Table 6.

Observational properties of the brightest three GCs in each sample galaxy.

IDRADECI(BI)0(BV)0(UB)0FWHMAREACIMF814Wrgc (kpc)FLAG
(1)(2)(3)(4)(5)(6)(7)(8)(9)(10)(11)(12)(13)
M81-GC1148.8412569.11042516.13 ± 0.032.06 ± 0.101.10 ± 0.101.63 ± 0.103.62−11.663.0302
M81-GC2148.9412369.05009716.75 ± 0.032.24 ± 0.101.27 ± 0.102.05 ± 0.103.45−11.031.5403
M81-GC3149.1144069.01938016.95 ± 0.031.78 ± 0.101.00 ± 0.101.43 ± 0.105.82−10.845.8702
M101-GC1210.82494654.31872317.63 ± 0.022.51 ± 0.001.20 ± 0.171.31 ± 0.413.074491.30−11.574.0003
M101-GC2210.88465154.41416618.57 ± 0.022.74 ± 0.001.14 ± 0.173.383941.50−10.639.8200
M101-GC3210.88450854.36923719.10 ± 0.022.48 ± 0.001.46 ± 0.172.923011.39−10.106.3100
NGC 4258-GC1184.72927047.26486817.83 ± 0.001.63 ± 0.000.79 ± 0.102.693111.16−11.575.2500
NGC 4258-GC2184.86570047.21038917.89 ± 0.003.37 ± 0.011.13 ± 0.102.791651.18−11.5016.7800
NGC 4258-GC3184.74597047.30106717.97 ± 0.002.15 ± 0.010.99 ± 0.100.43 ± 0.054.034401.65−11.420.6902
M51-GC1202.45958447.17471018.90 ± 0.032.05 ± 0.001.07 ± 0.10−0.06 ± 0.173.104621.44−10.763.2302
M51-GC2202.50711747.24184519.18 ± 0.033.50 ± 0.001.52 ± 0.101.17 ± 0.172.772711.35−10.487.9603
M51-GC3202.46942047.25390619.31 ± 0.031.75 ± 0.001.25 ± 0.102.472811.24−10.358.8000
NCG628-GC124.22142915.78891418.28 ± 0.032.51 ± 0.001.08 ± 0.161.82 ± 0.073.334711.56−11.667.8403
NCG628-GC224.17102315.78250019.13 ± 0.031.90 ± 0.000.68 ± 0.160.28 ± 0.092.752431.37−10.810.5202
NCG628-GC324.21297315.73498719.71 ± 0.033.15 ± 0.001.25 ± 0.162.621831.16−10.2310.4800
IDRADECI(BI)0(BV)0(UB)0FWHMAREACIMF814Wrgc (kpc)FLAG
(1)(2)(3)(4)(5)(6)(7)(8)(9)(10)(11)(12)(13)
M81-GC1148.8412569.11042516.13 ± 0.032.06 ± 0.101.10 ± 0.101.63 ± 0.103.62−11.663.0302
M81-GC2148.9412369.05009716.75 ± 0.032.24 ± 0.101.27 ± 0.102.05 ± 0.103.45−11.031.5403
M81-GC3149.1144069.01938016.95 ± 0.031.78 ± 0.101.00 ± 0.101.43 ± 0.105.82−10.845.8702
M101-GC1210.82494654.31872317.63 ± 0.022.51 ± 0.001.20 ± 0.171.31 ± 0.413.074491.30−11.574.0003
M101-GC2210.88465154.41416618.57 ± 0.022.74 ± 0.001.14 ± 0.173.383941.50−10.639.8200
M101-GC3210.88450854.36923719.10 ± 0.022.48 ± 0.001.46 ± 0.172.923011.39−10.106.3100
NGC 4258-GC1184.72927047.26486817.83 ± 0.001.63 ± 0.000.79 ± 0.102.693111.16−11.575.2500
NGC 4258-GC2184.86570047.21038917.89 ± 0.003.37 ± 0.011.13 ± 0.102.791651.18−11.5016.7800
NGC 4258-GC3184.74597047.30106717.97 ± 0.002.15 ± 0.010.99 ± 0.100.43 ± 0.054.034401.65−11.420.6902
M51-GC1202.45958447.17471018.90 ± 0.032.05 ± 0.001.07 ± 0.10−0.06 ± 0.173.104621.44−10.763.2302
M51-GC2202.50711747.24184519.18 ± 0.033.50 ± 0.001.52 ± 0.101.17 ± 0.172.772711.35−10.487.9603
M51-GC3202.46942047.25390619.31 ± 0.031.75 ± 0.001.25 ± 0.102.472811.24−10.358.8000
NCG628-GC124.22142915.78891418.28 ± 0.032.51 ± 0.001.08 ± 0.161.82 ± 0.073.334711.56−11.667.8403
NCG628-GC224.17102315.78250019.13 ± 0.031.90 ± 0.000.68 ± 0.160.28 ± 0.092.752431.37−10.810.5202
NCG628-GC324.21297315.73498719.71 ± 0.033.15 ± 0.001.25 ± 0.162.621831.16−10.2310.4800

Note. (1) Assigned name, which follows the convention of GAL-GCn, where GAL stands for galaxy name and n is 1 for the brightest object in the F814W filter, and increases sequentially as the magnitude increases. (2,3) Right ascension, Declination, coordinates in J2000. (4) Magnitude in F814W-band and magnitude error from SExtractor and aperture correction, added in quadrature, (5) (F435WF814W)0 colour, the error is the quadrature sum of the error in each band from SExtractor. (6) (F435WF555W)0 colour, error is quadrature sum as in column 5. In the case of M81 the colour is (F435WF606W)0. (7) (F336WF435W)0 colour, the error is the quadrature sum of the error in each band. In the case of M81 the colour is. (ug)0. (8) FWHM in pixel units from SExtractor. (9) AREA in pixels from SExtractor. (10) Concentration index, defined as the difference between magnitudes measured in 1 and 3 pixel radius apertures. (11) Absolute magnitude in F814W-band. (12) Galactocentric distance of the GC in kiloparsec. (13) FLAG classification: 00 clusters without U-band photometry; 01 determined as a reddened young cluster from U-band photometry; 02 – determined as bonafide GC from U-band photometry; and 03 – error in U-B is likely to be larger than the indicated formal error.

Table 6.

Observational properties of the brightest three GCs in each sample galaxy.

IDRADECI(BI)0(BV)0(UB)0FWHMAREACIMF814Wrgc (kpc)FLAG
(1)(2)(3)(4)(5)(6)(7)(8)(9)(10)(11)(12)(13)
M81-GC1148.8412569.11042516.13 ± 0.032.06 ± 0.101.10 ± 0.101.63 ± 0.103.62−11.663.0302
M81-GC2148.9412369.05009716.75 ± 0.032.24 ± 0.101.27 ± 0.102.05 ± 0.103.45−11.031.5403
M81-GC3149.1144069.01938016.95 ± 0.031.78 ± 0.101.00 ± 0.101.43 ± 0.105.82−10.845.8702
M101-GC1210.82494654.31872317.63 ± 0.022.51 ± 0.001.20 ± 0.171.31 ± 0.413.074491.30−11.574.0003
M101-GC2210.88465154.41416618.57 ± 0.022.74 ± 0.001.14 ± 0.173.383941.50−10.639.8200
M101-GC3210.88450854.36923719.10 ± 0.022.48 ± 0.001.46 ± 0.172.923011.39−10.106.3100
NGC 4258-GC1184.72927047.26486817.83 ± 0.001.63 ± 0.000.79 ± 0.102.693111.16−11.575.2500
NGC 4258-GC2184.86570047.21038917.89 ± 0.003.37 ± 0.011.13 ± 0.102.791651.18−11.5016.7800
NGC 4258-GC3184.74597047.30106717.97 ± 0.002.15 ± 0.010.99 ± 0.100.43 ± 0.054.034401.65−11.420.6902
M51-GC1202.45958447.17471018.90 ± 0.032.05 ± 0.001.07 ± 0.10−0.06 ± 0.173.104621.44−10.763.2302
M51-GC2202.50711747.24184519.18 ± 0.033.50 ± 0.001.52 ± 0.101.17 ± 0.172.772711.35−10.487.9603
M51-GC3202.46942047.25390619.31 ± 0.031.75 ± 0.001.25 ± 0.102.472811.24−10.358.8000
NCG628-GC124.22142915.78891418.28 ± 0.032.51 ± 0.001.08 ± 0.161.82 ± 0.073.334711.56−11.667.8403
NCG628-GC224.17102315.78250019.13 ± 0.031.90 ± 0.000.68 ± 0.160.28 ± 0.092.752431.37−10.810.5202
NCG628-GC324.21297315.73498719.71 ± 0.033.15 ± 0.001.25 ± 0.162.621831.16−10.2310.4800
IDRADECI(BI)0(BV)0(UB)0FWHMAREACIMF814Wrgc (kpc)FLAG
(1)(2)(3)(4)(5)(6)(7)(8)(9)(10)(11)(12)(13)
M81-GC1148.8412569.11042516.13 ± 0.032.06 ± 0.101.10 ± 0.101.63 ± 0.103.62−11.663.0302
M81-GC2148.9412369.05009716.75 ± 0.032.24 ± 0.101.27 ± 0.102.05 ± 0.103.45−11.031.5403
M81-GC3149.1144069.01938016.95 ± 0.031.78 ± 0.101.00 ± 0.101.43 ± 0.105.82−10.845.8702
M101-GC1210.82494654.31872317.63 ± 0.022.51 ± 0.001.20 ± 0.171.31 ± 0.413.074491.30−11.574.0003
M101-GC2210.88465154.41416618.57 ± 0.022.74 ± 0.001.14 ± 0.173.383941.50−10.639.8200
M101-GC3210.88450854.36923719.10 ± 0.022.48 ± 0.001.46 ± 0.172.923011.39−10.106.3100
NGC 4258-GC1184.72927047.26486817.83 ± 0.001.63 ± 0.000.79 ± 0.102.693111.16−11.575.2500
NGC 4258-GC2184.86570047.21038917.89 ± 0.003.37 ± 0.011.13 ± 0.102.791651.18−11.5016.7800
NGC 4258-GC3184.74597047.30106717.97 ± 0.002.15 ± 0.010.99 ± 0.100.43 ± 0.054.034401.65−11.420.6902
M51-GC1202.45958447.17471018.90 ± 0.032.05 ± 0.001.07 ± 0.10−0.06 ± 0.173.104621.44−10.763.2302
M51-GC2202.50711747.24184519.18 ± 0.033.50 ± 0.001.52 ± 0.101.17 ± 0.172.772711.35−10.487.9603
M51-GC3202.46942047.25390619.31 ± 0.031.75 ± 0.001.25 ± 0.102.472811.24−10.358.8000
NCG628-GC124.22142915.78891418.28 ± 0.032.51 ± 0.001.08 ± 0.161.82 ± 0.073.334711.56−11.667.8403
NCG628-GC224.17102315.78250019.13 ± 0.031.90 ± 0.000.68 ± 0.160.28 ± 0.092.752431.37−10.810.5202
NCG628-GC324.21297315.73498719.71 ± 0.033.15 ± 0.001.25 ± 0.162.621831.16−10.2310.4800

Note. (1) Assigned name, which follows the convention of GAL-GCn, where GAL stands for galaxy name and n is 1 for the brightest object in the F814W filter, and increases sequentially as the magnitude increases. (2,3) Right ascension, Declination, coordinates in J2000. (4) Magnitude in F814W-band and magnitude error from SExtractor and aperture correction, added in quadrature, (5) (F435WF814W)0 colour, the error is the quadrature sum of the error in each band from SExtractor. (6) (F435WF555W)0 colour, error is quadrature sum as in column 5. In the case of M81 the colour is (F435WF606W)0. (7) (F336WF435W)0 colour, the error is the quadrature sum of the error in each band. In the case of M81 the colour is. (ug)0. (8) FWHM in pixel units from SExtractor. (9) AREA in pixels from SExtractor. (10) Concentration index, defined as the difference between magnitudes measured in 1 and 3 pixel radius apertures. (11) Absolute magnitude in F814W-band. (12) Galactocentric distance of the GC in kiloparsec. (13) FLAG classification: 00 clusters without U-band photometry; 01 determined as a reddened young cluster from U-band photometry; 02 – determined as bonafide GC from U-band photometry; and 03 – error in U-B is likely to be larger than the indicated formal error.

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