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We present the results of a CO(1-0) emission survey with the IRAM 30m of 30galaxies at moderate redshift (z ~ 0.2-0.6) to explore galaxy evolution and inparticular the star formation efficiency, in the redshift range filling the gapbetween local and very high-z objects. Our detection rate is about 50%. One ofthe bright objects was mapped at high resolution with the IRAM interferometer,and about 50% of the total emission found in the 27 arcsec (97 kpc) single dishbeam is recovered by the interferometer, suggesting the presence of extendedemission. The FIR-to-CO luminosity ratio is enhanced, following the increasingtrend observed between local and high-z ultra-luminous starbursts.

Galaxy Evolution and Star Formation Efficiency in the Last Half of the Universe