Example #1
0
    def test_fill_pswf_to_convolutionfunction(self):
        oversampling = 8
        support = 6
        gcf, cf = create_pswf_convolutionfunction(self.image,
                                                  oversampling=oversampling,
                                                  support=support)
        assert numpy.max(numpy.abs(cf.data)) > 0.0
        if self.persist:
            export_image_to_fits(
                gcf, "%s/test_convolutionfunction_pswf_gcf.fits" % self.dir)

        cf_image = convert_convolutionfunction_to_image(cf)
        cf_image.data = numpy.real(cf_image.data)
        if self.persist:
            export_image_to_fits(
                cf_image,
                "%s/test_convolutionfunction_pwsf_cf.fits" % self.dir)

        peak_location = numpy.unravel_index(numpy.argmax(numpy.abs(cf.data)),
                                            cf.shape)
        assert numpy.abs(cf.data[peak_location] - 0.1871722034219655 +
                         0j) < 1e-7, cf.data[peak_location]

        assert peak_location == (0, 0, 0, 4, 4, 3, 3), peak_location
        u_peak, v_peak = cf.grid_wcs.sub([1, 2]).wcs_pix2world(
            peak_location[-2], peak_location[-1], 0)
        assert numpy.abs(u_peak) < 1e-7, u_peak
        assert numpy.abs(v_peak) < 1e-7, u_peak
def weight_blockvisibility(vis,
                           model,
                           gcfcf=None,
                           weighting="uniform",
                           robustness=0.0,
                           **kwargs):
    """ Weight the visibility data

    This is done collectively so the weights are summed over all vis_lists and then
    corrected

    :param vis_list:
    :param model_imagelist: Model required to determine weighting parameters
    :param weighting: Type of weighting
    :param kwargs: Parameters for functions in graphs
    :return: List of vis_graphs
   """

    assert isinstance(vis, BlockVisibility), vis
    assert image_is_canonical(model)

    if gcfcf is None:
        gcfcf = create_pswf_convolutionfunction(model)

    griddata = create_griddata_from_image(model, vis)
    griddata, sumwt = grid_blockvisibility_weight_to_griddata(
        vis, griddata, gcfcf[1])
    vis = griddata_blockvisibility_reweight(vis,
                                            griddata,
                                            gcfcf[1],
                                            weighting=weighting,
                                            robustness=robustness)
    return vis
Example #3
0
def invert_2d(vis: Visibility,
              im: Image,
              dopsf: bool = False,
              normalize: bool = True,
              gcfcf=None,
              **kwargs) -> (Image, numpy.ndarray):
    """ Invert using 2D convolution function, using the specified convolution function

    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 vis: Visibility to be inverted
    :param im: image template (not changed)
    :param dopsf: Make the psf instead of the dirty image
    :param normalize: Normalize by the sum of weights (True)
    :param gcfcf: (Grid correction function i.e. in image space, Convolution function i.e. in uv space)
    :return: resulting image

    """
    assert isinstance(vis, Visibility), vis

    svis = copy_visibility(vis)

    if dopsf:
        svis.data['vis'][...] = 1.0 + 0.0j

    svis = shift_vis_to_image(svis, im, tangent=True, inverse=False)

    if gcfcf is None:
        gcf, cf = create_pswf_convolutionfunction(
            im,
            support=get_parameter(kwargs, "support", 6),
            oversampling=get_parameter(kwargs, "oversampling", 128))
    else:
        gcf, cf = gcfcf

    griddata = create_griddata_from_image(im)
    griddata, sumwt = grid_visibility_to_griddata(svis,
                                                  griddata=griddata,
                                                  cf=cf)

    imaginary = get_parameter(kwargs, "imaginary", False)
    if imaginary:
        result0, result1 = fft_griddata_to_image(griddata,
                                                 gcf,
                                                 imaginary=imaginary)
        log.debug("invert_2d: retaining imaginary part of dirty image")
        if normalize:
            result0 = normalize_sumwt(result0, sumwt)
            result1 = normalize_sumwt(result1, sumwt)
        return result0, sumwt, result1
    else:
        result = fft_griddata_to_image(griddata, gcf)
        if normalize:
            result = normalize_sumwt(result, sumwt)
        return result, sumwt
Example #4
0
 def test_griddata_predict_pswf(self):
     self.actualSetUp(zerow=True)
     gcf, cf = create_pswf_convolutionfunction(self.model,
                                               support=6,
                                               oversampling=256)
     griddata = create_griddata_from_image(self.model)
     griddata = fft_image_to_griddata(self.model, griddata, gcf)
     newvis = degrid_visibility_from_griddata(self.vis,
                                              griddata=griddata,
                                              cf=cf)
     newvis.data['vis'][...] -= self.vis.data['vis'][...]
     qa = qa_visibility(newvis)
     assert qa.data['rms'] < 0.7, str(qa)
Example #5
0
 def test_griddata_invert_pswf_w(self):
     self.actualSetUp(zerow=False)
     gcf, cf = create_pswf_convolutionfunction(self.model)
     griddata = create_griddata_from_image(self.model, self.vis)
     griddata, sumwt = grid_visibility_to_griddata(self.vis,
                                                   griddata=griddata,
                                                   cf=cf)
     cim = fft_griddata_to_image(griddata, gcf)
     cim = normalize_sumwt(cim, sumwt)
     im = convert_polimage_to_stokes(cim)
     if self.persist:
         export_image_to_fits(
             im, '%s/test_gridding_dirty_pswf_w.fits' % self.dir)
     self.check_peaks(im, 97.13240718331633, tol=1e-7)
Example #6
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 def test_griddata_invert_pswf_stokesIQ(self):
     self.actualSetUp(zerow=True, image_pol=PolarisationFrame("stokesIQ"))
     gcf, cf = create_pswf_convolutionfunction(self.model)
     griddata = create_griddata_from_image(self.model, self.vis)
     griddata, sumwt = grid_visibility_to_griddata(self.vis,
                                                   griddata=griddata,
                                                   cf=cf)
     cim = fft_griddata_to_image(griddata, gcf)
     cim = normalize_sumwt(cim, sumwt)
     im = convert_polimage_to_stokes(cim)
     if self.persist:
         export_image_to_fits(im,
                              '%s/test_gridding_dirty_pswf.fits' % self.dir)
     self.check_peaks(im, 97.10594988491545, tol=1e-7)
Example #7
0
 def test_griddata_invert_pswf_w(self):
     self.actualSetUp(zerow=False)
     gcf, cf = create_pswf_convolutionfunction(self.model,
                                               support=6,
                                               oversampling=32)
     griddata = create_griddata_from_image(self.model)
     griddata, sumwt = grid_visibility_to_griddata(self.vis,
                                                   griddata=griddata,
                                                   cf=cf)
     im = fft_griddata_to_image(griddata, gcf)
     im = normalize_sumwt(im, sumwt)
     if self.persist:
         export_image_to_fits(
             im, '%s/test_gridding_dirty_pswf_w.fits' % self.dir)
     self.check_peaks(im, 97.01838776845877, tol=1e-7)
Example #8
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 def test_griddata_predict_pswf(self):
     self.actualSetUp(zerow=True, image_pol=PolarisationFrame("stokesIQUV"))
     gcf, cf = create_pswf_convolutionfunction(self.model,
                                               support=8,
                                               oversampling=255)
     modelIQUV = convert_stokes_to_polimage(self.model,
                                            self.vis.polarisation_frame)
     griddata = create_griddata_from_image(modelIQUV, self.vis)
     griddata = fft_image_to_griddata(modelIQUV, griddata, gcf)
     newvis = degrid_visibility_from_griddata(self.vis,
                                              griddata=griddata,
                                              cf=cf)
     newvis.data['vis'][...] -= self.vis.data['vis'][...]
     qa = qa_visibility(newvis)
     assert qa.data['rms'] < 1.06, str(qa)
Example #9
0
 def test_griddata_visibility_weight_IQ(self):
     self.actualSetUp(zerow=True, image_pol=PolarisationFrame("stokesIQUV"))
     gcf, cf = create_pswf_convolutionfunction(self.model)
     gd = create_griddata_from_image(self.model, self.vis)
     gd_list = [
         grid_visibility_weight_to_griddata(self.vis, gd, cf)
         for i in range(10)
     ]
     gd, sumwt = griddata_merge_weights(gd_list, algorithm='uniform')
     self.vis = griddata_visibility_reweight(self.vis, gd, cf)
     gd, sumwt = grid_visibility_to_griddata(self.vis, griddata=gd, cf=cf)
     cim = fft_griddata_to_image(gd, gcf)
     cim = normalize_sumwt(cim, sumwt)
     im = convert_polimage_to_stokes(cim)
     if self.persist:
         export_image_to_fits(
             im, '%s/test_gridding_dirty_2d_IQ_uniform.fits' % self.dir)
     self.check_peaks(im, 99.40822097133994)
Example #10
0
def predict_2d(vis: Union[BlockVisibility, Visibility],
               model: Image,
               gcfcf=None,
               **kwargs) -> Union[BlockVisibility, Visibility]:
    """ Predict using convolutional degridding.

    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 vis: Visibility to be predicted
    :param model: model image
    :param gcfcf: (Grid correction function i.e. in image space, Convolution function i.e. in uv space)
    :return: resulting visibility (in place works)
    """

    if model is None:
        return vis

    assert isinstance(vis, Visibility) or isinstance(vis, BlockVisibility), vis

    _, _, ny, nx = model.data.shape

    if gcfcf is None:
        gcf, cf = create_pswf_convolutionfunction(
            model,
            support=get_parameter(kwargs, "support", 8),
            oversampling=get_parameter(kwargs, "oversampling", 127))
    else:
        gcf, cf = gcfcf

    griddata = create_griddata_from_image(model, vis)
    polmodel = convert_stokes_to_polimage(model, vis.polarisation_frame)
    griddata = fft_image_to_griddata(polmodel, griddata, gcf)
    if isinstance(vis, Visibility):
        vis = degrid_visibility_from_griddata(vis, griddata=griddata, cf=cf)
    else:
        vis = degrid_blockvisibility_from_griddata(vis,
                                                   griddata=griddata,
                                                   cf=cf)

    # Now we can shift the visibility from the image frame to the original visibility frame
    svis = shift_vis_to_image(vis, model, tangent=True, inverse=True)

    return svis
Example #11
0
 def test_griddata_blockvisibility_weight(self):
     self.actualSetUp(zerow=True,
                      block=True,
                      image_pol=PolarisationFrame("stokesIQUV"))
     gcf, cf = create_pswf_convolutionfunction(self.model)
     gd = create_griddata_from_image(self.model, self.vis)
     gd_list = [
         grid_blockvisibility_weight_to_griddata(self.vis, gd, cf)
         for i in range(10)
     ]
     assert numpy.max(numpy.abs(gd_list[0][0].data)) > 10.0
     gd, sumwt = griddata_merge_weights(gd_list, algorithm='uniform')
     self.vis = griddata_blockvisibility_reweight(self.vis, gd, cf)
     gd, sumwt = grid_blockvisibility_to_griddata(self.vis,
                                                  griddata=gd,
                                                  cf=cf)
     cim = fft_griddata_to_image(gd, gcf)
     cim = normalize_sumwt(cim, sumwt)
     im = convert_polimage_to_stokes(cim)
     if self.persist:
         export_image_to_fits(
             im, '%s/test_gridding_dirty_2d_uniform_block.fits' % self.dir)
     self.check_peaks(im, 100.13540418821904)