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Table 8

GES calibrating globular clusters, with basic properties from the Harris Galactic GC catalog (Harris 1996, 2010), except where noted.

Cluster [Fe/H] E(BV) (mM)V RV σ0 Status Notes
(dex) (mag) (mag) (km s-1) (km s-1)

NGC 1851 –1.18 0.02 15.47 320.5 10.4 in iDR1 GALAH
NGC 4372 –2.17 0.39 15.03 72.3 3.9a in iDR1 metal-poor
NGC 5927 –0.49 0.45 15.82 –107.5 5.1a in iDR1 metal-rich
NGC 2808 –1.14 0.22 15.59 101.6 13.4 in iDR2 well studied
NGC 7078 (M 15) –2.37 0.10 15.39 –107.0 13.5 in iDR2 APOGEE, GALAH
NGC 4833 –1.85 0.32 15.08 200.2 3.9a in iDR2 metal-poor
NGC 6752 –1.54 0.02 13.13 –26.7 4.9 in iDR3 RAVE, GALAH
NGC 104 (47 Tuc) –0.72 0.04 13.37 –18.0 11.0 in iDR3/4 GALAH
NGC 362 –1.26 0.05 14.83 223.5 6.4 in iDR4 GALAH
NGC 1904 (M 79) –1.60 0.01 15.59 205.8 5.3 in iDR4 well studied
NGC 7089 (M 2) –1.65 0.06 15.50 –5.3 8.2 in iDR4 APOGEE
NGC 6553 –0.18 0.63 15.83 –3.2 6.1 observed metal-rich
NGC 1261 –1.27 0.01 16.09 68.2 ... observed well studied
NGC 6218 (M 12) –1.37 0.19 14.01 –41.4 4.5 observed RAVE

Notes. The status column specifies the processing cycle in which each GC was analyzed for the first time (see Sect. 2), and the last column indicates other surveys using each GC as calibrator, along with other useful annotations.

(a)

Radial velocity dispersion from Lardo et al. (2015).

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