STELLAR MASS–GAS-PHASE METALLICITY RELATION AT 0.5 ≤ z ≤ 0.7: A POWER LAW WITH INCREASING SCATTER TOWARD THE LOW-MASS REGIME

We present the stellar mass (M-*)-gas-phase metallicity relation (MZR) and its scatter at intermediate redshifts (0.5 <= z <= 0.7) for 1381 field galaxies collected from deep spectroscopic surveys. The star formation rate (SFR) and color at a given M-* of this magnitude-limited (R less than or...

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Bibliographic Details
Main Authors:	Guo, Yicheng, Koo, David C., Lu, Yu, Forbes, John C., Rafelski, Marc, Trump, Jonathan R., Amorín, Ricardo, Barro, Guillermo, Davé, Romeel, Faber, S. M., Hathi, Nimish P., Yesuf, Hassen, Cooper, Michael C., Dekel, Avishai, Guhathakurta, Puragra, Kirby, Evan N., Koekemoer, Anton M., Pérez-González, Pablo G., Lin, Lihwai, Newman, Jeffery A., Primack, Joel R., Rosario, David J., Willmer, Christopher N. A., Yan, Renbin
Other Authors:	Univ Arizona, Steward Observ
Language:	en
Published:	IOP PUBLISHING LTD 2016
Subjects:	galaxies: abundances galaxies: dwarf galaxies: evolution galaxies: formation galaxies: fundamental parameters galaxies: ISM
Online Access:	http://hdl.handle.net/10150/621237 http://arizona.openrepository.com/arizona/handle/10150/621237

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http://hdl.handle.net/10150/621237
http://arizona.openrepository.com/arizona/handle/10150/621237

STELLAR MASS–GAS-PHASE METALLICITY RELATION AT 0.5 ≤ z ≤ 0.7: A POWER LAW WITH INCREASING SCATTER TOWARD THE LOW-MASS REGIME

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