MASTER OT J001204.00-412337.4: strange behavior
Josch Hambsch has reported new observations.
The object started fading rapidly on Aug. 8.
The duration of the superoutburst (8 d) is
too short for a WZ Sge star. Observations of subsequent
behavior are very important (the object still shows
superhumps).
ASASSN-22jz = AT 2022qwf (UG:)
(submitted to VSX)
Discovery circumstances:
https://www.wis-tns.org/object/2022qwf
Complete ASAS-SN Sky Patrol (Shappee et al. 2014ApJ...788...48S
and Kochanek et al. 2017PASP..129j4502K) light curve and data:
https://asas-sn.osu.edu/sky-patrol/coordinate/6863cfab-4837-4bdd-bffb-552ee…
ASASSN-22jz 20220805.9828 <16.47g ASN
ASASSN-22jz 20220808.0109 10.22g ASN
ASASSN-22jz 20220808.0121 9.74g ASN
ASASSN-22jz 20220808.0133 9.77g ASN
A DASCH search revealed a previous (super?)outburst recorded
on Harvard plates:
1920 April 14.205 UT, mpg. 10.92
1920 April 14.250 UT, mpg. 11.01
1920 April 22.085 UT, mpg. 11.83
1920 April 22.216 UT, mpg. 11.33
ASASSN-22jz looks like a WZ Sge-type dwarf nova outburst
(amplitude 9 magnitudes) at a distance of ~230 pc.
Time-resolved photometry is urgently required.
Clear skies,
Patrick
ASASSN-19oc
Noise? WZ Sge star with a dip in the early stage of
the superoutburst.
YYYYMMDD(UT) mag observer
20220726.5640 <162c (Yutaka Maeda)
20220802.5037 128:c (Yutaka Maeda)
MASTER OT J001204.00-412337.4: superhump period
Josch Hambsch and Berto Monard have reported new
observations. The current superhump period is 0.06105(6) d
(probably still stage A). The low amplitude (0.08 mag)
is consistent with a period bouncer.
Single-night observation by Berto Monard during
the initial plateau did not show a strong signature
of early superhumps (but had some hint). Early superhumps
had probably already decayed at the time of Monard's
observation.
Re: MASTER OT J001204.00-412337.4: new SU UMa-type dwarf nova
> According to ASAS-SN Sky Patrol (Shappee et al. 2014ApJ...788...48S and
> Kochanek et al. 2017PASP..129j4502K) data the current superoutburst started
> on (or shortly before) 2022 July 16. A dip was recorded (also by
> Josch Hambsch, HMB) from July 28 to 30:
Then looks likely a period-bouncer WZ Sge star.
ASASSN-16hg: https://ui.adsabs.harvard.edu/abs/2018PASJ...70...47K/abstract
ASASSN-15jd: https://ui.adsabs.harvard.edu/abs/2016PASJ...68...55K/abstract
MASTER OT J001204.00-412337.4: new SU UMa-type dwarf nova
Josch Hambsch has reported observations on three nights.
The object was faint (17 mag) on July 29 and was rising
rapidly on July 30 (with superhumps). Superhumps were
apparent on July 31 at mag 14.9. The period is about
0.063 d.