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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 10.

Left: dependence of [Fe/H], [Mg/Fe], and [Mg/H] on the SSP age (first column) and galaxy formation time (second column). Right: dependence of abundances on the galaxy formation time with the stellar mass dependence removed (see Section 5.1). The gray shaded regions show the 68% confidence interval for z ∼ 0 SDSS galaxies. The symbols for galaxies at different redshifts are the same as in Figure 8.

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