Supernova SN 2024abfo‘s brightness increased steadily from our first measurement at 16.91 mag on 17 Nov 2024 until peak brightness was reached during the night 06 Dec 2024, at 13.81 mag, more than fifteenfold. Meanwhile, brightness is back at 16.73 mag on 11 Apr 2025 (all values median mag of the dataset).
Discovery by ATLAS (ATLAS-STH_ATLAS-03) on 15 Nov 2024 reported a brightness of 16.79 mag with filter “orange-ATLAS”, measurements by Pan-STARRS (PS1_GPC1) two days later on 17 Nov 2024 reported 16.63 mag with filter “i-P1”.
Our amateur measurement with 137 datasets in total now cover a period of 146 days, quite an achievement I’d say. ;-)
Due to using an L filter (Baader UV/IR cut) and not a V band filter, the measurements here overestimate the brightness by approx. 0.2 mag. With almost full moon and low altitude (meanwhile NGC 1493 is setting quite early), the last two measurement have a higher uncertainty, up to 0.08 mag.
IAS – Internationale Amateursternwarte e.V. – Hakos Observatory, Namibia
IAS remote telescope “Dieter”
Data aquisition by Martin Junius and Stephan Messner.
Technical details see previous post. Photometry measurements with L filter.
