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Early Results from GLASS-JWST. XXVI. Spatially Resolved Star Formation and Balmer Decrements at 1.1 < z < 2.3 from NIRISS Slitless Spectroscopy

  • Authors: Pengfei Ren, Xin Wang, Yuxuan Pang, Mengting Ju, Tucker Jones, Karl Glazebrook, Matthew A. Malkan, Gabriel Brammer, Victoria Strait, Themiya Nanayakkara, Tommaso Treu, Benedetta Vulcani, Peter J. Watson

Pengfei Ren et al 2026 The Astrophysical Journal Letters 1005 .

  • Provider: AAS Journals

Caption: Figure 1.

SFR and stellar mass (M*) for our galaxy samples, which are corrected for lensing magnification using the mass model of P. Bergamini et al. (2023). Blue and red dots correspond to the galaxies for the 1.10 ≤ z ≤ 1.53 and 1.76 ≤ z ≤ 2.29 samples, respectively. The stellar mass ranges adopted for stacking are denoted by the gray shaded regions, and medians for each bin are indicated by dark squares. The thick solid lines represent SFMS from K. E. Whitaker et al. (2014).

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