Fig. 1.
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F356W grism spectra for six Hα emitters in our sample. At the top of each panel, we report the stellar mass of the galaxy. The shaded region shows the uncertainty on the flux, and the 1.5″ × 1.5″ insets show false-color rest-frame optical RGB images constructed from NIRCam F115W/F200W/F356W. The green and brown lines highlight the Hαλ6564.6 and [N II] λλ6549.9, 6585.4 wavelengths, respectively.
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