The unusual N IV] -emitter galaxy GDS J033218.92-275302.7: star formation or AGN-driven winds from a massive galaxy at z = 5.56

E. Vanzella; A. Grazian; M. Hayes; L. Pentericci; D. Schaerer; M. Dickinson; S. Cristiani; M. Giavalisco; A. Verhamme; M. Nonino; P. Rosati

doi:10.1051/0004-6361/200913042

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Volume 513 (April 2010)

A&A, 513 (2010) A20

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Table 2:

Summary of the photometric information (magnitudes and 1- $\sigma$ errors) for our source.
$U_{\rm VIMOS}$ $^{\dag }$	B₄₃₅	V₆₀₆	R	i₇₇₅	z₈₅₀	Js	H	Ks	3.6 $\mu{\rm m}$	4.5 $\mu{\rm m}$	5.8 $\mu{\rm m}$	8.0 $\mu{\rm m}$	24 $\mu{\rm m}$
29.49	29.86	27.86	27.11	25.22	24.61	24.68	24.80	24.21	22.82	23.00	23.37	23.18	22.61
1 $\sigma$ l.m	1 $\sigma$ l.m	0.179	0.195	0.039	0.031	0.116	0.151	0.140	0.014	0.024	0.235	0.198	1 $\sigma$ l.m.

Notes. $^{(\dag )}$ Other two WFI U bands are available, U35 and U38 with slightly different filter shape. The lower limits are 27.84 and 26.75, respectively much shallower than the limit provided by the $U_{\rm VIMOS}$ .

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