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Table B.3.

IR and FIR fluxes used during the analysis.

Object S60μm L60μm S100μm L100μm L(FIR) MW4 S22
[mJy] [erg s−1] [mJy] [erg s−1] [erg s−1] [mJy]
J00418+4021 2100 ± 170 1.16 ± 0.09 E+45 3200 ± 1000 1.8 ± 0.5 E+45 5 ± 2 E+45 3.96 ± 0.02 219 ± 4
J00457+0410 < 200 < 3 E+45 < 300 < 6 E+45 < 4 E+45 6.19 ± 0.09 28 ± 2
J00535+1241 2160 ± 50 8.2 ± 0.2 E+44 2960 ± 50 1.12 ± 0.2 E+44 3.9 ± 0.2 E+45 2.37 ± 0.02 940 ± 20
J10255+5140 150 ± 40 3.4 ± 0.9 E+43 200 ± 100 4 ± 2 E+43 2 ± 2 E+44 5.57 ± 0.03 50 ± 2
J11292-0424 670 ± 30 2.8 ± 0.1 E+44 1200 ± 100 4.9 ± 0.6 E+44 1.4 ± 0.2 E+45 3.71 ± 0.02 275 ± 6
J11420+6030 - - - - - 7.7 ± 0.2 7 ± 1
J12075+1506 - - - - - 6.46 ± 0.06 22 ± 1
J12091+5611 - - - - - 9.2 ± 0.5 1.8 ± 0.9
J12366+5630 - - - - - 8.5 ± 0.2 3.5 ± 0.7
J12562+5652 32000 ± 2000 6.2 ± 0.3 E+45 30000 ± 1000 5.9 ± 0.2 E+45 3.5 ± 0.5 E+46 0.27 ± 0.01 6530 ± 70
J13012+5902 30 ± 50 1 ± 2 E+45 - - 8 ± 200 E+44 6.40 ± 0.05 23 ± 1
J14052+2555 230 ± 50 7 ± 2 E+44 - - 1± 4 E+45 4.65 ± 0.03 115 ± 3
J14063+2223 < 100 < 1.5 E+44 < 100 < 1.3 E+44 < 4.0 E+44 6.04 ± 0.05 32 ± 1
J14170+4456 110 ± 30 1.6 ± 0.5 E+44 150 ± 70 2± 1 E+44 4± 4 E+44 5.28 ± 0.03 65 ± 2
J14258+3946 - - - - - 8.4 ± 0.3 3.6 ± 0.9
J14475+3455 < 200 < 1.5 E+46 < 600 < 4.1 E+46 < 1.4 E+46 5.37 ± 0.03 59 ± 1
J15455+4846 350 ± 30 7.0 ± 0.5 E+45 370 ± 80 7.0 ± 2 E+45 7± 2 E+45 4.72 ± 0.02 109 ± 3
J17014+5149 480 ± 40 4.8 ± 0.4 E+45 400 ± 100 4 ± 1 E+45 6 ± 2 E+45 4.09 ± 0.02 193 ± 3

Notes. Column 1: Object coordinate name. Column 2: 60μm flux densities from IRAS or ISO data. Column 3: 60μm luminosity derived from equation 7. Column 4: 100μm flux densities from IRAS or ISO data. Column 5: 100μm luminosity derived from equation 7. Column 6: L(FIR) defined from a linear combination of the 60μm and 100μm fluxes according to Helou et al. (1985). Column 7: WISE band 4 (22μm) magnitude. Column 8: 22μm flux densities derived from Column 7 magnitudes, using Fν0 × 10MW4/2.5, where Fν0 = 8.363Jy (Jarrett et al. 2011) is the zero magnitude flux density in band 4 corresponding to the constant that gives the same response as that of Vega.

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