Table 2: Photometric completeness f and the associated $1~\sigma$ uncertainty, both in percent, in the four regions in which we have divided our NGC 6218 field.
  Centre Ring 1 Ring 2 Ring 3
V f $\sigma$ f $\sigma$ f $\sigma$ f $\sigma$
18.25 91 2 94 1 95 2 96 1
18.75 86 3 93 2 94 2 96 1
19.25 79 6 92 4 93 2 95 1
19.75 76 5 90 2 91 1 94 1
20.25 75 4 86 4 89 1 92 1
20.75 67 7 82 2 86 2 90 1
21.25 59 9 77 2 83 2 88 2
21.75 47 6 70 2 80 2 84 2
22.25 34 5 62 5 74 2 80 2
22.75 22 4 48 4 63 2 72 1
23.25 13 4 31 3 49 3 59 2
23.75 6 3 18 3 33 2 42 2
24.25 2 1 7 3 19 4 23 2


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