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Table 2.

Confirmed and candidate cool stars in the MUSE field.

MSB α (J2000) δ (J2000) V I F475W F814W J K Classification Comments
18 10 21 42.33 +18 05 46.87 23.27 21.70 24.129 21.823 20.972 20.254 AGB? Cand. M-AGB (L16)
10 10 21 43.85 +18 05 30.70 23.00 20.97 24.175 21.029 20.073 18.773 Carbon star Cand. C-AGB (L16)
8 10 21 44.24 +18 05 46.50 22.97 20.90 24.099 20.878 19.464 18.451 Carbon star Cand. M-AGB (L16)
13 10 21 44.83 +18 05 30.87 22.63 21.20 23.430 21.308 20.495 19.691 AGB? Cand. M-AGB (L16)
21 10 21 44.73 +18 05 48.13 23.30 21.97 23.959 22.040 21.198 20.311 ? Cand. M-AGB (L16)

1 10 21 43.27 +18 05 13.36 20.02 20.03 ... ... 15.692 14.979 M (f/g?) 2MASS: J10214334+1805133
... 10 21 43.32 +18 05 03.22 ... ... ... ... 16.156 15.362 K (f/g) 2MASS: J10214332+1805032
5 10 21 43.48 +18 05 09.43 22.05 20.27 22.975 19.796 ... ... M (f/g)

Notes.

Identifiers and V- and I-band photometry are from McQuinn et al. (2013); F475W and F814W photometry is from HST imaging by McQuinn et al. (2015). IR photometry is from Lee (2016, with his classifications in the final column), and 2MASS (Skrutskie et al. 2006) for two of the foreground objects.

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