Ultrahigh-redshift or closer-by, dust-obscured galaxies? - Deciphering the nature of faint, previously missed F200W dropouts in CEERS

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Table G.2.

F356W effective radii of our UHR galaxy candidate sample assuming their z > 8 solutions.

ID	Name	z_high	R_e [arcsec]	R_e [kpc]	n_s	q_s
U-31863	BUDIARA	$17 . 76_{- 1.5}^{+ 1.6}$ $Mathematical equation: $ 17.76^{+1.6}_{-1.5} $$	0.050	0.145 ± 0.067	0.346	0.319
U-34120	VICIADGO	$17 . 56_{- 1.3}^{+ 1.4}$ $Mathematical equation: $ 17.56^{+1.4}_{-1.3} $$	0.109	0.3 ± 0.1	0.307	0.319
U-75985	LIZZAN	$17 . 80_{- 1.45}^{+ 1.48}$ $Mathematical equation: $ 17.80^{+1.48}_{-1.45} $$	0.028	≤0.087	3.052	0.319
U-80918	NASPE	$17 . 55_{- 1.30}^{+ 1.47}$ $Mathematical equation: $ 17.55^{+1.47}_{-1.30} $$	0.049	0.143 ± 0.037	0.558	0.319
A-22691	ARCERIO	$17 . 32_{- 2.98}^{+ 2.05}$ $Mathematical equation: $ 17.32^{+2.05}_{-2.98} $$	0.026	≤0.087	5.2	0.371

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