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Table 2:

12CO(1-0) flux values for NGC 5953.

Reference 		Telescope Diameter Primary beam or FOVa Beam Flux
    [m] [ $^{\prime \prime }$] [ $^{\prime \prime }$$\times $ $^{\prime \prime }$] [Jy km s-1]
Iono et al. (2005) OVRO   60 $4.4 \times 3.6$ 233
Zhu et al. (1999) NRAO 12 55   365
Young et al. (1995) FCRAO 14 45   320
This paper PdBI+30 m   42 $2.1 \times 1.4$ 254
This paper PdBI+30 m   22 $^{{\rm b}}$ $2.1 \times 1.4$ 185
This paper PdBI   22 $^{{\rm b}}$ $2.0 \times 1.4$ 150
This paper 30 m 30 22 (central position)   167 $^{{\rm c}}$
This paper 30 m 30 22 (inner $50^{\prime\prime} \times 50^{\prime\prime}$)   377 $^{{\rm d}}$

Notes. (a) Primary beam is considered for single dish observations, while field-of-view (FOV) for interferometric or combined (interferometric+single dish) ones; (b) the photometry has been performed within 22 $^{\prime \prime }$, the 12CO(1-0) primary beam for the 30 m telescope; (c) the 12CO(1-0) recovered flux for the central position (0 $^{\prime \prime }$, 0 $^{\prime \prime }$); (d) the 12CO(1-0) recovered flux for inner $50^{\prime\prime} \times 50^{\prime\prime}$, $5 \times 5$ mapping with 7 $^{\prime \prime }$ spacing (see Sect. 2.2).


Source LaTeX | All tables | In the text

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