Image Details
Caption: Figure 2.
The radio light curves of SN 2025ulz compared to that of Type IIb SNe. For SN 2025ulz, we plot 5σ detections with dots, detections at ≥3σ (but <5σ) with open circles, and upper limits (including detections dominated by host-galaxy light) with downward triangles (Table 1). The data for SNe Type IIb are taken from N. A. J. et al. (2022), A. Gangopadhyay et al. (2023).
© 2026. The Author(s). Published by the American Astronomical Society.