Probing high-redshift quasars with ALMA - I. Expected observables and potential number of sources

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Table 2:

Frequency range, angular resolution $\theta _{{\rm res}}$ at the largest baseline, line sensitivity $S_{\rm l}$ for a linewidth of 300 km s^-1 and continuum sensitivity $S_{\rm c}$ for $3\sigma$ detection in one hour of integration time and primary beam size $\theta _{{\rm beam}}$ .
Band	Freq. [GHz]	$\theta _{{\rm res}}$ ['']	$S_{\rm c}$ [mJy]	$S_{\rm l}$ [mJy]	$\theta _{{\rm beam}}$ ['']
3	84-116	0.034	0.019	0.163	56
4	125-169	0.023	0.023	0.174	48
5	163-211	0.018	0.298	2.63	35
6	211-275	0.014	0.039	0.225	27
7	275-373	0.011	0.077	0.372	18
8	385-500	0.008	0.143	0.620	12
9	602-720	0.005	0.232	0.813	9

Notes. 3 more bands might be added in the future, band 1 around 40 GHz, band 2 around 80 GHz and band 10 around 920 GHz, which will have similar properties as the neighbouring bands.

Source LaTeX | All tables | In the text

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