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Table 2.

Log of the GTC OSIRIS spectroscopic observations.

Name RA Dec J G Date Date SNR
hh:mm:ss.ss °:′:″ mag mag yyyy-mm-dd s 6750–6800 Å
cbd67 12:18:32.71 +27:37:31.3 17.551 22.485 13-04-2018 2 × 1800 4.9
cbd34 12:23:57.37 +24:53:29.0 15.940 20.140 13-04-2018 2 × 1500 12.9
cbd34 12:23:57.37 +24:53:29.0 15.940 20.140 13-05-2018 2 × 1500 7.8
cbd10 12:21:02.46 +26:22:04.2 16.814 21.139 12-04-2018 2 × 1500 2.0
ComaBer 4 12:35:56.59 +25:21:11.2 17.993 22.928 13-05-2018 2 × 1800 4.9
ComaBer 5 12:45:25.19 +28:18:16.2 17.801 22.736 13-05-2018 6 × 1800 7.0
ComaBer 7 12:18:27.25 +31:15:53.3 17.162 > 21.36 12-05-2018 2 × 1500 3.6
T159 12:11:14.90 +23:35:39.9 16.787 22.736 29-04-2018 2 × 1800 3.9
T191 12:42:53.70 +24:55:07.1 17.530 22.736 29-04-2018 4 × 1960 4.1
T191 12:42:53.70 +24:55:07.1 17.530 22.736 01-05-2018 2 × 1960 3.2
T191 12:42:53.70 +24:55:07.1 17.530 22.736 11-05-2018 2 × 1960 7.6

DENIS1228 12:28:15.20 −15:47:34.2 14.378 13-04-2018 2 × 370 10.1

Notes. The names of the targets as given in Casewell et al. (2006) and Tang et al. (2018), and this paper, respectively, are listed along with their coordinates, magnitudes, dates of observations, instrumental set-up, weather conditions, and spectral types derived in this work. The last row is a well-known field lithium L-dwarf template (Martín et al. 1997, 1999) observed as part of our programme GTC55-19A.

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