The equal-charge branch of supersymmetric rotating AdS black holes has . The corresponding microcanonical sector of the superconformal index is obtained by projecting to equal charges, or equivalently by extracting the constant term in the two charge-difference fugacities. We prove that for the large- multigraviton sector the projected index factorizes exactly as where is the partition function. This factorization gives, for every spin sector, an explicit onset energy below which the large- coefficient is zero. Exact computations show that finite-rank coefficients can nevertheless appear at energies where the large- coefficient vanishes, including beyond the classical black-hole bound. We also determine the full line . In particular, with denoting this large- onset energy, and the first giant-graviton sector already contributes one unit at this point. All coefficients are coefficients of the -graded index, not positive degeneracies. The main conclusion is that the high-spin tail survives the exact equal-charge projection.

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