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[vsnet-campaign-dn 1772] Re: [vsnet-alert 6798] SDSSp_J173008.38+624754.7 period analysis
Dear colleagues,
I have now completed a period analysis of
SDSSp_J173008.38+624754.7, using the complete set of
observations obtained at CBA Belgium Observatory last
night, October 22/23 (5.25 hours).
The PDM technique yields a superhump period value of
0.0801 +/- 0.0009 d, which is close to the value
reported by Taichi below, although not yet completely
in line.
I will post the complete light curve to my Web site
later today.
Please continue your follow-up observations, as multi-
longitude coverage is needed to secure the outbursting
characteristics of this new UGSU CV.
With kind regards,
Tonny Vanmunster
CBA Belgium Observatory
http://vsnet.lunarpages.com/cbabelgium
In antwoord op: Taichi Kato <tkato@kusastro.kyoto-
u.ac.jp>:
> SDSSp_J173008.38+624754.7 period analysis
>
> Dear Colleagues,
>
> We have analyzed the Nyrola observation, and
obtained the best
> superhump
> period of 0.0819(8) d. The value is one of the
longest among SU UMa-type
> dwarf novae below the period gap.
>
> Regards,
> VSNET Collaboration team
>
>
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