Image Details
Caption: Figure 3.
Best-fit BayeSN model to each of the observed filters and epochs for SN 2025ogs. The measured photometry is shown as circles with errors, and the shaded region represents the BayeSN model + fitting uncertainty. The epoch of our NIRSpec observation is noted by the dashed black vertical line.
© 2026. The Author(s). Published by the American Astronomical Society.