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frequency [GHz]<br />
practical issues<br />
CO transitions as function of redshift, f(T, ρ)<br />
PdBI/ALMA<br />
submm band<br />
PdBI/ALMA<br />
1mm band<br />
significant coverage in frequency space<br />
PdBI 2mm band<br />
PdBI/ALMA 3mm band<br />
<strong>at</strong> high redshift: can only detect high-J CO<br />
transitions<br />