autolens/model/inversion/convolution.py
def convolve_mapping_matrix(self, mapping_matrix):
        """For a given inversion mapping matrix, convolve every pixel's mapped regular with the PSF kernel.

        A mapping matrix provides non-zero entries in all elements which map two pixels to one another
        (see *inversions.mappers*).

        For example, lets take an regular which is masked using a 'cross' of 5 pixels:

        [[ True, False,  True]],
        [[False, False, False]],
        [[ True, False,  True]]

        As example mapping matrix of this cross is as follows (5 regular pixels x 3 source pixels):

        [1, 0, 0] [0->0]
        [1, 0, 0] [1->0]
        [0, 1, 0] [2->1]
        [0, 1, 0] [3->1]
        [0, 0, 1] [4->2]

        For each source-pixel, we can create an regular of its unit-surface brightnesses by mapping the non-zero
        entries back to masks. For example, doing this for source pixel 1 gives:

        [[0.0, 1.0, 0.0]],
        [[1.0, 0.0, 0.0]]
        [[0.0, 0.0, 0.0]]

        And source pixel 2:

        [[0.0, 0.0, 0.0]],
        [[0.0, 1.0, 1.0]]
        [[0.0, 0.0, 0.0]]

        We then convolve each of these regular with our PSF kernel, in 2 dimensions, like we would a normal regular. For
        example, using the kernel below:

        kernel:

        [[0.0, 0.1, 0.0]]
        [[0.1, 0.6, 0.1]]
        [[0.0, 0.1, 0.0]]

        Blurred Source Pixel 1 (we don't need to perform the convolution into masked pixels):

        [[0.0, 0.6, 0.0]],
        [[0.6, 0.0, 0.0]],
        [[0.0, 0.0, 0.0]]

        Blurred Source pixel 2:

        [[0.0, 0.0, 0.0]],
        [[0.0, 0.7, 0.7]],
        [[0.0, 0.0, 0.0]]

        Finally, we map each of these blurred regular back to a blurred mapping matrix, which is analogous to the
        mapping matrix.

        [0.6, 0.0, 0.0] [0->0]
        [0.6, 0.0, 0.0] [1->0]
        [0.0, 0.7, 0.0] [2->1]
        [0.0, 0.7, 0.0] [3->1]
        [0.0, 0.0, 0.6] [4->2]

        If the mapping matrix is sub-gridded, we perform the convolution on the fractional surface brightnesses in an
        identical fashion to above.

        Parameters
        -----------
        mapping_matrix : ndarray
            The 2D mapping matix describing how every inversion pixel maps to an datas_ pixel.
        """
        return self.convolve_matrix_jit(mapping_matrix, self.image_frame_indexes,
                                        self.image_frame_psfs, self.image_frame_lengths)
def convolve_mapping_matrix(self, mapping_matrix):
        """For a given inversion mapping matrix, convolve every pixel's mapped regular with the PSF kernel.

        A mapping matrix provides non-zero entries in all elements which map two pixels to one another
        (see *inversions.mappers*).

        For example, lets take an regular which is masked using a 'cross' of 5 pixels:

        [[ True, False,  True]],
        [[False, False, False]],
        [[ True, False,  True]]

        As example mapping matrix of this cross is as follows (5 regular pixels x 3 source pixels):

        [1, 0, 0] [0->0]
        [1, 0, 0] [1->0]
        [0, 1, 0] [2->1]
        [0, 1, 0] [3->1]
        [0, 0, 1] [4->2]

        For each source-pixel, we can create an regular of its unit-surface brightnesses by mapping the non-zero
        entries back to masks. For example, doing this for source pixel 1 gives:

        [[0.0, 1.0, 0.0]],
        [[1.0, 0.0, 0.0]]
        [[0.0, 0.0, 0.0]]

        And source pixel 2:

        [[0.0, 0.0, 0.0]],
        [[0.0, 1.0, 1.0]]
        [[0.0, 0.0, 0.0]]

        We then convolve each of these regular with our PSF kernel, in 2 dimensions, like we would a normal regular. For
        example, using the kernel below:

        kernel:

        [[0.0, 0.1, 0.0]]
        [[0.1, 0.6, 0.1]]
        [[0.0, 0.1, 0.0]]

        Blurred Source Pixel 1 (we don't need to perform the convolution into masked pixels):

        [[0.0, 0.6, 0.0]],
        [[0.6, 0.0, 0.0]],
        [[0.0, 0.0, 0.0]]

        Blurred Source pixel 2:

        [[0.0, 0.0, 0.0]],
        [[0.0, 0.7, 0.7]],
        [[0.0, 0.0, 0.0]]

        Finally, we map each of these blurred regular back to a blurred mapping matrix, which is analogous to the
        mapping matrix.

        [0.6, 0.0, 0.0] [0->0]
        [0.6, 0.0, 0.0] [1->0]
        [0.0, 0.7, 0.0] [2->1]
        [0.0, 0.7, 0.0] [3->1]
        [0.0, 0.0, 0.6] [4->2]

        If the mapping matrix is sub-gridded, we perform the convolution on the fractional surface brightnesses in an
        identical fashion to above.

        Parameters
        -----------
        mapping_matrix : ndarray
            The 2D mapping matix describing how every inversion pixel maps to an datas_ pixel.
        """
        return self.convolve_matrix_jit(mapping_matrix, self.image_frame_indexes,
                                        self.image_frame_psfs, self.image_frame_lengths)
def convolve_mapping_matrix ( self , mapping_matrix ) : return self . convolve_matrix_jit ( mapping_matrix , self . image_frame_indexes , self . image_frame_psfs , self . image_frame_lengths )
For a given inversion mapping matrix, convolve every pixel's mapped regular with the PSF kernel.

        A mapping matrix provides non-zero entries in all elements which map two pixels to one another
        (see *inversions.mappers*).

        For example, lets take an regular which is masked using a 'cross' of 5 pixels:

        [[ True, False,  True]],
        [[False, False, False]],
        [[ True, False,  True]]

        As example mapping matrix of this cross is as follows (5 regular pixels x 3 source pixels):

        [1, 0, 0] [0->0]
        [1, 0, 0] [1->0]
        [0, 1, 0] [2->1]
        [0, 1, 0] [3->1]
        [0, 0, 1] [4->2]

        For each source-pixel, we can create an regular of its unit-surface brightnesses by mapping the non-zero
        entries back to masks. For example, doing this for source pixel 1 gives:

        [[0.0, 1.0, 0.0]],
        [[1.0, 0.0, 0.0]]
        [[0.0, 0.0, 0.0]]

        And source pixel 2:

        [[0.0, 0.0, 0.0]],
        [[0.0, 1.0, 1.0]]
        [[0.0, 0.0, 0.0]]

        We then convolve each of these regular with our PSF kernel, in 2 dimensions, like we would a normal regular. For
        example, using the kernel below:

        kernel:

        [[0.0, 0.1, 0.0]]
        [[0.1, 0.6, 0.1]]
        [[0.0, 0.1, 0.0]]

        Blurred Source Pixel 1 (we don't need to perform the convolution into masked pixels):

        [[0.0, 0.6, 0.0]],
        [[0.6, 0.0, 0.0]],
        [[0.0, 0.0, 0.0]]

        Blurred Source pixel 2:

        [[0.0, 0.0, 0.0]],
        [[0.0, 0.7, 0.7]],
        [[0.0, 0.0, 0.0]]

        Finally, we map each of these blurred regular back to a blurred mapping matrix, which is analogous to the
        mapping matrix.

        [0.6, 0.0, 0.0] [0->0]
        [0.6, 0.0, 0.0] [1->0]
        [0.0, 0.7, 0.0] [2->1]
        [0.0, 0.7, 0.0] [3->1]
        [0.0, 0.0, 0.6] [4->2]

        If the mapping matrix is sub-gridded, we perform the convolution on the fractional surface brightnesses in an
        identical fashion to above.

        Parameters
        -----------
        mapping_matrix : ndarray
            The 2D mapping matix describing how every inversion pixel maps to an datas_ pixel.
For a given inversion mapping matrix convolve every pixel s mapped regular with the PSF kernel .