--- Alon Retter <ar@astro.keele.ac.uk> wrote: (in part) The full amplitude of the variation was ~0.03 mag, so I don't expect that amateurs will be able to detect it. In addition, in outbursts, I believe that it might be even more difficult to observe it due to the noise. === While finding a 0.03 mag periodic variation in lots of noise may be difficult, it certainly is not impossible. The variation in XTE J1118+480 is only about twice that and it was immediately apparent in its light curves - which have a lot of intrinsic scatter due to its 9.9 second flickering. By running a period finding routine (such as is available from GEA in their AVE package) on the data you can find those periodic variations. By phase averaging the data, you can plainly see the nature of the variation. See the curves on my XTE J1118+480 web page for an example. DO LOOK for those periodic wobbles. While they may be more subtle than being run over by a truck, you can find them! ===== Regards, Lew === NEW! HOT Star! Shines in X-Rays!=== Check out Lew's work on "The noisiest star in the Universe" http://vsnet.lewcook.com/xte1118.htm __________________________________________________ Do You Yahoo!? Send instant messages & get email alerts with Yahoo! Messenger. http://im.yahoo.com/