WcsNDMap¶
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class
gammapy.maps.
WcsNDMap
(geom, data=None, dtype='float32', meta=None)[source]¶ Bases:
gammapy.maps.WcsMap
Representation of a N+2D map using WCS with two spatial dimensions and N non-spatial dimensions.
This class uses an ND numpy array to store map values. For maps with non-spatial dimensions and variable pixel size it will allocate an array with dimensions commensurate with the largest image plane.
Parameters: geom :
WcsGeom
WCS geometry object.
data :
ndarray
Data array. If none then an empty array will be allocated.
dtype : str, optional
Data type, default is float32
meta :
OrderedDict
Dictionary to store meta data.
Attributes Summary
data
Data array ( ndarray
)geom
Map geometry ( MapGeom
)Methods Summary
coadd
(map_in)Add the contents of map_in
to this map.create
([map_type, npix, binsz, width, proj, …])Factory method to create an empty WCS map. crop
(crop_width)Crop the spatial dimension of the map by removing a number of pixels from the edge of the map. downsample
(factor[, preserve_counts])Downsample the spatial dimension of the map by a given factor. fill_by_coord
(coords[, weights])Fill pixels at the given map coordinates with values in weights
vector.fill_by_idx
(idx[, weights])Fill pixels at the given pixel indices with values in weights
vector.fill_by_pix
(pix[, weights])Fill pixels at the given pixel coordinates with values in weights
vector.from_geom
(geom[, meta, map_type])Generate an empty map from a Geom
instance.from_hdu
(hdu[, hdu_bands])Make a WcsNDMap object from a FITS HDU. from_hdu_list
(hdulist[, hdu, hdu_bands, …])from_hdulist
(hdu_list[, hdu, hdu_bands])Make a WcsMap object from a FITS HDUList. get_by_coord
(coords)Return map values at the given map coordinates. get_by_idx
(idx)Return map values at the given pixel indices. get_by_pix
(pix)Return map values at the given pixel coordinates. interp_by_coord
(coords[, interp])Interpolate map values at the given map coordinates. interp_by_pix
(pix[, interp])Interpolate map values at the given pixel coordinates. interp_image
(coords[, order])iter_by_coord
([buffersize])Iterate over elements of the map returning a tuple with values and map coordinates. iter_by_image
()Iterate over image planes of the map returning a tuple with the image array and image plane index. iter_by_pix
([buffersize])Iterate over elements of the map returning a tuple with values and pixel coordinates. make_hdu
([hdu, hdu_bands, sparse, conv])Make a FITS HDU from this map. pad
(pad_width[, mode, cval, order])Pad the spatial dimension of the map by extending the edge of the map by the given number of pixels. plot
([ax, idx])Quickplot method. read
(filename[, hdu, hdu_bands, map_type])Read a map from a FITS file. reproject
(geom[, order, mode])Reproject this map to a different geometry. set_by_coord
(coords, vals)Set pixels at the given map coordinates to the values in vals
vector.set_by_idx
(idx, vals)Set pixels at the given pixel indices to the values in vals
vector.set_by_pix
(pix, vals)Set pixels at the given pixel coordinates to the values in vals
vector.sum_over_axes
()Reduce to a 2D image by summing over non-spatial dimensions. to_hdulist
([hdu, hdu_bands, sparse, conv])Convert to HDUList
.upsample
(factor[, order, preserve_counts])Upsample the spatial dimension of the map by a given factor. write
(filename, **kwargs)Write to a FITS file. Attributes Documentation
Methods Documentation
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coadd
(map_in)¶ Add the contents of
map_in
to this map. This method can be used to combine maps containing integral quantities (e.g. counts) or differential quantities if the maps have the same binning.Parameters: map_in :
Map
Input map.
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create
(map_type='wcs', npix=None, binsz=0.1, width=None, proj='CAR', coordsys='CEL', refpix=None, axes=None, skydir=None, dtype='float32', conv='gadf', meta=None)¶ Factory method to create an empty WCS map.
Parameters: map_type : {‘wcs’, ‘wcs-sparse’}
Map type. Selects the class that will be used to instantiate the map.
npix : int or tuple or list
Width of the map in pixels. A tuple will be interpreted as parameters for longitude and latitude axes. For maps with non-spatial dimensions, list input can be used to define a different map width in each image plane. This option supersedes width.
width : float or tuple or list
Width of the map in degrees. A tuple will be interpreted as parameters for longitude and latitude axes. For maps with non-spatial dimensions, list input can be used to define a different map width in each image plane.
binsz : float or tuple or list
Map pixel size in degrees. A tuple will be interpreted as parameters for longitude and latitude axes. For maps with non-spatial dimensions, list input can be used to define a different bin size in each image plane.
skydir : tuple or
SkyCoord
Sky position of map center. Can be either a SkyCoord object or a tuple of longitude and latitude in deg in the coordinate system of the map.
coordsys : {‘CEL’, ‘GAL’}, optional
Coordinate system, either Galactic (‘GAL’) or Equatorial (‘CEL’).
axes : list
List of non-spatial axes.
proj : string, optional
Any valid WCS projection type. Default is ‘CAR’ (cartesian).
refpix : tuple
Reference pixel of the projection. If None then this will be chosen to be center of the map.
dtype : str, optional
Data type, default is float32
conv : {‘fgst-ccube’,’fgst-template’,’gadf’}, optional
FITS format convention. Default is ‘gadf’.
meta :
OrderedDict
Dictionary to store meta data.
Returns: map :
WcsMap
A WCS map object.
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crop
(crop_width)[source]¶ Crop the spatial dimension of the map by removing a number of pixels from the edge of the map.
Parameters: crop_width : {sequence, array_like, int}
Number of pixels cropped from the edges of each axis. Defined analogously to
pad_with
frompad
.Returns: map :
Map
Cropped map.
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downsample
(factor, preserve_counts=True)[source]¶ Downsample the spatial dimension of the map by a given factor.
Parameters: factor : int
Downsampling factor.
preserve_counts : bool
Preserve the integral over each bin. This should be true if the map is an integral quantity (e.g. counts) and false if the map is a differential quantity (e.g. intensity).
Returns: map :
Map
Downsampled map.
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fill_by_coord
(coords, weights=None)¶ Fill pixels at the given map coordinates with values in
weights
vector.Parameters: coords : tuple or
MapCoord
MapCoord
object or tuple of coordinate arrays for each dimension of the map. Tuple should be ordered as (lon, lat, x_0, …, x_n) where x_i are coordinates for non-spatial dimensions of the map.weights :
ndarray
Weights vector. If None then a unit weight will be assumed for each element in
coords
.
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fill_by_idx
(idx, weights=None)[source]¶ Fill pixels at the given pixel indices with values in
weights
vector.Parameters: idx : tuple
Tuple of pixel index arrays for each dimension of the map. Tuple should be ordered as (I_lon, I_lat, I_0, …, I_n) for WCS maps and (I_hpx, I_0, …, I_n) for HEALPix maps.
weights :
ndarray
Weights vector. If None then a unit weight will be assumed for each element in
idx
.
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fill_by_pix
(pix, weights=None)¶ Fill pixels at the given pixel coordinates with values in
weights
vector.Parameters: pix : tuple
Tuple of pixel index arrays for each dimension of the map. Tuple should be ordered as (I_lon, I_lat, I_0, …, I_n) for WCS maps and (I_hpx, I_0, …, I_n) for HEALPix maps. Pixel indices can be either float or integer type. Float indices will be rounded to the nearest integer.
weights :
ndarray
Weights vector. If None then a unit weight will be assumed for each element in
pix
.
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from_geom
(geom, meta=None, map_type='auto')¶ Generate an empty map from a
Geom
instance.Parameters: geom :
MapGeom
Map geometry.
meta :
OrderedDict
Dictionary to store meta data.
map_type : {‘wcs’, ‘wcs-sparse’, ‘hpx’, ‘hpx-sparse’, ‘auto’}
Map type. Selects the class that will be used to instantiate the map. The map type should be consistent with the geometry. If map_type is ‘auto’ then an appropriate map type will be inferred from type of
geom
.Returns: map_out :
Map
Map object
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classmethod
from_hdu
(hdu, hdu_bands=None)[source]¶ Make a WcsNDMap object from a FITS HDU.
Parameters: hdu :
BinTableHDU
orImageHDU
The map FITS HDU.
hdu_bands :
BinTableHDU
The BANDS table HDU.
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from_hdu_list
(hdulist, hdu=None, hdu_bands=None, map_type='auto')¶
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from_hdulist
(hdu_list, hdu=None, hdu_bands=None)¶ Make a WcsMap object from a FITS HDUList.
Parameters: hdu_list :
HDUList
HDU list containing HDUs for map data and bands.
hdu : str
Name or index of the HDU with the map data.
hdu_bands : str
Name or index of the HDU with the BANDS table.
Returns: wcs_map :
WcsMap
Map object
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get_by_coord
(coords)¶ Return map values at the given map coordinates.
Parameters: coords : tuple or
MapCoord
MapCoord
object or tuple of coordinate arrays for each dimension of the map. Tuple should be ordered as (lon, lat, x_0, …, x_n) where x_i are coordinates for non-spatial dimensions of the map.Returns: vals :
ndarray
Values of pixels in the map. np.nan used to flag coords outside of map.
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get_by_idx
(idx)[source]¶ Return map values at the given pixel indices.
Parameters: idx : tuple
Tuple of pixel index arrays for each dimension of the map. Tuple should be ordered as (I_lon, I_lat, I_0, …, I_n) for WCS maps and (I_hpx, I_0, …, I_n) for HEALPix maps.
Returns: vals :
ndarray
Array of pixel values. np.nan used to flag coordinate outside of map
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get_by_pix
(pix)¶ Return map values at the given pixel coordinates.
Parameters: pix : tuple
Tuple of pixel index arrays for each dimension of the map. Tuple should be ordered as (I_lon, I_lat, I_0, …, I_n) for WCS maps and (I_hpx, I_0, …, I_n) for HEALPix maps. Pixel indices can be either float or integer type.
Returns: vals :
ndarray
Array of pixel values. np.nan used to flag coordinates outside of map
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interp_by_coord
(coords, interp=None)[source]¶ Interpolate map values at the given map coordinates.
Parameters: coords : tuple or
MapCoord
MapCoord
object or tuple of coordinate arrays for each dimension of the map. Tuple should be ordered as (lon, lat, x_0, …, x_n) where x_i are coordinates for non-spatial dimensions of the map.interp : {None, ‘nearest’, ‘linear’, ‘cubic’, 0, 1, 2, 3}
Method to interpolate data values. By default no interpolation is performed and the return value will be the amplitude of the pixel encompassing the given coordinate. Integer values can be used in lieu of strings to choose the interpolation method of the given order (0=’nearest’, 1=’linear’, 2=’quadratic’, 3=’cubic’). Note that only ‘nearest’ and ‘linear’ methods are supported for all map types.
Returns: vals :
ndarray
Interpolated pixel values.
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iter_by_coord
(buffersize=1)[source]¶ Iterate over elements of the map returning a tuple with values and map coordinates.
Parameters: buffersize : int
Set the size of the buffer. The map will be returned in chunks of the given size.
Returns: val :
ndarray
Map values.
coords : tuple
Tuple of map coordinates.
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iter_by_image
()[source]¶ Iterate over image planes of the map returning a tuple with the image array and image plane index.
Returns: val :
ndarray
Array of image plane values.
idx : tuple
Index of image plane.
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iter_by_pix
(buffersize=1)[source]¶ Iterate over elements of the map returning a tuple with values and pixel coordinates.
Parameters: buffersize : int
Set the size of the buffer. The map will be returned in chunks of the given size.
Returns: val :
ndarray
Map values.
pix : tuple
Tuple of pixel coordinates.
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make_hdu
(hdu='SKYMAP', hdu_bands=None, sparse=False, conv=None)¶ Make a FITS HDU from this map.
Parameters: hdu : str
The HDU extension name.
hdu_bands : str
The HDU extension name for BANDS table.
sparse : bool
Set INDXSCHM to SPARSE and sparsify the map by only writing pixels with non-zero amplitude.
Returns: hdu :
BinTableHDU
orImageHDU
HDU containing the map data.
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pad
(pad_width, mode='constant', cval=0, order=1)[source]¶ Pad the spatial dimension of the map by extending the edge of the map by the given number of pixels.
Parameters: pad_width : {sequence, array_like, int}
Number of pixels padded to the edges of each axis.
mode : {‘edge’, ‘constant’, ‘interp’}
Padding mode. ‘edge’ pads with the closest edge value. ‘constant’ pads with a constant value. ‘interp’ pads with an extrapolated value.
cval : float
Padding value when mode=’consant’.
order : int
Order of interpolation when mode=’constant’ (0 = nearest-neighbor, 1 = linear, 2 = quadratic, 3 = cubic).
Returns: map :
Map
Padded map.
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plot
(ax=None, idx=None, **kwargs)[source]¶ Quickplot method.
Parameters: norm : str
Set the normalization scheme of the color map.
idx : tuple
Set the image slice to plot if this map has non-spatial dimensions.
**kwargs : dict
Keyword arguments passed to
imshow
.Returns: fig :
Figure
Figure object.
ax :
WCSAxes
WCS axis object
im :
AxesImage
Image object.
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read
(filename, hdu=None, hdu_bands=None, map_type='auto')¶ Read a map from a FITS file.
Parameters: filename : str
Name of the FITS file.
hdu : str
Name or index of the HDU with the map data.
hdu_bands : str
Name or index of the HDU with the BANDS table. If not defined this will be inferred from the FITS header of the map HDU.
map_type : {‘wcs’, ‘wcs-sparse’, ‘hpx’, ‘hpx-sparse’, ‘auto’}
Map type. Selects the class that will be used to instantiate the map. The map type should be consistent with the format of the input file. If map_type is ‘auto’ then an appropriate map type will be inferred from the input file.
Returns: map_out :
Map
Map object
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reproject
(geom, order=1, mode='interp')¶ Reproject this map to a different geometry.
Parameters: geom :
MapGeom
Geometry of projection.
mode : {‘interp’, ‘exact’}
Method for reprojection. ‘interp’ method interpolates at pixel centers. ‘exact’ method integrates over intersection of pixels.
order : int or str
Order of interpolating polynomial (0 = nearest-neighbor, 1 = linear, 2 = quadratic, 3 = cubic).
Returns: map :
Map
Reprojected map.
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set_by_coord
(coords, vals)¶ Set pixels at the given map coordinates to the values in
vals
vector.Parameters: coords : tuple or
MapCoord
MapCoord
object or tuple of coordinate arrays for each dimension of the map. Tuple should be ordered as (lon, lat, x_0, …, x_n) where x_i are coordinates for non-spatial dimensions of the map.vals :
ndarray
Values vector. Pixels at
coords
will be set to these values.
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set_by_idx
(idx, vals)[source]¶ Set pixels at the given pixel indices to the values in
vals
vector.Parameters: idx : tuple
Tuple of pixel index arrays for each dimension of the map. Tuple should be ordered as (I_lon, I_lat, I_0, …, I_n) for WCS maps and (I_hpx, I_0, …, I_n) for HEALPix maps.
vals :
ndarray
Values vector. Pixels at
idx
will be set to these values.
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set_by_pix
(pix, vals)¶ Set pixels at the given pixel coordinates to the values in
vals
vector.Parameters: pix : tuple
Tuple of pixel index arrays for each dimension of the map. Tuple should be ordered as (I_lon, I_lat, I_0, …, I_n) for WCS maps and (I_hpx, I_0, …, I_n) for HEALPix maps. Pixel indices can be either float or integer type. Float indices will be rounded to the nearest integer.
vals :
ndarray
Values vector. Pixels at
pix
will be set to these values.
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to_hdulist
(hdu=None, hdu_bands=None, sparse=False, conv=None)¶ Convert to
HDUList
.Parameters: hdu : str
Name or index of the HDU with the map data.
hdu_bands : str
Name or index of the HDU with the BANDS table.
sparse : bool
Sparsify the map by only writing pixels with non-zero amplitude.
conv : {‘fgst-ccube’,’fgst-template’,’gadf’,None}, optional
FITS format convention. If None this will be set to the default convention of the map.
Returns: hdu_list :
HDUList
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upsample
(factor, order=0, preserve_counts=True)[source]¶ Upsample the spatial dimension of the map by a given factor.
Parameters: factor : int
Upsampling factor.
order : int
Order of the interpolation used for upsampling.
preserve_counts : bool
Preserve the integral over each bin. This should be true if the map is an integral quantity (e.g. counts) and false if the map is a differential quantity (e.g. intensity).
Returns: map :
Map
Upsampled map.
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write
(filename, **kwargs)¶ Write to a FITS file.
Parameters: filename : str
Output file name.
hdu : str
Set the name of the image extension. By default this will be set to SKYMAP (for BINTABLE HDU) or PRIMARY (for IMAGE HDU).
hdu_bands : str
Set the name of the bands table extension. By default this will be set to BANDS.
conv : str
FITS format convention. By default files will be written to the gamma-astro-data-formats (GADF) format. This option can be used to write files that are compliant with format conventions required by specific software (e.g. the Fermi Science Tools). Supported conventions are ‘gadf’, ‘fgst-ccube’, ‘fgst-ltcube’, ‘fgst-bexpcube’, ‘fgst-template’, ‘fgst-srcmap’, ‘fgst-srcmap-sparse’, ‘galprop’, and ‘galprop2’.
sparse : bool
Sparsify the map by dropping pixels with zero amplitude. This option is only compatible with the ‘gadf’ format.
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