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[vsnet-alert 6398] Re: WZ Sge results of August 21/22 run at CBA Belgium



Hi Tonny et al,

Observations here in Kaitaia more or less confirmed what you said. I ran
from 22 August 0706 UT to about 1110 UT when cloud suddenly arrived. The
humps were ~0.05 at around phase 0.4. Two eclipses were visible, the third
was a little distorted. Overall, the star fell by about 0.12 in 4 hours. I
used a 10 second exposure time but should have stuck with the 20 seconds
I've been using lately. The S/N ratio might have been better. The weather
doesn't look promising at the moment but let's hope.

Regards,
Stan


----- Original Message -----
From: <tonny.vanmunster@wanadoo.be>
To: <vsnet-alert@kusastro.kyoto-u.ac.jp>;
<vsnet-campaign@kusastro.kyoto-u.ac.jp>;
<vsnet-superoutburst@kusastro.kyoto-u.ac.jp>
Cc: <news@cba.phys.columbia.edu>
Sent: Wednesday, August 22, 2001 11:48 PM
Subject: WZ Sge results of August 21/22 run at CBA Belgium


> Dear colleagues,
>
> I have just uploaded the August 21/22 light curve of WZ
> Sge, that I obtained at CBA Belgium Observatory, to my
> web site (see address below).
>
> It was not a particularly favourable photometric night,
> hampered also by low clouds. I nevertheless managed to
> collect a dense time-series, over a period of about 6
> hours. The resulting light curve clearly shows a number
> of interesting features. First, the rebrightening of WZ
> Sge, which was still very obvious in the hours
> preceding our observations, seems to have come to an
> end. The superhumps are much smaller than in any of our
> previous observing nights, having an amplitude
> of \'barely\' 0.06 mag. In between superhumps, there are
> a number of dips. The most pronounced dip (the one
> immediately preceding the superhump peaks) likely is to
> be attributed to eclipses.
>
> Best regards,
> Tonny Vanmunster
> CBA Belgium Observatory
> http://vsnet.lunarpages.com/cbabelgium
>
> ------------------------------------------------------------------
> This mail sent through Wanadoo WebMail: http://webmail.wanadoo.be/
>

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