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Table B.1.

Known and well-characterized GCs we used to derive the total luminosity for each Sgr GC.

Cluster ID [Fe/H]a E(B − V) (m − M)0 References
[dex] [mag] [mag]
Liller 1 −0.33 3.09 14.48 Valenti et al. (2010) (V10)
NGC 6440 −0.36 1.15 14.58 Valenti et al. (2004) (V04)
NGC 6441 −0.46 0.52 15.65 V04
NGC 6624 −0.44 0.31 17.33 Siegel et al. (2011) (S11)
Terzan 6 −0.56 2.35 14.13 Valenti et al. (2007) (V07)
Terzan 12 −0.50 2.06 12.65 Ortolani et al. (1998)
NGC 6637 −0.64 0.22 17.35 S11
Terzan 2 −0.69 1.40 14.30 Christian & Friel (1992)
BH 261 −0.76 0.36 13.90 Ortolani et al. (2006)
NGC 6569 −0.76 0.49 15.40 V07
UKS 1 −0.98 2.2 16.01 Minniti et al. (2011)
NGC 6638 −0.95 0.43 15.07 V07
Terzan 9 −1.05 1.79 13.73 V10
NGC 6642 −1.26 0.42 14.30 Barbuy et al. (2006)
NGC 6626 −1.32 0.42 13.70 Kerber et al. (2018)
NGC 6540 −1.35 0.66 13.57 V10
NGC 6558 −1.32 0.50 14.59 Barbuy et al. (2018)
NGC 6453 −1.50 0.69 15.15 V10
NGC 6715 −1.49 0.14 17.27 S11
Terzan 8 −2.16 0.14 17.26 S11

Notes.

a

The [Fe/H] values are taken from the 2010 version of the Harris (1996) catalog.

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