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Early Results from GLASS-JWST. XXIV. The Mass–Metallicity Relation in Lensed Field Galaxies at Cosmic Noon with NIRISS

  • Authors: Xianlong He, Xin Wang, Tucker Jones, Tommaso Treu, K. Glazebrook, Matthew A. Malkan, Benedetta Vulcani, Benjamin Metha, Maruša Bradač, Gabriel Brammer, Guido Roberts-Borsani, Victoria Strait, Andrea Bonchi, Marco Castellano, Adriano Fontana, Charlotte Mason, Emiliano Merlin, Takahiro Morishita, Diego Paris, Paola Santini, Michele Trenti, Kristan Boyett, K. Grasha

Xianlong He et al 2024 The Astrophysical Journal Letters 960 .

  • Provider: AAS Journals

Caption: Figure 4.

Stacked grism spectra for galaxies residing in several mass bins at two redshift ranges, as shown in the upper (1.8 < z < 2.3) and lower (2.6 < z < 3.4) panels, respectively. Each mass bin contains 5 ∼ 11 galaxies, with the exact number of galaxies and corresponding mass range highlighted above each stacked spectrum. In each set of spectra, the blue curves represent the median stacked spectrum, the cyan bands mark the standard deviation flux uncertainties, and the red dashed curves show the best-fit Gaussian fits to multiple emission lines, while [S II] and Hα are across a discontinuous range among other lines (i.e., the [O III] λ λ 4960,5008 doublets, Hβ, Hγ, Hδ, [Ne III], and [O II]) in the broken axes at the right parts. The details of the stacking procedures are presented in Section 3.5.

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