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Table 1

Fundamental parameters of the studied LMC cluster candidates.

ID RA Dec r E(BV) log(t/yr) [Fe/H] Notes
(°) (°) () (mag) (dex)

LMC 5_5

BSDL 1504 80.775 –71.422 0.4 0.065 9.55 –0.7
BSDL 1355 80.342 –70.900 0.4 0.064 9.50 –0.7
BSDL 1341 80.249 –70.318 0.5 0.085 9.45 –0.7
SL 435 80.875 –71.428 0.4 0.065 9.40 –0.7 8.70 ± 0.20, –0.4 (1)
KMHK 897 81.492 –70.459 0.7 0.085 9.40 –0.7
KMHK 835 80.533 –71.175 0.5 0.064 9.40 –0.7
HS 329 82.442 –71.001 0.4 0.070 9.30 –0.7 9.25 ± 0.04 (4)
KMHK 750 79.577 –70.721 0.4 0.086 9.30 –0.4
SL 472 81.562 –70.380 0.4 0.085 9.20 –0.7
BSDL 1672 81.375 –71.087 0.25 0.070 9.20 –0.4
HS 323 82.215 –70.207 0.6 0.071 9.20 –0.4
HS 264 80.805 –70.778 0.4 0.082 9.10 –0.4 9.20 ± 0.04 (4)
KMHK 997 82.576 –70.420 0.5 0.076 9.10 –0.4
NGC 1987 81.821 –70.738 0.8 0.080 9.00 –0.4 9.05 ± 0.05, 0.010 (3)
SL 389 79.905 –71.211 0.7 0.064 8.90 –0.4
HS 214 79.460 –70.801 0.3 0.086 8.90 –0.4 8.15 ± 0.04, –0.4 (1)
KMHK 907 81.553 –70.981 0.3 0.070 8.80 –0.4
HS 238 80.033 –70.156 0.3 0.100 8.80 –0.4
SL 441 80.925 –71.037 0.5 0.064 8.80 0.0
BSDL 2123 82.775 –70.168 0.5 0.071 8.80 –0.4
SL 399 80.087 –70.768 0.5 0.064 8.50 –0.4 8.30 ± 0.05, –0.4 (1)
KMK 88_55 80.923 –70.096 0.3 0.084 8.50 –0.4
HS 304 81.814 –71.172 0.4 0.074 8.50 –0.4
SL 406 80.258 –70.873 0.3 0.064 8.45 –0.4 8.50 ± 0.05, –0.4 (1)
SL 395 79.996 –70.665 0.3 0.083 8.40 –0.4 8.30 ± 0.20, –0.4 (1)
HS 324 82.229 –71.120 0.3 0.070 8.40 –0.4
SL 364 79.423 –71.066 0.3 0.094 8.30 –0.4 8.00 ± 0.20, –0.4 (1)
NGC 1943 80.623 –70.155 0.5 0.085 8.30 –0.4 8.35 ± 0.05, –0.4 (1)
SL 487e 81.788 –71.023 0.4 0.070 8.30 –0.4
KMHK 764 79.720 –70.602 0.4 0.091 8.30 –0.4
SL 431 80.800 –70.2805 0.4 0.050 8.30 –0.4
NGC 2010 82.641 –70.819 0.5 0.078 8.20 –0.4 8.20 ± 0.05, –0.4 (2)
SL 510 82.340 –70.579 0.5 0.076 8.10 –0.4 8.10 ± 0.10, –0.4 (5)
KMHK 999 82.553 –71.557 0.3 0.076 8.00 –0.4
BSDL 1949 82.345 –70.237 0.4 0.071 7.70 –0.4
BSDL 1876 81.977 –71.522 0.2 0.076 7.50 –0.4 8.20 ± 0.40, –0.4 (1)
BSDL 2008 82.460 –71.068 0.3 0.070 7.50 –0.4
SL 539 82.733 –70.695 0.4 0.078 7.50 –0.4 7.40 ± 0.20, –0.4 (1)
BSDL 2199 82.942 –70.253 0.4 0.071 7.50 –0.4
KMHK 979 82.412 –70.986 0.4 0.070 7.30 –0.4 7.30 ± 0.40, –0.4 (1)
BSDL 1955 82.332 –71.031 0.3 0.070 7.30 –0.4 7.30 ± 0.40, –0.4 (1)
BSDL 1980 82.387 –70.994 0.5 0.070 7.30 –0.4 7.30 ± 0.40, –0.4 (1)
BSDL 1830 81.892 –70.614 0.2 0.076 7.30 –0.4 7.50 ± 0.60, –0.4 (1)
BSDL 1875 81.976 –71.547 0.3 0.076 7.30 –0.4 8.60 ± 0.60, –0.4 (1)
SL 528 82.670 –70.223 0.2 0.071 >9.00 ... cluster-like asterism?
OGLE 545 82.663 –70.217 0.2 0.071 >9.00 ... cluster-like asterism?
BSDL 1182 79.568 –71.435 0.15 0.065 ... ... unresolved cluster?
HS 232 80.155 –70.964 0.2 0.064 ... ... possible non-cluster; 9.20 ± 0.10, –0.4 (1)
HS 265 80.817 –70.234 0.25 0.085 ... ... possible non-cluster
BSDL 1790 81.720 –70.211 0.4 0.085 ... ... possible non-cluster
OGLE 534 82.515 –70.126 0.2 0.063 ... ... possible non-cluster
OGLE 536 82.517 –70.205 0.2 0.071 ... ... possible non-cluster
KMHK 801 80.114 –70.450 0.3 0.085 ... ... possible non-cluster
HS 295 81.524 –70.092 0.3 0.085 ... ... possible non-cluster
HS 282 81.318 –70.099 0.3 0.085 ... ... possible non-cluster
BSDL 2196 82.932 –70.201 0.2 0.071 ... ... possible non-cluster
BSDL 2063 82.618 –70.560 0.5 0.076 ... ... possible non-cluster
OGLE 471 81.573 –70.222 0.3 0.085 ... ... possible non-cluster
HS 345 82.956 –70.287 0.25 0.071 ... ... possible non-cluster
KMHK 819 80.333 –71.407 0.3 0.065 ... ... possible non-cluster
HS 342 82.940 –70.308 0.3 0.071 ... ... possible non-cluster
SL 542 82.825 –70.216 0.4 0.071 ... ... possible non-cluster

Reference. (1) Glatt et al. (2010); (2) Gouliermis et al. (2010); (3) Milone et al. (2009); (4) Piatti (2011); (5) Piatti (2012).

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