Dear colleagues,
I have just finished analysing my unfiltered CMOS observations of MASTER OT
J052622.61+734629.7, obtained on 2021, September 03/04 at CBA Belgium
Observatory, using a 0.40-m f/10.0 telescope and QHY-268M CMOS camera under
clear skies.
Regular superhumps with an amplitude of 0.29 mag are clearly visible in the
resulting light curve, establishing MASTER OT J052622.61+734629.7 as a new
SU UMa-type dwarf nova. A period analysis using the ANOVA, Lomb-Scargle,
Generalized-Lomb-Scargle and PDM methods (Peranso 3.0), yields a combined
superhump period of 0.0665 +/- 0.0003d. The object was at mag CV = 16.2 on
Sep 04th.
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
ASASSN-19wz possible superoutburst
Past ZTF data suggest an SU UMa star (possible superoutburst
in 2020 Nov.).
YYYYMMDD(UT) mag observer
20210901.2558 15.276zg (Zwicky Transient Facility Lasair (Masci+ 2019))
NSV 1440 (AM CVn star)
Orbital period: 0.0252329 d (36.3354 min)
https://www.aavso.org/vsx/index.php?view=detail.top&oid=40064
A precursor outburst was recorded on 2021 August 26, according
to 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/7915bb9f-d7c9-4e0c-b378-02749…
The most recently observed superoutburst occurred in 2019 February.
Time-resolved photometry is urgently required.
Clear skies,
Patrick
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Am Montag, 30. August 2021, 18:23:06 MESZ hat Rod Stubbings Folgendes geschrieben:
The AM CVn-type object NSV 1440 is in bright outburst.
NSV 1440 210830.519 129
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Rod Stubbings
Tetoora Road Observatory
Victoria, Australia
Telescope: "Infinity" 22" f/3.8
stubbo(a)dcsi.net.au
http://rodstubbingsobservatory.wordpress.com/
ASASSN-21qg: new SU UMa-type dwarf nova
Berto Monard and Josch Hambsch have reported observations.
This object shows superhumps with a period of 0.05539(5) d
since Aug. 26.