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A survey detection channel overrides the pixels in an astronomical foundation model, and biases tomographic mean redshifts

Via ArXiv cs.AI
Wednesday, Aug 26, 2026 · 4:00AM
Summary

arXiv:2608.23626v1 Announce Type: new Abstract: Foundation models for astronomy are trained on survey pixels together with the catalogue products derived from those pixels. Those catalogues are incomplete at a measurable rate, and a model trained on both inherits that incompleteness as a systematic.

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arxiv.org
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