Table 10
Input data for the investigation of 160 μm photometric flux contamination of faint stars by background confusion.
| HD | l | b |  |
OBSIDs | f160, excess |  |
 |
 |
 |
|---|---|---|---|---|---|---|---|---|---|
| (°) | (°) | (MJy sr−1) | (mJy) | (mJy) | (mJy) | (mJy) | |||
| 148387 | 92.6 | +41.0 | 2.44 ± 0.13 | 1342186146+..47+..55+..56 | 8.5 | 106.7 ± 1.4 | 124.9 ± 2.1 | 130.7 ± 2.6 | 1.17 |
| 180711 | 98.7 | +23.0 | 6.04 ± 0.02 | 1342212497+.498+.499+.500 | 5.5 | 87.4 ± 0.9 | 91.8 ± 1.1 | 94.8 ± 1.2 | 1.05 |
| – | – | – | – | 1342222147+..48+..49+..50 | – | 90.8 ± 1.0 | 94.4 ± 1.1 | 95.3 ± 1.3 | 1.04 |
| – | – | – | – | 1342233571+..72+..73+..74 | – | 92.0 ± 1.0 | 95.9 ± 1.1 | 99.0 ± 1.2 | 1.04 |
| – | – | – | – | 1342250093+..94+..95+..96 | – | 87.2 ± 0.9 | 85.9 ± 1.0 | 84.2 ± 1.1 | 0.99 |
| – | – | – | – | 1342257987+..88+..89+..90 | – | 86.2 ± 0.9 | 91.4 ± 1.1 | 95.2 ± 1.3 | 1.06 |
| 139669 | 112.9 | +36.5 | 2.67 ± 0.07 | 1342191982+..83 | 8.0 | 61.3 ± 0.7 | 66.5 ± 0.9 | 68.4 ± 1.0 | 1.08 |
| 138265 | 95.8 | +47.4 | 1.27 ± 0.03 | 1342188841+42 | 9.0 | 30.1 ± 0.4 | 33.3 ± 0.5 | 34.9 ± 0.6 | 1.11 |
| 39608 | 269.6 | −30.9 | 5.22 ± 0.17 | 1342198535+..36+..37+..38 | 6.0 | 10.7 ± 0.2 | 13.5 ± 0.3 | 15.9 ± 0.4 | 1.26 |
| 152222 | 98.5 | +36.7 | 2.57 ± 0.15 | 1342227973+..74 | – | 8.2 ± 0.2 | 7.0 ± 0.3 | 5.9 ± 0.4 | 0.85 |
Notes. The determination of 
is described in the text. The OBSID combinations of the deepest maps are used for this investigation. f160, excess is estimated as the difference of the measured f160 minus model fmodel flux from Table 7. Listed fluxes 
are not colour corrected. Uncertainties of the flux estimates include a 1% uncertainty of the aperture correction to obtain the total flux, which is quadratically added to σaper (c.f. Eq. (2)).
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