**Table 2:** Redshifts for the first 10 galaxies $^{{\rm *}}$ in the sample of 143 measured with 2dF in the cluster A3667 and falling in the redshift range $0.044 \leq z \leq 0.068$ .
ID	RA	Dec	$m_{\rm B}$	$z_{\rm abs}$	$z_{\rm em}$	$z_{\rm ave}$	$z_{\rm lit}$	morphological
	(J2000)	(J2000)						type
1	20 05 37.49	-56 41 06.1	16.89	0.0558				2
2	20 06 26.98	-56 19 50.9	18.16	0.0586				3
3	20 07 22.03	-56 39 44.0	16.41	0.0535				2
4	20 07 29.09	-57 28 46.2	18.09	0.0553	0.0553	0.0553		5
5	20 07 30.08	-57 22 58.6	16.75	0.0521	0.0518	0.0520		3
6	20 07 32.50	-56 34 45.9	17.43	0.0560	0.0557	0.0559		4
7	20 07 56.06	-56 16 01.3	16.65	0.0543	0.0545	0.0544	0.0535	5
8	20 08 01.56	-56 06 07.6	17.60	0.0594	0.0594	0.0594		3
9	20 08 09.17	-56 30 21.7	16.80	0.0523			0.0524	2
10	20 08 27.61	-56 20 42.5	17.79	0.0572	0.0569	0.05705		3

$^{{\rm *}}$ The full data table contains 143 objects and is available in electronic form at CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/479/1. Column 1 gives the source ID number; Cols. 2 and 3 are the Right Ascension and Declination in J2000 coordinates; Col. 4 is the blue magnitude; Cols. 6 and 7 are the redshifts as determined by absorption and emission features, respectively, and Col. 8 is the average redshift for cases where a redshift could be determined by both emission and absoprtion features; Col. 9 is the previously published redshift and Col. 10 is the morphological type determined by the best correlation to the spectral templates used by 2dfdr, numbers correspond to those listed in Colless et al. (2001).

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