TCP J16294031-4022063: unusually reddened SU UMa-type dwarf nova?
Josch Hambsch has reported observations.
The data showed regular 0.23-mag superhumps with a period
of 0.0543(4) d.
This result, however, is strange since this object
is apparently reddened like a nova:
YYYYMMDD(UT) mag observer
20230716.5893 14.73V (Masayuki Moriyama)
20230716.5904 14.21Rc (Masayuki Moriyama)
20230716.5914 13.68Ic (Masayuki Moriyama)
20230716.5925 15.06B (Masayuki Moriyama)
If this is a reddened SU UMa-type dwarf nova, the object
should be fairly close. The absence of a bright quiescent
counterpart would be problematic. Further observations
are strongly encouraged.