The evolution of the mass-metallicity relation up to z≈0.9 from the VIMOS/VLT Deep Survey

Details The evolution of the mass-metallicity relation up to z≈0.9 from the VIMOS/VLT Deep Survey The evolution of the mass-metallicity relation up to z≈0.9 from the VIMOS/VLT Deep Survey

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006sf2a.conf..351l&link_type=abstract

SF2A-2006: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics Eds.: D. Barret, F. Casoli, G.

Astronomy and Astrophysics

Astrophysics

Scientific paper

We present the first results derived from the spectrophotometric
properties of the VIMOS VLT Deep Survey (VVDS) first epoch data. We have
measured the spectral features (emission/absorption lines, 4000Å
break) of a sample of ≈8000 galaxies taken from the VVDS deep 02h and
CDFS fields using the platefit_VVDS pipeline.

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