[vsnet-alert 23874] Re: ATO J061.1478-31.0634 = Gaia19fes: orbital period

[Patrick Schmeer pasc1312-aavso@yahoo.de via vsnet-alert]

 ATO J061.1478-31.0634 (UGSU:)
https://www.aavso.org/vsx/index.php?view=detail.top&oid=1499859

Should we take 0.122641(4) d as the orbital period?
And has the UGSU classification been confirmed?
The two recorded outbursts were shorter than
usual superoutbursts of SU UMa-type dwarf novae
(which typically last ~14 days) – e.g. the one in 2019
November lasted only 7 days.
 
Regards,
Patrick
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     Am Donnerstag, 26. Dezember 2019, 00:35:31 MEZ hat Taichi Kato <tkato at kusastro.kyoto-u.ac.jp> Folgendes geschrieben:  
 
 ATO J061.1478-31.0634 = Gaia19fes: orbital period

  Berto Monard reported time-resolved photometry
mainly following the outburst.
The object shows almost sinusoidal (full amplitude
0.09 mag) orbital variations.  The period has been
determined to be 0.122641(4) d (one-day alias of
the previously reported period).