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(cba:news) TT Ari, take 1... and filter selection (Joe Patterson) [2009-10-23T21:39:30Z]



Or at least publicly take one. We decided to jump out with a quick "what we learned on the first day" note, and here it is:

	http://www.astronomerstelegram.org/?read=2254

I limited the author list to those with light curves coincident with the X-ray observation. However, there are some really beautiful light curves rolling in now, and such beauties are hard to keep cooped up in a computer for long. We'll figure out some way to get 'em out in the light of day pretty soon.

At this early stage, the ~0.38 day waves are the most interesting aspect of the light curve, and this timescale forces us to worry about how we take our data. In particular, our longest/best light curves last 8-9 hours, and this is practically the same as the signals we wish to measure. Thus uncorrected extinction effects will certainly contaminate our data. It's *differential* extinction that matters, and this can be pretty large for clear-filter data, since the effective wavelength for TT Ari will be much bluer than that for an average field star (about 0.10 mag/airmass). I can satisfactorily correct your data if you supply the airmass - and the need is minimal if you observe in a decently narrow band (like V). So one of those strategies would be helpful. But if software/hardware limitations mean that you're a clear-filter guy, that's all right. I learn a lot about how to make these corrections from experience.

It remains desirable, IN PRINCIPLE, to get B and I - or some similar well-spaced blue and infrared - light curves. But we already know roughly that the light curves are similar - as is true for practically every CV. So no quick riches for this approach. Nevertheless, really extensive coverage like this would probably teach us a lot; I don't recommend it, but a very extensive set of B/I light curves would make a liar out of me.

Whew, tomorrow I promise to cover the rest of the CV goodies in the October sky.

joe