THE MASS–METALLICITY AND LUMINOSITY–METALLICITY RELATIONS FROM DEEP2 AT z ∼ 0.8
By H. Zahid, Lisa J. Kewley, F. Bresolin. 2010
153 citations recorded by the source corpus.
We present the mass–metallicity (MZ) and luminosity–metallicity (LZ) relations at z ∼ 0.8 from ∼1350 galaxies in the Deep Extragalactic Evolutionary Probe 2 survey. We determine stellar masses by fitting the spectral energy distribution inferred from photometry with current stellar population synthesis models. This work raises the number of galaxies with metallicities at z ∼0.8 by more than an order of magnitude. We investigate the evolution in the MZ and LZ relations in comparison with local MZ and LZ relations determined in a consistent manner using ∼21, 000 galaxies in the Sloan Digital Sky Survey. We show that high stellar mass galaxies (M ∼ 1010.6 M☉) at z ∼0.8 have attained the chemical enrichment seen in the local universe, while lower stellar mass galaxies (M ∼ 109.2 M☉) at z ∼0.8 have lower metallicities (Δlog(O/H) ∼ 0.15 dex) than galaxies at the same stellar mass in the local universe. We find that the LZ relation evolves in both metallicity and B-band luminosity between z ∼0.8 and z ∼ 0, with the B-band luminosity evolving as a function of stellar mass. We emphasize that the B-band luminosity should not be used as a proxy for stellar mass in chemical evolution studies of star-forming galaxies. Our study shows that both the metallicity evolution and the B-band luminosity evolution for emission-line galaxies between the epochs are a function of stellar mass, consistent with the cosmic downsizing scenario of galaxy evolution.
Subfields: Astronomy and Astrophysics, Instrumentation
View Paper: https://www.semanticscholar.org/paper/24edaa8e26a3fb6ffc6aca7815fc7032af6cd1b9
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In Astronomy and Astrophysics
In Instrumentation
- Lisa J. Kewley
- T. Yuan
- M. Dopita
- M. Akiyama
- Margaret J. Geller
- Sara L. Ellison
- David R. Patton
- Christy A. Tremonti
Citations in the corpus
- THE COSMIC BPT DIAGRAM: CONFRONTING THEORY WITH OBSERVATIONS (2013, background): “…for star-forming galaxies (Noeske et al. 2007), understanding the metal- kewley@mso.anu.edu.au licity history of galaxies (Kobulnicky & Kewley 2004; Zahid et al. 2011; Yuan et al. 2013), and disentangling the cosmic evolution of the starburst versus AGN fraction (Ramos Almeida et al. 2013).”