def test_wcsndmap_fill_by_coord(npix, binsz, coordsys, proj, skydir, axes):
geom = WcsGeom.create(npix=npix,
binsz=binsz,
skydir=skydir,
proj=proj,
coordsys=coordsys,
axes=axes)
m = WcsNDMap(geom)
coords = m.geom.get_coord()
fill_coords = tuple([np.concatenate((t, t)) for t in coords])
fill_vals = fill_coords[1]
m.fill_by_coord(fill_coords, fill_vals)
assert_allclose(m.get_by_coord(coords), 2.0 * coords[1])
# Test with SkyCoords
m = WcsNDMap(geom)
coords = m.geom.get_coord()
skydir = SkyCoord(coords[0],
coords[1],
unit="deg",
frame=coordsys_to_frame(geom.coordsys))
skydir_cel = skydir.transform_to("icrs")
skydir_gal = skydir.transform_to("galactic")
fill_coords_cel = (skydir_cel, ) + tuple(coords[2:])
fill_coords_gal = (skydir_gal, ) + tuple(coords[2:])
m.fill_by_coord(fill_coords_cel, coords[1])
m.fill_by_coord(fill_coords_gal, coords[1])
assert_allclose(m.get_by_coord(coords), 2.0 * coords[1])
def test_wcsndmap_set_get_by_coord(npix, binsz, coordsys, proj, skydir, axes):
geom = WcsGeom.create(npix=npix,
binsz=binsz,
skydir=skydir,
proj=proj,
coordsys=coordsys,
axes=axes)
m = WcsNDMap(geom)
coords = m.geom.get_coord()
m.set_by_coord(coords, coords[0])
assert_allclose(coords[0], m.get_by_coord(coords))
if not geom.is_allsky:
coords[1][...] = 0.0
assert_allclose(np.nan * np.ones(coords[0].shape),
m.get_by_coord(coords))
# Test with SkyCoords
m = WcsNDMap(geom)
coords = m.geom.get_coord()
skydir = SkyCoord(coords[0],
coords[1],
unit="deg",
frame=coordsys_to_frame(geom.coordsys))
skydir_cel = skydir.transform_to("icrs")
skydir_gal = skydir.transform_to("galactic")
m.set_by_coord((skydir_gal, ) + tuple(coords[2:]), coords[0])
assert_allclose(coords[0], m.get_by_coord(coords))
assert_allclose(
m.get_by_coord((skydir_cel, ) + tuple(coords[2:])),
m.get_by_coord((skydir_gal, ) + tuple(coords[2:])),
)
# Test with MapCoord
m = WcsNDMap(geom)
coords = m.geom.get_coord()
coords_dict = dict(lon=coords[0], lat=coords[1])
if axes:
for i, ax in enumerate(axes):
coords_dict[ax.name] = coords[i + 2]
map_coords = MapCoord.create(coords_dict, coordsys=coordsys)
m.set_by_coord(map_coords, coords[0])
assert_allclose(coords[0], m.get_by_coord(map_coords))
def test_hpxmap_set_get_by_coord(nside, nested, coordsys, region, axes):
m = create_map(nside, nested, coordsys, region, axes)
coords = m.geom.get_coord(flat=True)
m.set_by_coord(coords, coords[0])
assert_allclose(coords[0], m.get_by_coord(coords))
# Test with SkyCoords
m = create_map(nside, nested, coordsys, region, axes)
coords = m.geom.get_coord(flat=True)
skydir = SkyCoord(coords[0],
coords[1],
unit="deg",
frame=coordsys_to_frame(m.geom.coordsys))
skydir_cel = skydir.transform_to("icrs")
skydir_gal = skydir.transform_to("galactic")
m.set_by_coord((skydir_gal, ) + tuple(coords[2:]), coords[0])
assert_allclose(coords[0], m.get_by_coord(coords))
assert_allclose(
m.get_by_coord((skydir_cel, ) + tuple(coords[2:])),
m.get_by_coord((skydir_gal, ) + tuple(coords[2:])),
)
def _make_tsmap_fast(self, prefix, **kwargs):
"""
Make a TS map from a GTAnalysis instance. This is a
simplified implementation optimized for speed that only fits
for the source normalization (all background components are
kept fixed). The spectral/spatial characteristics of the test
source can be defined with the src_dict argument. By default
this method will generate a TS map for a point source with an
index=2.0 power-law spectrum.
Parameters
----------
model : dict or `~fermipy.roi_model.Source`
Dictionary or Source object defining the properties of the
test source that will be used in the scan.
"""
loglevel = kwargs.get('loglevel', self.loglevel)
src_dict = copy.deepcopy(kwargs.setdefault('model', {}))
src_dict = {} if src_dict is None else src_dict
multithread = kwargs.setdefault('multithread', False)
threshold = kwargs.setdefault('threshold', 1E-2)
max_kernel_radius = kwargs.get('max_kernel_radius')
loge_bounds = kwargs.setdefault('loge_bounds', None)
use_pylike = kwargs.setdefault('use_pylike', True)
if loge_bounds:
if len(loge_bounds) != 2:
raise Exception('Wrong size of loge_bounds array.')
loge_bounds[0] = (loge_bounds[0] if loge_bounds[0] is not None else
self.log_energies[0])
loge_bounds[1] = (loge_bounds[1] if loge_bounds[1] is not None else
self.log_energies[-1])
else:
loge_bounds = [self.log_energies[0], self.log_energies[-1]]
# Put the test source at the pixel closest to the ROI center
xpix, ypix = (np.round(
(self.npix - 1.0) / 2.), np.round((self.npix - 1.0) / 2.))
cpix = np.array([xpix, ypix])
map_geom = self._geom.to_image()
frame = coordsys_to_frame(map_geom.coordsys)
skydir = SkyCoord(*map_geom.pix_to_coord((cpix[0], cpix[1])),
frame=frame,
unit='deg')
skydir = skydir.transform_to('icrs')
src_dict['ra'] = skydir.ra.deg
src_dict['dec'] = skydir.dec.deg
src_dict.setdefault('SpatialModel', 'PointSource')
src_dict.setdefault('SpatialWidth', 0.3)
src_dict.setdefault('Index', 2.0)
src_dict.setdefault('Prefactor', 1E-13)
counts = []
bkg = []
model = []
c0_map = []
eslices = []
enumbins = []
model_npred = 0
for c in self.components:
imin = utils.val_to_edge(c.log_energies, loge_bounds[0])[0]
imax = utils.val_to_edge(c.log_energies, loge_bounds[1])[0]
eslice = slice(imin, imax)
bm = c.model_counts_map(
exclude=kwargs['exclude']).data.astype('float')[eslice, ...]
cm = c.counts_map().data.astype('float')[eslice, ...]
bkg += [bm]
counts += [cm]
c0_map += [cash(cm, bm)]
eslices += [eslice]
enumbins += [cm.shape[0]]
self.add_source('tsmap_testsource',
src_dict,
free=True,
init_source=False,
use_single_psf=True,
use_pylike=use_pylike,
loglevel=logging.DEBUG)
src = self.roi['tsmap_testsource']
# self.logger.info(str(src_dict))
modelname = utils.create_model_name(src)
for c, eslice in zip(self.components, eslices):
mm = c.model_counts_map('tsmap_testsource').data.astype('float')[
eslice, ...]
model_npred += np.sum(mm)
model += [mm]
self.delete_source('tsmap_testsource', loglevel=logging.DEBUG)
for i, mm in enumerate(model):
dpix = 3
for j in range(mm.shape[0]):
ix, iy = np.unravel_index(np.argmax(mm[j, ...]), mm[j,
...].shape)
mx = mm[j, ix, :] > mm[j, ix, iy] * threshold
my = mm[j, :, iy] > mm[j, ix, iy] * threshold
dpix = max(dpix, np.round(np.sum(mx) / 2.))
dpix = max(dpix, np.round(np.sum(my) / 2.))
if max_kernel_radius is not None and \
dpix > int(max_kernel_radius / self.components[i].binsz):
dpix = int(max_kernel_radius / self.components[i].binsz)
xslice = slice(max(int(xpix - dpix), 0),
min(int(xpix + dpix + 1), self.npix))
model[i] = model[i][:, xslice, xslice]
ts_values = np.zeros((self.npix, self.npix))
amp_values = np.zeros((self.npix, self.npix))
wrap = functools.partial(_ts_value_newton,
counts=counts,
bkg=bkg,
model=model,
C_0_map=c0_map)
if kwargs['map_skydir'] is not None:
map_offset = wcs_utils.skydir_to_pix(kwargs['map_skydir'],
map_geom.wcs)
map_delta = 0.5 * kwargs['map_size'] / self.components[0].binsz
xmin = max(int(np.ceil(map_offset[1] - map_delta)), 0)
xmax = min(int(np.floor(map_offset[1] + map_delta)) + 1, self.npix)
ymin = max(int(np.ceil(map_offset[0] - map_delta)), 0)
ymax = min(int(np.floor(map_offset[0] + map_delta)) + 1, self.npix)
xslice = slice(xmin, xmax)
yslice = slice(ymin, ymax)
xyrange = [range(xmin, xmax), range(ymin, ymax)]
wcs = map_geom.wcs.deepcopy()
npix = (ymax - ymin, xmax - xmin)
crpix = (map_geom._crpix[0] - ymin, map_geom._crpix[1] - xmin)
wcs.wcs.crpix[0] -= ymin
wcs.wcs.crpix[1] -= xmin
# FIXME: We should implement this with a proper cutout method
map_geom = WcsGeom(wcs, npix, crpix=crpix)
else:
xyrange = [range(self.npix), range(self.npix)]
xslice = slice(0, self.npix)
yslice = slice(0, self.npix)
positions = []
for i, j in itertools.product(xyrange[0], xyrange[1]):
p = [[k // 2, i, j] for k in enumbins]
positions += [p]
self.logger.log(loglevel, 'Fitting test source.')
if multithread:
pool = Pool()
results = pool.map(wrap, positions)
pool.close()
pool.join()
else:
results = map(wrap, positions)
for i, r in enumerate(results):
ix = positions[i][0][1]
iy = positions[i][0][2]
ts_values[ix, iy] = r[0]
amp_values[ix, iy] = r[1]
ts_values = ts_values[xslice, yslice]
amp_values = amp_values[xslice, yslice]
ts_map = WcsNDMap(map_geom, ts_values)
sqrt_ts_map = WcsNDMap(map_geom, ts_values**0.5)
npred_map = WcsNDMap(map_geom, amp_values * model_npred)
amp_map = WcsNDMap(map_geom, amp_values * src.get_norm())
o = {
'name': utils.join_strings([prefix, modelname]),
'src_dict': copy.deepcopy(src_dict),
'file': None,
'ts': ts_map,
'sqrt_ts': sqrt_ts_map,
'npred': npred_map,
'amplitude': amp_map,
'loglike': -self.like(),
'config': kwargs
}
return o
def _make_ts_cube(self, prefix, **kwargs):
map_skydir = kwargs.get('map_skydir')
map_size = kwargs.get('map_size')
exclude = kwargs.get('exclude', [])
# We take the coordinate system and the bin size from the underlying map
skywcs = self._geom.wcs
galactic = wcs_utils.is_galactic(skywcs)
pixsize = max(np.abs(skywcs.wcs.cdelt))
# If the map_size is not specified we need to find the right number of pixels
if map_size is None:
npix = max(self._geom.npix)[0]
map_size = pixsize * npix
else:
npix = int(np.round(map_size / pixsize))
saved_state = LikelihoodState(self.like)
for ex_src in exclude:
self.zero_source(ex_src)
if map_skydir is None:
# Take the center of the wcs
map_geom = self._geom.to_image()
frame = coordsys_to_frame(map_geom.coordsys)
map_skydir = SkyCoord(*map_geom.pix_to_coord(
self._geom.wcs.wcs.crpix),
frame=frame,
unit='deg')
map_skydir = map_skydir.transform_to('icrs')
refdir = pyLike.SkyDir(map_skydir.ra.deg, map_skydir.dec.deg)
src_dict = copy.deepcopy(kwargs.setdefault('model', {}))
src_dict = {} if src_dict is None else src_dict
src_dict['ra'] = map_skydir.ra.deg
src_dict['dec'] = map_skydir.dec.deg
src_dict.setdefault('SpatialModel', 'PointSource')
src_dict.setdefault('SpatialWidth', 0.3)
src_dict.setdefault('Index', 2.0)
src_dict.setdefault('Prefactor', 1.0)
src_dict['name'] = 'tscube_testsource'
src = Source.create_from_dict(src_dict)
if 'Prefactor' in src.spectral_pars:
src.spectral_pars['Prefactor']['scale'] = 1.0e-10
modelname = utils.create_model_name(src)
pylike_src = self.components[0]._create_source(src)
pylike_src.spectrum().normPar().setBounds(0, 1E6)
skyproj = pyLike.FitScanner.buildSkyProj(str("AIT"), refdir, pixsize,
npix, galactic)
optFactory = pyLike.OptimizerFactory_instance()
optObject = optFactory.create(str("MINUIT"), self.like.composite)
fitScanner = pyLike.FitScanner(self.like.composite, optObject, skyproj,
npix, npix)
fitScanner.set_quiet(True)
fitScanner.setTestSource(pylike_src)
self.logger.info("Running tscube")
outfile = utils.format_filename(self.config['fileio']['workdir'],
'tscube.fits',
prefix=[prefix])
fitScanner.run_tscube(True, kwargs['do_sed'], kwargs['nnorm'],
kwargs['norm_sigma'], kwargs['cov_scale_bb'],
kwargs['cov_scale'], kwargs['tol'],
kwargs['max_iter'], kwargs['tol_type'],
kwargs['remake_test_source'],
kwargs['st_scan_level'], str(''),
kwargs['init_lambda'])
self.logger.info("Writing FITS output")
fitScanner.writeFitsFile(str(outfile), str("gttscube"), "", False,
pyLike.FitScanner.TSMAP_ONLY)
saved_state.restore()
convert_tscube(str(outfile), str(outfile))
tscube = castro.TSCube.create_from_fits(outfile)
ts_map = tscube.tsmap
norm_map = tscube.normmap
npred_map = copy.deepcopy(norm_map)
npred_map.data *= tscube.refSpec.ref_npred.sum()
amp_map = copy.deepcopy(norm_map)
amp_map.data *= pylike_src.spectrum().normPar().getValue()
sqrt_ts_map = copy.deepcopy(ts_map)
sqrt_ts_map.data[...] = np.abs(sqrt_ts_map.data)**0.5
o = {
'name': utils.join_strings([prefix, modelname]),
'src_dict': copy.deepcopy(src_dict),
'file': os.path.basename(outfile),
'ts': ts_map,
'sqrt_ts': sqrt_ts_map,
'npred': npred_map,
'amplitude': amp_map,
'config': kwargs,
'tscube': tscube
}
if not kwargs['write_fits']:
os.remove(outfile)
o['file'] = None
self.logger.info("Done")
return o
def _make_tsmap_fast(self, prefix, **kwargs):
"""
Make a TS map from a GTAnalysis instance. This is a
simplified implementation optimized for speed that only fits
for the source normalization (all background components are
kept fixed). The spectral/spatial characteristics of the test
source can be defined with the src_dict argument. By default
this method will generate a TS map for a point source with an
index=2.0 power-law spectrum.
Parameters
----------
model : dict or `~fermipy.roi_model.Source`
Dictionary or Source object defining the properties of the
test source that will be used in the scan.
"""
loglevel = kwargs.get('loglevel', self.loglevel)
src_dict = copy.deepcopy(kwargs.setdefault('model', {}))
src_dict = {} if src_dict is None else src_dict
multithread = kwargs.setdefault('multithread', False)
threshold = kwargs.setdefault('threshold', 1E-2)
max_kernel_radius = kwargs.get('max_kernel_radius')
loge_bounds = kwargs.setdefault('loge_bounds', None)
use_pylike = kwargs.setdefault('use_pylike', True)
if loge_bounds:
if len(loge_bounds) != 2:
raise Exception('Wrong size of loge_bounds array.')
loge_bounds[0] = (loge_bounds[0] if loge_bounds[0] is not None
else self.log_energies[0])
loge_bounds[1] = (loge_bounds[1] if loge_bounds[1] is not None
else self.log_energies[-1])
else:
loge_bounds = [self.log_energies[0], self.log_energies[-1]]
# Put the test source at the pixel closest to the ROI center
xpix, ypix = (np.round((self.npix - 1.0) / 2.),
np.round((self.npix - 1.0) / 2.))
cpix = np.array([xpix, ypix])
map_geom = self._geom.to_image()
frame = coordsys_to_frame(map_geom.coordsys)
skydir = SkyCoord(*map_geom.pix_to_coord((cpix[0], cpix[1])),
frame=frame, unit='deg')
skydir = skydir.transform_to('icrs')
src_dict['ra'] = skydir.ra.deg
src_dict['dec'] = skydir.dec.deg
src_dict.setdefault('SpatialModel', 'PointSource')
src_dict.setdefault('SpatialWidth', 0.3)
src_dict.setdefault('Index', 2.0)
src_dict.setdefault('Prefactor', 1E-13)
counts = []
bkg = []
model = []
c0_map = []
eslices = []
enumbins = []
model_npred = 0
for c in self.components:
imin = utils.val_to_edge(c.log_energies, loge_bounds[0])[0]
imax = utils.val_to_edge(c.log_energies, loge_bounds[1])[0]
eslice = slice(imin, imax)
bm = c.model_counts_map(exclude=kwargs['exclude']).data.astype('float')[
eslice, ...]
cm = c.counts_map().data.astype('float')[eslice, ...]
bkg += [bm]
counts += [cm]
c0_map += [cash(cm, bm)]
eslices += [eslice]
enumbins += [cm.shape[0]]
self.add_source('tsmap_testsource', src_dict, free=True,
init_source=False, use_single_psf=True,
use_pylike=use_pylike,
loglevel=logging.DEBUG)
src = self.roi['tsmap_testsource']
# self.logger.info(str(src_dict))
modelname = utils.create_model_name(src)
for c, eslice in zip(self.components, eslices):
mm = c.model_counts_map('tsmap_testsource').data.astype('float')[
eslice, ...]
model_npred += np.sum(mm)
model += [mm]
self.delete_source('tsmap_testsource', loglevel=logging.DEBUG)
for i, mm in enumerate(model):
dpix = 3
for j in range(mm.shape[0]):
ix, iy = np.unravel_index(
np.argmax(mm[j, ...]), mm[j, ...].shape)
mx = mm[j, ix, :] > mm[j, ix, iy] * threshold
my = mm[j, :, iy] > mm[j, ix, iy] * threshold
dpix = max(dpix, np.round(np.sum(mx) / 2.))
dpix = max(dpix, np.round(np.sum(my) / 2.))
if max_kernel_radius is not None and \
dpix > int(max_kernel_radius / self.components[i].binsz):
dpix = int(max_kernel_radius / self.components[i].binsz)
xslice = slice(max(int(xpix - dpix), 0),
min(int(xpix + dpix + 1), self.npix))
model[i] = model[i][:, xslice, xslice]
ts_values = np.zeros((self.npix, self.npix))
amp_values = np.zeros((self.npix, self.npix))
wrap = functools.partial(_ts_value_newton, counts=counts,
bkg=bkg, model=model,
C_0_map=c0_map)
if kwargs['map_skydir'] is not None:
map_offset = wcs_utils.skydir_to_pix(kwargs['map_skydir'],
map_geom.wcs)
map_delta = 0.5 * kwargs['map_size'] / self.components[0].binsz
xmin = max(int(np.ceil(map_offset[1] - map_delta)), 0)
xmax = min(int(np.floor(map_offset[1] + map_delta)) + 1, self.npix)
ymin = max(int(np.ceil(map_offset[0] - map_delta)), 0)
ymax = min(int(np.floor(map_offset[0] + map_delta)) + 1, self.npix)
xslice = slice(xmin, xmax)
yslice = slice(ymin, ymax)
xyrange = [range(xmin, xmax), range(ymin, ymax)]
wcs = map_geom.wcs.deepcopy()
npix = (ymax - ymin, xmax - xmin)
crpix = (map_geom._crpix[0] - ymin, map_geom._crpix[1] - xmin)
wcs.wcs.crpix[0] -= ymin
wcs.wcs.crpix[1] -= xmin
# FIXME: We should implement this with a proper cutout method
map_geom = WcsGeom(wcs, npix, crpix=crpix)
else:
xyrange = [range(self.npix), range(self.npix)]
xslice = slice(0, self.npix)
yslice = slice(0, self.npix)
positions = []
for i, j in itertools.product(xyrange[0], xyrange[1]):
p = [[k // 2, i, j] for k in enumbins]
positions += [p]
self.logger.log(loglevel, 'Fitting test source.')
if multithread:
pool = Pool()
results = pool.map(wrap, positions)
pool.close()
pool.join()
else:
results = map(wrap, positions)
for i, r in enumerate(results):
ix = positions[i][0][1]
iy = positions[i][0][2]
ts_values[ix, iy] = r[0]
amp_values[ix, iy] = r[1]
ts_values = ts_values[xslice, yslice]
amp_values = amp_values[xslice, yslice]
ts_map = WcsNDMap(map_geom, ts_values)
sqrt_ts_map = WcsNDMap(map_geom, ts_values**0.5)
npred_map = WcsNDMap(map_geom, amp_values * model_npred)
amp_map = WcsNDMap(map_geom, amp_values * src.get_norm())
o = {'name': utils.join_strings([prefix, modelname]),
'src_dict': copy.deepcopy(src_dict),
'file': None,
'ts': ts_map,
'sqrt_ts': sqrt_ts_map,
'npred': npred_map,
'amplitude': amp_map,
'loglike': -self.like(),
'config': kwargs
}
return o
