[vsnet-newvar 8011] ASASSN-16iz: most likely SU UMa star

[Taichi Kato]

ASASSN-16iz: most likely SU UMa star

   ZTF recorded superoutburst + rebrightening.

  YYYYMMDD(UT)   mag  observer
  20190827.4718 15.271zg  (Zwicky Transient Facility (Masci et al., 2019))
  20190827.5018 15.353zr  (Zwicky Transient Facility (Masci et al., 2019))
  20190830.4742 15.451zg  (Zwicky Transient Facility (Masci et al., 2019))
  20190830.5047 15.676zr  (Zwicky Transient Facility (Masci et al., 2019))
  20190906.4522 16.117zg  (Zwicky Transient Facility (Masci et al., 2019))
  20190906.5140 16.235zr  (Zwicky Transient Facility (Masci et al., 2019))
  20190909.4771 16.418zg  (Zwicky Transient Facility (Masci et al., 2019))
  20190909.5198 16.521zr  (Zwicky Transient Facility (Masci et al., 2019))
  20190912.4892 17.264zg  (Zwicky Transient Facility (Masci et al., 2019))
  20190915.4628 19.397zr  (Zwicky Transient Facility (Masci et al., 2019))
  20190918.4655 17.005zr  (Zwicky Transient Facility (Masci et al., 2019))
  20190918.5166 17.069zg  (Zwicky Transient Facility (Masci et al., 2019))

   Relatively bright object and time-resolved photometry
is wanted during the next superoutburst.