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Probing the 3D Structures of Supernovae through IR Signatures of CO and SiO

  • Authors: T. Mera, P. Hoeflich, C. R. Burns, C. Ashall, K. Medler, E. Fereidouni, W. B. Hoogendam, M. Shahbandeh, S. Shiber, C. M. Pfeffer, E. Baron, J. Lu, N. Morrell, E. Y. Hsiao, M. M. Phillips

T. Mera et al 2026 The Astrophysical Journal 1003 .

  • Provider: AAS Journals

Caption: Figure 14.

Demonstration of the χ2 convergence for the fundamental band for each of the six primary parameters for Model PP at day 385. For each panel we keep the optimized parameters the same except for the parameter being varied. For panels (A)–(F) we only show χ2 of the fundamental band because the overtone is virtually nonexistent. (A) Density structure (n), (B) inner velocity edge (v1), (C) width of the molecular region (Δv), (D) clump density contrast (fc), (E) clump size (rR), and (F) clump shape (ϵ). For discussion, see Section 4.2.

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