Table 2: Adopted template carbon stars used for deriving radial velocities by cross-correlation. Their velocities, noted $v_{\rm helio}$ , are in km s^-1.

Star $v_{\rm helio}$ Run

APM 1019-1136
+126 $\pm ~4$ April

APM 1406+0520 -21 $\pm ~5$ April

APM 1519-0614 +105 $\pm ~4$ April

IRAS 17446-7809 -5 $\pm ~5$ August

APM 2213-0017 -44 $\pm ~3$ August

APM 0207-0211 -140 $\pm ~5$ August

**Table 2:** Adopted template carbon stars used for deriving radial velocities by cross-correlation. Their velocities, noted $v_{\rm helio}$ , are in km s^-1.
Star	$v_{\rm helio}$	Run
APM 1019-1136	+126 $\pm ~4$	April
APM 1406+0520	-21 $\pm ~5$	April
APM 1519-0614	+105 $\pm ~4$	April
IRAS 17446-7809	-5 $\pm ~5$	August
APM 2213-0017	-44 $\pm ~3$	August
APM 0207-0211	-140 $\pm ~5$	August

Source LaTeX | All tables | In the text

	1 Introduction
	2 Selection of candidates
	3 Observations
	4 General properties of the observed stars
	5 Spectra
	6 Radial velocities
	7 Proper motions
	8 Distances
	9 Analysis and discussion
	10 Concluding remarks
	References
	Online Material
	Appendix A: Spectra