Next went to color-color. Here's a diagram of the residuals from the plot, with different colors indicating different annuli as before. Now full color-color residuals from the whole dataset. The color color plot of the BHB stars without the residuals is also informative. Just to confirm, plotted g'-r' Vs r'-r with fits.
Turned my attention to M92, plotting the first color-color plot of Clem's ugriz and u'g'r'i'z' data. The plot seems to have a slight upward curve to it.
Finally, got the annuli program to work on it, and plotted the color-color with the annuli marked and linear fitted.
6/30:
Plotted the residuals to a 45 degree line for the color color diagram of M92, color coded like the other plots.
Went back to M13, made g'-r' vs g'-g transform plots for stars far away from the center of the cluster. Made more transforms: here's u'-u, i'-i, and z'-z for the horizontal branch. Did the transforms again for all the stars: u'-u, g'-g, r'-r, i'-i, and z'-z.
Switched again to M92. Made lots of transforms: u'-u, g'-g, r'-r, i'-i, and z'-z, all against g'-r'.
The above plots had a few outliers that made it hard to tell what was going on in the meat of the data, so i cut them out
and plotted the transforms again (for all but u'-u, where the data was so weird I decided not to clip any of it):
g'-g, r'-r, i'-i, and z'-z.
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