Dear colleagues, The WZ Sge-star candidate, TSS 022216.4+412260 start fading. The Kyoto Team (Kubota, Imada, and Kato) detected superhump also on Nov. 27 and...
I have made a probable detection of this star, which is on the Recurrent Objects Programme: 2005 Dec 3.967 16.2C I last visited this field on 2005 Dec 29,...
Jeremy, EUVEJ0854+390 is a polar (AM Herculis star), we got the orbital period of 113.3min this year from photometry. It varies by a whopping 1.5mag over the...
Boris.Gaensicke@...
Dec 4, 2005 11:57 am
812
Outbursts and activity. CAROQ 051204.515 150 Stu.RASNZ outburst CARV436 051204.517 142 Stu.RASNZ active CETWW 051204.507 145...
Hello Boris, thanks for that information as it makes my results easier to understand. It's clearly a fascinating object. I obtained about 45 mins of time...
Dr. Boris, Do you happen to have any sequence values for the EUVEJ0854+390 field? Or anyone else for that matter... Thank you To The Stars Tim Crawford CTX ...
Jeremy, Polars tend to show large amplitude (> 0.5 mag) variations during their orbital cycle, even periodic snapshot observations, nightly or twice a week,...
Berto Monard
LAGMonar@...
Dec 5, 2005 8:55 am
816
Dear Jeremy, ... that seems about 1mag brighter than during our observations obtained at with the 2.5m INT on La Palma. ... We have two nights of good...
Boris.Gaensicke@...
Dec 5, 2005 9:28 am
817
Dear Tim, ... I don't have a sequence, but you may find the SDSS data around this object useful, which provides u,g,r,i,z magnitudes for all objects. ...
Boris.Gaensicke@...
Dec 5, 2005 9:28 am
818
... I have a BV field calibration for this SDSS CV, as I do for almost all of the SDSS CVs. I've placed this one, only based on a single photometric night, at...
Dear colleagues, The Kyoto Team (Kubota, Imada, and Kato) detect that the WZ Sge-star candidate, TSS 022216.4+412260 rebrightning now. The magnitude of the...
Kaori Kubota
kaori.k@...
Dec 6, 2005 1:28 pm
822
I have detected the Recurrent Objects Programme star, V701 Tau, in outburst in an unfiltered CCD image: 2005 Dec 6 22.11UT 15.1C Takahashi FS102, 0.1 m...
Preliminary evidence of 0.25 mag peak-to-trough superhumps with a (very preliminary) period of 0.0678 days (ANOVA method using Peranso). Note that Taichi Kato...
Arne: In your previous post- ~ than that. As Boris indicates, all of the SDSS CVs also have ~ ugriz data, and the paper by Smith et al. 2002, AJ 123,2121 ~...
... Nope. There are transformations using, say, V and (V-K) to various J-C filter passbands, but not from strictly J,H,K. You cannot extrapolate magnitude...
I imaged FS Aur over the time span JD 712.76 - 713.05. During this time it brightened 0.8 mag in 7 hrs, and at the end of the run it was 1.5 mag brighter than...
3.3hrs of unfiltered photometry tonight shows sharply-peaked superhumps still present with an amplitude of 0.2 mag. Mean magnitude = 15.4C. Period analysis ...
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