[vsnet-campaign-dn 5423] Superhumps in CSS080304:090240+052500
Hiroyuki Maehara
maehara at kwasan.kyoto-u.ac.jp
Thu Mar 6 12:56:00 JST 2008
Dear colleagues,
I performed time-series photometry of the object last night.
The data show superhumps with an amplitude of ~0.5 mag.
The superhump period is around 0.057 d.
CSS080304:090240+052500 is a new large-amplitude SU UMa-type (or
WZ Sge-type) dwarf nova.
Further observations are encouraged.
Best regards,
Hiroyuki Maehara
VSNET Collaboration Team
On Thu, Mar 06, 2008 at 01:00:59AM +0900, Akira Arai wrote:
> We observed a new optical transient CSS080304:090240+052500
> using our 25cm telescope at Higashi-Hiroshma Observatory, Japan.
> The object is now aboue 16.8mag in V-band.
>
> YYYYMMDD(UT) mag. err.
> 20080305.59146 16.8V 0.1 Higashi-Hiroshima Observatory
>
> We started a time-series observation of the object using nofiltered CCD.
>
> Regards,
> A. Arai and M. Uemura
> on behalf of the KANATA team
> Hiroshima University
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