Re: AT2022sfe: likely highly reddened nova
Accoring to
> https://www.wis-tns.org/object/2022sfe
The Gaia object appears to be the northern component
of the pair.
200029.264 +345308.30 (2000.0) Gaia_EDR3_2059315910815578496 plx=-(-) dismod=- pmra=-(-) pmdec=-(-) G=21.008 BP=21.178 RP=19.371
The location 20:00:29.256 +34:53:09.14 is very slightly
different from this location. A faint object not in Gaia
may be outbursting now.
AT2022sfe: likely highly reddened nova
Moriyama-san has pointed out the red color.
YYYYMMDD(UT) mag observer
20220827.5919 15.53C (Masayuki Moriyama)
20220828.6528 15.34C (Masayuki Moriyama)
20220828.6559 14.99Rc (Masayuki Moriyama)
20220828.6576 13.51Ic (Masayuki Moriyama)
20220828.6593 <16.39B (Masayuki Moriyama)
20220828.6638 16.92:V (Masayuki Moriyama)
See:
https://www.wis-tns.org/object/2022sfe
The object is located very close to the northern component
of a close pair in the PS1 image.
The Gaia object appears to be the southern component
of the pair.
200029.264 +345308.30 (2000.0) Gaia_EDR3_2059315910815578496 plx=-(-) dismod=- pmra=-(-) pmdec=-(-) G=21.008 BP=21.178 RP=19.371
The outbursting object may not be related to them.
ASASSN-22jz: revised period of early superhumps
Using the period of ordinary superhumps, I re-analyzed
the data reported in [vsnet-alert 26907]. The correct
period of early superhumps was an one-day alias
to vsnet-alert 26907. P(ESH)=0.05700(3) d.
PS1-3PIJ035747.16-063851.1 = Gaia DR3 324488617195639360 = ASASSN-22kc = ZTF19abuskjw: new SU UMa-type dwarf nova
Josch Hambsch and Itoh-san have reported observations.
The object shows superhumps with a period of 0.05761(3) d
(amplitude 0.10 mag).
MASTER OT J001204.00-412337.4: rebrightening
Josch Hambsch has detected a rebrightening on Aug. 17.
Having unusual outburst property, this object deserves
continuous attention and time-resolved photometry.