Fig. 1.

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RGB mosaic of CEERS DR v.1.0 NIRCam data showing the position of our sample of dropouts, which is described in Sect. 4. Sources belonging to the UHR galaxy candidate sample are represented by colored star markers (see Sect. 7.1), while the strong line emitter CURION is depicted with a diamond marker (see Sect. 7.4). All other F200W dropouts are instead indicated by gray circles. The available CEERS DR 0.6 MIRI pointings overlapping with the EGS NIRCam-covered area are shown as red contours.
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