Table 3: Galactic column density (from Dickey & Lockman 1990), BMW count rates and fluxes for galaxies in the complete serendipitous sample, ordered by increasing flux.
LEDA name $N_{{\rm H}}$ Count rate F0.5 - 2
  (1020 cm-2) (10-3 count s-1) (10-13 erg cm-2 s-1)
0157406 4.9 0.37$\pm$0.07 0.12$\pm$0.02
0068536 2.5 1.11$\pm$0.34 0.32$\pm$0.09
0025825 4.2 1.12$\pm$0.22 0.35$\pm$0.06
0042833 2.0 1.31$\pm$0.23 0.35$\pm$0.05
0028990 0.8 1.50$\pm$0.30 0.36$\pm$0.07
0005323 3.8 1.33$\pm$0.28 0.41$\pm$0.09
0010446 3.1 1.48$\pm$0.24 0.43$\pm$0.06
0057078 2.3 1.63$\pm$0.28 0.44$\pm$0.08
0069338 8.8 1.24$\pm$0.20 0.46$\pm$0.07
0038773 2.0 1.70$\pm$0.11 0.46$\pm$0.03
0001333 4.2 1.55$\pm$0.27 0.48$\pm$0.09
0007289 5.5 1.71$\pm$0.26 0.56$\pm$0.10
0070861 2.6 2.11$\pm$0.38 0.61$\pm$0.12
0018991 5.4 2.18$\pm$0.32 0.70$\pm$0.10
0004117 4.0 2.36$\pm$0.23 0.73$\pm$0.06
0043675 3.9 2.49$\pm$0.37 0.77$\pm$0.12
0002204 1.9 3.23$\pm$0.23 0.87$\pm$0.05
0045318 1.0 3.78$\pm$0.60 0.91$\pm$0.14
0046432 3.2 3.13$\pm$0.66 0.91$\pm$0.20
0047432 2.3 3.61$\pm$0.64 0.97$\pm$0.16
0130966 2.4 4.41$\pm$0.81 1.19$\pm$0.22
0016574 5.9 3.73$\pm$0.51 1.23$\pm$0.17
0005324 3.8 4.34$\pm$0.51 1.35$\pm$0.16
0057728 1.5 5.11$\pm$0.39 1.38$\pm$0.11
0013368 1.4 7.22$\pm$1.41 1.73$\pm$0.24
0029050 0.8 10.20$\pm$0.70 2.45$\pm$0.17
0002362 2.7 9.06$\pm$0.99 2.63$\pm$0.29
0004848 6.1 9.26$\pm$2.43 3.06$\pm$0.66
0063122 7.9 11.02$\pm$1.42 3.97$\pm$0.36
0006367 3.0 14.80$\pm$0.60 4.29$\pm$0.17
0017451 7.5 15.66$\pm$1.72 5.64$\pm$0.72
0028995 4.8 34.20$\pm$2.00 10.94$\pm$0.64


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