Table 9.
Calculated source counts and associated errors for our observations of the XMM-LSS field using completeness correction Method 2.
S | Sc | N | ![]() |
FDR | Completeness | Corrected ![]() |
Completeness | Completeness | Completeness |
---|---|---|---|---|---|---|---|---|---|
(mJy) | (mJy) | (Jy1.5) | Correction | (Jy1.5) | SFG | Small | Large | ||
2.00−2.51 | 2.24 |
![]() |
![]() |
0.98 ± 0.01 |
![]() |
![]() |
![]() |
![]() |
![]() |
2.51−3.16 | 2.82 |
![]() |
![]() |
0.98 ± 0.01 |
![]() |
![]() |
![]() |
![]() |
![]() |
3.16−3.98 | 3.55 |
![]() |
![]() |
0.98 ± 0.01 |
![]() |
![]() |
![]() |
![]() |
![]() |
3.98−5.01 | 4.47 |
![]() |
![]() |
0.98 ± 0.01 |
![]() |
![]() |
![]() |
![]() |
![]() |
5.01−6.31 | 5.62 |
![]() |
![]() |
0.98 ± 0.01 |
![]() |
![]() |
![]() |
![]() |
![]() |
6.31−7.94 | 7.08 |
![]() |
![]() |
0.98 ± 0.01 |
![]() |
![]() |
![]() |
![]() |
![]() |
7.94−10.00 | 8.91 |
![]() |
![]() |
0.98 ± 0.01 |
![]() |
![]() |
![]() |
![]() |
![]() |
10.00−12.59 | 11.22 |
![]() |
![]() |
0.99 ± 0.01 |
![]() |
![]() |
![]() |
![]() |
![]() |
12.59−15.85 | 14.13 |
![]() |
![]() |
1.00 |
![]() |
![]() |
![]() |
![]() |
![]() |
15.85−19.95 | 17.78 |
![]() |
![]() |
1.00 |
![]() |
![]() |
![]() |
![]() |
![]() |
19.95−25.12 | 22.39 |
![]() |
![]() |
0.99 ± 0.01 |
![]() |
![]() |
![]() |
![]() |
![]() |
25.12−31.62 | 28.18 |
![]() |
![]() |
1.00 |
![]() |
![]() |
![]() |
![]() |
![]() |
31.62−39.81 | 35.48 |
![]() |
![]() |
1.00 |
![]() |
![]() |
![]() |
![]() |
![]() |
39.81−50.12 | 44.67 |
![]() |
![]() |
0.99 ± 0.01 |
![]() |
![]() |
![]() |
![]() |
![]() |
50.12−63.10 | 56.23 |
![]() |
![]() |
1.00 |
![]() |
![]() |
![]() |
![]() |
![]() |
63.10−79.43 | 70.79 |
![]() |
![]() |
1.00 |
![]() |
![]() |
![]() |
![]() |
![]() |
79.43−100.00 | 89.13 |
![]() |
![]() |
1.00 |
![]() |
![]() |
![]() |
![]() |
![]() |
Notes. This includes information on the flux densities of the bin, raw counts (and associated error) in the given flux density bin, source counts, and correction factors (Method 2) as described in Sects. 6.1 and 6.2. Finally the corrected source counts using these corrections are presented, as well as estimates for the completeness corrections using the models in Sect. 6.4.
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