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Table 9.

Candidate ACs in GGCs. “Flag NIR” indicates the source of the NIR photometry, and “ID” lists the Gaia DR3 identification according to Gavras et al. (2023).

Name ID Gaia DR3 RA Dec P J σJ Ks σKs E(B − V) μ σμ Flag NIR
deg deg days mag mag mag mag mag mag mag
ω Cen V68 6083718920208854528 201.55333 −47.32658 0.54 13.20 0.01 12.94 0.01 0.12 13.67 0.02 BR16
Terzan1 V4 4055452878472660480 263.98826 −30.49802 2.46 14.27 0.01 12.91 0.02 1.99 13.77 0.07 VVVDR2
NGC6752 V1 6638377937476917376 287.85367 −59.94009 1.38 11.67 0.05 11.04 0.03 0.04 13.08 0.01 2MASS
NGC6388 V18 5955269337621694592 264.06388 −44.73400 1.87 12.02 0.15 11.24 0.15 0.37 15.24 0.03 VSH
NGC5466 V19 1452625254531322752 211.41857 +28.48674 0.82 14.16 0.08 13.97 0.07 0.00 16.04 0.02 2MASS
NGC2808 V29 5248759277665209472 138.00335 −64.86095 1.97 12.19 0.15 11.56 0.15 0.22 15.01 0.02 VHS
M92 V7 1360405396085147008 259.28171 +43.12267 1.06 13.00 0.03 12.63 0.03 0.02 14.65 0.02 DP05
M22 V11 4077588452718318080 279.09468 −23.90256 1.69 10.52 0.09 10.08 0.10 0.34 12.59 0.02 2MASS

Notes. RA and Dec refer at Epoch of the first observation J2016.0. The E(B − V) values are from Harris (2010), while the μ values are from Baumgardt & Vasiliev (2021). FLag NIR indicates the origin of the NIR photometry: “VVVDR2” refers to Minniti et al. (2017), “VSH_DR5” refers to McMahon et al. (2021), “BR16” refers to Braga et al. (2016), “2MASS” refers to Skrutskie et al. (2006), and “DP05” refers to Del Principe et al. (2005).

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