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Mass-metallicity relation of zCOSMOS galaxies at z ≈ 0.7, its dependence on star formation rate, and the existence of massive low-metallicity galaxies

C. Maier 1 B. L. Ziegler 1 S. J. Lilly T. Contini 2 E. Pérez-Montero F. Lamareille 2 M. Bolzonella E. Le Floc’h 3
1 University of Vienna [Vienna]
2 IRAP - Institut de recherche en astrophysique et planétologie
3 DAP - Département d'Astrophysique (ex SAP)
Abstract : Aims. The knowledge of the number and physical nature of low-metallicity massive galaxies is crucial for determining and interpreting the mass-metallicity relation (MZR).Methods. Using VLT-ISAAC near-infrared (NIR) spectroscopy of 39 zCOSMOS 0.5
Keywords : galaxies: high-redshift galaxies: star formation galaxies: evolution
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https://hal-cea.archives-ouvertes.fr/cea-01300564
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Submitted on : Monday, April 11, 2016 - 11:29:12 AM
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C. Maier, B. L. Ziegler, S. J. Lilly, T. Contini, E. Pérez-Montero, et al.. Mass-metallicity relation of zCOSMOS galaxies at z ≈ 0.7, its dependence on star formation rate, and the existence of massive low-metallicity galaxies. Astronomy and Astrophysics - A&A, EDP Sciences, 2015, 577, pp.A14. ⟨10.1051/0004-6361/201425224⟩. ⟨cea-01300564⟩

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