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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 />
Mgas (fuel for SF, evol. st<strong>at</strong>e, tdep)<br />
Excit<strong>at</strong>ion => ngas , Tkin (phys. conditions for SF)<br />
Imaging => Σgas ,Mdyn (sys. potential => Mtot)
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