Table 12
PACS fluxes with 1σ errors of non-excess sources, together with the photospheric predictions (Sλ).
| HIP | SpT | PACS70 | S70 | χ 70 | PACS100 | S100 | χ 100 | PACS160 | S160 | χ 160 | Ld/L⋆ | MIPS70 |
|
|
||||||||||||
| 910 | F5V | 29.51 ± 0.19 | 17.66 ± 1.38 | 14.46 ± 0.09 | 2.32 | <7.5 | 5.61 ± 0.04 | 8.9e-07 | 37.50 ± 4.48 | |||
| 2941 | K1V+... | 24.09 ± 0.43 | 11.20 ± 1.82 | 11.80 ± 0.21 | –0.33 | <5.7 | 4.61 ± 0.08 | 2.0e-06 | 25.80 ± 11.93 | |||
| 3093 | K0V | 21.93 ± 1.69 | 22.50 ± 0.34 | –0.33 | 8.21 ± 1.23 | 11.02 ± 0.17 | –2.26 | 3.76 ± 3.43 | 4.31 ± 0.07 | –0.16 | 1.7e-06 | 14.90 ± 5.69 |
| 3497 | G3V | 7.97 ± 0.95 | 8.72 ± 0.10 | –0.78 | 5.23 ± 1.01 | 4.27 ± 0.05 | 0.95 | <4.8 | 1.67 ± 0.02 | 2.8e-06 | 5.20 ± 4.41 | |
| 3821 | G0V SB | 131.05 ± 2.06 | 60.80 ± 2.04 | 64.21 ± 1.01 | –1.50 | 15.75 ± 2.66 | 25.08 ± 0.39 | –3.47 | 3.3e-07 | 122.3 ± 10.74 | ||
Notes.The significance at each band is given. Figures without errors in the PACS160 column give 3σ upper limits. Figures in the column Ld/L⋆ give upper limits of the fractional luminosity of the dust. The last column gives Spitzer fluxes at 70 μm. Units for fluxes and photospheric predictions are mJy. Only the first 5 lines of the table are given here. The full version is available at the CDS.
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