[vsnet-alert 22502] V1024 Per: SU UMa-type dwarf nova with highly variable mass-transfer rate

[Taichi Kato]

V1024 Per: SU UMa-type dwarf nova with highly variable mass-transfer rate

   No outburst in the 2016-2017 season (system faded).
High activity in the 2017-2018 season, but without
a superoutburst.  Currently lower activity again.

ASAS-SN data:
https://asas-sn.osu.edu/light_curves/fe300934-6d6e-4bbb-b4f6-2dce3779987e

Most recent outburst:

  YYYYMMDD(UT)   mag  observer
  20180906.5309 16.119V  (ASAS-SN survey (Shappee+ 2014; Kochanek+ 2017))
  20180906.5322 16.217V  (ASAS-SN survey (Shappee+ 2014; Kochanek+ 2017))
  20180906.5335 16.241V  (ASAS-SN survey (Shappee+ 2014; Kochanek+ 2017))
  20180907.9931  128  (Eddy Muyllaert)