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Table 1

M 31 GCs analysed in the present work.

ID RA (J2000.0) Dec (J2000.0) dp S/N Reference
(kpc) (pixel-1)

B126 00:42:43.481 +41:12:42.47 0.79 73 a
B134 00:42:51.678 +41:44:03.42 0.52 70 a
B158 00:43:14.406 +41:47:21.28 2.40 120 a
B163 00:43:17.640 +41:27:44.91 3.01 170 a
B222 00:44:25.380 +41:14:11.62 4.37 30 a
B225 00:44:29.560 +41:21:35.27 4.69 169 a
B234 00:44:46.375 +41:29:17.77 6.03 71 a
B292 00:36:16.666 +40:58:26.58 17.15 32 a
B301 00:38:21.581 +40:03:37.16 20.09 31 a
B302 00:38:33.500 +41:20:52.29 10.81 28 a
B304 00:38:56.940 +41:10:28.41 9.85 34 a
B305 00:38:58.922 +40:16:31.78 16.74 15 a
B307 00:39:18.477 +40:32:58.05 13.27 20 a
B310 00:39:25.752 +41:23:33.14 8.67 35 a
B313 00:39:44.599 +40:52:55.05 9.38 52 a
B314 00:39:44.599 +40:14:07.95 16.15 17 a
B316 00:39:53.604 +40:41:39.29 10.78 20 a
B321 00:40:15.545 +40:27:46.50 12.78 30 a
B322 00:40:17.270 +40:39:04.70 10.57 69 a
B324 00:40:20.477 +41:40:49.38 8.33 71 a
B327 00:40:24.107 +40:36:22.52 10.91 30 a
B328 00:40:24.529 +41:40:23.15 8.13 30 a
B331 00:40:26.642 +41:42:04.28 8.35 15 a
B337 00:40:48.477 +42:12:11.06 13.71 178 a
B347 00:42:22.892 +41:24:27.58 8.79 61 a
B350 00:42:28.442 +40:24:51.12 11.73 39 a
B354 00:42:47.645 +42:00:24.73 10.10 30 a
B365 00:44:36.445 +42:17:20.57 14.77 60 a
B380 00:46:06.238 +42:00:53.13 13.36 43 a
B383 00:46:11.498 +41:19:41.48 8.94 85 a
B393 00:47:01.204 +41:24:66.39 11.16 43 a
B398 00:47:57.786 +41:48:45.66 15.32 44 a
B401 00:48:08.508 +41:40:41.93 14.96 54 a
MGC1 00:50:42.459 +32:54:58.78 116.05 20 b
MCGC5 00:35:59.700 +35:11:03.60 78.49 20 b
MCGC10 01:07:26.318 +35:46:48.41 99.85 20 b
NB16 00:42:33.094 +41:20:16.41 1.05 142 a
NB89 00:42:44.780 +41:14:44.20 0.34 110 a

Notes. The first column gives the GC identification, as in the Bologna catalogue (Galleti et al. 2004). Second and third columns give the coordinates of the objects, in J2000. Fourth column shows the projected distance of the cluster to the centre of M 31 (see text in Sect. 2.1). Fifth column shows the S/N of the spectra as given in the corresponding paper; when this information was not available (clusters B302, B305, B307, B316, B331, B354), we estimated the S/N around 5000 Å using standard IRAF2 routines. Sixth column gives the reference of the spectra: (a) for Beasley et al. (2004) and (b) for Alves-Brito et al. (2009).

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