The spectral admissibility sub-programme of the Cosmochrony corpus addresses a single central question: which spectral sectors of the Weil representation of Heis₃ (Z/qZ) survive the Born–Infeld bounded-flux constraint? The answer organises the entire O-series (papers O1–O32 and five precursor papers) into a logically closed derivation chain: \ bounded flux \;\; admissibility envelope \;\; Weil-sector capacity \;\; ₀₈ₑ \;\; ^* 0. 126. \ This note maps the constituent papers, identifies four internal phases, records the status of every result as proved, structural, or open, and states the two remaining open deliverables: the pointwise analytical proof of hypothesis H-color (partially resolved at three levels in O32) and the extension of the numerical campaign to q = 401.
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Jérôme Beau (Sun,) studied this question.
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