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 array (
ndarray
)Map geometry (
Geom
)Map meta (
dict
)Map data times unit (
Quantity
)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
.fill_events
(self, events)Fill event coordinates (
EventList
).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.
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
- **kwargsdict
Keyword arguments to overwrite in the map constructor.
- Returns
- copy
Map
Copied Map.
- copy
-
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
- nsideint or
ndarray
HEALPix NSIDE parameter. This parameter sets the size of the spatial pixels in the map.
- binszfloat 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.
- nestbool
True for HEALPix “NESTED” indexing scheme, False for “RING” scheme.
- coordsys{‘CEL’, ‘GAL’}, optional
Coordinate system, either Galactic (‘GAL’) or Equatorial (‘CEL’).
- skydirtuple 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.
- widthfloat
Diameter of the map in degrees. If None then an all-sky geometry will be created.
- axeslist
List of
MapAxis
objects for each non-spatial dimension.- meta
dict
Dictionary to store meta data.
- unitstr or
Unit
The map unit
- nsideint or
- Returns
- map
HpxMap
A HPX map object.
- map
-
downsample
(self, factor, preserve_counts=True)[source]¶ Downsample the spatial dimension by a given factor.
- Parameters
- factorint
Downsampling factor.
- preserve_countsbool
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).
- axisstr
Which axis to downsample. By default spatial axes are downsampled.
- Returns
- map
Map
Downsampled map.
- map
-
fill_by_coord
(self, coords, weights=None)¶ Fill pixels at
coords
with givenweights
.
-
fill_by_idx
(self, idx, weights=None)[source]¶ Fill pixels at
idx
with givenweights
.- Parameters
- idxtuple
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
- pixtuple
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
.- unitstr or
Unit
Data unit.
- geom
- Returns
- map_out
Map
Map object
- map_out
-
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.
- hdustr
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_bandsstr
Name or index of the HDU with the BANDS table.
- hdu_list
- Returns
- hpx_map
HpxMap
Map object
- hpx_map
-
get_by_coord
(self, coords)¶ Return map values at the given map coordinates.
-
get_by_idx
(self, idx)[source]¶ Return map values at the given pixel indices.
- Parameters
- idxtuple
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
- vals
-
get_by_pix
(self, pix)¶ Return map values at the given pixel coordinates.
- Parameters
- pixtuple
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
- vals
-
get_image_by_coord
(self, coords)¶ Return spatial map at the given axis coordinates.
- Parameters
- coordstuple 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.
- map_out
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
- idxtuple
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.
- map_out
See also
-
get_image_by_pix
(self, pix)¶ Return spatial map at the given axis pixel coordinates
- Parameters
- pixtuple
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.
- map_out
See also
-
interp_by_coord
(self, coords, interp=1)[source]¶ Interpolate map values at the given map coordinates.
- Parameters
- coordstuple 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_valueNone or float value
The value to use for points outside of the interpolation domain. If None, values outside the domain are extrapolated.
- coordstuple or
- Returns
- vals
ndarray
Interpolated pixel values.
- vals
-
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
- hdustr
The HDU extension name.
- hdu_bandsstr
The HDU extension name for BANDS table.
- sparsebool
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.
- hdu_out
-
make_wcs_mapping
(self, sum_bands=False, proj='AIT', oversample=2, width_pix=None)[source]¶ Make a HEALPix to WCS mapping object.
- Parameters
- sum_bandsbool
sum over non-spatial dimensions before reprojecting
- projstr
WCS-projection
- oversamplefloat
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_pixint
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
- hpx2wcs
-
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.
- cvalfloat
Padding value when mode=’consant’.
- orderint
Order of interpolation when mode=’constant’ (0 = nearest-neighbor, 1 = linear, 2 = quadratic, 3 = cubic).
- Returns
- map
Map
Padded map.
- 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.
- projstring, optional
Any valid WCS projection type.
- oversamplefloat
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_pixint
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
.- **kwargsdict
Keyword arguments passed to
imshow
.
- Returns
- fig
Figure
Figure object.
- ax
WCSAxes
WCS axis object
- im
AxesImage
orPatchCollection
Image object.
- fig
-
plot_interactive
(self, rc_params=None, **kwargs)¶ Plot map with interactive widgets to explore the non spatial axes.
- Parameters
- rc_paramsdict
Passed to
matplotlib.rc_context(rc=rc_params)
to style the plot.- **kwargsdict
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
- filenamestr or
Path
Name of the FITS file.
- hdustr
Name or index of the HDU with the map data.
- hdu_bandsstr
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.
- filenamestr or
- Returns
- map_out
Map
Map object
- map_out
-
set_by_coord
(self, coords, vals)¶ Set pixels at
coords
with givenvals
.
-
set_by_idx
(self, idx, vals)[source]¶ Set pixels at
idx
with givenvals
.- Parameters
- idxtuple
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
- pixtuple
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.
-
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
- hdustr
The HDU extension name.
- hdu_bandsstr
The HDU extension name for BANDS table.
- sparsebool
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
- hdu_list
-
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
- nsideint
NSIDE parameter of the new map.
- preserve_countsbool
Choose whether to preserve counts (total amplitude) or intensity (amplitude per unit solid angle).
- Returns
- map
HpxMap
Map object.
- map
-
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_bandsbool
Sum over non-spatial axes before reprojecting. If False then the WCS map will have the same dimensionality as the HEALPix one.
- normalizebool
Preserve integral by splitting HEALPIX values between bins?
- projstr
WCS-projection
- oversamplefloat
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_pixint
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.
- map_out
-
upsample
(self, factor, preserve_counts=True)[source]¶ Upsample the spatial dimension by a given factor.
- Parameters
- factorint
Upsampling factor.
- orderint
Order of the interpolation used for upsampling.
- preserve_countsbool
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).
- axisstr
Which axis to upsample. By default spatial axes are upsampled.
- Returns
- map
Map
Upsampled map.
- map
-
write
(self, filename, overwrite=False, **kwargs)¶ Write to a FITS file.
- Parameters
- filenamestr
Output file name.
- overwritebool
Overwrite existing file?
- hdustr
Set the name of the image extension. By default this will be set to SKYMAP (for BINTABLE HDU) or PRIMARY (for IMAGE HDU).
- hdu_bandsstr
Set the name of the bands table extension. By default this will be set to BANDS.
- convstr
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’.
- sparsebool
Sparsify the map by dropping pixels with zero amplitude. This option is only compatible with the ‘gadf’ format.