Flipped back to M13, did the same thing for those transforms as I did for M92: u'-u, g'-g, r'-r, i'-i, z'-z.
Now went to overlays. Added u'u, r'-r, i'-i, and z'-z to g'-g from Monday.
7/06:
Moved to color-color plots. Made several for M13: u-g, g-r, g-i, and r-i.
Next, I overlaid PM members onto the transforms for M13: u'-u, g'-g, r'-r, i'-i, and z'-z.
Back to M13 color-colors - this time I made residuals for the above plots: g-r, g-i, and r-i (u-g is so bad it's useless to plot a residual).
Got new data from Zeljko, plotted a comparison of the residuals of g'-r' Vs. g-r for M13, M92, and Zeljko's field stars (which have no error or sep estimates, and are not a part of a cluster-so no CMD cut either).
Took the linear fit from the full 0 to .2 degree field for M13, then plotted the residuals of the individual .05 degree annuli
to the line and found the median residual. Did the same for r'-r.
Looked at M13's turnoff and giant branch next, plotting the same things for g'-g and r'-r again.
7/07:
Did the median residual plots for M13's i'-i and z'-z on the horizontal branch, and for i'-i and z'-z on the turnoff/giant branch. Figured u'-u
was a lost cause, so didnt bother making those plots.
Went to M92, made g'-g and r'-r for the HB.
Spent quite awhile trying to match up the field stars, but I finally got it. The result is a field/M92/M13 transform overlay.
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