Study computes stability map in orbital eccentricity and dataset size, indicating implications for astrophysical measurements.
We compute a two-phase stability map of the COCM oscillatory parametrisation in the space of orbital eccentricity e and dataset size n. Using mock catalogs with Gaussian noise (A_0=0.091, φ=−0.956), we measure the fraction f_S of free optimisations that recover ω_z = 11.1991±1.0. The regime boundary is found at n_crit = 12.8 ± 1.5, nearly independent of e. DR2+CC (n=14) lies marginally above n_crit under Gaussian noise — the non-recovery observed in real DR2 data is not primarily a statistical-resolution effect but reflects displacement by a compact high-tension substructure (ELG2, −13.4σ). This result formally revises the qualitative interpretation of NT16 §2.
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José Luis Vázquez González (2026) studied this question.
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