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Galaxy evolution: SFR tracers<br />
SFR [M/yr] = K • Luminosity<br />
<br />
<br />
<br />
<br />
<br />
<br />
U band<br />
UV continuum<br />
Hydrogen recombination lines<br />
Forbidden lines<br />
Far-infrared<br />
1.4 GHz Radio<br />
R=Light / SFR<br />
R STANDARD<br />
:<br />
- Salpeter IMF, Z <br />
- Mmax=100M <br />
- A V<br />
=1, dust screen<br />
Charlot et al 98<br />
Local SFR calibrations valid for high<br />
redshift? (see Cardiel+03, Moustakas+06)
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