StackedObsImageMaker¶
-
class
gammapy.scripts.
StackedObsImageMaker
(empty_image=None, energy_band=None, offset_band=None, data_store=None, obs_table=None, exclusion_mask=None, ncounts_min=0, save_bkg_scale=True)[source]¶ Bases:
object
Compute stacked images for many observations.
The computed images are stored in a
images
attribute of typeSkyImageList
with the following keys:counts
: Countsbkg
: Background modelexposure
: Exposureexcess
: Excesssignificance
: Significance
Parameters: empty_image :
SkyImage
Reference image
energy_band :
Energy
Energy band selection
offset_band :
astropy.coordinates.Angle
Offset band selection
data_store :
DataStore
Data store
obs_table :
Table
Required columns: OBS_ID
exclusion_mask :
SkyImage
Exclusion mask
ncounts_min : int
Minimum counts required for the observation
save_bkg_scale: bool
- True if you want to save the normalisation of the bkg for each run in a
Table
table_bkg_norm with two columns: “OBS_ID” and “bkg_scale”
Methods Summary
excess_image
()Compute excess between counts and bkg image. make_images
([make_background_image, …])Compute the counts, bkg, exposure, excess and significance images for a set of observation. significance_image
(radius)Make the significance image from the counts and bkg images. Methods Documentation
-
make_images
(make_background_image=False, bkg_norm=True, spectral_index=2.3, for_integral_flux=False, radius=10)[source]¶ Compute the counts, bkg, exposure, excess and significance images for a set of observation.
Parameters: make_background_image : bool
True if you want to compute the background and exposure images
bkg_norm : bool
If true, apply the scaling factor to the bkg image
spectral_index : float
Assumed power-law spectral index
for_integral_flux : bool
True if you want that the total excess / exposure gives the integrated flux
radius : float
Disk radius in pixels for the significance image