WcsMap¶
-
class
gammapy.maps.
WcsMap
(geom, data, meta=None, unit='')[source]¶ Bases:
gammapy.maps.Map
Base class for WCS map classes.
Parameters: Attributes Summary
data
Data array ( ndarray
)geom
Map geometry ( MapGeom
)meta
Map meta ( OrderedDict
)quantity
Map data times unit ( Quantity
)unit
Map unit ( Unit
)Methods Summary
coadd
(self, map_in)Add the contents of map_in
to this map.copy
(self, \*\*kwargs)Copy map instance and overwrite given attributes, except for geometry. create
([map_type, npix, binsz, width, proj, …])Factory method to create an empty WCS map. crop
(self, crop_width)Crop the spatial dimension of the map by removing a number of pixels from the edge of the map. downsample
(self, factor[, preserve_counts, axis])Downsample the spatial dimension by a given factor. fill_by_coord
(self, coords[, weights])Fill pixels at coords
with givenweights
.fill_by_idx
(self, idx[, weights])Fill pixels at idx
with givenweights
.fill_by_pix
(self, pix[, weights])Fill pixels at pix
with givenweights
.from_geom
(geom[, meta, data, map_type, unit])Generate an empty map from a MapGeom
instance.from_hdulist
(hdu_list[, hdu, hdu_bands])Make a WcsMap object from a FITS HDUList. get_by_coord
(self, coords)Return map values at the given map coordinates. get_by_idx
(self, idx)Return map values at the given pixel indices. get_by_pix
(self, pix)Return map values at the given pixel coordinates. get_image_by_coord
(self, coords)Return spatial map at the given axis coordinates. get_image_by_idx
(self, idx)Return spatial map at the given axis pixel indices. get_image_by_pix
(self, pix)Return spatial map at the given axis pixel coordinates interp_by_coord
(self, coords[, interp, …])Interpolate map values at the given map coordinates. interp_by_pix
(self, pix[, interp, fill_value])Interpolate map values at the given pixel coordinates. iter_by_coord
(self[, buffersize])Iterate over elements of the map returning a tuple with values and map coordinates. iter_by_image
(self)Iterate over image planes of the map returning a tuple with the image array and image plane index. iter_by_pix
(self[, buffersize])Iterate over elements of the map returning a tuple with values and pixel coordinates. make_hdu
(self[, hdu, hdu_bands, sparse, conv])Make a FITS HDU from this map. pad
(self, 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_interactive
(self[, rc_params])Plot map with interactive widgets to explore the non spatial axes. read
(filename[, hdu, hdu_bands, map_type])Read a map from a FITS file. reproject
(self, geom[, order, mode])Reproject this map to a different geometry. set_by_coord
(self, coords, vals)Set pixels at coords
with givenvals
.set_by_idx
(self, idx, vals)Set pixels at idx
with givenvals
.set_by_pix
(self, pix, vals)Set pixels at pix
with givenvals
.slice_by_idx
(self, slices)Slice sub map from map object. sum_over_axes
(self[, keepdims])Reduce to a 2D image by summing over non-spatial dimensions. to_hdulist
(self[, hdu, hdu_bands, sparse, conv])Convert to HDUList
.upsample
(self, factor[, order, …])Upsample the spatial dimension by a given factor. write
(self, filename[, overwrite])Write to a FITS file. Attributes Documentation
-
meta
¶ Map meta (
OrderedDict
)
Methods Documentation
-
coadd
(self, 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.
- map_in :
-
copy
(self, **kwargs)¶ Copy map instance and overwrite given attributes, except for geometry.
Parameters: - **kwargs : dict
Keyword arguments to overwrite in the map constructor.
Returns: - copy :
Map
Copied Map.
-
classmethod
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, unit='')[source]¶ 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.
- unit : str or
Unit
The unit of the map
Returns: - map :
WcsMap
A WCS map object.
-
crop
(self, crop_width)¶ 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
fromnumpy.pad
.
Returns: - map :
Map
Cropped map.
-
downsample
(self, factor, preserve_counts=True, axis=None)¶ Downsample the spatial dimension 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).
- axis : str
Which axis to downsample. By default spatial axes are downsampled.
Returns: - map :
Map
Downsampled map.
-
fill_by_coord
(self, coords, weights=None)¶ Fill pixels at
coords
with givenweights
.Parameters:
-
fill_by_idx
(self, idx, weights=None)¶ Fill pixels at
idx
with givenweights
.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. Default is weight of one.
-
fill_by_pix
(self, pix, weights=None)¶ Fill pixels at
pix
with givenweights
.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. Default is weight of one.
-
static
from_geom
(geom, meta=None, data=None, map_type='auto', unit='')¶ Generate an empty map from a
MapGeom
instance.Parameters: - geom :
MapGeom
Map geometry.
- data :
numpy.ndarray
data array
- 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
.- unit : str or
Unit
Data unit.
Returns: - map_out :
Map
Map object
- geom :
-
classmethod
from_hdulist
(hdu_list, hdu=None, hdu_bands=None)[source]¶ 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
- hdu_list :
-
get_by_coord
(self, coords)¶ Return map values at the given map coordinates.
Parameters: - coords : tuple or
MapCoord
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.
- coords : tuple or
-
get_by_idx
(self, idx)¶ 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
-
get_by_pix
(self, 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
-
get_image_by_coord
(self, coords)¶ Return spatial map at the given axis coordinates.
Parameters: - coords : tuple or dict
Tuple should be ordered as (x_0, …, x_n) where x_i are coordinates for non-spatial dimensions of the map. Dict should specify the axis names of the non-spatial axes such as {‘axes0’: x_0, …, ‘axesn’: x_n}.
Returns: - map_out :
Map
Map with spatial dimensions only.
See also
Examples
import numpy as np from gammapy.maps import Map, MapAxis from astropy.coordinates import SkyCoord from astropy import units as u # Define map axes energy_axis = MapAxis.from_edges( np.logspace(-1., 1., 4), unit='TeV', name='energy', ) time_axis = MapAxis.from_edges( np.linspace(0., 10, 20), unit='h', name='time', ) # Define map center skydir = SkyCoord(0, 0, frame='galactic', unit='deg') # Create map m_wcs = Map.create( map_type='wcs', binsz=0.02, skydir=skydir, width=10.0, axes=[energy_axis, time_axis], ) # Get image by coord tuple image = m_wcs.get_image_by_coord(('500 GeV', '1 h')) # Get image by coord dict with strings image = m_wcs.get_image_by_coord({'energy': '500 GeV', 'time': '1 h'}) # Get image by coord dict with quantities image = m_wcs.get_image_by_coord({'energy': 0.5 * u.TeV, 'time': 1 * u.h})
-
get_image_by_idx
(self, idx)¶ Return spatial map at the given axis pixel indices.
Parameters: - idx : tuple
Tuple of scalar indices for each non spatial dimension of the map. Tuple should be ordered as (I_0, …, I_n).
Returns: - map_out :
Map
Map with spatial dimensions only.
See also
-
get_image_by_pix
(self, pix)¶ Return spatial map at the given axis pixel coordinates
Parameters: - pix : tuple
Tuple of scalar pixel coordinates for each non-spatial dimension of the map. Tuple should be ordered as (I_0, …, I_n). Pixel coordinates can be either float or integer type.
Returns: - map_out :
Map
Map with spatial dimensions only.
See also
-
interp_by_coord
(self, coords, interp=None, fill_value=None)¶ Interpolate map values at the given map coordinates.
Parameters: - coords : tuple or
MapCoord
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.
- fill_value : None or float value
The value to use for points outside of the interpolation domain. If None, values outside the domain are extrapolated.
Returns: - vals :
ndarray
Interpolated pixel values.
- coords : tuple or
-
interp_by_pix
(self, pix, interp=None, fill_value=None)¶ Interpolate map values at the given pixel coordinates.
Parameters: - pix : tuple
Tuple of pixel coordinate arrays for each dimension of the map. Tuple should be ordered as (p_lon, p_lat, p_0, …, p_n) where p_i are pixel 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.
- fill_value : None or float value
The value to use for points outside of the interpolation domain. If None, values outside the domain are extrapolated.
Returns: - vals :
ndarray
Interpolated pixel values.
-
iter_by_coord
(self, buffersize=1)¶ 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.
-
iter_by_image
(self)¶ Iterate over image planes of the map returning a tuple with the image array and image plane index.
The image plane index is in data order, so that the data array can be indexed directly. See Iterating on a Map for further information.
Returns: - val :
ndarray
Array of image plane values.
- idx : tuple
Index of image plane.
- val :
-
iter_by_pix
(self, buffersize=1)¶ 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.
-
make_hdu
(self, hdu='SKYMAP', hdu_bands=None, sparse=False, conv=None)[source]¶ 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.
-
pad
(self, pad_width, mode='constant', cval=0, order=1)¶ 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.
-
plot_interactive
(self, rc_params=None, **kwargs)¶ Plot map with interactive widgets to explore the non spatial axes.
Parameters: - rc_params : dict
Passed to
matplotlib.rc_context(rc=rc_params)
to style the plot.- **kwargs : dict
Keyword arguments passed to
WcsNDMap.plot
.
Examples
You can try this out e.g. using a Fermi-LAT diffuse model cube with an energy axis:
from gammapy.maps import Map m = Map.read("$GAMMAPY_DATA/fermi_3fhl/gll_iem_v06_cutout.fits") m.plot_interactive(add_cbar=True, stretch="sqrt")
If you would like to adjust the figure size you can use the
rc_params
argument:rc_params = {'figure.figsize': (12, 6), 'font.size': 12} m.plot_interactive(rc_params=rc_params)
-
static
read
(filename, hdu=None, hdu_bands=None, map_type='auto')¶ Read a map from a FITS file.
Parameters: - filename : str or
Path
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
- filename : str or
-
reproject
(self, geom, order=1, mode='interp')¶ Reproject this map to a different geometry.
Only spatial axes are reprojected, if you would like to reproject non-spatial axes consider using
Map.interp_by_coord()
instead.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.
- geom :
-
set_by_coord
(self, coords, vals)¶ Set pixels at
coords
with givenvals
.Parameters:
-
set_by_idx
(self, idx, vals)¶ Set pixels at
idx
with givenvals
.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.
-
set_by_pix
(self, pix, vals)¶ Set pixels at
pix
with givenvals
.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.
-
slice_by_idx
(self, slices)¶ Slice sub map from map object.
For usage examples, see Indexing and Slicing.
Parameters: - slices : dict
Dict of axes names and integers or
slice
object pairs. Contains one element for each non-spatial dimension. For integer indexing the corresponding axes is dropped from the map. Axes not specified in the dict are kept unchanged.
Returns: - map_out :
Map
Sliced map object.
-
sum_over_axes
(self, keepdims=False)¶ Reduce to a 2D image by summing over non-spatial dimensions.
-
to_hdulist
(self, hdu=None, hdu_bands=None, sparse=False, conv=None)[source]¶ 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
-
upsample
(self, factor, order=0, preserve_counts=True, axis=None)¶ Upsample the spatial dimension 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).
- axis : str
Which axis to upsample. By default spatial axes are upsampled.
Returns: - map :
Map
Upsampled map.
-
write
(self, filename, overwrite=False, **kwargs)¶ Write to a FITS file.
Parameters: - filename : str
Output file name.
- overwrite : bool
Overwrite existing file?
- 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.
-