Dear colleagues,
I have just finished analysing my unfiltered CCD observations of TCP
J19470832-0924198, obtained on 2024, Aug 13/14 at CBA Extremadura
Observatory using a 0.40-m f/5.1 telescope and SX-46 CCD camera under clear
skies.
The resulting light curve clearly shows the presence of superhumps with an
amplitude of 0.30 mag, establishing TCP J19470832-0924198 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) yields a combined
superhump period of 0.0565 +/- 0.0012d. The object was at mag CV = 15.0 on
Aug 13th.
Image calibration and photometry were done using my new photometry software
Phoranso 1.0.4.6
I will send my observations to AAVSO, CBA and VSNET for further analysis.
Best regards
Tonny
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Tonny Vanmunster
CBA Belgium Observatory
CBA Extremadura Observatory
http://www.cbabelgium.co <http://www.cbabelgium.com/> m
PERANSO : The Light Curve and Period Analysis Software
http://www.peranso.co <http://www.peranso.com/> m
PHORANSO: Photometric Reduction and Analysis Software *** NEW ***
http://www.phoranso.com <http://www.phoranso.com/>