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Table 5.

Main parameters of the SCs investigated in this work.

ID(*) RA Dec R log t Nstars G n0 rc rc Tile Flag Simbad name
[J2000] [J2000] [′] [arcmin−2] [′] [pc]
YMCA-0049 11.8554 −68.9199 1.10 9.60 422 47.7 676 ± 7 0.32 ± 0.13 5.6 ± 2.2 6_5 A L 32; OGLE-CL SMC 310
YMCA-0050 14.7444 −68.9153 0.85 9.70 210 31.6 382 ± 5 0.28 ± 0.03 4.8 ± 0.5 6_6 A ESO 51-9; OGLE-CL SMC 309
YMCA-0051 25.4233 −71.1624 0.70 9.20 165 22.9 249 ± 8 0.34 ± 0.19 5.0 ± 2.7 4_9 A HW 84; OGLE-CL SMC 305
YMCA-0052 28.2998 −70.7526 0.95 9.85 79 14.0 187 ± 9 0.14 ± 0.02 2.0 ± 0.4 4_10 A OGLE-CL MBR 6
YMCA-0053 66.7160 −67.2567 0.50 9.75 54 6.6 83 ± 9 0.24 ± 0.12 3.5 ± 1.7 7_26 B
YMCA-0054 67.3571 −67.4461 0.40 9.40 62 6.9 337 ± 10 0.14 ± 0.05 2.0 ± 0.7 7_26 A OGLE-CL LMC 0841
YMCA-0055 67.6149 −67.7673 0.25 9.45 27 5.2 136 ± 17 0.16 ± 0.12 2.4 ± 1.7 7_26 C
YMCA-0056 67.6596 −66.9542 0.35 9.25 77 15.7 486 ± 10 0.16 ± 0.05 2.3 ± 0.7 7_26 A HS 8; KMHK 5
YMCA-0057 67.8233 −67.7799 0.20 9.40 22 5.5 228 ± 16 0.12 ± 0.10 1.8 ± 1.4 7_26 C OGLE-CL LMC 0834
YMCA-0058 68.8670 −67.7115 0.50 9.30 112 9.2 284 ± 10 0.17 ± 0.02 2.5 ± 0.3 7_27 A HS 13; KMHK 11
YMCA-0059 69.4153 −66.1983 1.30 9.25 836 33.8 692 ± 25 0.38 ± 0.06 5.5 ± 0.9 8_28 A ESO 84-30; LW 11; NGC 1644; SL 9
YMCA-0060 69.7900 −67.4985 0.25 9.40 38 5.9 164 ± 14 0.19 ± 0.06 2.8 ± 0.9 7_27 C
YMCA-0061 69.9930 −67.3831 0.35 9.80 62 6.0 176 ± 21 0.21 ± 0.13 3.1 ± 1.9 7_27 C
YMCA-0062 93.9911 −64.9733 0.60 9.25 178 17.0 615 ± 19 0.19 ± 0.06 2.7 ± 0.8 9_40 A KMHK 1710; LW 444
YMCA-0063 94.4250 −65.5469 0.40 9.45 86 11.2 456 ± 9 0.15 ± 0.02 2.1 ± 0.3 9_40 A OGLE-CL LMC 0758
YMCA-0064 94.4670 −65.3440 0.30 9.45 33 5.0 85 ± 8 0.21 ± 0.16 3.1 ± 2.4 9_40 C
YMCA-0065 96.1209 −66.5061 0.45 9.20 109 13.7 448 ± 18 0.18 ± 0.05 2.7 ± 0.7 8_39 A OHSC 34; KMHK 1751
YMCA-0066 96.2493 −66.5821 0.40 9.40 58 6.6 235 ± 14 0.12 ± 0.02 1.8 ± 0.4 8_39 B
YMCA-0067 97.0305 −67.2605 0.35 9.35 35 6.2 139 ± 6 0.18 ± 0.07 2.7 ± 1.1 7_38 B
YMCA-0068 97.4257 −70.5889 0.80 9.25 226 13.4 309 ± 12 0.25 ± 0.04 3.6 ± 0.6 4_33 A OHSC 36; KMHK 1757
YMCA-0069 97.4821 −70.4781 0.35 9.45 39 6.1 124 ± 6 0.19 ± 0.15 2.8 ± 2.1 4_33 C
YMCA-0070 97.5571 −64.3277 2.50 10.10 3291 227.8 1013 ± 10 0.74 ± 0.05 10.8 ± 0.8 10_43 A ESO 87-24; KMHK 1756; LW 481;
NGC 2257 ; SL 895
YMCA-0071 98.0190 −70.5724 0.40 9.35 42 5.0 176 ± 12 0.11 ± 0.02 1.7 ± 0.4 4_33 B
YMCA-0072 98.2564 −71.1269 1.00 9.00 417 32.8 377 ± 7 0.43 ± 0.11 6.3 ± 1.5 4_33 A KMHK 1760; LW 483; SL 897
YMCA-0073 106.9160 −69.9839 0.50 9.75 51 23.9 355 ± 8 0.16 ± 0.06 2.3 ± 0.9 5_38 A KMHK 1762; OHSC 37

Notes. The meaning of the different columns is ID, RA, Dec: YMCA identifier and the coordinates of the SCs; R: estimated radius; log t: logarithm of the age; Nstars: number of stars within the SC radius; G: value of the parameter defined in Eq. (2); n0 central number surface density as derived from the fit of the radial density function (Eq. (3)); rc estimated core radius expressed in arcmin and parsec (Eq. (4)); Tile: tile in which each SC resides; Flag: robustness ranking of SC: A and B represent the highest and the intermediate confidence level; C reports SCs which necessitate deeper follow-up images to be confirmed. The last column reports additional IDs of already catalogued SCs as reported in SIMBAD Astronomical Database. (*): ID numbers begin from 49 since SCs from YMCA-0001 up to YMCA-0048 were presented in Gatto et al. (2020). To properly match the position of the stars in the CMD of NGC 2257 (YMCA-0070), we adopted Z = 0.0006 and a distance modulus of DM = 18.37 mag, as reported in Milone et al. (2023).

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