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Table 2

Observation parameters.

Transition Frequencya Feff HPBW rms in Tmb Tsys Modej Dates
(GHz) (′′) (km s−1) (K) (K)
N2H+(1–0) 93.1737637b 0.95 0.80 26.5 0.063 0.075–0.140 155–176 OTF 09–14.07.2014
N2D+(2–1) 154.2171805c 0.93 0.72 16.3 0.038 0.040–0.100 203–627 OTF 09–14.07.2014
H13CO+(1–0) 86.7542884d 0.95 0.81 28.5 0.068 0.110–0.190 102–129 OTF 02–08.12.2014
0.140–0.190 122–126 OTF 03–04.06.2015
DCO+(2–1) 144.0772804e 0.93 0.73 17.2 0.041 0.150–0.250 115–155 OTF 02–08.12.2014
0.310–0.500 198–220 OTF 03–04.06.2015
HC18O+(1–0) 85.1622231f 0.95 0.81 28.5 0.069 0.026–0.039 96–105 SP 08.12.2014
0.020–0.038 99–109 SP 04.06.2015
D13CO+(2–1) 141.4651331g 0.93 0.74 17.5 0.041 0.028–0.039 90–96 SP 08.12.2014
0.029–0.059 142–164 SP 04.06.2015

Notes. (a) Frequency of the main hyperfine component; (b)from Pagani et al. (2009); (c) from Pagani et al. (2009) and Dore, priv. comm.; (d)from Schmid-Burgk et al. (2004); (e)from Caselli& Dore (2005); (f)from Schmid-Burgk et al. (2004); (g)from Caselli& Dore (2005); (h)Beff and Feff values are available at the 30 m antenna efficiencies web page http://www.iram.es/IRAMES/mainWiki/Iram30mEfficiencies; (i) Δvres is the velocity resolution; (j)observational mode: OTFis an on-the-fly map, SP is a single-pointing on-off observation towards the DCO+(2–1) emission peak.

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