Table D.1
DUNES stars whose apparent excesses are very likely due to contamination by background galactic extended structures or extragalactic objects.
| HIP | SpT | PACS70 | S70 | χ 70 | PACS100 | S100 | χ 100 | PACS160 | S160 | χ 160 | MIPS70 |
| (mJy) | (mJy) | (mJy) | (mJy) | (mJy) | (mJy) | (mJy) | |||||
|
|
|||||||||||
| 29568 | G5V | 10.48 ± 0.19 | 7.83 ± 1.16 | 5.13 ± 0.10 | 1.92 | 8.28 ± 2.11 | 2.01 ± 0.04 | 3.00 | 15.3 ± 2.3 | ||
| 38784 | G8V | 8.66 ± 2.65 | 9.47 ± 0.10 | –0.31 | 4.19 ± 0.74 | 4.64 ± 0.05 | –0.61 | 5.98 ± 1.28 | 1.81 ± 0.02 | 3.26 | 10.6 ± 3.0 |
| 40843 | F6V | 22.59 ± 0.13 | 33.17 ± 2.76 | 11.07 ± 0.06 | 8.03 | 53.35 ± 3.17 | 4.32 ± 0.02 | 15.47 | 32.5 ± 5.3 | ||
| 71908 | F1Vp | 68.58 ± 4.16 | 38.54 ± 1.58 | 33.60 ± 2.04 | 3.13 | 13.13 ± 0.80 | |||||
| 85295 | K7V | 21.14 ± 0.46 | 12.94 ± 1.12 | 10.36 ± 0.22 | 2.30 | 14.15 ± 3.29 | 4.05 ± 0.09 | 3.07 | 13.8 ± 4.6 | ||
| 105312 | G5V | 12.44 ± 1.72 | 11.86 ± 0.66 | 0.34 | 7.84 ± 0.76 | 5.81 ± 0.32 | 2.67 | 9.20 ± 1.74 | 2.27 ± 0.13 | 3.98 | 13.6 ± 5.7 |
| 113576 | K5/M0V | 19.01 ± 0.97 | 9.43 ± 0.79 | 9.32 ± 0.48 | 0.14 | 12.66 ± 1.50 | 3.64 ± 0.19 | 6.01 | 19.1 ± 2.9 | ||
Notes.PACS and predicted photospheric fluxes, and the significance of the measured apparent excesses are given. The last column gives Spitzer MIPS fluxes at 70 μm.
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