Dear colleagues,
I have just finished analysing my unfiltered CMOS observations of
ASASSN-14lb, obtained on 2021, October 08/09 at CBA Belgium Observatory,
using a 0.40-m f/10.0 telescope and QHY-268M CMOS camera under clear skies.
My observations were triggered by [vsnet-alert 26304].
Regular superhumps with an amplitude of 0.28 mag are clearly visible in the
resulting light curve, establishing ASASSN-14lb as a new SU UMa-type dwarf
nova. A period analysis using the ANOVA, Lomb-Scargle,
…
[View More]Generalized-Lomb-Scargle and PDM methods (Peranso 3.0), yields a combined
superhump period of 0.0704 +/- 0.0006d. The object was at mag CV = 16.5 on
Oct 09th.
I will send my observations to AAVSO, CBA and VSNET for further analysis.
Best regards
Tonny
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Tonny Vanmunster
CBA Belgium Observatory
CBA Extremadura Observatory
http://www.cbabelgium.com
PERANSO : The Light Curve and Period Analysis Software
http://www.peranso.com
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LL And outburst
Of course, this is a top-priority target!
The 2004 superoutburst occurred in June and no good observations
were reported.
See
https://ui.adsabs.harvard.edu/abs/2004PASJ...56S.135K/abstract
for the 1993 superoutburst. Determination of the superhump
period is very important.
YYYYMMDD(UT) mag observer
20210908.9111 <139 (Eddy Muyllaert)
20210909.701 <153 (Hiroyuki Maehara)
20210909.9424 <146 (Eddy Muyllaert)
20210910.219 <17.90C (Gary Poyner)
…
[View More] 20210910.9257 <146 (Eddy Muyllaert)
20210910.9375 <146 (Jose Ripero)
20210911.9299 <146 (Eddy Muyllaert)
20210914.901 128C (Jeremy Shears)
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