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render: point-source fit.png with the Fit Source Plane panel - #13
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…ens#789) Re-render point_source_image_chi_squared, point_source_source_chi_squared and cluster fit.png against PyAutoLens#790 / PyAutoArray#653; producer docstrings and AGENTS.md describe the new panel. Co-Authored-By: Claude Opus 5.5 <noreply@anthropic.com>
… (PyAutoLens#790) Co-Authored-By: Claude Opus 5.5 <noreply@anthropic.com>
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Summary
Re-renders every point-source
fit.pngwith the new Fit Source Plane panel (PyAutoLabs/PyAutoLens#789): the observed positions traced to the point's own plane, numbered 1..N as on the image plane andpoint_solver.png, with the source centre, caustics and a tangential-caustic inset.point_source_image_chi_squared/fit.png— image-plane χ²: context-only panel, no noise footprints or χ².point_source_source_chi_squared/fit.png— source-plane χ² (magnification weighting): σ/|μ| circles primary, dashed darker-orange A·σ ellipses as propagated-noise reference,χ² = 10,023in the legend (the only χ² shown); the "Model (source plane)" crosses are gone from the image plane.cluster/point_0,point_1fit.png— each point against its own plane's caustics (point_0 at z=1, point_1 at z=2); inset frames the tangential caustic only; milli-arcsecond ticks distinct (e.g. 1.1997″ / 1.2004″ / 1.2011″).point_solver.pngfiles are byte-identical (shared numbering refactor is behaviour-preserving). Producer docstrings + AGENTS.md describe the panel.Upstream PR
This PR merges last. Its
lintjob renders against library mains, so it is red until both library PRs merge — re-run then.Scripts Changed
scripts/point_source_image_chi_squared/visualization.py(docstring)scripts/point_source_source_chi_squared/visualization.py(docstring)scripts/cluster/visualization.py(docstring)gallery/viz_manifest.yaml;AGENTS.mdTest Plan
ruff check .,ruff format --check .,python gallery/gallery_build.py --checkclean🤖 Generated with Claude Code