Complete paper (Markdown + DOCX) on the C3 high-variability ISP blazar subpopulation. v5 adds the formatted DOCX version of the full paper. Key results: GMM identification of C3 (N=129, 4LAC-DR3); spectral softening confirmed in ON 246 (KS p=7.5e-4) and 3C 66A (KS p=1.15e-13, 27,059 photons); shared physical signature across different variability characters. OSF: https://osf.io/7b5t2
Yoshimitsu Katayama (Sun,) studied this question.