Observer-frame spectrum of a $\rm 4\times 10^{12} L_{\odot}$ galaxy
with increasing redshifts from $z$=0.3 to 12. The figure is based
on the observed spectrum of M82 including
the ISO spectral data and all available radio- and submillimeter data,
and assumes a cosmology with
        $H_o = 50$ km s$^{-1}$ Mpc$^{-1}$, $\Omega_0=0.3$ and 
        $\Omega_\Lambda=0.7$ (Beelen \& Cox 2001, in preparation). 
The strongest emission line is the [C~II] 
fine-structure line at 158~$\mu$m.
The positions of the ALMA Bands are shown at the bottom.
The thick dashed curves are 5 sigma 
        detection limits after 1 hour of integration time.