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Table 5

Published ground-based [C I] and CO line fluxes.

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

IC10 0.89 1.00 0.52 0.84 25 1.4 GP00, Ba06
NGC 253 101 31.5 1210 104 IWB, IB02
NGC 278 0.89 0.54 17.9 1.9 IB02, I09b
NGC 660 8.39 3.37 154 11 IB02, I09b
NGC 891 0.79 118 12 Ba06, I
Maffei 2 40.6 2.17 275 22 IB02, IB03
NGC 1068 10.8 5.33 247 17 IB02, I09a
IC 342 20.6 2.94 193 24 IB02, IB03
Henize2-10 1.40 4.00 0.36 20 1.2 GP00, Ba06
NGC 3079 11.4 7.61 189 11 IB02, I09b, GP00
NGC 3628 10.9 4.13 169 13 IB02, I09b
NGC 4038 2.6 0.6 0.94 110 14 GP00, Ba06
NGC 4736/M94 0.57 69 5.9 GP00, Ba06
NGC 4826/M64 8.49 5.11 126 15 IB02, I09a
NGC 4945 56.8 80.4 1300 131 H08
NGC 5194/M51 2.76 1.41 43.5 5.7 IB02, ITB, GP00
NGC 5236/M83 26.7 5.98 291 28 IB01, IB02
Circinus 18.0 26.1 8.20 592 56 H08, Z14
NGC 6090/Mrk496 0.38 43 GP00, Ba06
NGC 6946 21.3 4.78 249 22 IB01, IB02, GP00

Notes. In this table only, all fluxes refer to the same beamwidth of 22”, except in the cases of NGC 4945 and the Circinus galaxy where beamwidths of 38” apply, similar to the SPIRE aperture.

(b)

Reference to line fluxes: Ba06 = Bayet et al. (2006); GP00 = Gerin & Phillips (2000); H08 = Hitschfeld et al. (2008); IWB = Israel et al. (1995); ITB = Israel et al. (2006); IB01 = Israel & Baas (2001); IB02 = Israel & Baas (2002); IB03 = Israel & Baas (2003); I09a = Israel (2009a); I09b = Israel (2009b); Z14 = Zhang et al. (2014).

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