MASTER OT J183342.09+654019.1 superoutburst
Superhumps of this object were observed in 2021 Apr.,
but not so well.
YYYYMMDD(UT) mag observer
20230803.2927 17.662g (ASAS-SN Sky Patrol Photom. DB (Hart+2023; Shappee+2014))
20230805.3107 17.534g (ASAS-SN Sky Patrol Photom. DB (Hart+2023; Shappee+2014))
20230814.4402 17.555g (ASAS-SN Sky Patrol Photom. DB (Hart+2023; Shappee+2014))
20230822.4005 15.150g (ASAS-SN Sky Patrol Photom. DB (Hart+2023; Shappee+2014))
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From: <andrew_simon(a)univ.kiev.ua>
Date: Fri, 25 Aug 2023 22:43:27 +0300
Dear Dr. Taichi Kato,
According to my observations in the Lisnyky observational station during
the last two nights it looks like the object Gaia19cuu now in
superoutburst. From the observations superhumps can be easily detected on
the images attached to this letter.
Data from the Gaia shows previous outbursts with the amplitude of 4-5
magnitudes (https://gsaweb.ast.cam.ac.uk/alerts/alert/Gaia19cuu/)
Also data from Gaia Followup for 7 Jul 2019 submitted by Liam Hardy shows
superhumps, due to these data I started to follow this object. (
https://gsaweb.ast.cam.ac.uk/alerts/alert/Gaia19cuu/followup)
ZTF also detected multiple outbursts in the light curve as well as current
outburst. https://lasair-ztf.lsst.ac.uk/objects/ZTF18aatluwz/
After analysing the data I found 0.068d period for 2023-08-23 and 0.077d
period for 2023-08-24. But due to the relatively short duration of
observations these determinations can be not precise. Obtained data
relatively to the comp.star I also attached to this letter.
This night it is cloudy in Kyiv so I have no possibility to
continue observations. But I hope that the object will appear to be
interesting for observations over the world.
Best regards,
Andrew Simon.
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TCP J16294031-4022063: superhump period
Superhump period is 0.05378(1) d (shorter one-day
alias is less likely considering the Porb distribution
of CVs).
Observers:
Josch Habmsch