SkyDiffuseMap¶
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class
gammapy.image.models.SkyDiffuseMap(map, norm=1, meta=None, normalize=True, interp_kwargs=None)[source]¶ Bases:
gammapy.image.models.SkySpatialModelSpatial sky map template model (2D).
This is for a 2D image. Use
SkyDiffuseCubefor 3D cubes with an energy axis.Parameters: - map :
Map Map template
- norm : float
Norm parameter (multiplied with map values)
- meta : dict, optional
Meta information, meta[‘filename’] will be used for serialization
- normalize : bool
Normalize the input map so that it integrates to unity.
- interp_kwargs : dict
Interpolation keyword arguments passed to
gammapy.maps.Map.interp_by_coord. Default arguments are {‘interp’: ‘linear’, ‘fill_value’: 0}.
Attributes Summary
evaluation_radiusReturns the effective radius of the sky region where the model evaluates to non-zero. framemapmetanormparametersParameters ( Parameters)positionSkyCoordMethods Summary
__call__(self, lon, lat)Call evaluate method copy(self)A deep copy. evaluate(self, lon, lat, norm)Evaluate model. normalize(self)Normalize the diffuse map model so that it integrates to unity. read(filename[, normalize])Read spatial template model from FITS image. Attributes Documentation
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evaluation_radius¶ Returns the effective radius of the sky region where the model evaluates to non-zero. For a DiffuseMap source, we fix it to half of the maximal dimension of the map.
Returns: - radius :
Angle Radius in angular units.
- radius :
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frame¶
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map¶
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meta¶
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norm¶
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parameters¶ Parameters (
Parameters)
Methods Documentation
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__call__(self, lon, lat)¶ Call evaluate method
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copy(self)¶ A deep copy.
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classmethod
read(filename, normalize=True, **kwargs)[source]¶ Read spatial template model from FITS image.
The default unit used if none is found in the file is
sr-1.Parameters: - filename : str
FITS image filename.
- normalize : bool
Normalize the input map so that it integrates to unity.
- kwargs : dict
Keyword arguments passed to
Map.read().
- map :