Table 6: The candidate list of the WFILAS survey after the selection as described in Sect. 4. From left to right are the object name, the B, R, M815, New A, N817 and N824 AB-magnitudes, line flux calculated from the narrowband magnitude in which the object was detected and line luminosity. For all measurements less than $2\sigma $ the $2\sigma $ upper limit has been given.
SExtractor ID Object ID B R M815 New A N817 N824 Line flux Luminosity
                (10-17 erg s-1 cm-2) (1043 erg s-1)
CDFS_1864a J033215.14-280013.9 >26.25 >26.56 24.72 $\pm$ 0.46 23.14 $\pm$ 0.26 >24.27 >23.93 6.5 $\pm$ 1.5 2.3 $\pm$ 0.5
CDFS_4928a J033145.97-275316.4 >26.25 >26.56 24.59 $\pm$ 0.41 23.38 $\pm$ 0.32 24.11 $\pm$ 0.47 23.61 $\pm$ 0.41 5.2 $\pm$ 1.6 1.8 $\pm$ 0.5
CDFS_5388a J033202.37-275211.3 >26.25 >26.56 24.70 $\pm$ 0.45 23.32 $\pm$ 0.31 >24.27 >23.93 5.5 $\pm$ 1.5 1.9 $\pm$ 0.5
S11_5236a b J114334.98-014433.7 >26.63 >26.59 24.31 $\pm$ 0.42 >24.13 23.05 $\pm$ 0.18 >23.74 7.0 $\pm$ 1.2 2.5 $\pm$ 0.4
S11_8921c J114218.90-013544.6 >26.63 26.38 $\pm$ 0.45 23.88 $\pm$ 0.28 23.98 $\pm$ 0.47 23.41 $\pm$ 0.26 >23.75 5.0 $\pm$ 1.2 1.8 $\pm$ 0.4
S11_10595 J114312.46-013049.6 >26.63 >26.60 24.44 $\pm$ 0.47 >24.13 23.52 $\pm$ 0.28 >23.75 4.5 $\pm$ 1.2 1.6 $\pm$ 0.4
SGP_8884d J004525.38-292402.8 >26.07 >26.41 23.33 $\pm$ 0.20 22.73 $\pm$ 0.16   >24.06 9.5 $\pm$ 1.4 3.3 $\pm$ 0.5
a Galaxy is in the complete sample. b Confirmed LAE at z = 5.721. See text and Westra et al. (2005) for details. c Signal-to-noise in the range $2{-}3\sigma$ for R band in the 10 pixel aperture, but ${<}2\sigma$ in the 6 pixel aperture. d Confirmed LAE at z = 5.652. See text for details.

Source LaTeX | All tables | In the text