Image Details
Caption: Figure 5.
MZR measurements for the star-forming field galaxies behind the A2744 cluster. Left: the individual (hollow) and the stacked (solid) result of our galaxy sample at z ∈ [1.8, 2.3] (blue triangles) and z ∈ [2.6, 3.4] (red squares), with their linear fits represented by shaded regions and solid lines. Right: comparison to other observational works, along with the IllustrisTNG100 simulation (Torrey et al. 2019) and the FIRE simulation (Ma et al. 2016). These colored lines are linear regressions of their respective results, with their parameters summarized in Table 3.
© 2024. The Author(s). Published by the American Astronomical Society.