Gaia24amv: SU UMa-type dwarf nova near the period gap

Gaia24amv/AT 2019dkz was discovered on 2019-04-13 11:19:45.000 by J. Nordin, V. Brinnel, M. Giomi, J. van Santen (HU Berlin), A. Gal-Yam, O. Yaron, S. Schulze (Weizmann) on behalf of ZTF.

Follow-up observations were started on 2026 June 26 with a 0.7-m f/4 telescope at Observational Station Lisnyky of Taras Shevchenko National University of Kyiv. The main dataset was obtained on 2026 June 26–July 4 using the 0.7-m f/4 AZT-8 telescope at the Observational Station Lisnyky of Taras Shevchenko National University of Kyiv, the 0.6-m f/6.5 ADYU60 reflector at the Observatory of Adıyaman University and 0.7-m f/6.5 Planewave CDK-700 telescope of Planetarium Slaskie in Chorzów. Results were published in The Astronomer's Telegram .

Light curve obtained on 26 of June 2026

Period of superhumps detected from detrending data obtained during 2026 June 26-30