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Table 2.

Constants to model the photometric uncertainty as a function of magnitude in our fields.

Hot DOGs filters β A(10−11)
g 0.903 0.789
W0410–0913 r 0.896 2.031
i 0.901 3.396

g 0.906 0.940
W0831+0140 r 0.891 3.227
i 0.902 3.386

r 0.919 0.274
W2246–0526 i 0.920 0.519
z 0.920 0.850

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