HpxNDMap¶
-
class
gammapy.maps.
HpxNDMap
(geom, data=None, dtype='float32', meta=None, unit='')[source]¶ Bases:
gammapy.maps.HpxMap
HEALPix map with any number of non-spatial dimensions.
This class uses a N+1D numpy array to represent the sequence of HEALPix image planes. Following the convention of WCS-based maps this class uses a column-wise ordering for the data array with the spatial dimension being tied to the last index of the array.
Parameters: Attributes Summary
data
Data array ( ndarray
)geom
Map geometry ( Geom
)meta
Map meta ( dict
)quantity
Map data times unit ( Quantity
)unit
Map unit ( Unit
)Methods Summary
coadd
(self, map_in[, weights])Add the contents of map_in
to this map.copy
(self, \*\*kwargs)Copy map instance and overwrite given attributes, except for geometry. create
([nside, binsz, nest, map_type, …])Factory method to create an empty HEALPix map. crop
(self, crop_width)Crop the spatial dimensions of the map. downsample
(self, factor[, preserve_counts])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, …])Generate an empty map from a Geom
instance.from_hdu
(hdu[, hdu_bands])Make a HpxNDMap object from a FITS HDU. from_hdulist
(hdu_list[, hdu, hdu_bands])Make a HpxMap 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])Interpolate map values at the given pixel coordinates. iter_by_image
(self)Iterate over image planes of the map. make_hdu
(self[, hdu, hdu_bands, sparse, conv])Make a FITS HDU with input data. make_wcs_mapping
(self[, sum_bands, proj, …])Make a HEALPix to WCS mapping object. pad
(self, pad_width[, mode, cval, order])Pad the spatial dimensions of the map. plot
(self[, method, ax, normalize, proj, …])Quickplot method. 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)Sum over all non-spatial dimensions. to_hdulist
(self[, hdu, hdu_bands, sparse, conv])Convert to HDUList
.to_swapped
(self)Return a new map with the opposite scheme (ring or nested). to_ud_graded
(self, nside[, preserve_counts])Upgrade or downgrade the resolution of the map to the chosen nside. to_wcs
(self[, sum_bands, normalize, proj, …])Make a WCS object and convert HEALPIX data into WCS projection. upsample
(self, factor[, preserve_counts])Upsample the spatial dimension by a given factor. write
(self, filename[, overwrite])Write to a FITS file. Attributes Documentation
Methods Documentation
-
coadd
(self, map_in, weights=None)¶ 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.
- weights: `Map` or `~numpy.ndarray`
The weight factors while adding
- 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
(nside=None, binsz=None, nest=True, map_type='hpx', coordsys='CEL', data=None, skydir=None, width=None, dtype='float32', region=None, axes=None, meta=None, unit='')¶ Factory method to create an empty HEALPix map.
Parameters: - nside : int or
ndarray
HEALPix NSIDE parameter. This parameter sets the size of the spatial pixels in the map.
- binsz : float or
ndarray
Approximate pixel size in degrees. An NSIDE will be chosen that correponds to a pixel size closest to this value. This option is superseded by nside.
- nest : bool
True for HEALPix “NESTED” indexing scheme, False for “RING” scheme.
- coordsys : {‘CEL’, ‘GAL’}, optional
Coordinate system, either Galactic (‘GAL’) or Equatorial (‘CEL’).
- 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.
- map_type : {‘hpx’, ‘hpx-sparse’}
Map type. Selects the class that will be used to instantiate the map.
- width : float
Diameter of the map in degrees. If None then an all-sky geometry will be created.
- axes : list
List of
MapAxis
objects for each non-spatial dimension.- meta :
dict
Dictionary to store meta data.
- unit : str or
Unit
The map unit
Returns: - map :
HpxMap
A HPX map object.
- nside : int or
-
crop
(self, crop_width)[source]¶ Crop the spatial dimensions 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)[source]¶ 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)[source]¶ 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='', dtype='float32')¶ Generate an empty map from a
Geom
instance.Parameters: - geom :
Geom
Map geometry.
- data :
numpy.ndarray
data array
- meta :
dict
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_hdu
(hdu, hdu_bands=None)[source]¶ Make a HpxNDMap object from a FITS HDU.
Parameters: - hdu :
BinTableHDU
The FITS HDU
- hdu_bands :
BinTableHDU
The BANDS table HDU
- hdu :
-
classmethod
from_hdulist
(hdu_list, hdu=None, hdu_bands=None)¶ Make a HpxMap 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. If None then the method will try to load map data from the first BinTableHDU in the file.
- hdu_bands : str
Name or index of the HDU with the BANDS table.
Returns: - hpx_map :
HpxMap
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)[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
-
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=1)[source]¶ 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)[source]¶ Interpolate map values at the given pixel coordinates.
-
iter_by_image
(self)¶ Iterate over image planes of the map.
This is a generator yielding
(data, idx)
tuples, wheredata
is anumpy.ndarray
view of the image plane data, andidx
is a tuple of int, the index of the image plane.The image plane index is in data order, so that the data array can be indexed directly. See Iterating by image for further information.
-
make_hdu
(self, hdu=None, hdu_bands=None, sparse=False, conv=None)¶ Make a FITS HDU with input data.
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.
- 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_out :
BinTableHDU
orImageHDU
Output HDU containing map data.
-
make_wcs_mapping
(self, sum_bands=False, proj='AIT', oversample=2, width_pix=None)[source]¶ Make a HEALPix to WCS mapping object.
Parameters: - sum_bands : bool
sum over non-spatial dimensions before reprojecting
- proj : str
WCS-projection
- oversample : float
Oversampling factor for WCS map. This will be the approximate ratio of the width of a HPX pixel to a WCS pixel. If this parameter is None then the width will be set from
width_pix
.- width_pix : int
Width of the WCS geometry in pixels. The pixel size will be set to the number of pixels satisfying
oversample
orwidth_pix
whichever is smaller. If this parameter is None then the width will be set fromoversample
.
Returns: - hpx2wcs :
HpxToWcsMapping
-
pad
(self, pad_width, mode='constant', cval=0, order=1)[source]¶ Pad the spatial dimensions of the map.
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
(self, method='raster', ax=None, normalize=False, proj='AIT', oversample=2, width_pix=1000, **kwargs)[source]¶ Quickplot method.
This will generate a visualization of the map by converting to a rasterized WCS image (method=’raster’) or drawing polygons for each pixel (method=’poly’).
Parameters: - method : {‘raster’,’poly’}
Method for mapping HEALPix pixels to a two-dimensional image. Can be set to ‘raster’ (rasterization to cartesian image plane) or ‘poly’ (explicit polygons for each pixel). WARNING: The ‘poly’ method is much slower than ‘raster’ and only suitable for maps with less than ~10k pixels.
- proj : string, optional
Any valid WCS projection type.
- oversample : float
Oversampling factor for WCS map. This will be the approximate ratio of the width of a HPX pixel to a WCS pixel. If this parameter is None then the width will be set from
width_pix
.- width_pix : int
Width of the WCS geometry in pixels. The pixel size will be set to the number of pixels satisfying
oversample
orwidth_pix
whichever is smaller. If this parameter is None then the width will be set fromoversample
.- **kwargs : dict
Keyword arguments passed to
imshow
.
Returns: - fig :
Figure
Figure object.
- ax :
WCSAxes
WCS axis object
- im :
AxesImage
orPatchCollection
Image object.
-
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 :
Geom
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)[source]¶ 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)[source]¶ Sum over all non-spatial dimensions.
Returns: - map_out :
HpxNDMap
Summed map.
- map_out :
-
to_hdulist
(self, hdu='SKYMAP', hdu_bands=None, sparse=False, conv='gadf')¶ Convert to
HDUList
.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.
- 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
-
to_swapped
(self)[source]¶ Return a new map with the opposite scheme (ring or nested).
Returns: - map :
HpxMap
Map object.
- map :
-
to_ud_graded
(self, nside, preserve_counts=False)[source]¶ Upgrade or downgrade the resolution of the map to the chosen nside.
Parameters: - nside : int
NSIDE parameter of the new map.
- preserve_counts : bool
Choose whether to preserve counts (total amplitude) or intensity (amplitude per unit solid angle).
Returns: - map :
HpxMap
Map object.
-
to_wcs
(self, sum_bands=False, normalize=True, proj='AIT', oversample=2, width_pix=None, hpx2wcs=None)[source]¶ Make a WCS object and convert HEALPIX data into WCS projection.
Parameters: - sum_bands : bool
Sum over non-spatial axes before reprojecting. If False then the WCS map will have the same dimensionality as the HEALPix one.
- normalize : bool
Preserve integral by splitting HEALPIX values between bins?
- proj : str
WCS-projection
- oversample : float
Oversampling factor for WCS map. This will be the approximate ratio of the width of a HPX pixel to a WCS pixel. If this parameter is None then the width will be set from
width_pix
.- width_pix : int
Width of the WCS geometry in pixels. The pixel size will be set to the number of pixels satisfying
oversample
orwidth_pix
whichever is smaller. If this parameter is None then the width will be set fromoversample
.- hpx2wcs :
HpxToWcsMapping
Set the HPX to WCS mapping object that will be used to generate the WCS map. If none then a new mapping will be generated based on
proj
andoversample
arguments.
Returns: - map_out :
WcsMap
WCS map object.
-
upsample
(self, factor, preserve_counts=True)[source]¶ 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.
-