Unfiltered plane screening creates actual compatible dust context

Can the frozen stellar screen retrieve candidates where cached dust clumps actually occur?

Two deterministic class-free cloud centers, fixed rectangles and unchanged E112 classifier; all-source3/15/30arcsec dust alternatives and60arcsec controls.

Preserve terminal zero-byte restricted DNS failure; separately registered network execution retains exact plans. Independent2,745-native-primitive review and scalar/proper-motion/haversine replay checks583 exported scalars,6,133 cached motion references and12,469,620 geometry admissions.

61 new nativeWISE IDs,53 supported,8 unknown,50 candidates;118,848bytes downloaded.13 selected candidates near cached clumps at30arcsec versus7 controls;6 versus3 at15arcsec;zero at3arcsec. Existing cached Gaia/YSO point queries provide no alternatives. Sharded collection3,225 distinct candidates without copying old rows.

Next: Obtain actual field-specific stellar/young/contaminant reference evidence; preserve all missing inputs, fixed flags and radii; then deeper native catalogue/image/temporal refinement.

Small cloud-centered sample, not large-survey validation. High burden9,854–22,508 candidates/deg2. Dust proximity is ambiguous; absent cached references are a coverage gap. No adopted ownership, physical class, membership or birth.