[vsnet-outburst 17251] CC Scl: eclipsing SU UMa-type dwarf nova

[Taichi Kato]

CC Scl: eclipsing SU UMa-type dwarf nova

   Josch Hambsch has reported observations up to 28 d
after the termination of the superoutburst.
An analysis of the data now revealed that this object
is eclipsing.  The ephemeris using the all the available
data (including the CRTS data) is:

Min(BJD) = 2456668.00638(9) + 0.058567233(8) E

The mean orbital light curve:
http://www.kusastro.kyoto-u.ac.jp/vsnet/tmp/ccsclorb.png

   The orbital period reported in Woudt et al. (2012)
MNRAS 427, 1004 has turned out to be incorrect.