Table 5
Published ground-based [C I] and CO line fluxes.
Name | Observed line fluxa | Ref.b | |||||
CO (4−3) | CO (7−6) | [C I] (1−0) | [C I] (2−1) | CO (2−1) | 13CO (2−1) | ||
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.
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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