[vsnet-outburst 25997] MASTER OT J193922.39+665346.0: new SU UMa-type dwarf nova
Tonny Vanmunster tonny.vanmunster@gmail.com via vsnet-outburst
vsnet-outburst at ooruri.kusastro.kyoto-u.ac.jp
Sat Nov 7 08:43:10 JST 2020
Dear colleagues,
I have just finished analysing my (ongoing) unfiltered CCD observations of MASTER OT J193922.39+665346.0, obtained tonight (2020, Nov 06/07) at CBA Belgium Observatory, using a 0.40-m f/10.0 telescope and STT-3200ME CCD camera under clear skies.
Superhumps with an amplitude of 0.20 mag are clearly in the resulting light curve, establishing MASTER OT J193922.39+665346.0 as a new SU UMa-type dwarf nova. A period analysis using the ANOVA, Lomb-Scargle, Generalized-Lomb-Scargle and PDM methods (Peranso 3.0, in beta testing), yields a combined superhump period of 0.0717 +/- 0.0023d. The object was at mag 16.4 (CV) on Nov 06th.
I will send my observations (currently large backlog) to AAVSO, CBA and VSNET for further analysis.
Follow-up observations are recommended to refine the superhump period.
Best regards
Tonny
--
Tonny Vanmunster
CBA Belgium Observatory
CBA Extremadura Observatory
www.cbabelgium.com
www.peranso.com
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