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Announcement: New Applications
We are excited to announce the launch of our new applications! We're opening up early access to our new applications for searching, downloading, and submitting photometric observations. You can now access these applications through these links:
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One of the criteria used by Taichi Kato in his paper is:
"the presence of early superhumps (reflecting the 2:1 resonance) and long or multiple rebrightenings are the best distinguishing properties of WZ Sge-type dwarf novae."
I suspect the reason for not including this star is that such early superhaumps have not been detected (yet)
We must continue to observe (when weather permits!!!!!!)
Kind regards
Stephen [HSP]
Hi Eddy
Where can I access this paper? Thanks
Stephen [HSP]
Look at the CVnet
Hi Stephen,
Look at the CVnet site.
Regards,
Eddy
Thanks, Eddie. Got it.
XY Psc is given as UG: in VSX. Is it proven to be a UGWZ? If so, do you have a refrence?
Stephen [HSP]
No Stephen it's not proven but it looks like it is a UGWZ. Look at :
http://www.konkoly.hu/cgi-bin/IBVS?5140
Cheers,
Eddy
One of the criteria used by Taichi Kato in his paper is:
"the presence of early superhumps (reflecting the 2:1 resonance) and long or multiple rebrightenings are the best distinguishing properties of WZ Sge-type dwarf novae."
I suspect the reason for not including this star is that such early superhaumps have not been detected (yet)
We must continue to observe (when weather permits!!!!!!)
Kind regards
Stephen [HSP]