Add subplot_fit_quick for interferometer quick updates - #549
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6-panel (2x3) fast-render subplot for interferometer data: Top row: Dirty Image, Dirty Model Image, Dirty Normalized Residual Bottom row: Vis Norm Residual (Real) scatter, Vis Norm Residual (Imag) scatter, Source Plane / Reconstruction Uses raw imshow + scatter on pre-converted numpy arrays (same approach as imaging subplot_fit_quick). Visibility scatter panels use rasterized rendering for speed with large UV datasets. Quick updates now call subplot_fit_quick instead of the heavier subplot_fit_dirty_images. Co-Authored-By: Claude Opus 4.7 <noreply@anthropic.com>
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Summary
Adds a 6-panel
subplot_fit_quickfor interferometer data, matching the imaging equivalent. Layout:Uses raw
imshow+scatteron pre-converted numpy arrays for sub-second rendering. Visibility scatter panels userasterized=Truefor speed with large UV datasets. Quick updates now callsubplot_fit_quickinstead ofsubplot_fit_dirty_images.API Changes
New function
autolens.interferometer.plot.fit_interferometer_plots.subplot_fit_quick. The plotter's quick-update branch now calls this instead ofsubplot_fit_dirty_images.Test Plan
fit_quick.pngoutput for interferometer datapytest test_autolens/🤖 Generated with Claude Code