Table 11: Determination of the star formation rates.
DLA system SFR for the best "spiral'' model SFR for the best "dwarf irregular'' model

[ $M_{\odot}$ yr^-1 kpc^-2] [ $M_{\odot}$ yr^-1 kpc^-2]

Q0100+13, $z_{\rm abs} = 2.309$ $8.5\times 10^{-3}$ $1.0\times 10^{-2}$

Q1331+17, $z_{\rm abs} = 1.776$ $7.5\times 10^{-3}$ $9.2\times 10^{-5}$

Q2231-00, $z_{\rm abs} = 2.066$ - $4.0\times 10^{-2}$

**Table 11:** Determination of the star formation rates.
DLA system	SFR for the best "spiral'' model	SFR for the best "dwarf irregular'' model
	[ $M_{\odot}$ yr^-1 kpc^-2]	[ $M_{\odot}$ yr^-1 kpc^-2]
Q0100+13, $z_{\rm abs} = 2.309$	$8.5\times 10^{-3}$	$1.0\times 10^{-2}$
Q1331+17, $z_{\rm abs} = 1.776$	$7.5\times 10^{-3}$	$9.2\times 10^{-5}$
Q2231-00, $z_{\rm abs} = 2.066$	-	$4.0\times 10^{-2}$

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