Forget the face runs made on proxies too small to see a face
The floor added in the previous commit stops this happening again; it does nothing about the 1,824 images in the reference library that already carry a face_index row written against a proxy of 1024 or less. Those rows are why the damage is permanent rather than merely past. The work list is "images with no row for this model", so an image examined against a 1024px proxy -- 0.078 faces per image, nine in ten finding nothing -- is indistinguishable from one examined properly, and no later pass will ever offer it to the detector again. V12 deletes exactly those markers, and nothing else. The faces those runs did find stay in place and keep drawing the People screen until a better pass replaces them, and record_detections re-attaches the user's confirmed names across that replacement by box overlap, so a library somebody has spent an evening naming does not lose that evening. The cost is a re-fetch of the affected images. Deleting the marker rather than teaching the work-list query to select on source_edge, which was the other option and is worse. A standing `source_edge < floor` predicate never lets go: an image whose largest embedded preview is genuinely smaller than the floor would be re-fetched on every sweep for ever, because the next pass cannot do any better than the last one did. A one-off deletion gives each affected image exactly one more attempt through the good path and then lets the ordinary "has a row" rule settle it. The threshold is written out in the SQL instead of referring to dr_face::MIN_DETECT_EDGE. A migration has to keep meaning what it meant when it ran; binding it to a constant someone may raise later would quietly change what an old catalog gets migrated to. Co-Authored-By: Claude Opus 5 (1M context) <noreply@anthropic.com>
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