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Panchromatic JWST Observations and Models of the Dim Type Iax Supernova SN 2024vjm at 200 days

  • Authors: E. Baron, J. M. DerKacy, C. Ashall, M. Shahbandeh, Peter H. Hauschildt, T. Barman, J. P. Aufdenberg, C. R. Burns, N. Morrell, M. D. Stritzinger, P. Hoeflich, K. Medler, E. Fereidouni, C. M. Pfeffer, T. Mera, W. B. Hoogendam, S. Shiber, P. J. Brown, Divya Mishra, Inma Dominguez, L. Galbany, Paolo Mazzali, E. Y. Hsiao, Huangfei Xiao, T. de Jaeger, S. Kumar

E. Baron et al 2026 The Astrophysical Journal Letters 1008 .

  • Provider: AAS Journals

Caption: Figure 6.

(a) The observed Day +196.1 SN 2024vjm JWST spectrum plotted against the best-fit blackbody. (b) The observed Day +196.1 SN 2024vjm JWST spectrum plotted against the best-fit dust model. The two components of the model, consisting of cold, 0.15 μm and hot, 0.01 μm graphite, are also shown. (c) The observed Day +196.1 SN 2024vjm JWST spectrum with the best fit dust model (b) removed.

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