Table 1: Observing runs. The first column gives the month and year of the observations, the second column lists the instrumental combination utilized. The third column gives the number of spectra.

Date
Instr. configuration n

High-resolution spectra

Feb.-97
Echelle-REOSC, 2.15-m, CASLEO 2
Mar.-97 CES+LC, CAT 1.4-m, ESO 4
Feb.-98 Echelle-REOSC, 2.15-m, CASLEO 5
Feb.-99 Echelle-REOSC, 2.15-m, CASLEO 3
May-01 FEROS, 1.5-m, ESO 4
Mar.-02 FEROS, 1.5-m, ESO 4
Mar.-02 EMMI-REMD/Ech, NTT, ESO 2
Apr.-02 FEROS, 1.5-m, ESO 1
Jan.-03 Echelle-REOSC, 2.15-m, CASLEO 4
Mar.-03 Echelle-REOSC, 2.15-m, CASLEO 3
Apr.-03 Echelle-REOSC, 2.15-m, CASLEO 5
May-03 FEROS, 2.2-m, ESO 3
Dec.-03 Echelle-REOSC, 2.15-m, CASLEO 2
May-04 FEROS, 2.2-m, ESO 3
Apr.-05 Echelle, 2.5-m, LCO 4
Feb.-06 Echelle, 2.5-m, LCO 1

Medium-resolution spectra

Feb.-94
2D-Frutti, 1-m, CTIO 2
Apr.-96 B&C, 1.5-m, ESO 2
Feb.-02 CSpec, 1.5-m, CTIO 4

Low-resolution spectra

May-73
Cass, 0.9-m, CTIO 2
Dec.-97 B&C, 2.15-m, CASLEO 4
Apr.-01 REOSC-DS, 2.15-m, CASLEO 6


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