This dwarf nova in Lacerta was discovered by 9th-grade student Alexandra
Rybka in November 2020 while data mining from the URAT1 catalog (due to
outburst at Epoch 2013.708). It was also in outburst on 1989-09-03 DSS red
plate and on several PanSTARRS-1 images. AAVSO VSX entry:
https://www.aavso.org/vsx/index.php?view=detail.top&oid=2214231
According to ATLAS data (Tonry et al., 2018) the latest superoutburst
started on 2021 October 20th and peaked at 16.6o on Oct. 21st. Light curve
from ATLAS forced photometry server in orange and cyan filters:
http://scan.sai.msu.ru/~denis/Rybka2-ATLAS-LC.gif
During the outbursts this variable is showing the eclipses as deep as 2
magnitudes. See, for example, the light curve of October 2019 outburst from
ZTF data (Masci et al., 2018):
http://scan.sai.msu.ru/~denis/Rybka2-ZTF-Oct2019.gif
Using the combined ATLAS and ZTF data from four outbursts, I have found the
best value of period to be P=0.0819486 d (118.006 minutes) and the epoch of
mid-eclipse MJD=59513.379. After the linear detrending of outbursts (some
for 0.15 mag/day, one for 0.12, the other for 0.10 mag/day) the following
phased light curve was obtained:
http://scan.sai.msu.ru/~denis/Rybka2-phased_LC.gif
Denis Denisenko
ASASSN-21uy: superhump period
Josch Hambsch has reported further observations.
The superhump period is 0.06057(4) d.
The profile is still doubly humped with the second
maximum fainter.
ASASSN-21uw: new SU UMa-type dwarf nova
Josch Hambsch and Berto Monard have reported observations.
Superhumps started to appear on Nov. 20 and the current
period is 0.0557(1) d (probably stage A).
CS Ind outburst
SU UMa star with a long (0.124 d) superhump period.
YYYYMMDD(UT) mag observer
20211007.485 170 (Rod Stubbings)
20211105.442 168 (Rod Stubbings)
20211108.442 170 (Rod Stubbings)
20211120.457 120 (Rod Stubbings)