ASASSN-22jz: new WZ Sge-type dwarf nova
Berto Monard has reported observations on two nights.
The object was fading rather rapidly (0.3 mag/d),
probably in viscous fading phase.
Although there were much irregularity, I could detect
a period of 0.05404(4) d (double wave, 0.035 mag).
Although the profile is not very typical for early superhumps,
the period appears to be real based on the appearance of
one-day aliases. The rather unusual profile of
early superhumps a result of their low …
[View More]amplitude and
overlapping irregularity. Considering the outburst
amplitude and peak M_V, this object can be identified
to be a WZ Sge star.
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ZTFJ061429.37+793024.1=ZTF18accmhht: polar
Using ZTF data, I obtained a period of 0.0822436(2) d
(single hump per orbit). The overall behavior also
does not resemble that of a VY Scl star (too rapid fading
and flat bottom).
ZTFJ050541.47+680015.1=ZTF18abwcfvv: NL+E
https://www.aavso.org/vsx/index.php?view=detail.top&oid=2228287
According to Gaia variable stars, it was classified as
050541.4 +680014 (2000.0) Gaia_DR3_483798207282350976 ECL (score=0.48)
050541.4 +680014 (2000.0) Gaia_DR3_483798207282350976 vtype=E P=0.20496893(0.00000043)
I obtained a period of 0.2049695(3) d using ZTF data.
Typical NL+E light curve.
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
…
[View More]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
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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)