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Re: Analyzing Data
Tom,
I suspect that a very successful minor modification to the
WS statistic would be for it to calculate residuals from a
given night's mean magnitude instead of a global mean magnitude.
This would get rid of the effects of zero-point changes which
aren't currently calibrated out.
Cheers,
Doug
On Sun, 4 Aug 2002, Tom Droege wrote:
> Since I did not get data last night, I spent some time this morning looking
> at data I took on August 2. A first look had found just 3 variable
> stars. This applying WS and looking at those with large statistic. > 10 I
> recall.
>
> This morning I reprocessed the data and looked at WS > 1. I found 13
> pretty likely variables. One with a WS statistic of 1.2.
>
> When I send out data sets, they contain a number of evenings of
> observations for each star. This causes WS to generate big numbers for
> what amounts to day to day variations, or for long term variation. This
> swamps the short term variations, so if you look at the data the way I have
> passed it out, it is hard to find the short term variables where the
> variation is small.
>
> I started thinking about this when I noticed that we were finding mostly
> variables abound mag 10 and lower. There should be more around mag
> 11-13. So why was I not finding them?
>
> The answer is that they are there, one just has to look carefully with
> something better than WS. OK, Doug has done a good job getting us a start,
> but something more is needed, I think. We need a way to look at the data
> with WS over 1 and see what I can see if I look at it by eye.
>
> Sometimes there is a big WS statistic and one look shows it is due to 1 bad
> point. Well, it may be real, but not likely. Mostly stars are not
> expected to brighten .2 mag for one measurement point. So one can throw
> such things out. But something has to look and see what is happening.
>
> I think there is a lot of work to be done to develop better algorithms to
> find the variables.
>
> Tom Droege
>
>