Ly emitters in the GOODS-S field - A powerful pure nebular SED with N IV] emission at z = 5.563

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Volume 510 (February 2010)

A&A, 510 (2010) A109

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Table 4:

Photometry (AB magnitudes) of sample sources in the GOODS passbands with their 1 $\sigma$ errors.
GDS-id	$r_{\rm e}$ ('')	z	IRAC4	IRAC3	IRAC2	IRAC1	Ks	H	J	z	i	V	B
J033229.14-274852.6	0.138	3.597	-24.54	-24.40	24.15 $\pm$ 0.21	24.32 $\pm$ 0.15	24.20 $\pm$ 0.10	24.56 $\pm$ 0.13	24.60 $\pm$ 0.13	24.40 $\pm$ 0.03	24.48 $\pm$ 0.03	24.89 $\pm$ 0.02	26.25 $\pm$ 0.09
J033201.84-274206.6	0.169	3.603	...	...	23.32 $\pm$ 0.14	23.59 $\pm$ 0.11	23.77 $\pm$ 0.08	25.21 $\pm$ 0.18	-25.90	25.00 $\pm$ 0.06	25.06 $\pm$ 0.05	25.14 $\pm$ 0.03	27.16 $\pm$ 0.37
J033217.13-274217.8	0.127	3.617	-24.50	-24.50	24.80 $\pm$ 0.27	25.04 $\pm$ 0.22	25.04 $\pm$ 0.15	24.67 $\pm$ 0.13	25.72 $\pm$ 0.22	24.98 $\pm$ 0.05	25.03 $\pm$ 0.04	25.12 $\pm$ 0.03	26.92 $\pm$ 0.17
J033233.33-275007.4	0.138	3.791	-24.44	-24.96	25.03 $\pm$ 0.30	25.21 $\pm$ 0.23	24.99 $\pm$ 0.15	24.81 $\pm$ 0.14	24.62 $\pm$ 0.13	24.70 $\pm$ 0.04	24.72 $\pm$ 0.03	24.99 $\pm$ 0.02	27.35 $\pm$ 0.12
J033236.83-274558.0	0.153	3.797	-23.97	-24.57	24.11 $\pm$ 0.24	24.10 $\pm$ 0.16	24.55 $\pm$ 0.13	24.57 $\pm$ 0.13	24.55 $\pm$ 0.13	24.54 $\pm$ 0.02	24.62 $\pm$ 0.02	25.16 $\pm$ 0.02	27.50 $\pm$ 0.14
J033240.38-274431.0	0.111	4.12	-24.48	-24.82	25.10 $\pm$ 0.37	24.59 $\pm$ 0.21	24.93 $\pm$ 0.15	24.59 $\pm$ 0.13	25.38 $\pm$ 0.19	24.99 $\pm$ 0.04	25.07 $\pm$ 0.03	25.64 $\pm$ 0.04	-28.70
J033234.36-274855.8	0.251	4.138	-23.91	23.70 $\pm$ 0.40	23.47 $\pm$ 0.15	23.34 $\pm$ 0.10	23.63 $\pm$ 0.08	24.03 $\pm$ 0.10	24.29 $\pm$ 0.11	24.10 $\pm$ 0.02	24.25 $\pm$ 0.02	25.23 $\pm$ 0.03	28.00 $\pm$ 0.29
J033248.24-275136.9	0.146	4.374	-24.54	-24.54	25.00 $\pm$ 0.31	24.46 $\pm$ 0.14	24.93 $\pm$ 0.15	25.82 $\pm$ 0.25	24.75 $\pm$ 0.13	24.81 $\pm$ 0.04	24.91 $\pm$ 0.03	25.78 $\pm$ 0.05	-28.51
J033257.17-275145.0	0.173	4.76	-24.55	-24.54	24.87 $\pm$ 0.25	24.32 $\pm$ 0.13	24.36 $\pm$ 0.11	24.77 $\pm$ 0.14	25.22 $\pm$ 0.17	24.54 $\pm$ 0.03	24.53 $\pm$ 0.03	25.79 $\pm$ 0.06	-28.60
J033229.29-275619.5	0.156	4.762	21.31 $\pm$ 0.24	22.52 $\pm$ 0.25	23.05 $\pm$ 0.12	23.00 $\pm$ 0.08	...	...	...	24.86 $\pm$ 0.05	25.12 $\pm$ 0.04	26.93 $\pm$ 0.14	-28.86
J033210.03-274132.7	0.112	4.811	-24.5	-24.60	24.46 $\pm$ 0.31	24.27 $\pm$ 0.16	25.25 $\pm$ 0.18	24.54 $\pm$ 0.13	25.02 $\pm$ 0.19	24.94 $\pm$ 0.05	25.12 $\pm$ 0.05	26.78 $\pm$ 0.12	-28.61
J033221.30-274051.2	0.155	5.292	-24.5	-24.29	25.15 $\pm$ 0.32	25.68 $\pm$ 0.29	25.32 $\pm$ 0.18	...	25.71 $\pm$ 0.22	25.14 $\pm$ 0.08	25.13 $\pm$ 0.10	28.33 $\pm$ 0.25	-29.50
J033245.43-275438.5	0.190	5.375	-24.5	-24.50	24.02 $\pm$ 0.19	24.71 $\pm$ 0.18	24.86 $\pm$ 0.14	24.94 $\pm$ 0.15	24.88 $\pm$ 0.14	25.00 $\pm$ 0.05	25.70 $\pm$ 0.07	-28.97	-28.76
J033237.63-275022.4	0.263	5.518	-24.24	-24.24	24.57 $\pm$ 0.30	24.69 $\pm$ 0.24	25.40 $\pm$ 0.31	24.60 $\pm$ 0.20	25.82 $\pm$ 0.25	25.71 $\pm$ 0.10	26.28 $\pm$ 0.22	-29.50	-29.50
J033218.92-275302.7	0.109	5.563	23.15 $\pm$ 0.20	23.70 $\pm$ 0.31	23.37 $\pm$ 0.08	23.20 $\pm$ 0.07	24.45 $\pm$ 0.11	24.96 $\pm$ 0.14	24.73 $\pm$ 0.11	24.53 $\pm$ 0.04	25.18 $\pm$ 0.05	27.48 $\pm$ 0.03	-28.75
J033225.61-275548.7	0.110	5.786	-24.61	-24.60	24.45 $\pm$ 0.19	24.04 $\pm$ 0.11	25.04 $\pm$ 0.15	24.81 $\pm$ 0.14	24.61 $\pm$ 0.12	24.42 $\pm$ 0.04	26.32 $\pm$ 0.17	27.67 $\pm$ 0.23	-29.51
J033246.04-274929.7	0.120	5.787	-24.49	-24.49	25.65 $\pm$ 0.39	26.10 $\pm$ 0.32	25.49 $\pm$ 0.19	25.66 $\pm$ 0.21	25.85 $\pm$ 0.22	26.26 $\pm$ 0.14	27.83 $\pm$ 0.45	-29.08	-29.21
J033240.01-274815.0	0.120	5.828	-24.6	-24.80	24.48 $\pm$ 0.20	24.49 $\pm$ 0.14	25.32 $\pm$ 0.17	25.00 $\pm$ 0.13	25.07 $\pm$ 0.15	25.21 $\pm$ 0.06	26.52 $\pm$ 0.15	-29.65	-29.46

Notes. Negative numbers indicate upper limits. Also given are the half-light radii and the redshift measured from Ly $\alpha$ .

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