Transients in the Palomar Observatory Sky Survey

There are more stars near the ecliptic plane, therefore more emulsion flaws would be removed from the full data set, making the distribution non-random.
I agree, and that is the point I was trying to make (although probably in a hamfisted and unclear way). The distribution of emulsion flaws was presumably random before the ones closest to the ecliptic were removed.

I note that Villaroel says that only northern hemisphere plates were considered; if so that removes the big bulge in Sagittarius, which is in the southern celestial hemisphere. I may have to think again.
 
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