SDSS J094002.56+274942.0: another long-Porb SU UMa star
ZTF time-resolved data recorded superhumps during
the 2019 Feb. outburst. T. Vanmunster's observation
also detected 0.3-mag superhump(s) on 2019 Feb. 11.
Probably due to the long Porb=0.16352 d, this variation
was not regarded as superhump(s).
The 2009 outburst (Krajci and Wils JAAVSO 38, 33)
was a normal one. The secondary is probably somewhat
evolved as reported as a possible spectral class early M-type
in Krajci and Wils (2010).