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Re: Soliciting criticism
Just looking at the thumbnail pictures of the two graphs
I can see the slopes are diferent. I think you have a good,
graphic and intuitive way to compare data reduction pipelines.
You want all the green and red points to lie on a straight
horizontal line on the bottom of the graph.
sps2x uses,sps2x uses, I think PSF fitting while sextrator does aperature
photometery. I think PSF fitting while sextrator does aperature
One thing required by the psf fitting technique is a good psf
"Creager, Robert S" wrote:
> > Hey folks,
> > I'm hoping some of you have the desire to critique, and offer suggestion
> > about the graphs here: http://robertcreager.mystarband.net/ . The are all
> > from Tom's data, night 2157 (from a few weeks ago). As the graph titles
> > imply, one is reduced from source extractor, and one from sps2x.
> > Speaking of source extractor, does anyone have a set of values which might
> > be appropriate for reducing Mark IV images? I grabbed Glenn Gombert setup
> > from 1996, but at this point, I'm shooting in the dark as to how to
> > improve the reduction. If anyone wants to direct, I'll be happy to make
> > changes and keep re-running the reduction. It takes about 4 hours from
> > start to finish for reducing night 2157, so I can get two runs per day at
> > home.
> > The basic steps are:
> > * Create master dark and flats from median data
> > * Adjust the object data by: mean * (object[i][i] - dark[i][j] ) /
> > flat[i][j] where mean is the mean of a central box of the flat field
> > * Do the reduction (sps2x, source extractor) in V-I pairs
> > * Match the reduction data to transform into ra/dec
> > * Try to match both to subset of Tycho2 data
> > * If both match, use in next step
> > * If only one matches, match other band to the matching one to
> > calculate ra/dec
> > * Collate the V-I pairs from previous
> > * Solve for magnitude adjustment from collated data
> > * Use stars which match the Tycho2 subset
> > * Fit a line to the raw color (V-I) vs. magnitude delta (Tycho2 -
> > measured) for each V and I
> > * Iterate over the line fit, removing 4 sigma data, until either no
> > more data was removed, we've removed too much data (10% removed) or the
> > RMS error is below 0.05
> > * Import star list into database, and match stars within 0.004
> > degrees.
> > * Produce graphs included from the previous data
> > The majority of the stars in the graph have 30+ measurements.
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