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,...
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...
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 3:09 pm
585
Z UMi has commenced a fade: 17 Nov 1749GMT A(2)V(1)B 11.3 C8 22 Nov 2214GMT equal B 11.4 C8 28 Nov 2034GMT B(1)V(3)C 11.7...
EnootnhoJ@...
Dec 4, 2005 5:09 pm
586
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 ...
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
588
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
589
... AM Her may be the best covered, but one of the most interesting is BY Cam, which I've been monitoring visually for just over ten years. There is a light...
... 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...
Arne, thank you for the sequence data file... I should have started with you! however, just a tiny little problem that I need to solve.... I can never open...
... pure ASCII text files, space delimited. You can change the name to j0854.txt or something and see if that helps. Often Windoze assumes a particular...
2005 Dec 6.870 15.9C Best regards, Jeremy Shears _________________________________________________________________ Be the first to hear what's new at MSN -...
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...
V701 Tau has faded since I last saw it 2 nights ago. I have just started a time series at 21.45UT on 2005 Dec 8 and it's at 15.6C (however, since I have only...
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 ...
W Cyg is very faint and AF Cyg is very bright at the moment: W Cyg Latest observation: 8 Dec 1005 1837GMT K(4)V(1)L 7.4 12X50B I have been...
EnootnhoJ@...
Dec 9, 2005 12:15 pm
600
John, I had the same estimates as you on the night of 6th December 2005 at 1845UT for AF Cyg and 19.45UT for W Cyg. Looking back at my estimates of AF Cyg I...
Scatter in red stars by visual observers is quite normal and sometimes it can amount to as much as a magnitude. This is due to the individual observers ...
EnootnhoJ@...
Dec 11, 2005 12:18 am
603
Issue #5700 of The Information Bulletin on Variable Stars contains information on 20 new variable stars discovered by BAA member Martin Nicholson. ...
Des, I only observe red variables at 10 day intervals and try to avoid doing them in moonlight as red stars generally appear brighter (compared with non red ...
EnootnhoJ@...
Dec 13, 2005 9:22 pm
605
150 years ago, on December 15th, J. R. Hind discovered U Gem while searching for asteroids in Gemini. To honor U Gem's century and a half of amazing, ...
Visual magnitude estimate by P. Schmeer, Bischmisheim, Germany: UMABZ 20051217.895 116 SPK Sequence: AAVSO Instrument: 203-mm SCT Regards, Patrick ...
Patrick Schmeer
pasc1312-aavso@...
Dec 17, 2005 9:37 pm
607
BZ Uma was reported in outburst earlier this evening by Patrick Schmeer. This is a (proposed) UGSU star, although a superoutburst with superhumps has never...
BZ UMa this evening... Dec 17.941 11.3 18.004 11.3 BZ UMa is a ROP star. The last outburst occured on Jan 16, 2005. There is still some debate as to...
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