Dear colleagues,
I have just finished analysing my unfiltered CMOS observations of TCP
J17321088+0807243 obtained on 2023, Jun 15/16 and June 16/17 at CBA
Belgium Observatory using a 0.40-m f/10.0 telescope and QHY-268M CMOS camera
under clear skies. My observations were triggered by Taichi Kato's post in
vsnet-alert 27850.
The resulting light curve clearly shows the presence of superhumps with an
amplitude of 0.32 mag, establishing TCP J17321088+0807243 as either a new SU
UMa-type or …
[View More]WZ Sge-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 0.0612 +/- 0.0011d. The object was at mag CV
= 17.0 on Jun 17th.
Image calibration and photometry were done using a beta version of Phoranso.
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.com> http://www.cbabelgium.com
PERANSO: The Light Curve and Period Analysis Software
http://www.peranso.com
PHORANSO: Photometric Reduction and Analysis Software *** NEW - in beta
mode ***
http://www.phoranso.com
[View Less]
BraTS-SON-T2-046 = TCPJ17294472-4236232: new SU UMa (probable WZ Sge) star
Josch Hambsch reported observations. Superhumps are
clearly seen (period about 0.06 d, will be refined later).