Table A.3
Measured continuum fluxes, in Jy, from mid-IR to millimeter wavelengths.
| Spectral Energy Distributions for our sources | |||||||||||||||||||
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| #01 | #02 | #03 | #04 | #05 | #06 | #07 | #08 | #09 | #10 | #11 | #12 | #13 | #14 | ||||||
|
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| MSXa | 8.3 μm | 10.3 | <0.2 | <0.2 | 0.2 | 0.6 | <0.2 | 19.5 | <0.2 | <0.2 | <0.1 | 1.2 | <0.2 | 2.0 | 2.1 | ||||
| IRASb | 12 μm | 19.0 | − | − | 2.9 | 2.9 | − | 22.8 | − | <5 | <1.4 | <1.4 | − | 5.3 | 2.9 | ||||
| MSXa | 12.1 μm | 21.8 | <0.6 | <0.6 | <0.5 | <0.5 | <0.6 | 15.6 | <0.6 | <0.6 | <0.8 | 1.8 | <0.6 | 3.1 | 3.0 | ||||
| MSXa | 14.7 μm | 33.0 | <0.6 | <0.6 | 0.9 | 0.7 | <0.6 | 26.3 | <0.6 | <0.6 | <0.6 | 2.2 | <0.6 | 6.1 | 5.4 | ||||
| MSXa | 21.3 μm | 61.8 | <1.1 | <1.1 | 5.5 | 3.4 | <1.1 | 69.7 | <1.1 | <1.1 | 4.1 | 13.6 | <1.1 | 46.7 | 24.3 | ||||
| MIPSc | 24 μm | − | 0.02 | 0.24 | >6 | 5.4 | 0.22 | − | 1.8 | 4.4 | >6 | >10 | 0.25 | >18 | − | ||||
| IRASb | 25 μm | 98.6 | − | − | 14.3 | 11.1 | − | 137.6 | − | 5.9 | <27.2 | <27.2 | − | 129.1 | 50.1 | ||||
| IRASb | 60 μm | 891 | − | − | 324 | 317 | − | 958 | − | 187 | <765 | <765 | − | 1725 | 367 | ||||
| MIPSc | 70 μm | − | − | − | 260 | 291 | 15 | − | 44 | 245 | 479 | 321 | 14 | − | − | ||||
| HiGALd | 70 μm | − | − | 14.3 | 280.8 | 386.3 | 33.7 | 1200 | 98.4 | 659.8 | 942.0 | 338.4 | 38.7 | 2212 | − | ||||
| IRASb | 100 μm | 1891 | − | − | 1028 | 1104 | − | 2136 | − | 727 | <1948 | <1948 | − | 2744 | <686 | ||||
| HiGALd | 160 μm | − | − | 55.6 | 400.2 | 725.5 | 139.5 | 1590 | 169.2 | 866.0 | 1120 | 587.0 | 91.7 | 1598 | − | ||||
| HiGALd | 250 μm | − | − | 63.8 | 328.8 | 464.5 | 165.0 | 623 | 117.6 | 496.3 | 585.5 | 538.6 | 97.0 | 682.2 | − | ||||
| HiGALd | 350 μm | − | − | 29.3 | 130.4 | 229.2 | 81.7 | 359 | 44.2 | 229.1 | 326.3 | 270.1 | 52.1 | 385.8 | − | ||||
| JCMTe | 450 μm | 83 | 14 | 25 | 194 | − | − | − | − | − | 148 | − | 38 | <351 | 76 | ||||
| HiGALd | 500 μm | − | 23.3 | 13.1 | 47.3 | 66.4 | 32.8 | 116 | 13.6 | 73.7 | 82.3 | 95.5 | 20.5 | 84.9 | − | ||||
| JCMTe | 850 μm | 9.53 | 2.88 | 3.83 | 20.4 | 13.4 | − | − | − | − | 16.7 | − | 5.26 | 16.7 | 6.32 | ||||
| APEXf | 850 μm | − | 3.13 | 3.43 | 16.8 | 20.6 | 5.95 | 25.6 | 3.29 | 9.75 | − | − | − | − | − | ||||
| −g | 1.2 mm | 3.60 | 0.92 | 0.91 | 10.4 | 7.6 | 1.11 | 10.6 | 0.71 | 2.03 | 4.01 | 13.2 | 1.02 | 5.3 | 2.30 | ||||
Notes.
Fluxes obtained from the catalog of the Midcourse Space Experiment (MSX; Price et al. 1999).
Fluxes obtained from the point source catalog v2.1 of the Infrared Astronomical Satellite (IRAS; Neugebauer et al. 1984).
Fluxes obtained from the Spitzer satellite, and the instrument Multiband Imaging Photometer for Spitzer (MIPS; Rieke et al. 2004).
Fluxes obtained from the Hi-GAL/Herschel project (Molinari et al. 2010a,b).
Fluxes obtained from the SCUBA Legacy survey (Di Francesco et al. 2008).
Fluxes obtained from the ATLASGAL project (Schuller et al. 2009).
At 1.2 mm we used the single-dish surveys of Beuther et al. (2002a); Faúndez et al. (2004); Hill et al. (2005); Rathborne et al. (2006), carried out with the IRAM 30 m telescope or with the SEST (Swedish-ESO 15 m Submillimeter Telescope).
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