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Table 6

Integrated mid- and far-IR photometry.

Name Spitzer/IRAC Spitzer/MIPS Herschel/PACS Herschel/SPIRE
5.8 μm 8.0 μm 24 μm 70 μm 100 μm 160 μm 250 μm 350 μm 500 μm
NGC 23 0.17 0.43 0.86 10 14 13 5.2 2.1 0.63
MCG +12-02-001 0.20 0.58 2.9 25 29 22 7.5 2.8 0.96
NGC 876 0.045 0.10 0.17 3.3 5.0 5.5 2.6 1.1 0.39
NGC 877 0.29 0.77 0.88 12 23 28 14 5.8 1.9
UGC 01845 0.12 0.34 0.84 13 17 15 4.8 1.8 0.56
NGC 992 0.19 0.55 1.0 12 16 15 5.4 2.1 0.66
UGC 02982 0.19 0.56 0.60 9.9 16 16 7.2 3.1 1.2
NGC 1614 0.30 0.88 5.7 36 36 23 6.5 2.3 0.65
CGCG 468-002 NED01 0.056 0.088 0.33 2.4 2.9 2.5 0.82 0.30 <0.19a
CGCG 468-002 NED02 0.033 0.086 0.60 9.2 9.6 6.8 2.0 0.73 <0.19a
NGC 1961 0.32 0.73 0.71 11 24 36 18 8.1 3.0
UGC 03351 0.19 0.52 0.66 18 31 32 14 5.5 1.6
UGC 03405 0.054 0.14 0.12 2.1 4.3 5.6 2.9 1.3 0.45
UGC 03410 0.19 0.51 0.62 9.9 17 20 8.8 3.6 1.2
NGC 2388 0.15 0.42 1.6 20 25 21 7.4 3.0 0.97
NGC 2389 0.079 0.20 0.27 3.2 6.3 5.2 2.3 1.1 0.50
MCG +02-20-002 0.021 0.057 <0.50b 0.85 1.6 2.1 0.96 0.43 0.16
MCG +02-20-003 0.11 0.22 <0.73b 10 13 10 3.5 1.4 0.45
NGC 3110 0.21 0.60 0.91 13 20 20 7.9 3.1 0.94
NGC 3221 0.24 0.64 0.72 10 19 25 12 5.1 1.7
Arp 299 1.1 2.4 23c 130 120 72 22 7.6 2.3
MCG –02-33-098 0.076 0.21 1.1 7.2 8.4 6.5 2.6 1.1 0.34
IC 860 0.018 0.038 0.87 20 18 11 3.6 1.5 0.47
NGC 5653 0.22 0.62 1.1 14 21 21 8.1 3.1 1.0
Zw 049-057 0.028 0.071 0.54 28 32 24 7.9 3.0 0.98
NGC 5936 0.17 0.48 1.0 11 16 16 6.7 2.6 0.87
NGC 5990 0.23 0.48 1.2 12 16 15 6.3 2.4 0.84
NGC 6052 0.075 0.20 0.66 7.4 9.9 8.9 3.3 1.3 0.43
NGC 6701 0.17 0.45 0.98 12 19 18 7.4 2.9 0.97
NGC 6921 0.060 0.077 0.086 2.2 3.1 2.3 0.79 0.30 0.10 ± 0.03
MCG +04-48-002 0.17 0.46 0.68 10 14 12 4.1 1.5 0.49
NGC 7591 0.10 0.28 0.65 8.9 13 13 6.4 2.7 0.91
NGC 7679 0.14 0.40 0.81 8.0 10 8.4 3.1 1.2 0.42
NGC 7752 0.052 0.14 0.28 3.4 4.9 4.5 1.7 0.70 0.21
NGC 7753 0.11 0.26 0.34 4.1 8.6 12 6.5 3.0 1.1
NGC 7769 0.14 0.35 0.49 ··· <13.58b ··· 4.9 1.9 0.61
NGC 7770 0.060 0.14 0.38 2.9 3.8 3.2 1.2 0.44 ± 0.07 0.14 ± 0.03
NGC 7771 0.26 0.63 1.2 23 38 39 17 6.6 2.1

Notes. The units of the fluxes are Jy. Uncertainties are included only when they are greater than 10% of the flux.

(a)

The two components of CGCG 468-002 are not resolved in the 500 μm Herschel/SPIRE image, therefore we assume the integrated flux of the two components as an upper limit.

(b)

These upper limits are the IRAS 25 μm and 100 μm fluxes measured by Surace et al. (2004).

(c)

The MIPS 24 μm image of Arp 299 is saturated, so we took the IRAS 25 μm flux from Sanders et al. (2003) corrected by the conversion factor between IRAS 25 μm and MIPS 24 μm fluxes given Calzetti et al. (2010).

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