Detection of superhumps in the ER UMa-type dwarf nova Gaia24aeg
According to the data from TRANSIENT Name Service (TNS) Gaia24aes/AT 2024re was discovered on 2024-01-05 14:00:57.600 by S.T. Hodgkin, E. Breedt, A. Delgado, D.L. Harrison, M. van Leeuwen, G. Rixon, T. Wevers, A. Yoldas (IoA Cambridge), N. Ihanec, K. Kruszyńska, K.A. Rybicki, Ł. Wyrzykowski (Warsaw University Astronomical Observatory), Z. Kostrzewa-Rutkowska (Leiden Observatory), D. Eappachen (SRON/RU), G. Marton (Konkoly Observatory), on behalf of the Gaia Alerts team.
Our follow-up observations were provided on 09 August, 2026 with 0.7-m f/4 AZT-8 telescope at the Observational Station Lisnyky of Taras Shevchenko National University of Kyiv. On the reulted lightcurve we can clearly detected superhumps. Period detection gives us a result of Psh = 0.077(3)d. Results were published in The Astronomer's Telegram.
Light curve obtained on 09 of August 2026 and processed with BHTOM
Period determinationfor the data obtained on 09 of August 2026
Period of superhumps detected from the data obtained on 09 of August 2026