slitflow.loc.fit module
- class Gauss2D(info_path=None)[source]
Bases:
TableFit spot localizations with 2D Gaussian distribution.
Caution
The input image should be split into a single frame image. In other words, the shape of reqs[0] in
process()should be (1, height, width).- Parameters:
reqs[0] (Image) – Image to fit. Required params;
pitch,length_unit.reqs[1] (Table) – Roughly predicted X,Y-coordinate.
param["half_width"] (int) – Half width of the clipping rectangle in pixel to fit the spot image. The shape of clipped image is (2 * half_width + 1, 2 * half_width + 1).
param["split_depth"] (int) – File split depth number.
- Returns:
Refined X,Y-coordinate
- Return type:
- static process(reqs, param)[source]
Fit spot localizations with 2D Gaussian distribution.
- Parameters:
reqs[0] (numpy.ndarray) – Numpy 3D array with the shape of (1, height, width).
reqs[1] (pandas.DataFrame) – Roughly predicted X,Y-coordinate.
param["calc_cols"] (list of str) – X,Y-coordinate column names.
param["use_cols"] (list of str) – Column names to use. Index column names + calc_cols.
param["half_width"] (int) – Half width of the clipping rectangle in pixel to fit the spot image. The shape of clipped image is (2 * half_width + 1, 2 * half_width + 1).
param["split_depth"] (int) – File split depth number.
- Returns:
Refined X,Y-coordinate
- Return type:
- fit_gauss_2d(clip, half_width)[source]
Fit clip image with 2D Gaussian.
- Parameters:
clip (numpy.ndarray) – Two-dimensional array for fitting.
half_width (int) – Half width of the clipping rectangle. clip.shape = (2 * half_width + 1, 2 * half_width + 1).
- Returns:
tuples containing
amplitude (float): Amplitude of 2D Gaussian
y_center (float): Y-coordinate of 2D Gaussian center
x_center (float): X-coordinate of 2D Gaussian center
sigma (float): Standard deviation of 2D Gaussian
back (float): Background offset of 2D Gaussian
se_amplitude (float): Standard deviation error of amplitude
se_y_center (float): Standard deviation error of Y-coordinate
se_x_center (float): Standard deviation error of X-coordinate
se_sigma (float): Standard deviation error of sigma
se_back (float): Standard deviation error of background
rmsr (float): Root mean square of residual (Background)
rsqr (float): R-squared
If fitting is failed, this function returns (amp_ini, half_width, half_width, half_width / 3, back_ini, 100, 100, 100, 100, 100, 1, 1)