Based on observation made at the European Southern Observatory, Paranal, Chile (ESO LP 164.O-0560).

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Full Table 3 is only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/437/883

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... 2004

http://www.mpe.mpg.de/~mara/surveys/

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... added

For five galaxies the redshift has been obtained from ESO/GOODS data.

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... respectively

See the ESO web page http://www.eso.org/instruments/fors/inst/grisms.html for more details.

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... IRAF

IRAF is distributed by the National Optical Astronomy Observatories, which are operated by the Association of Universities for Research in Astronomy, Inc., under cooperative agreement with the National Science Foundation.

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... package

Deep Infrared Mosaicking Software, a package written by Eisenhardt, Dickinson, Stanford and Ward, available at http://iraf.noao.edu/contrib/dimsumV2

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... 6583

Our spectral resolution did not allow to separate the doublet [NII] $\lambda \lambda$ 6548,6583 from H $\alpha$ .

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... bin

At the median redshift of the analyzed galaxy sample (z=0.73), a rest frame bin of 2 Å is only slightly less than the typical pixel size used in the spectroscopic observations.

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... variation

$(spe1-spe2)/\langle spe1,spe2\rangle$ .

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... et al.

See http://www.cida.ve/~magris/ademis/datafile1.txt

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