Table 2
Herschel/PACS 70, 100, and 160 μm fluxes for our sample stars.
Source | F70μm ± σ (Jy) | qF70μm | F100μm ± σ (Jy) | qF100μm | F160μm ± σ (Jy) | qF160μm |
---|---|---|---|---|---|---|
Cyg OB2#7 | – | – | – | |||
HD 66811 | 0.32 ± 0.045 | A | 0.220 ± 0.025 | A | 0.3 ± 0.1 | B |
Cyg OB2#11 | ≲0.253 | U | ≲0.51 | U | ≲2.53 | U |
HD 210839 | 0.07 ± 0.01 | A | 0.06 ± 0.01 | A | 0.06 ± 0.03 | B |
HD 151804 | 0.092 ± 0.011 | A | 0.076 ± 0.01 | A | ≲0.03 | U |
HD 152408 | 0.16 ± 0.02 | A | 0.14 ± 0.02 | A | – | |
HD 149404 | 0.147 ± 0.017 | A | 0.18 ± | B | ≲0.67 | U |
HD 30614 | 0.07 ± 0.01 | A | 0.042 ± 0.005 | A | – | |
HD 37128 | 0.32 ± 0.04 | A | 0.212 ± 0.025 | A | ≲0.43 | U |
HD 38771 | 0.122 ± 0.015 | A | 0.063 ± 0.01 | A | – | |
HD 154090 | 0.058 ± 0.008 | A | 0.038 ± 0.005 | A | – | |
HD 193237 | 1.4 ± 0.1 | A | 1.27 ± 0.13 | A | 0.875 ± 0.075 | A |
HD 24398 | 0.093 ± 0.013 | A | 0.043 ± 0.006 | A | ≲0.054 | U |
HD 169454 | 0.21 ± 0.03 | A | ≲0.36 | U | – | |
HD 152236 | 0.34 ± 0.04 | A | ≲0.8 | U | – | |
HD 190603 | – | – | – | |||
HD 41117 | 0.07 ± 0.01 | A | 0.045 ± 0.006 | A | – | |
HD 194279 | 0.046 ± 0.020 | B | 0.0167 ± 0.008 | B | – | |
HD 198478 | 0.086 ± 0.017 | A | 0.043 ± 0.006 | A | – | |
HD 80077 | 0.135 ± 0.017 | A | 0.14 ± 0.07 | B | – | |
HD 53138 | 0.08 ± 0.01 | A | 0.054 ± 0.007 | A | ≲0.0345 | U |
Cyg OB2#12 | 0.49 ± 0.06 | A | 0.44 ± 0.08 | A | ≲1.98 | U |
HD 24912 | 0.045 ± 0.007 | A | 0.034 ± 0.004 | A | ≲0.041 | U |
HD 36861 | 0.024 ± 0.008 | A | 0.020 ± 0.012 | B | – | |
HD 37043 | 0.019 ± 0.006 | B | – | – | ||
HD 149757 | 0.079 ± 0.011 | A | 0.041 ± 0.005 | A | ≲0.054 | U |
HD 149438 | 0.053 ± 0.06 | A | 0.039 ± 0.005 | A | ≲0.067 | U |
Notes. Sources are listed as in Table 1. The 1σ error of the flux includes the uncertainty in flux calibration from PACS, the error in the photometric procedure and the error arising from the apertureand colour corrections (see Sect. 2). The quality of each of these flux densities is designated by the quality flags (qFλ) and is either of high quality (qFλ = A; S∕N ≥ 10), of moderate quality (qFλ = B; 5 ≤ S∕N < 10), or an upper limit (qFλ = U; S∕N ≤ 5 and/or confused detection).
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