Image Details
Caption: Figure 5.
The γ-ray escape time t0 and 56Ni mass of SN 2022an in the context of the SN Ia population. The comparison samples are taken from N. Wygoda et al. (2019) and A. Sharon et al. (2025). The asterisk symbol indicates the result obtained without accounting for the error budget due to the uncertain distance to SN 202an.
© 2026. The Author(s). Published by the American Astronomical Society.