All Tables

Table 1: Values of the parameters adopted for the test case. The upper part reports the values of the three free parameters of the model, whereas the lower part reports the value of the hidden parameters.
Table 2: Conversion factors of the line intensity in erg s^-1 cm^-2 into the velocity integrated main beam temperature $T_{\rm mb} \Delta v$ observed at the IRAM and JCMT telescopes respectively, for the five lines observed towards IRAS 16293-2422 (Parise et al. 2005). Last column quotes the $T_{\rm mb} \Delta v$ observed towards IRAS 16293-2422 (Parise et al. 2005).^a Predicted flux from the model simply converted into K km s^-1 using the conversion factor. ^b Predicted flux derived using an accurate convolution of the signal with the telescope beam.
Table 3: Integration time required to detect the HDO lines with a peak signal over noise of 5 (see text). Note that only one receiver was assumed, so in principle those times can be lowered by a factor $\sqrt {2}$ by using a double polarization setup.
Table A.1: Predicted fluxes for the IRAS 16293-2422 test case.