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

Open Access

Table C.1.

Photometry of our F200W dropouts.

ID	Names	f_F435W [nJy]	f_F606W [nJy]	f_F814W [nJy]	f_F105W [nJy]	f_F125W [nJy]	f_F140W [nJy]	f_F160W [nJy]
U-31863	BUDIARA	−	−3.60 ± 5.20	2.39 ± 5.90	−	−	−	−
U-34120	VICIADGO	−	5.23 ± 5.04	−0.78 ± 3.79	−	2.78 ± 5.82	−12.64 ± 14.84	−23.42 ± 5.60
U-53105	-	−0.16 ± 4.45	3.72 ± 4.20	0.89 ± 4.95	−	−8.68 ± 7.16	23.44 ± 12.48	−14.71 ± 6.42
U-75985	LIZZAN	6.49 ± 4.21	2.83 ± 1.79	3.54 ± 2.84	−	−6.22 ± 3.19	−0.41 ± 4.01	−0.58 ± 2.75
U-80918	NASPE	1.41 ± 5.50	0.82 ± 4.33	−3.99 ± 5.51	−	12.79 ± 7.30	12.96 ± 13.28	−1.67 ± 6.48
U-100588	-	0.96 ± 4.16	−3.88 ± 5.46	0.20 ± 5.79	−	11.57 ± 7.28	−3.61 ± 13.06	−6.38 ± 6.68
U-106373	-	−1.85 ± 5.60	0.50 ± 3.81	1.17 ± 6.25	−	4.08 ± 4.60	−	7.77 ± 4.18
U-112842	CURION	−	−1.33 ± 3.25	−1.35 ± 4.02	−10.16 ± 6.45	6.15 ± 5.87	6.68 ± 9.75	−13.74 ± 4.78
A-22691	ARCERIO	−	3.06 ± 3.55	4.13 ± 3.66	−	5.74 ± 10.02	−	5.39 ± 8.89
A-26130	-	−	0.00 ± 5.17	−6.18 ± 5.62	−	17.32 ± 14.25	−	12.02 ± 11.93
A-76468	-	−	−1.23 ± 4.62	5.85 ± 7.08	−	12.42 ± 12.55	−	−9.45 ± 10.53



ID	Names	$f_{F 090 W} [nJy]$ $Mathematical equation: $ \mathrm{f}_{\mathrm{F090W}} \, \mathrm{[nJy]} $$	$f_{F 115 W} [nJy]$ $Mathematical equation: $ \mathrm{f}_{\mathrm{F115W}} \, \mathrm{[nJy]} $$	$f_{F 150 W} [nJy]$ $Mathematical equation: $ \mathrm{f}_{\mathrm{F150W}} \, \mathrm{[nJy]} $$	$f_{F 200 W} [nJy]$ $Mathematical equation: $ \mathrm{f}_{\mathrm{F200W}} \, \mathrm{[nJy]} $$	$f_{F 277 W} [nJy]$ $Mathematical equation: $ \mathrm{f}_{\mathrm{F277W}} \, \mathrm{[nJy]} $$	$f_{F 356 W} [nJy]$ $Mathematical equation: $ \mathrm{f}_{\mathrm{F356W}} \, \mathrm{[nJy]} $$	$f_{F 410 M} [nJy]$ $Mathematical equation: $ \mathrm{f}_{\mathrm{F410M}} \, \mathrm{[nJy]} $$	$f_{F 444 W} [nJy]$ $Mathematical equation: $ \mathrm{f}_{\mathrm{F444W}} \, \mathrm{[nJy]} $$

U-31863	BUDIARA	−	5.64 ± 3.55	4.61 ± 2.53	3.18 ± 1.98	10.18 ± 1.33	11.66 ± 1.49	−	11.70 ± 1.56
U-34120	VICIADGO	5.78 ± 3.46	3.14 ± 1.73	2.84 ± 2.54	1.57 ± 1.91	10.04 ± 1.84	9.28 ± 1.32	12.34 ± 2.49	7.30 ± 1.30
U-53105	-	3.31 ± 3.97	3.74 ± 3.62	7.66 ± 4.04	6.33 ± 3.53	9.41 ± 2.10	13.24 ± 2.02	16.02 ± 4.58	23.06 ± 3.91
U-75985	LIZZAN	1.15 ± 1.17	1.43 ± 2.01	−0.54 ± 1.89	1.64 ± 1.17	5.47 ± 1.07	9.40 ± 1.23	3.38 ± 2.13	4.32 ± 1.03
U-80918	NASPE	4.14 ± 3.60	−	−10.81 ± 9.89	3.98 ± 2.81	12.56 ± 2.13	16.43 ± 2.43	14.88 ± 3.94	8.44 ± 2.06
U-100588	-	−2.86 ± 4.14	−1.75 ± 3.02	5.01 ± 4.11	0.58 ± 3.34	−1.12 ± 2.18	−0.93 ± 2.11	23.04 ± 5.03	27.83 ± 2.22
U-106373	-	2.83 ± 1.88	2.75 ± 3.08	3.08 ± 2.83	4.31 ± 2.34	1.03 ± 1.35	6.67 ± 1.86	18.34 ± 2.64	17.20 ± 1.86
U-112842	CURION	−	0.83 ± 2.41	0.99 ± 2.80	−0.49 ± 1.74	−0.81 ± 1.77	5.18 ± 1.46	31.34 ± 3.37	32.08 ± 1.64
A-22691	ARCERIO	−	1.02 ± 2.16	0.59 ± 2.09	2.65 ± 1.79	7.9 ± 1.83	9.32 ± 1.66	−	8.99 ± 2.97
A-26130	-	−	4.05 ± 2.95	1.09 ± 4.63	0.98 ± 3.63	11.21 ± 3.12	14.38 ± 2.23	25.04 ± 5.45	19.46 ± 4.87
A-76468	-	−	4.37 ± 2.94	3.75 ± 3.41	3.56 ± 2.79	6.55 ± 2.12	8.87 ± 2.13	18.45 ± 4.25	24.66 ± 3.36

Notes. We flagged with “-” all those observations that are not available in a certain band. Negative flux values are likely produced by local over-subtractions of the background, and they were treated in our analysis as upper limits.

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