[vsnet-alert 18045] Re: bright outburst of 2QZ J015940.6-281040 in ASAS-SN data

Patrick Schmeer pasc1312-aavso at yahoo.de
Tue Dec 9 17:18:57 JST 2014


In 2005 I reported this set of ASAS data of the
2003 outburst to Ron Downes. He then added
the following lines in the Catalog and Atlas of
Cataclysmic Variables:
"Magnitude Range: 12.0 V - 19.7 b
Notes: large outburst (Schmeer, private
communication) indicates ug or ugwz type
Last Updated: 2005-10-11"
http://archive.stsci.edu/prepds/cvcat/query_processor.cgi?setup_file=varcat.setup.cgi&query_decision=single_record&uid=8553&query_select=everything

Regards,
Patrick

--------------------------------------------
Taichi Kato <tkato at kusastro.kyoto-u.ac.jp> wrote:

Subject: [vsnet-alert 18042] Re: bright outburst of 2QZ J015940.6-281040 in ASAS-SN data
  
Re: bright outburst of 2QZ J015940.6-281040 in ASAS-SN data
 
This object was recorded in bright outburst in ASAS-3 data in 2003.
 
YYYYMMDD(UT)   mag  observer
20030619.4205 <14.50V  (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
20030619.4205 <14.50V  (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
20030619.4205 <14.50V  (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
20030622.3791 12.084V  (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
20030622.3791 12.113V  (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
20030622.3791 12.120V  (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
20030630.3847 12.880V  (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
20030630.3847 12.889V  (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
20030630.3847 12.997V  (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
20030710.3264 <14.50V  (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
20030710.3264 <14.50V  (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
20030712.3685 <14.50V  (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
20030712.3685 <14.50V  (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
20030712.3685 <14.50V  (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
 
The outburst was most likely a superoutburst (even a WZ Sge-type outburst).
Time-series observations of the current outburst are encouraged!


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