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⟩ | σ⟨J⟩ | ⟨Ks⟩ | σ⟨Ks⟩ | 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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