Table 2
12CO(1–0) flux values, both obtained by our observations and extracted from the literature, for NGC 3627.
| Reference | Telescope | Diameter | Primary beam or FOVa | Beam | Flux |
| [m] | [″] | [″ × ″] | [Jy km s-1] | ||
|
|
|||||
| Young et al. (1995) | FCRAO | 14 | 45 | 786 | |
| This paper | PdBI+30 m | 42 | 2.1 × 1.3 | 668 | |
| This paper | PdBI+30 m | 22b | 2.1 × 1.3 | 359 | |
| This paper | PdBI | 22b | 2.0 × 1.3 | 251 | |
| This paper | 30 m | 30 | 22 (central position) | 343c | |
| Helfer et al. (2003) | NRAO | 12 | 55 (inner 50″ × 50″) | 1100–1200 | |
| This paper | 30 m | 30 | 22 (inner 50″ × 50″) | 1097d | |
Notes.
Primary beam is considered for single-dish observations, while field-of-view (FOV) for interferometric or combined (interferometric+single-dish) ones.
The photometry has been performed within 22″, the 12CO(1–0) primary beam for the 30 m telescope.
The 12CO(1–0) recovered flux for inner ~50″ × 50″, 5 × 5 mapping with 7″spacing (see Sect. 2.2).
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