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 | – |
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– |
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22.37 ± 0.02 | 21.95 ± 0.02 |
GC59 | 40.45037 | −8.41578 | – |
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– |
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22.87 ± 0.03 | 22.31 ± 0.03 |
GC71 | 40.43809 | −8.40620 | – |
![]() |
– |
![]() |
22.65 ± 0.02 | 22.19 ± 0.03 |
GC73 | 40.45093 | −8.40486 |
![]() |
![]() |
![]() |
![]() |
21.53 ± 0.02 | 21.06 ± 0.02 |
GC77 | 40.44396 | −8.40371 |
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![]() |
![]() |
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22.10 ± 0.02 | 21.70 ± 0.02 |
GC85 | 40.44896 | −8.40147 |
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![]() |
![]() |
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22.37 ± 0.02 | 21.84 ± 0.02 |
GC91 | 40.42571 | −8.39813 | – |
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– |
![]() |
22.51 ± 0.02 | 22.09 ± 0.03 |
GC92 | 40.44536 | −8.39741 |
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![]() |
![]() |
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22.13 ± 0.02 | 21.63 ± 0.02 |
GC93 | 40.44467 | −8.39743 |
![]() |
– |
![]() |
– | 22.82 ± 0.03 | 22.35 ± 0.03 |
GC98 | 40.44726 | −8.39293 |
![]() |
![]() |
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22.76 ± 0.02 | 22.29 ± 0.03 |
GC101 | 40.43832 | −8.39104 | – |
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– |
![]() |
22.86 ± 0.03 | 22.38 ± 0.03 |
GCNEW2 | 40.44836 | −8.40506 |
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– | – | – | 23.76 ± 0.04 | 23.25 ± 0.04 |
GCNEW3 | 40.44264 | −8.40203 |
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– |
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– | 22.58 ± 0.02 | 22.16 ± 0.03 |
GCNEW4 | 40.45166 | −8.40222 |
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– | – | – | 24.08 ± 0.04 | 23.51 ± 0.05 |
GCNEW5 | 40.44270 | −8.40079 |
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– | – | – | 23.90 ± 0.04 | 23.43 ± 0.05 |
GCNEW9 | 40.44205 | −8.40753 |
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– | – | – | 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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