The metallicity-luminosity relation at medium redshift based on faint CADIS emission line galaxies
Abstract
The emission line survey within the Calar Alto Deep Imaging Survey (CADIS) detects galaxies with very low continuum brightness by using an imaging Fabry-Perot interferometer. With spectroscopic follow-up observations of MB>~-19 CADIS galaxies using FORS2 at the VLT and DOLORES at TNG we obtained oxygen abundances of 5 galaxies at z~0.4 and 10 galaxies at z~0.64. Combining these measurements with published oxygen abundances of galaxies with MB<~-19 we find evidence that a metallicity-luminosity relation exists at medium redshift, but it is displaced to lower abundances and higher luminosities compared to the metallicity-luminosity relation in the local universe. Comparing the observed metallicities and luminosities of galaxies at z<3 with Pegase2 chemical evolution models we have found a favoured scenario in which the metallicity of galaxies increases by a factor of ~2 between z~0.7 and today, and their luminosity decreases by ~0.5-0.9mag.
Keywords
Cite
@article{arxiv.astro-ph/0402048,
title = {The metallicity-luminosity relation at medium redshift based on faint CADIS emission line galaxies},
author = {C. Maier and K. Meisenheimer and H. Hippelein},
journal= {arXiv preprint arXiv:astro-ph/0402048},
year = {2009}
}
Comments
Accepted for publication in A&A; 12 pages, 9 figures