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A Glimpse of the Stellar Populations and Elemental Abundances of Gravitationally Lensed, Quiescent Galaxies at z ≳ 1 with Keck Deep Spectroscopy

  • Authors: Zhuyun Zhuang, Nicha Leethochawalit, Evan N. Kirby, J. W. Nightingale, Charles C. Steidel, Karl Glazebrook, Tania M. Barone, Hannah Skobe, Sarah M. Sweet, Themiya Nanayakkara, Rebecca J. Allen, Keerthi Vasan G. C., Tucker Jones, Glenn G. Kacprzak, Kim-Vy H. Tran, Colin Jacobs

Zhuyun Zhuang et al 2023 The Astrophysical Journal 948 .

  • Provider: AAS Journals

Caption: Figure 8.

[Fe/H] (top), [Mg/Fe] (middle), and [Mg/H] (bottom) as a function of the stellar mass for quiescent galaxies. AGEL1323 at z = 1.016 and AGEL0014 at z = 1.37 are plotted as a filled square and a pentagon, respectively. The SDSS galaxies at z ∼ 0.05 (open green triangles) are taken from Leethochawalit et al. (2019) but remeasured with alf for consistency. The open yellow stars show the measurements for the LEGA-C sample at 0.59 < z < 0.75 by Beverage et al. (2021). The abundances of individual high-z quiescent galaxies measured by Kriek et al. (2016; blue open down triangle) and Kriek et al. (2019; black open circles) as well as that of a stacked spectrum at z = 1.15 determined by Carnall et al. (2022) are plotted for comparison. The green solid lines and shaded regions represent the best-fit linear relations and intrinsic scatter of the z ∼ 0.05 SDSS galaxies.

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