[vsnet-alert 21073] ASASSN-15fv: new SU UMa type dwarf nova

Tonny Vanmunster tonny.vanmunster at gmail.com
Thu Jun 1 07:50:40 JST 2017


Dear colleagues,

I have just concluded the analysis of my 2017, May 24/25 unfiltered CCD photometry session of ASASSN-15fv. Observations were made at CBA Belgium Observatory,  using a 0.40-m f/10.0 telescope and STT-3200ME CCD camera, under a clear sky. The resulting light curve clearly shows the presence of superhumps with an amplitude of 0.28 mag. A period analysis using the ANOVA, Lomb-Scargle and PDM methods (Peranso), yields a combined preliminary superhump period of 0.0692 +/- 0.0010d, hence establishing this object as a new SU UMa type dwarf nova. The object was at mag 16.6 (unfiltered) on May 24th.


Observations will be sent to CBA and VSNET for further analysis.

Best regards
Tonny

-- 

Tonny Vanmunster
CBABelgium Observatory
 <http://www.cbabelgium.com> www.cbabelgium.com
 <http://www.peranso.com> www.peranso.com



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