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; B. L. Ziegler; S. J. Lilly; T. Contini; E. Pérez-Montero; F. Lamareille; M. Bolzonella; E. Le Floc’h

doi:10.1051/0004-6361/201425224

Journal Articles Astronomy and Astrophysics - A&A Year : 2015

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

(1) , (1) , , (2) , , (2) , , (3)

1
2
3

C. Maier

Function : Author

University of Vienna [Vienna]

B. L. Ziegler

Function : Author

University of Vienna [Vienna]

S. J. Lilly

Function : Author

T. Contini

Function : Author
PersonId : 178293
IdHAL : thierry-contini
ORCID : 0000-0003-0275-938X
IdRef : 112340571

Institut de recherche en astrophysique et planétologie

E. Pérez-Montero

Function : Author

F. Lamareille

Function : Author

Institut de recherche en astrophysique et planétologie

M. Bolzonella

Function : Author

E. Le Floc’h

Function : Author

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: evolution galaxies: high-redshift galaxies: star formation

Domains

Physics [physics] Astrophysics [astro-ph]

Fichier principal

aa25224-14.pdf (1.64 Mo)

Origin : Publication funded by an institution

EDP Sciences : Connect in order to contact the contributor

https://hal-cea.archives-ouvertes.fr/cea-01300564

Submitted on : Monday, April 11, 2016-11:29:12 AM

Last modification on : Wednesday, February 8, 2023-5:10:59 PM

Dates and versions

cea-01300564 , version 1 (11-04-2016)

Identifiers

HAL Id : cea-01300564 , version 1
DOI : 10.1051/0004-6361/201425224

Cite

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, 2015, 577, pp.A14. ⟨10.1051/0004-6361/201425224⟩. ⟨cea-01300564⟩

Export

BibTeX TEI Dublin Core DC Terms EndNote Datacite

Collections

IRD CEA INSU METEO CNRS OMP OMP-IRAP DSM-IRFU IRFU-SAP CEA-UPSAY UNIV-PARIS-SACLAY CEA-DRF UNIV-UT3 UT3-TOULOUSEINP

1904 View

5181 Download