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\@writefile{toc}{\contentsline {section}{\numberline {2}Thermal continuum emission of high redshift galaxies}{1}}
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\@writefile{lof}{\contentsline {figure}{\numberline {1}{\ignorespaces Redshift Coverage for CO transitions for the ALMA Bands 7, 6, 3 and 4.}}{2}}
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\@writefile{lof}{\contentsline {figure}{\numberline {2}{\ignorespaces CO (1--0) emission (left panel) in the face-on spiral M51 is distributed smoothly along the spiral arms. The higher J CO transitions require the density and temperatures found only in the immediate vicinity of bright HII regions (as traced by H$\alpha $ on the right panel). }}{3}}
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