autolens.plot.subplot_fit_interferometer#

subplot_fit_interferometer(fit, output_path=None, output_format=None, colormap=None, image_plane_lines=None, image_plane_line_colors=None, source_plane_lines=None, source_plane_line_colors=None, title_prefix=None)#

Produce a 12-panel subplot summarising an interferometer fit.

Arranges the following panels in a 3 × 4 grid:

  • Amplitudes vs UV-distance (scatter)

  • Dirty image

  • Dirty signal-to-noise map

  • Dirty model image

  • Source plane image (final plane)

  • Normalised residual (real part) vs UV-distance (scatter)

  • Normalised residual (imaginary part) vs UV-distance (scatter)

  • Source plane image zoomed (final plane)

  • Dirty normalised residual map

  • Dirty normalised residual map clipped to ± 1 σ

  • (panel 9 re-used for 1σ clip — see implementation note)

  • Dirty chi-squared map

  • Source plane image (full extent)

Parameters:

  • fit (FitInterferometer) – The interferometer fit to visualise.

  • output_path (Optional[str]) – Directory in which to save the figure. If None the figure is not saved to disk.

  • output_format (str) – Image format passed to save_figure.

  • colormap (Optional[str]) – Matplotlib colormap name applied to all image panels.