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Table 2

[C I] and CO line fluxes from HerCULES galaxies.

Name Observed line flux Herschel Ref.a
CO (43) CO (76) [C I] (10) [C I] (21) CO (21) 13CO (21) obsid
461 GHz 807 GHz 492 GHz 809 GHz 230 GHz 220 GHz
(10-17 W m-2) (10-19 W m-2)

NGC 34 2.54 0.75 1.25 10 1342199253 PS14
NGC 253 128 182 41.5 114 2355 229 1342210847 R14, *
MGC+12-02-001 3.07 2.69 1.05 2.59 1342213377
IC 1623 4.25 3.41 2.40 3.83 1342212314
IRAS F05189-2524 0.87 0.25 0.61 10 1.5 1342192833 P12, PS14
NGC 1365 41.7 26.2 19.6 31.8 385 34 1342204021 I, *
NGC 1614 2.61 3.43 1.10 2.67 95 1342192831 A95
NGC 2146 17.0 17.8 5.68 15.3 402 35 1342193810 I09a *
NGC 2623 1.92 2.84 0.86 2.44 21 1342219553 P12
NGC 3256 17.7 18.9 7.87 16.0 261 10 1342201201 S06
Arp 299C/IC 694 5.75 5.34 1.79 3.82 74 8.9 1342199250 S12, A95, *
Arp 299B 5.17 5.38 1.99 3.88 77 7.1 1342199249 S12, A95, *
Arp 299A/NGC 3690 8.71 12.0 2.44 7.81 139 6.9 1342199248 S12, A95, *
ESO 320-G030 4.39 4.54 1.72 3.44 1342210861
NGC 4418 1.17 5.17 1.83 1.08 1342187780
Mrk 231 2.46 0.58 1.34 24 0.45 1342210493 P12
IRAS 13120-5453 6.70 2.35 5.39 1342212342
Arp 193/IC 883 3.20 3.41 1.35 3.70 65 1.9 1342209853 P12, P14
NGC 5135 3.53 3.04 3.36 6.18 95 6.4 1342212344 P12, PS14
ESO 173-G015 12.1 17.5 4.90 14.5 1342202268
Mrk 273 2.82 0.51 1.76 21 2.6 1342209850 P12
CGCG 049-057 2.99 0.96 1.41 46 1.7 1342212346 P12
Arp 220 6.77 13.4 2.95 7.42 86 4.3 1342190674 P12
NGC 6240 7.78 16.6 3.04 9.54 114 1.9 1342214831 P14
IRAS F17207-0014 4.47 1.12 2.66 53 1342192829 P12
IC 4687 1.67 1.56 0.91 1.57 1342192993
IRAS F18293-3413 5.88 6.24 4.26 7.43 1342192830
NGC 7469 3.24 3.74 2.14 4.63 73 5.3 1342199252 P12, I09a, *
NGC 7552 12.4 11.6 5.46 10.8 208 22 1342198428 A95
NGC 7771 4.49 3.49 5.86 7.29 1342212317
Mrk 331 2.45 2.30 1.34 2.57 1342212316

Notes.

(a)

References to ground-based J = 2−112CO and 13CO observations: A95 = Aalto et al. (1995), I09a = Israel (2009a); I = Israel (JCMT, this paper); P12 = Papadopoulos et al. (2012); P14 = Papadopoulos et al. (2014), PS14 = Pereira-Santaella et al. (2014); R14 = Rosenberg et al. (2014a); S06 = Sakamoto et al. (2006). S12 = Sliwa et al. (2012). For galaxies marked by an asterisk (*) we have determined J = 2−112CO and 13CO fluxes corresponding to the SPIRE aperture by integration over the (JCMT) map.

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