Table 13: Comparison with MACHO photometry for the non-variable stars with 18.25<V<21, from Alves subsample.
Bin $\langle \Delta V\rangle $ $\sigma$ N
Field A
18.25-18.50 0.030 0.027 123
18.50-18.75 0.032 0.030 133
18.75-19.00 0.024 0.031 188
19.00-19.25 0.035 0.037 502
19.25-19.50 0.037 0.042 673
19.50-19.75 0.013 0.049 329
19.75-20.00 0.035 0.063 327
20.00-20.25 0.035 0.065 445
20.25-20.50 0.033 0.098 603
20.50-20.75 0.054 0.110 753
20.75-21.00 0.045 0.129 826
Field B
18.25-18.50 0.001 0.030 98
18.50-18.75 0.012 0.034 115
18.75-19.00 -0.001 0.032 164
19.00-19.25 0.014 0.040 438
19.25-19.50 0.028 0.055 426
19.50-19.75 0.019 0.060 268
19.75-20.00 0.017 0.057 280
20.00-20.25 0.020 0.074 373
20.25-20.50 0.027 0.087 466
20.50-20.75 0.041 0.119 647
20.75-21.00 0.057 0.116 694

Notes: $\langle \Delta V\rangle = \langle V_{\rm this~paper}-V_{\rm Alves}\rangle$.


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