Figure 4 from The MOSDEF Survey: A Stellar Mass–SFR–Metallicity Relation Exists at z ∼ 2.3

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The MOSDEF Survey: A Stellar Mass–SFR–Metallicity Relation Exists at z ∼ 2.3

Authors: Ryan L. Sanders, Alice E. Shapley, Mariska Kriek, William R. Freeman, Naveen A. Reddy, Brian Siana, Alison L. Coil, Bahram Mobasher, Romeel Davé, Irene Shivaei, Mojegan Azadi, Sedona H. Price, Gene Leung, Tara Fetherholf, Laura de Groot, Tom Zick, Francesca M. Fornasini, and Guillermo Barro

2018 The Astrophysical Journal 858 99.

Provider: AAS Journals

Caption: Figure 4.

Deviation plots for O32 and metallicity estimated using O32, with points and lines the same as in Figure 3. In each panel, the left vertical axis shows the scale of the residuals in each line ratio, while the right vertical axis displays the scale of the corresponding residuals in metallicity. The best-fit slope for the z ∼ 2.3 Δlog(O/H) (O32) versus Δlog(sSFR/yr⁻¹) relation is presented in Table 3.

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