[vsnet-alert 15747] CSS J174033.5+414756: rapid fading?

[Taichi Kato]

CSS J174033.5+414756: rapid fading?

   The most recent observation by the Kyoto team (Ohshima, Kato)
suggests that this object may have started fading more rapidly.
Observations of superhumps during the fading and post-superoutburst
phases are important since many WZ Sge-type dwarf novae show
longer superhump periods in this stage.
We have received other observations from various observers,
which will be reviewed later.