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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 2.

Example JWST/NIRISS data products for a galaxy (ID 02969) in the A2744 field. The top row shows the RGB thumbnail, F115W thumbnail, and emission-line maps, with observed wavelengths labeled. Each image spans 3″ × 3″ (∼25 kpc at z = 1.36) at ﹩0\mathop{.}\limits^{^{\prime\prime} }03﹩ per pixel. The bottom left panel shows the log p(z) plot, the unnormalized logarithm of the posterior redshift probability density, which is used to assess the relative likelihood of different redshift solutions, showing a sharp peak at z = 1.36 with a narrow redshift posterior uncertainty, indicating a well-constrained redshift solution. The bottom right panel shows the 1D NIRISS grism spectra covered in F115W, F150W, and F200W filters.

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