def calculate_sf_from_screen(screen):
""" Calculate structure function image from screen
Screen axes are ['XX', 'YY', 'TIME', 'FREQ']
:param screen:
:return:
"""
from scipy.signal import fftconvolve
nchan, ntimes, ny, nx = screen.data.shape
sf = numpy.zeros([nchan, 1, 2 * ny - 1, 2 * nx - 1])
for chan in range(nchan):
sf[chan, 0, ...] = fftconvolve(screen.data[chan, 0, ...],
screen.data[chan, 0, ::-1, ::-1])
for itime in range(ntimes):
sf += fftconvolve(screen.data[chan, itime, ...],
screen.data[chan, itime, ::-1, ::-1])
sf[chan, 0, ...] /= numpy.max(sf[chan, 0, ...])
sf[chan, 0, ...] = 1.0 - sf[chan, 0, ...]
sf_image = copy_image(screen)
sf_image.data = sf[:, :, (ny - ny // 4):(ny + ny // 4),
(nx - nx // 4):(nx + nx // 4)]
sf_image.wcs.wcs.crpix[0] = ny // 4 + 1
sf_image.wcs.wcs.crpix[1] = ny // 4 + 1
sf_image.wcs.wcs.crpix[2] = 1
return sf_image
def sum_invert_results(image_list):
""" Sum a set of invert results with appropriate weighting
:param image_list: List of [image, sum weights] pairs
:return: image, sum of weights
"""
if len(image_list) == 1:
return image_list[0]
first = True
sumwt = 0.0
im = None
for i, arg in enumerate(image_list):
if arg is not None:
if isinstance(arg[1], numpy.ndarray):
scale = arg[1][..., numpy.newaxis, numpy.newaxis]
else:
scale = arg[1]
if first:
im = copy_image(arg[0])
im.data *= scale
sumwt = arg[1]
first = False
else:
im.data += scale * arg[0].data
sumwt += arg[1]
assert not first, "No invert results"
im = normalize_sumwt(im, sumwt)
return im, sumwt
def test_calculate_image_frequency_moments(self):
frequency = numpy.linspace(0.9e8, 1.1e8, 9)
cube = create_low_test_image_from_gleam(npixel=512,
cellsize=0.0001,
frequency=frequency,
flux_limit=1.0)
log.debug(
export_image_to_fits(cube,
fitsfile='%s/test_moments_cube.fits' %
(self.dir)))
original_cube = copy_image(cube)
moment_cube = calculate_image_frequency_moments(cube, nmoment=3)
log.debug(
export_image_to_fits(moment_cube,
fitsfile='%s/test_moments_moment_cube.fits' %
(self.dir)))
reconstructed_cube = calculate_image_from_frequency_moments(
cube, moment_cube)
log.debug(
export_image_to_fits(
reconstructed_cube,
fitsfile='%s/test_moments_reconstructed_cube.fits' %
(self.dir)))
error = numpy.std(reconstructed_cube.data - original_cube.data)
assert error < 0.2
def invert_ng(bvis: BlockVisibility,
model: Image,
dopsf: bool = False,
normalize: bool = True,
**kwargs) -> (Image, numpy.ndarray):
""" Invert using nifty-gridder module
https://gitlab.mpcdf.mpg.de/ift/nifty_gridder
Use the image im as a template. Do PSF in a separate call.
This is at the bottom of the layering i.e. all transforms are eventually expressed in terms
of this function. . Any shifting needed is performed here.
:param bvis: BlockVisibility to be inverted
:param im: image template (not changed)
:param normalize: Normalize by the sum of weights (True)
:return: (resulting image, sum of the weights for each frequency and polarization)
"""
assert isinstance(bvis, BlockVisibility), bvis
im = copy_image(model)
nthreads = get_parameter(kwargs, "threads", 4)
epsilon = get_parameter(kwargs, "epsilon", 1e-12)
do_wstacking = get_parameter(kwargs, "do_wstacking", True)
verbosity = get_parameter(kwargs, "verbosity", 0)
sbvis = copy_visibility(bvis)
sbvis = shift_vis_to_image(sbvis, im, tangent=True, inverse=False)
vis = bvis.vis
freq = sbvis.frequency # frequency, Hz
nrows, nants, _, vnchan, vnpol = vis.shape
uvw = sbvis.uvw.reshape([nrows * nants * nants, 3])
ms = vis.reshape([nrows * nants * nants, vnchan, vnpol])
wgt = sbvis.imaging_weight.reshape(
[nrows * nants * nants, vnchan, vnpol])
if dopsf:
ms[...] = 1.0 + 0.0j
if epsilon > 5.0e-6:
ms = ms.astype("c8")
wgt = wgt.astype("f4")
# Find out the image size/resolution
npixdirty = im.nwidth
pixsize = numpy.abs(numpy.radians(im.wcs.wcs.cdelt[0]))
fuvw = uvw.copy()
# We need to flip the u and w axes.
fuvw[:, 0] *= -1.0
fuvw[:, 2] *= -1.0
nchan, npol, ny, nx = im.shape
im.data[...] = 0.0
sumwt = numpy.zeros([nchan, npol])
ms = convert_pol_frame(ms,
bvis.polarisation_frame,
im.polarisation_frame,
polaxis=2)
# There's a latent problem here with the weights.
# wgt = numpy.real(convert_pol_frame(wgt, bvis.polarisation_frame, im.polarisation_frame, polaxis=2))
# Set up the conversion from visibility channels to image channels
vis_to_im = numpy.round(model.wcs.sub([4]).wcs_world2pix(
freq, 0)[0]).astype('int')
for vchan in range(vnchan):
ichan = vis_to_im[vchan]
for pol in range(npol):
# Nifty gridder likes to receive contiguous arrays
ms_1d = numpy.array([
ms[row, vchan:vchan + 1, pol]
for row in range(nrows * nants * nants)
],
dtype='complex')
ms_1d.reshape([ms_1d.shape[0], 1])
wgt_1d = numpy.array([
wgt[row, vchan:vchan + 1, pol]
for row in range(nrows * nants * nants)
])
wgt_1d.reshape([wgt_1d.shape[0], 1])
dirty = ng.ms2dirty(fuvw,
freq[vchan:vchan + 1],
ms_1d,
wgt_1d,
npixdirty,
npixdirty,
pixsize,
pixsize,
epsilon,
do_wstacking=do_wstacking,
nthreads=nthreads,
verbosity=verbosity)
sumwt[ichan, pol] += numpy.sum(wgt[:, vchan, pol])
im.data[ichan, pol] += dirty.T
if normalize:
im = normalize_sumwt(im, sumwt)
return im, sumwt
def ingest_visibility(self,
freq=None,
chan_width=None,
times=None,
add_errors=False,
block=True,
bandpass=False):
if freq is None:
freq = [1e8]
if chan_width is None:
chan_width = [1e6]
if times is None:
times = (numpy.pi / 12.0) * numpy.linspace(-3.0, 3.0, 5)
lowcore = create_named_configuration('LOWBD2', rmax=750.0)
frequency = numpy.array(freq)
channel_bandwidth = numpy.array(chan_width)
phasecentre = SkyCoord(ra=+180.0 * u.deg,
dec=-60.0 * u.deg,
frame='icrs',
equinox='J2000')
if block:
vt = create_blockvisibility(
lowcore,
times,
frequency,
channel_bandwidth=channel_bandwidth,
weight=1.0,
phasecentre=phasecentre,
polarisation_frame=PolarisationFrame("stokesI"))
else:
vt = create_visibility(
lowcore,
times,
frequency,
channel_bandwidth=channel_bandwidth,
weight=1.0,
phasecentre=phasecentre,
polarisation_frame=PolarisationFrame("stokesI"))
cellsize = 0.001
model = create_image_from_visibility(
vt,
npixel=self.npixel,
cellsize=cellsize,
npol=1,
frequency=frequency,
phasecentre=phasecentre,
polarisation_frame=PolarisationFrame("stokesI"))
nchan = len(self.frequency)
flux = numpy.array(nchan * [[100.0]])
facets = 4
rpix = model.wcs.wcs.crpix - 1.0
spacing_pixels = self.npixel // facets
centers = [-1.5, -0.5, 0.5, 1.5]
comps = list()
for iy in centers:
for ix in centers:
p = int(round(rpix[0] + ix * spacing_pixels * numpy.sign(model.wcs.wcs.cdelt[0]))), \
int(round(rpix[1] + iy * spacing_pixels * numpy.sign(model.wcs.wcs.cdelt[1])))
sc = pixel_to_skycoord(p[0], p[1], model.wcs, origin=1)
comp = create_skycomponent(
direction=sc,
flux=flux,
frequency=frequency,
polarisation_frame=PolarisationFrame("stokesI"))
comps.append(comp)
if block:
predict_skycomponent_visibility(vt, comps)
else:
predict_skycomponent_visibility(vt, comps)
insert_skycomponent(model, comps)
self.comps = comps
self.model = copy_image(model)
self.empty_model = create_empty_image_like(model)
export_image_to_fits(
model, '%s/test_pipeline_functions_model.fits' % (self.dir))
if add_errors:
# These will be the same for all calls
numpy.random.seed(180555)
gt = create_gaintable_from_blockvisibility(vt)
gt = simulate_gaintable(gt, phase_error=1.0, amplitude_error=0.0)
vt = apply_gaintable(vt, gt)
if bandpass:
bgt = create_gaintable_from_blockvisibility(vt, timeslice=1e5)
bgt = simulate_gaintable(bgt,
phase_error=0.01,
amplitude_error=0.01,
smooth_channels=4)
vt = apply_gaintable(vt, bgt)
return vt