Below are a bunch of histograms of the distribution of the data (white) and randoms (green) for the two methods I have tried for making randoms, mine and Shirley's. You'll notice that the spectroscopic randoms mismatch the spectroscopic data much more than the photometric data/randoms (for both methods). This makes me perhaps think there is a problem with the mask I am using for the spectroscopic set. Martin White made this mask for me.. I've ask for a meeting with David this afternoon to look at this in more detail.
My randoms
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I've tried zooming in on regions in the data where the mismatch is greatest. For instance ( dec > 40, 110 < ra < 130). I've posted these on the blog too.
It does look like there are regions where there are data and not randoms, which would suggest a problem with the mask. (Note that the regular spacing of the randoms is because this is how Shirley generates randoms, by putting an object in the center of the grid). I plotted these because it is easier to see with the regular spacing that regions have been missed. For instance at ra ~129.4, dec ~ 49.4, There are several data points (red), but but randoms (blue). You can click on the below pictures to make them bigger.
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