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Table 1:

Morpho-kinematical classification of 52 $z_{\rm median}$ = 0.65 galaxies.

$z_{\rm median}$ = 0.65 $z_{\rm median}$ = 0.65 $z_{\rm median}$ = 0.65 z=0
  Starburst (60%) Quiescent (40%) All local
  $W_0({\rm OII})\ge$ 15 Å $W_0({\rm OII})<$ 15 Å All All
references N08 Z06 N08 N04
E/S0 0% 57% 23% 27%
Rotating spiral disks 23% 43% 31% 70%
Non-relaxed & 77% 0% 46% $\sim$3%
intermediate systems        
Galaxies with        
anomalous 68% 0% 41%  

From Neichel et al. (2008) (see their Table 4); for comparison, the last column shows the fractions derived from the SDSS (Nakamura et al. 2004) for galaxies in the same mass range (e.g. Hammer et al. 2005). CFRS (Hammer et al. 1997) found that 60% of $z_{\rm median}$ = 0.65 galaxies have spectra with $W_0({\rm OII})$ $\ge$ 15 Å and are classified as starbursts. References are Neichel et al. (2008): N08, Zheng et al. (2004): Z06, Nakamura et al. (2004): N04 and Hammer et al. (2005): H05.

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