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Table 2

Log of spectroscopic observations.

Target Date UTC Exp Airmass Seeing (S/N)/px vhel Corrhel
(s) (′′) km s-1 km s-1

#1 2010-05-05 09:49:21.971 2700 1.057 0.93 61 96.65 24.31
2010-05-06 08:10:16.920 5400 1.014 1.00 96.52 24.20
#2 2010-05-05 05:46:51.973 5400 1.160 1.22 54 90.01 24.67
#3 2010-05-05 07:30:43.969 5400 1.021 1.11 58 100.38 24.52
#4 2010-06-22 01:24:06.707 4600 1.450 1.47 37 99.78 6.14
2010-06-22 03:11:28.710 4600 1.103 1.77 99.82 6.01
#5 2010-06-22 04:33:50.710 4500 1.018 1.56 42 96.16 5.89
2010-06-22 05:50:02.710 4500 1.027 1.54 96.20 5.75
#6 2010-06-22 07:42:12.708 4500 1.211 1.47 26 94.08 5.57
2010-06-22 08:58:04.707 4500 1.540 1.62 94.25 5.46
#7 2010-06-23 04:18:17.468 4500 1.024 0.84 42 98.84 5.44
2010-06-25 05:06:03.250 3600 1.011 1.39 99.01 5.31
2010-06-25 06:06:55.251 3600 1.043 1.55 99.05 4.29
#8 2010-06-23 01:12:15.468 4500 1.500 1.07 31 7.29 5.71
2010-06-23 02:28:33.467 4500 1.191 0.91 7.35 5.63

Notes. For stars with several individual exposures, the signal-to-noise value corresponds to that of the final averaged spectrum.

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