KIC 11390659 bright outburst
(Porb is said to be below the period gap, no superhumps
have been detected)
https://www.aavso.org/vsx/index.php?view=detail.top&oid=297526
YYYYMMDD(UT) mag observer
20221012.1327 16.652zg (ZTF Alert DC mag (Masci+ 2019))
20221012.6669 <162C (Masayuki Moriyama)
20221013.6258 163:C (Masayuki Moriyama)
20221015.487 125 (Hiroyuki Maehara)
SDSS J001153.08-064739.1: superhump period
Josch Hambsch has reported further observations.
The superhump period has been determined tp be
0.10414(3) d. Amplitude 0.20 mag.
If these superhumps are of stage B, the expected
q=0.165 (table 4 in arXiv:2201.02945 = VSOLJ Variable
Star Bulletin No. 89). Even if they are of stage C,
q would be 0.18. This is very much in disagreement
with Rebassa-Mansergas et al. (2014) giving q=0.32(8).
ZTF18abtbrfb: polar below the period minimum?
Using ZTF data, I obtained a period of 0.0335541(1) d
(single peak, amplitude 1.0 mag).
Although the double period is acceptable, the two peaks
look too much alike.
SDSS J001153.08-064739.1 superhumps
Josch Hambsch detected superhumps also on Oct. 10.
Despite the brightness (still brighter than 14.0)
and 0.2-mag superhumps, no one else appears to be
observing. This object is in the period gap and has
an unusual secondary. Please pay more attention.