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Table 3

List of ISIS targets.

ID J H K S E(J − KS) V LSR Spectral
(km   s-1) type

18365544−0643364d 8.35 ± 0.02 7.34 ± 0.02 6.95 ± 0.03 0.51 +48 K4   II
18372648−0628397 8.88 ± 0.03 6.95 ± 0.02 6.09 ± 0.02 1.73 +68 M1   Ib
18372699−0628444 7.12 ± 0.02 5.90 ± 0.02 5.37 ± 0.02 0.50 +66 M6–7   II
18382442−0522521 8.14 ± 0.03 7.00 ± 0.03 6.57 ± 0.02 0.44 −21 M3.5   II–III
18383565−0603043 7.78 ± 0.02 6.64 ± 0.02 6.18 ± 0.02 0.47 +36 M3.5   III
18384011−0547537 7.42 ± 0.02 6.10 ± 0.03 5.48 ± 0.02 0.64 +24 M7   II–III
18391838−0600383 (D6) 7.72 ± 0.02 5.92 ± 0.03 5.07 ± 0.02 1.51 +108 M3.5   Iab
18391952−0559194 (D19) 8.28 ± 0.02 6.58 ± 0.04 5.80 ± 0.02 1.38 +111 M2   Ia
18391961−0600408 (D2) 6.90 ± 0.02 5.05 ± 0.02 4.12 ± 0.27 1.49 +121 M7.5   I
18392506−0610036 7.76 ± 0.05 6.53 ± 0.04 6.05 ± 0.02 0.58 +61 M3   II–III
18394635−0559473 7.05 ± 0.02 5.34 ± 0.02 4.51 ± 0.02 1.36 +110 M4   Ib
18395282−0535172 6.81 ± 0.02 5.41 ± 0.03 4.75 ± 0.03 0.74 +56 M8   I–II
18402741−0556336 12.09 ± 0.03 10.84 ± 0.02 10.38 ± 0.03 0.58 +21 M3   II
18402744−0556176 8.58 ± 0.02 7.44 ± 0.02 6.95 ± 0.02 0.50 +53 M3   II
18403179−0529522 7.88 ± 0.03 6.55 ± 0.04 5.98 ± 0.02 0.61 +36 M7   II–III
18405021−0552520 7.66 ± 0.03 6.49 ± 0.03 6.00 ± 0.02 0.41 +71 M6   II–III
18405351−0517488 8.42 ± 0.03 7.20 ± 0.04 6.74 ± 0.03 0.69 +71 K7   Iab
18405360−0525004 7.53 ± 0.02 6.12 ± 0.05 5.46 ± 0.02 0.93 +113 M3   Ib
18410764−0535045 8.16 ± 0.02 7.12 ± 0.03 6.67 ± 0.02 0.25 −26 M6–7   II
18410851−0555046 8.18 ± 0.02 6.98 ± 0.03 6.50 ± 0.02 0.51 +71 M4.5   II
18412383−0526073 7.79 ± 0.02 6.43 ± 0.03 5.87 ± 0.02 0.90 +103 M0   Iab
18414143−0531378 8.23 ± 0.04 7.23 ± 0.04 6.81 ± 0.02 0.61 +73 K3   Iab
18415112−0610503 7.99 ± 0.02 6.91 ± 0.03 6.48 ± 0.03 0.31 +21 M5   Ib–II
18415256−0611381 11.83 ± 0.02 10.13 ± 0.02 9.42 ± 0.02 1.78 −1 K0   III
18421965−0545389 10.32 ± 0.02 9.30 ± 0.03 8.87 ± 0.03 0.44 +49 M0   Iab
18422147−0545383 8.53 ± 0.02 7.41 ± 0.05 6.98 ± 0.02 0.37 +34 M4.5   III

Notes. Objects marked with a

were not primary targets and their identifications are based on slit reconstruction. Such objects felt in the slit by chance and do not necessarily fulfill the selection criteria.

(d)

The JHKS magnitudes are from 2MASS. Spectral types are based solely on our spectra. The colour excess has been calculated from the observed (J − KS) colour and the tabulated intrinsic colour, after Levesque et al. (2005).

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