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The First Radio View of a Type Ibn Supernova in SN 2023fyq: Understanding the Mass-loss History in the Last Decade before the Explosion

  • Authors: Raphael Baer-Way, Nayana A. J., Wynn Jacobson-Galán, Poonam Chandra, Maryam Modjaz, Samantha C. Wu, Daichi Tsuna, Raffaella Margutti, Ryan Chornock, Craig Pellegrino, Yize Dong, Maria R. Drout, Charles D. Kilpatrick, Dan Milisavljevic, Daniel Patnaude, Candice Stauffer

Raphael Baer-Way et al 2025 The Astrophysical Journal Letters 995 .

  • Provider: AAS Journals

Caption: Figure 4.

Radio SEDs of SN 2023fyq at Δt ≈ 58–525 days. The downward triangles represent 3σ flux density upper limits. The solid black lines denote the overall SSA+ external FFA model we derive self-consistently (see Section 3.1). The solid green lines denote the intrinsic SSA model using the calculated Fp/νp from Equation (5). The values of the best-fit parameters are displayed in Table 2. We also show the extrapolated models with dashed black and green lines at Δt ≈ 525 days with the flux density upper limits, to emphasize the discrepancy between the models and the nondetections, indicating a decrease in the mass-loss rate at ∼ 5–10 yr before the explosion.

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