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Table 11
SPIRE fluxes (Fλ) with 1σ errors, together with the photospheric predictions (Sλ).
HIP | F250 | S250 | χ250 | F350 | S350 | χ350 | F500 | S500 | χ500 |
(mJy) | (mJy) | (mJy) | (mJy) | (mJy) | (mJy) | ||||
|
|||||||||
544 | <22.5 | 1.20 ± 0.03 | <24.3 | 0.61 ± 0.02 | <27.6 | 0.30 ± 0.01 | |||
7978 | 312.30 ± 25.60 | 1.37 ± 0.08 | 12.15 | 179.90 ± 14.60 | 0.70 ± 0.04 | 12.27 | 78.40 ± 9.80 | 0.34 ± 0.02 | 7.97 |
13402 | <23.1 | 1.63 ± 0.03 | <23.1 | 0.83 ± 0.02 | <28.2 | 0.41 ± 0.01 | |||
15371 | 59.72 ± 6.70 | 2.03 ± 0.03 | 8.61 | 24.68 ± 6.89 | 1.04 ± 0.02 | 3.43 | 20.29 ± 7.66 | 0.51 ± 0.01 | 2.58 |
17439 | 53.00 ± 10.40 | 0.68 ± 0.01 | 5.03 | 32.20 ± 8.90 | 0.35 ± 0.01 | 3.58 | <21.6 | 0.17 ± 0.01 | |
22263 | 23.21 ± 6.81 | 1.66 ± 0.03 | 3.16 | 14.14 ± 6.87 | 0.85 ± 0.02 | 1.93 | <28.8 | 0.42 ± 0.01 | |
32480 | 90.00 ± 15.00 | 1.75 ± 0.02 | 5.88 | 25.00 ± 8.00 | 0.89 ± 0.01 | 3.01 | <24.0 | 0.44 ± 0.01 | |
40843 | <24.0 | 1.77 ± 0.01 | <23.7 | 0.90 ± 0.01 | <26.4 | 0.44 ± 0.01 | |||
51502 | 49.65 ± 8.29 | 1.30 ± 0.02 | 5.83 | 41.01 ± 8.15 | 0.66 ± 0.01 | 4.95 | 23.10 ± 9.41 | 0.33 ± 0.01 | 2.42 |
72603 | <24.0 | 1.43 ± 0.01 | <24.3 | 0.73 ± 0.01 | <30.9 | 0.36 ± 0.01 | |||
83389 | <20.1 | 0.64 ± 0.01 | <21.0 | 0.33 ± 0.01 | <24.0 | 0.16 ± 0.01 | |||
84862 | <20.1 | 1.95 ± 0.02 | <21.0 | 0.99 ± 0.01 | <24.3 | 0.49 ± 0.01 | |||
85235 | <22.2 | 1.00 ± 0.02 | <23.1 | 0.51 ± 0.01 | <29.4 | 0.25 ± 0.01 | |||
85295 | <19.8 | 1.66 ± 0.04 | <21.0 | 0.85 ± 0.02 | <24.0 | 0.42 ± 0.01 | |||
92043 | 12.12 ± 6.57 | 3.85 ± 0.05 | 1.26 | <21.9 | 1.96 ± 0.03 | <24.3 | 0.96 ± 0.01 | ||
101997 | <19.5 | 0.91 ± 0.02 | <21.0 | 0.46 ± 0.01 | <24.6 | 0.23 ± 0.01 | |||
105312 | <19.8 | 0.93 ± 0.05 | <20.7 | 0.47 ± 0.03 | <24.0 | 0.23 ± 0.01 | |||
106696 | <19.5 | 0.65 ± 0.01 | <20.7 | 0.33 ± 0.01 | <24.9 | 0.16 ± 0.01 | |||
107649 | 113.00 ± 18.00 | 1.44 ± 0.02 | 6.20 | 44.30 ± 9.00 | 0.73 ± 0.01 | 4.84 | 25.90 ± 8.00 | 0.36 ± 0.01 | 3.19 |
108870 | <19.8 | 9.86 ± 0.23 | <21.0 | 5.03 ± 0.12 | <23.4 | 2.47 ± 0.06 |
Notes.The significance at each band is given. Figures without errors in the SPIRE columns give 3σ upper limits for the corresponding stars.
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