XTE J1118+480 : Superhump still presence
According to IAU Circular 7617, J. Casares et al. detected
superhumps with a period of 0.17049(1) day using their data during
Dec. 2000 - Apr 2001. The data set obtained during the outburst in
2000 by VSNET team shows the mean superhump period during the outburst
is slightly longer than that reported in IAUC 7617, which may imply a
continuous period changing. In the case of SU UMa-type dwarf nova,
the "late superhump" is sometimes observed after superoutburst
(vsnet-campaign 894).