point for a single energy group.
Parameters
----------
datasets : `Datasets`
Datasets
energy_min, energy_max : `~astropy.units.Quantity`
Energy bounds to compute the flux point for.
Returns
-------
result : dict
Dict with results for the flux point.
"""
datasets_sliced = datasets.slice_by_energy(
energy_min=energy_min, energy_max=energy_max
)
if self.sum_over_energy_groups:
datasets_sliced = Datasets(
[_.to_image(name=_.name) for _ in datasets_sliced]
)
if len(datasets_sliced) > 0:
datasets_sliced.models = datasets.models.copy()
return super().run(datasets=datasets_sliced)
else:
log.warning(f"No dataset contribute in range {energy_min}-{energy_max}")
model = datasets.models[self.source].spectral_model
return self._nan_result(datasets, model, energy_min, energy_max)
def _nan_result(self, datasets, model, energy_min, energy_max):
"""NaN result"""
energy_axis = MapAxis.from_energy_edges([energy_min, energy_max])
with np.errstate(invalid="ignore", divide="ignore"):
result = model.reference_fluxes(energy_axis=energy_axis)
# convert to scalar values
result = {key: value.item() for key, value in result.items()}
result.update(
{
"norm": np.nan,
"stat": np.nan,
"success": False,
"norm_err": np.nan,
"ts": np.nan,
"counts": np.zeros(len(datasets)),
"npred": np.nan * np.zeros(len(datasets)),
"npred_excess": np.nan * np.zeros(len(datasets)),
"datasets": datasets.names,
}
)
if "errn-errp" in self.selection_optional:
result.update({"norm_errp": np.nan, "norm_errn": np.nan})
if "ul" in self.selection_optional:
result.update({"norm_ul": np.nan})
if "scan" in self.selection_optional:
norm = super()._set_norm_parameter()
norm_scan = norm.scan_values
result.update({"norm_scan": norm_scan, "stat_scan": np.nan * norm_scan})
return result