[vsnet-campaign-dn 15323] MASTER OT J172758.09+380021.5 outburst (since Feb. 8)
Patrick Schmeer pasc1312-aavso@yahoo.de via vsnet-campaign-dn
vsnet-campaign-dn at ooruri.kusastro.kyoto-u.ac.jp
Tue Feb 9 19:39:43 JST 2021
MASTER OT J172758.09+380021.5 (UGSU, EI Psc star?)
https://www.aavso.org/vsx/index.php?view=detail.top&oid=359271
Zwicky Transient Facility (ZTF) light curve and data:
https://lasair.roe.ac.uk/object/ZTF18aaiytds/
Recent 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/366ccedb-a673-4369-8728-7db8a373b623
The current outburst was also detected by Maeda-san (and
reported two hours ago, see vsnet-outburst 26607):
http://ooruri.kusastro.kyoto-u.ac.jp/mailarchive/vsnet-outburst/26607
Clear skies,
Patrick
-------
Am Donnerstag, 12. November 2020, 01:31:02 MEZ hat Taichi Kato <tkato at kusastro.kyoto-u.ac.jp> Folgendes geschrieben:
MASTER OT J172758.09+380021.5 outburst
According to the ZTF data, this object is not an ordinary
SU UMa star (see vsnet-alert 23720, 24112).
2018 Mar-Apr. superoutburst: two post-superoutburst rebrightenings
and a slow fading tail like a WZ Sge star.
2018 July-Aug. superoutburst: deep dip in the middle of
a superoutburst.
2019 Jan.-Feb: long rebrightening.
Currently, the supercycle appears to be ~70 d.
Thorstensen's spectrum did not show enhanced helium lines.
This object probably needs to be studied in detail.
(Could it be a WZ Sge star mimic or EI Psc-type object?)
YYYYMMDD(UT) mag observer
20201023.1179 17.890zr (Zwicky Transient Facility Lasair (Masci+ 2019))
20201028.1181 17.977zr (Zwicky Transient Facility Lasair (Masci+ 2019))
20201101.1589 16.600zr (Zwicky Transient Facility Lasair (Masci+ 2019))
20201104.0811 18.009zr (Zwicky Transient Facility Lasair (Masci+ 2019))
20201111.1389 14.521zr (Zwicky Transient Facility Lasair (Masci+ 2019))
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