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Table 4

Photometric properties of the IKN globular clusters (GCs) and the new candidates (GCCs).

ID Dec RA M V VI K S u g r i z
hh:mm:ss dd:mm:ss mag mag mag mag mag mag mag mag
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11)

GC-1 +68:23:36.06 10:08:07.12 −6.66 ± 0.06 0.911 ± 0.079 19.225 ± 0.089 ... 21.955 ± 0.097 21.087 ± 0.062 20.76 ± 0.087 19.876 ± 0.125
GC-2 +68:24:04.95 10:08:10.80 −7.16 ± 0.07 0.994 ± 0.078 18.622 ± 0.054 ... 21.321 ± 0.054 20.648 ± 0.052 20.372 ± 0.068 ...
GC-3 +68:24:33.16 10:08:05.27 −6.77 ± 0.06 1.085 ± 0.092 18.891 ± 0.071 ... ... ... ... ...
GC-4 +68:24:53.07 10:08:04.80 −7.42 ± 0.06 0.936 ± 0.077 18.321 ± 0.043 ... 20.997 ± 0.052 20.424 ± 0.044 20.098 ± 0.053 19.941 ± 0.135
GC-5 +68:24:57.35 10:08:05.52 −8.48 ± 0.06 0.906 ± 0.077 17.293 ± 0.019 21.435 ± 0.174 19.911 ± 0.025 19.312 ± 0.026 19.097 ± 0.044 18.769 ± 0.057
GCC-6 +68:25:29.13 10:08:05.16 −8.50 ± 0.04* ... ... 20.895 ± 0.124 19.675 ± 0.035 19.045 ± 0.03 18.651 ± 0.049 18.716 ± 0.086
GCC-7 +68:28:36.72 10:08:08.85 −7.48 ± 0.04* ... ... ... 20.766 ± 0.038 20.006 ± 0.08 19.895 ± 0.051 19.762 ± 0.107

Notes. Absolute magnitude in Col. (4) is calculated using the distance modulus of mM = 27.79 ± 0.02 mag adopted in the paper. The SDSS u,g,r,i,z are the PSF magnitudes derived in this work. Johnsons/Cousins V,I magnitudes are from Georgiev et al. (2009b).

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