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Re: Winter Project
Michael,
That is the plan. I have done this once before and it did not improve the
over all distribution but now that I understand that cause, perhaps it will
improve the individual star measurements.
The plan is to:
1) Group all the measurements of a star from all images together as at
present.
2) Look at the individual star measurement sets and copy the outlier (by
some definition) lines to a separate file.
3) Sort the outliers by measurement image.
4) Sort the whole data base by measurement image
5) Compute the ratio of outliers in each image as a percent
6) Add this outlier percentage to every measurement in each image by image.
Tom Droege
> [Original Message]
> From: Michael Koppelman <lolife@bitstream.net>
> To: <tdroege2@earthlink.net>
> Cc: tass <tass@listserv.wwa.com>
> Date: 10/31/2003 9:07:33 AM
> Subject: Re: Winter Project
>
> I don't know if this has been stated or not yet, but perhaps it's not
> the stars we need to flag but the images? i.e. can we determine if a
> given image is an outlier and then flag all the measurements from that
> image?
>
> Michael
>
>
> On Oct 29, 2003, at 11:51 AM, Thomas Droege wrote:
>
> > The plan is to find all the outliers - say all those measurements for
> > all
> > stars more than 3 sigma from the mean value for a star. Then compute
> > the
> > percentage of outliers in each frame. Then flag all the readings with
> > a
> > code as above. Or I might just put a number in the flag position
> > indicating the percent "outliers" which would allow you all to make
> > any cut
> > you like.
> >
> > Comments anyone?
>