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CECILIA: Ultradeep Rest-optical Spectra of Faint Galaxies at Cosmic Noon

  • Authors: Menelaos Raptis, Ryan F. Trainor, Allison L. Strom, Gwen C. Rudie, Noah S. J. Rogers, Charles C. Steidel, Michael V. Maseda, Caroline von Raesfeld, Nathalie A. Korhonen Cuestas

Menelaos Raptis et al 2025 The Astrophysical Journal Letters 989 .

  • Provider: AAS Journals

Caption: Figure 10.

N2 (left) and S2-BPT (right) diagrams. Our data points are compared to 11 galaxies at z ∼ 2–6 from R. L. Sanders et al. (2024; diamonds) and the stacked points from F. Bian et al. (2018; stars), both color-coded by their direct metallicities, as indicated by the color bar on the right. The F. Bian et al. (2018) sample was selected on the basis of N2-BPT line ratios, with the gray shading denoting the selection region. In the N2-BPT diagram, the stacked point from T16 and D40 from R24 (black and purple outlines, respectively) are shown as circles with the same O/H-based central color coding.

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