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Table 2.

Observed flux densities Fv in Jy and their corresponding errors.

Survey λ (μm) NGC 973 UGC 4277 IC 2531 NGC 4013 NGC 4217 NGC 5529 NGC 5907
FUV 0.15 0.001 ± 0.0005 0.0008 ± 0.0003 0.0007 ± 0.0003 0.0009 ± 0.0003 0.008 ± 0.001
NUV 0.23 0.0003 ±0.0001 0.002 ± 0.0004 0.002 ± 0.0003 0.002 ± 0.0004 0.002 ± 0.0002 0.01 ± 0.001
SDSS u 0.36 0.02 ± 0.002* 0.02 ± 0.002* 0.008 ± 0.0005* 0.05 ± 0.004*
WHT u 0.36 0.005 ± 0.0003* 0.004 ± 0.0002*
FTS B 0.45 0.040 ± 0.004*
SDSS g 0.47 0.07 ± 0.005* 0.08 ± 0.009* 0.03 ± 0.002* 0.18 ± 0.009*
WHT g 0.47 0.02 ± 0.001* 0.01 ± 0.001*
FTS V 0.55 0.070 ± 0.007*
SDSS r 0.62 0.15 ± 0.01* 0.17 ± 0.02* 0.07 ± 0.004* 0.34 ± 0.01*
WHT r 0.62 0.04 ± 0.002* 0.02 ± 0.001*
FTS R 0.66 0.098 ± 0.009*
SDSS i 0.75 0.23 ± 0.02* 0.26 ± 0.03* 0.1 ± 0.006* 0.51 ± 0.02*
WHT i 0.75 0.06 ± 0.003* 0.03 ± 0.001*
SDSS z 0.89 0.3 ± 0.02* 0.33 ± 0.03* 0.14 ± 0.008* 0.64 ± 0.03*
WHT z 0.89 0.09 ± 0.005* 0.04 ± 0.001*
2MASS J 1.25 0.17 ± 0.009* 0.08 ± 0.003* 0.250 ± 0.016* 0.51 ± 0.04* 0.51 ± 0.04* 0.23 ± 0.01* 1.09 ± 0.04*
2MASS H 1.65 0.24 ± 0.01* 0.1 ± 0.003* 0.347 ± 0.020* 0.69 ± 0.05* 0.71 ± 0.05* 0.32 ± 0.02* 1.48 ± 0.05*
2MASS K 2.20 0.2 ± 0.005 0.09 ± 0.003 0.291 ± 0.015* 0.59 ± 0.01 0.62 ± 0.02 0.29 ± 0.02* 1.36 ± 0.05*
TNG K 2.13 0.25 ± 0.02* 0.11 ± 0.006* 0.66 ± 0.06* 0.73 ± 0.06*
WISE 1 3.4 0.11 ± 0.006 0.05 ± 0.002* 0.127 ± 0.005 0.28 ± 0.02 0.33 ± 0.04 0.12 ± 0.009 0.65 ± 0.03
IRAC 1 3.6 0.14 ± 0.007* 0.156 ± 0.007* 0.38 ± 0.03* 0.41 ± 0.03* 0.15 ± 0.01* 0.85 ± 0.03*
IRAC 2 4.5 0.11 ± 0.004 0.25 ± 0.02 0.29 ± 0.03 0.1 ± 0.007 0.57 ± 0.03
WISE 2 4.60 0.1 ± 0.005 0.03 ± 0.002 0.088 ± 0.004 0.21 ± 0.02 0.25 ± 0.03 0.08 ± 0.006 0.47 ± 0.03
IRAC 3 5.8 0.14 ± 0.005 0.42 ± 0.01 1.17 ± 0.07
IRAC 4 8.0 0.2 ± 0.008 0.92 ± 0.04 2.36 ± 0.13
WISE 3 12.1 0.18 ± 0.01 0.06 ± 0.005 0.218 ± 0.007 0.62 ± 0.05 1.22 ± 0.13 0.25 ± 0.03 1.88 ± 0.13
IRAS 12 12 0.08 ± 0.02 0.54 ± 0.04 1.26 ± 0.07 0.26 ± 0.03 1.29 ± 0.07
WISE 4 22.2 0.32 ± 0.03 0.07 ± 0.008 0.188 ± 0.007 0.75 ± 0.07 1.48 ± 0.22 0.27 ± 0.03 2.19 ± 0.18
MIPS 1 24 0.66 ± 0.04 1.73 ± 0.13
IRAS 25 25 0.3 ± 0.02 0.77 ± 0.05 1.5 ± 0.08 0.24 ± 0.03 1.44 ± 0.08
IRAS 60 60 1.69 ± 0.12 0.35 ± 0.04 7.01 ± 0.35 11.6 ± 0.58 1.95 ± 0.17 9.14 ± 0.46
MIPS 2 70 10.01 ± 1.1 23.21 ± 2.66
IRAS 100 100 3.5 ±0.39 1.12 ±0.12 24.4 ± 1.23 41.2 ± 2.06 7.73 ± 0.55 37.4 ± 1.87
PACS 100 100 4.07 ± 0.36 1.64 ± 0.17 5.82 ± 0.51 24.17 ± 1.37 38.69 ± 1.94 8.52 ± 0.6 60.28 ± 3.2
MIPS 3 160 36.92 ± 5.5 86.16 ± 11.75
PACS 160 160 5.8 ± 0.35 2.74 ± 0.31 9.94 ± 0.65 32.44 ± 1.8 56.79 ± 2.84 12.3 ± 0.74 88.29 ± 4.69
ISO 170 170 62.27 ± 9.34 35.8 ± 5.37
SPIRE 250 250 3.6 ± 0.26 2.1 ± 0.16 6.72 ± 0.48 17. 67 ± 1.24 28.79 ± 2.07 8.04 ± 0.57 53.21 ± 3.73
SPIRE 350 350 1.7 ± 0.13 1.11 ± 0.09 3.51 ± 0.26 7.52 ± 0.53 12.27 ± 0.94 3.95 ± 0.28 24.45 ± 1.72
Planck 350 350 1.58 ± 0.94 3.50 ± 0.55 8.21 ± 0.41 4.46 ± 0.32 25.44 ± 0.42
SCUBA 450 450 13.2 ± 0.91
SPIRE 500 500 0.64 ± 0.06 0.43 ± 0.04 1.42 ± 0.12 2.52 ± 0.19 4.25 ± 0.39 1.54 ± 0.12 9.08 ± 0.64
Planck 550 550 1.18 ± 0.29 2.27 ± 0.22 1.61 ± 0.18 7.9 ± 0.24
Planck 850 850 0.31 ± 0.17 0.62 ± 0.09 0.52 ± 0.09 2.12 ± 0.13
SCUBA 850 850 1.96 ± 0.03

Notes. Correction for Galactic extinction (where applicable) has been applied according to Schlafly & Finkbeiner (2011). The masked objects were replaced by the interpolated values using a Gaussian weights kernel. No colour corrections to the retrieved fluxes were applied. The asterisk denotes the reference data.

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