ASASSN-14fe: new SU UMa-type dwarf nova
Berto Monard have reported observations. The data confirmed long-period (more than 0.08 d) superhumps. Re-analysis of the 2020 data yielded the most likely period of 0.08908(6) d (allowing one-day aliases) and an amplitude of 0.12 mag. The 2020 data were also obtained by Berto Monard. Let's hope that the correct alias will be established during the current superoutburst.
ASASSN-14fe (UGSU) https://www.aavso.org/vsx/index.php?view=detail.top&oid=399142
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/0b4de1f5-3a4c-4ce5-a276-0cf169...
The recent superoutburst started on 2022 January 28. A rapid fading occurred on February 9.
Regards, Patrick ------- T. Kato wrote (vsnet-alert 26564):
ASASSN-14fe: new SU UMa-type dwarf nova Berto Monard have reported observations. The data confirmed long-period (more than 0.08 d) superhumps. Re-analysis of the 2020 data yielded the most likely period of 0.08908(6) d (allowing one-day aliases) and an amplitude of 0.12 mag. The 2020 data were also obtained by Berto Monard. Let's hope that the correct alias will be established during the current superoutburst.
vsnet-outburst@ooruri.kusastro.kyoto-u.ac.jp
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Patrick Schmeer -
Taichi Kato