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Table 1:

Observation parameters of the PdBI maps shown in Fig. 1.

Molecule
Transition Frequency Instrument Config. Beam PA Vel. Resol. Int. Timea $T_\ensuremath{{\rm sys}} $ Noise $^{b,\dagger}$ Obs. date
    GHz     arcsec $\deg$ km s-1 hours K K  

H13CO+
1-0 86.754288 PdBI C & D $ 6.8 \times 4.7$ 13 0.2 6.5 150 0.10 2006-07
HCO 10,1 3/2, 2- 00,0 1/2,1 86.670760 PdBI C & D $ 6.7 \times 4.4$ 16 0.2 6.5 150 0.09 2006-07
a We observed a 7-field mosaic centered on the IR peak at $\alpha_{2000} = 05^{\rm h}40^{\rm m}54.27^{\rm s}$, $\delta_{2000} = -02\deg 28'00''$ (Abergel et al. 2003) with the following offsets: (-5.5'', -22.0''), (5.5'', -22.0''), (11.0'', 0.0''), (0.0'', 0.0''), (-11.0'', 0.0''), (-5.5'', 22.0'') and (5.5'', 22.0''). The total field-of-view is $80.1''\times 102.1''$ and the half power primary beam is 58.1''. The mosaic was Nyquist sampled in declination at 3.4 mm and largely oversampled in right ascension. This maximizes the field of view along the PDR edge while the oversampling in the perpendicular direction eases the deconvolution. On-source time was computed as if the source was always observed with 6 antennae; b the noise values refer to the mosaic phase center (mosaic noise is inhomogeneous due to primary beam correction; it steeply increases at the mosaic edges).

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