MGAB-V233: superhumps detected during a new superoutburst
According to the data from VSX AAVSO, MGAB-V233 was discovered by Gabriel Murawski.
Our follow-up observations were obtained on 17/18 September, 2026 with the 0.7-m f/4 AZT-8 telescope at the Observational Station Lisnyky of Taras Shevchenko National University of Kyiv, the 0.68-m telescope at the Horten Local Observatory, the 0.6-m Telescope of the University of Salerno Astronomical Observatory, the 0.4-m Telescope of the EEye Astronomical Complex and the 0.5-m OAUJ Cassegrain Telescope. On the reulted lightcurve we can clearly detected superhumps. The measured superhump period is Psh = 0.09565(6)d. The results were published in The Astronomer's Telegram.
Prediction of the SuperOtburts for MGAB-V233 with OASys
Period determination for the data obtained on 15-18 of September 2026
Superhump period determined from the data obtained on 15-18 of September 2026