Table 2: Calibration constants for the UV luminosities vs. SFR relations.
${M_{\rm up}}$ 100 $M_\odot$ 120 $M_\odot$

Z C₁₅₀₀ C₂₈₀₀ C₁₅₀₀ C₂₈₀₀

$\left[{\times10^{27}\frac{{\rm erg ~ s^{-1}~ Hz^{-1}}}{M_\odot ~ {\rm yr}^{-1}}}\right]$ $\left[{\times10^{27}\frac{{\rm erg ~ s^{-1}~ Hz^{-1}}}{M_\odot ~ {\rm yr}^{-1}}}\right]$

0.0004 14.6 13.7 14.8 13.9

0.004 12.8 11.8 13.1 12.0

0.008 11.9 10.8 12.2 11.0

0.02 10.6 10.0 11.0 10.3

0.05 9.3 8.9 9.8 9.2

**Table 2:** Calibration constants for the UV luminosities vs. SFR relations.
${M_{\rm up}}$	100 $M_\odot$	120 $M_\odot$
Z	C₁₅₀₀	C₂₈₀₀	C₁₅₀₀	C₂₈₀₀
	$\left[{\times10^{27}\frac{{\rm erg ~ s^{-1}~ Hz^{-1}}}{M_\odot ~ {\rm yr}^{-1}}}\right]$	$\left[{\times10^{27}\frac{{\rm erg ~ s^{-1}~ Hz^{-1}}}{M_\odot ~ {\rm yr}^{-1}}}\right]$
0.0004	14.6	13.7	14.8	13.9
0.004	12.8	11.8	13.1	12.0
0.008	11.9	10.8	12.2	11.0
0.02	10.6	10.0	11.0	10.3
0.05	9.3	8.9	9.8	9.2

Source LaTeX | All tables | In the text

	1 Introduction
	2 GALEV: galaxy evolution models
	3 Results
	4 Conclusions
	References