Cite
Stellar Mass--Gas-phase Metallicity Relation at $0.5\leq z\leq0.7$: A Power Law with Increasing Scatter toward the Low-mass Regime
MLA
J. A. Newman, et al. Stellar Mass--Gas-Phase Metallicity Relation at $0.5\leq Z\leq0.7$: A Power Law with Increasing Scatter toward the Low-Mass Regime. Jan. 2016. EBSCOhost, https://doi.org/10.48550/arxiv.1603.04863.
APA
J. A. Newman, Ricardo Amorín, Hassen M. Yesuf, Renbin Yan, Nimish P. Hathi, David J. Rosario, Marc Rafelski, Avishai Dekel, David C. Koo, Joel R. Primack, Romeel Davé, Jonathan R. Trump, Yu Lu, Puragra Guhathakurta, Christopher N. A. Willmer, Yicheng Guo, S. M. Faber, Pablo G. Pérez-González, Michael C. Cooper, … Anton M. Koekemoer. (2016). Stellar Mass--Gas-phase Metallicity Relation at $0.5\leq z\leq0.7$: A Power Law with Increasing Scatter toward the Low-mass Regime. https://doi.org/10.48550/arxiv.1603.04863
Chicago
J. A. Newman, Ricardo Amorín, Hassen M. Yesuf, Renbin Yan, Nimish P. Hathi, David J. Rosario, Marc Rafelski, et al. 2016. “Stellar Mass--Gas-Phase Metallicity Relation at $0.5\leq Z\leq0.7$: A Power Law with Increasing Scatter toward the Low-Mass Regime,” January. doi:10.48550/arxiv.1603.04863.