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Table 1.

Spectroscopically confirmed GCs.

ID RA Dec vMUSE vFLAMES vEmsellem+2019 vvan Dokkum+2018 VF606W IF814W
(J2000) (J2000) (km s−1) (km s−1) (km s−1) (km s−1) AB (mag) AB (mag)
(1) (2) (3) (4) (5) (6) (7) (8) (9)
GC39 40.43778 −8.42357 1800 . 6 1.8 + 1.3 $ 1800.6_{-1.8}^{+1.3} $ 1818 . 0 7.0 + 7.0 $ 1818.0_{-7.0}^{+7.0} $ 22.37 ± 0.02 21.95 ± 0.02
GC59 40.45037 −8.41578 1783 . 4 2.8 + 3.2 $ 1783.4_{-2.8}^{+3.2} $ 1799 . 0 15.0 + 16.0 $ 1799.0_{-15.0}^{+16.0} $ 22.87 ± 0.03 22.31 ± 0.03
GC71 40.43809 −8.40620 1794 . 4 3.7 + 4.1 $ 1794.4_{-3.7}^{+4.1} $ 1805 . 0 8.0 + 6.0 $ 1805.0_{-8.0}^{+6.0} $ 22.65 ± 0.02 22.19 ± 0.03
GC73 40.45093 −8.40486 1802 . 9 3.7 + 2.4 $ 1802.9_{-3.7}^{+2.4} $ 1797 . 5 1.3 + 1.6 $ 1797.5_{-1.3}^{+1.6} $ 1803 . 8 3.0 + 2.8 $ 1803.8_{-3.0}^{+2.8} $ 1814 . 0 3.0 + 3.0 $ 1814.0_{-3.0}^{+3.0} $ 21.53 ± 0.02 21.06 ± 0.02
GC77 40.44396 −8.40371 1791 . 0 4.1 + 4.2 $ 1791.0_{-4.1}^{+4.2} $ 1800 . 0 1.4 + 1.0 $ 1800.0_{-1.4}^{+1.0} $ 1792 . 6 4.7 + 4.4 $ 1792.6_{-4.7}^{+4.4} $ 1804 . 0 6.0 + 6.0 $ 1804.0_{-6.0}^{+6.0} $ 22.10 ± 0.02 21.70 ± 0.02
GC85 40.44896 −8.40147 1788 . 5 3.8 + 6.4 $ 1788.5_{-3.8}^{+6.4} $ 1792 . 1 0.9 + 0.8 $ 1792.1_{-0.9}^{+0.8} $ 1786 . 3 4.8 + 4.3 $ 1786.3_{-4.8}^{+4.3} $ 1801 . 0 6.0 + 5.0 $ 1801.0_{-6.0}^{+5.0} $ 22.37 ± 0.02 21.84 ± 0.02
GC91 40.42571 −8.39813 1796 . 7 3.3 + 4.9 $ 1796.7_{-3.3}^{+4.9} $ 1802 . 0 10.0 + 10.0 $ 1802.0_{-10.0}^{+10.0} $ 22.51 ± 0.02 22.09 ± 0.03
GC92 40.44536 −8.39741 1775 . 8 5.9 + 5.6 $ 1775.8_{-5.9}^{+5.6} $ 1780 . 2 1.0 + 1.3 $ 1780.2_{-1.0}^{+1.3} $ 1775 . 5 4.2 + 6.2 $ 1775.5_{-4.2}^{+6.2} $ 1789 . 0 7.0 + 6.0 $ 1789.0_{-7.0}^{+6.0} $ 22.13 ± 0.02 21.63 ± 0.02
GC93 40.44467 −8.39743 1812 . 4 10.1 + 6.6 $ 1812.4_{-10.1}^{+6.6} $ 1819 . 1 6.8 + 7.7 $ 1819.1_{-6.8}^{+7.7} $ 22.82 ± 0.03 22.35 ± 0.03
GC98 40.44726 −8.39293 1773 . 3 8.4 + 8.8 $ 1773.3_{-8.4}^{+8.8} $ 1777 . 4 5.2 + 4.3 $ 1777.4_{-5.2}^{+4.3} $ 1786 . 3 11.6 + 7.4 $ 1786.3_{-11.6}^{+7.4} $ 1784 . 0 10.0 + 10.0 $ 1784.0_{-10.0}^{+10.0} $ 22.76 ± 0.02 22.29 ± 0.03
GC101 40.43832 −8.39104 1836 . 0 2.6 + 3.3 $ 1836.0_{-2.6}^{+3.3} $ 1800 . 0 14.0 + 13.0 $ 1800.0_{-14.0}^{+13.0} $ 22.86 ± 0.03 22.38 ± 0.03
GCNEW2 40.44836 −8.40506 1793 . 0 9.4 + 9.8 $ 1793.0_{-9.4}^{+9.8} $ 23.76 ± 0.04 23.25 ± 0.04
GCNEW3 40.44264 −8.40203 1798 . 3 7.7 + 6.0 $ 1798.3_{-7.7}^{+6.0} $ 1788 . 7 10.9 + 16.9 $ 1788.7_{-10.9}^{+16.9} $ 22.58 ± 0.02 22.16 ± 0.03
GCNEW4 40.45166 −8.40222 1811 . 6 15.4 + 14.8 $ 1811.6_{-15.4}^{+14.8} $ 24.08 ± 0.04 23.51 ± 0.05
GCNEW5 40.44270 −8.40079 1804 . 9 7.2 + 9.4 $ 1804.9_{-7.2}^{+9.4} $ 23.90 ± 0.04 23.43 ± 0.05
GCNEW9 40.44205 −8.40753 1794 . 3 10.7 + 14.4 $ 1794.3_{-10.7}^{+14.4} $ 23.70 ± 0.04 23.32 ± 0.04

Notes. (1): Cluster identifier as in van Dokkum et al. (2018a) and Trujillo et al. (2019). (2), (3) right ascension and declination from HST data. (4) LOS velocity based on the here presented MUSE analysis, (5) velocities from the FLAMES spectra presented in Paper I, (6) velocities from MUSE as reported in Emsellem et al. (2019), (7) velocities from Keck DEIMOS and LRIS spectra as reported in van Dokkum et al. (2018a,b), (8), (9) apparent magnitudes from HST as detailed in Beasley et al. (2025).

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