ASASSN-24fo: new WZ Sge-type dwarf nova
ASASSN-24fo was discovered on 2024-08-25.14 by the ASAS-SN team with an
~8.5 mag outburst amplitude.
Sjoerd Dufoer and Josch Hambsch reported time-resolved observations.
These observations detected a double-waved variation with an amplitude of
0.04 mag and a period of 0.05691(5) d.
Therefore ASASSN-24fo is a new WZ Sge-type dwarf nova
Further observations are encouraged.
Best regards,
Yusuke
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South …
[View More]African Astronomical Observatory, Postdoc fellow
Yusuke TAMPO
MAIL: tampo(a)kusastro.kyoto-u.ac.jp
MAIL: yusuke(a)saao.ac.za
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Dear colleagues,
I have just finished analysing my unfiltered CCD observations of TCP
J19470832-0924198, obtained on 2024, Aug 13/14 at CBA Extremadura
Observatory using a 0.40-m f/5.1 telescope and SX-46 CCD camera under clear
skies.
The resulting light curve clearly shows the presence of superhumps with an
amplitude of 0.30 mag, establishing TCP J19470832-0924198 as a new SU
UMa-type dwarf nova. A period analysis, using the ANOVA, Lomb-Scargle,
Generalized-Lomb-Scargle and PDM …
[View More]methods (Peranso 3.0) yields a combined
superhump period of 0.0565 +/- 0.0012d. The object was at mag CV = 15.0 on
Aug 13th.
Image calibration and photometry were done using my new photometry software
Phoranso 1.0.4.6
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.co <http://www.cbabelgium.com/> m
PERANSO : The Light Curve and Period Analysis Software
http://www.peranso.co <http://www.peranso.com/> m
PHORANSO: Photometric Reduction and Analysis Software *** NEW ***
http://www.phoranso.com <http://www.phoranso.com/>
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A new eruption of the recurrent nova LMC V1341!
LMC V1341 240801.635 <140
LMC V1341 240803.666 132
LMC V1341 240803.712 132
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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/