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Open questions<br />
How the overall picture depends on SFR tracers?<br />
Why the SFR density is flat for z>1?<br />
Are we missing a significative fraction of objects?<br />
What is the role of the AGNs at different epochs?<br />
Are we really measuring downsizing?<br />
What are the new populations of galaxies?<br />
Jesús Gallego – UCM Granada 2008 9