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Table 2.

Observed data for U Ant, DR Ser, and V644 Sco.

U Ant
DR Ser
V644 Sco
Reference
λ Fλ ΔFλ Fλ ΔFλ Fλ ΔFλ
μm (Jy) (Jy) (Jy)
0.44 1.12 0.58 0.08 0.08 Kerschbaum & Olofsson (1999)
1.24 597.60 22.02 71.20 1.71 38.70 3.87
1.63 1127.52 41.54 85.22 3.14
1.66 85.90 8.59
2.16 103.00 10.30
2.19 1167.55 43.01 98.64 3.63
3.79 749.41 27.61 70.78 2.61
4.29 65.92 6.59
4.35 73.00 7.30
4.64 319.03 23.51
8.28 21.67 2.10 24.67 2.47
12.13 11.60 1.10 15.03 1.50
14.65 7.73 0.80 8.90 0.89
21.30 4.74 0.40 6.41 0.64
8.610 263.5 14.6 21.00 0.50 22.71 0.15 AKARI (archive)
18.40 61.5 2.3 6.16 0.13
65.00 25.8a 5.3 4.40 0.30
90.00 20.1a 4.2 3.68 0.51
140.00 8.4a 3.1
160.0 3.5a 2.2 1.28 0.19
12.00 167.50 12.23 15.95 1.16 17.62 1.76 IRAS (archive)
25.00 44.81 4.03 6.66 0.60 8.99 0.90
60.00 27.11 3.25 5.960 0.71 19.30 1.93
100.00 21.14 2.60
70.00 27.1 4.1 PACS (Kerschbaum et al. 2010)
160.00 7.4 1.2
250.00 1.89 0.28 SPIRE (archive, Sect. 2.5)
350.00 0.73 0.11
500.00 0.25 0.04
870.00 0.16 0.02 0.01 0.002 0.04 0.004 APEX LABOCA (this paper, Sect. 2.3)

Notes.Fλ and ΔFλ are the flux density and flux density error (1σ) at wavelength λ, respectively. For V644 Sco, the values of ΔFλ for some wavelengths are unavailable and are assumed to be 10% of Fλ. The origin of the data is indicated in the last column.

(a)

For U Ant the AKARI data from 65 μm to 160 μm was taken from Arimatsu et al. (2011) instead of from the AKARI archive.

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