Evolution in the properties of Lyman-α emitters from redshifts z ~ 3 to z ~ 2

K. K. Nilsson; C. Tapken; P. Møller; W. Freudling; J. P. U. Fynbo; K. Meisenheimer; P. Laursen; G. Östlin

doi:10.1051/0004-6361/200810881

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Volume 498 / No 1 (April IV 2009)

A&A, 498 1 (2009) 13-23

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Table 3:

COSMOS broad-bands used.
Band	Observatory	CWL (Å)	FWHM (Å)	Depth
u^*	CFHT	3798	720	26.4
Bj	SUBARU	4460	897	27.3
g⁺	SUBARU	4780	1265	27.0
Vj	SUBARU	5484	946	26.6
r⁺	SUBARU	6295	1382	26.8
i⁺	SUBARU	7641	1497	26.2
z⁺	SUBARU	9037	856	25.2
K_s	KPNO	21500	3200	21.6
The depths are $5\sigma$ AB magnitudes as measured in 3'' apertures
(Capak et al. 2007).

Source LaTeX | All tables | In the text

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