Table 1

Fraction of spurious detections.

EXI_ML Fraction bin all-sky Error Fraction NEP Error
(spurious, objects)

6.57.0 0.63 (11162, 17709) 0.03 0.34 0.08
7.07.5 0.55 (7657, 13989) 0.03 0.29 0.08
7.58.0 0.46 (4996, 10826) 0.03 0.15 0.06
8.08.5 0.40 (3475, 8612) 0.03 0.12 0.05
8.59.0 0.30 (2134, 6982) 0.02 0.12 0.06
9.09.5 0.23 (1311, 5692) 0.02 0.09 0.05
9.510.0 0.18 (869, 4685) 0.02 0.06 0.04
10.010.5 0.14 (555, 3917) 0.02 0.05 0.04
10.511.0 0.10 (326, 3373) 0.02 0.04 0.04
11.011.5 0.07 (193, 2908) 0.01 0.02 0.02
11.512.0 0.06 (148, 2548) 0.01 0.02 0.02
12.012.5 0.04 (84, 2245) 0.01 0.02 0.02
12.513.0 0.02 (45, 1993) 0.008 0.01 0.02
13.013.5 0.02 (36, 1805) 0.008 0.00 0.00
13.514.0 0.008 (13, 1637) 0.006 0.00 0.00
14.014.5 0.006 (9, 1553) 0.005 0.00 0.00
14.515.0 0.001 (2, 1437) 0.001 0.00 0.00

Notes. The first columns lists the EXI_ML bin. The numbers given in brackets refer to the number of spurious and catalogue objects in that EXI_ML bin. The error to the spurious detection per bin is given in the third column. Columns 4 and 5 give the fraction of spurious detections and the error for exposure times greater than 4000 s (fields close to NEP). We note that we here only consider fields without masked regions.

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