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Table B.2.

Cluster-center coordinates, average proper motions, distance modulus, reddening, metallicities, and ages for the studied clusters.

ID RA error Dec. error μα cos δ μδ (m−M)0 E(B−V) [M/H] agea ageb
h m s [arcsec] d m s [arcsec] [mas yr−1] [mas yr−1] [mag] [mag] [dex] [Gyr] [Gyr]
BRHT 5b 05 08 52.65 — −68 45 18.0 — 2.09±0.03 0.04±0.09 18.40 0.12 −0.4 0.015 —
BS 90 00 59 04.86 ±0.4 −72 09 10.3 ±4.7 0.67±0.05 −1.06±0.06 18.91 0.03 −0.7 4.2 —
BSDL 1650 05 25 50.01 — −68 49 16.0 — 1.54±0.19 0.34±0.15 18.38 0.18 −0.4 0.30 —
ESO 121-03 06 02 02.40 ±0.8 −60 31 26.0 ±1.2 1.61±0.04 0.92±0.06 18.34 0.05 −0.8 6.9 —
Hodge 02 05 17 48.88 ±0.1 −69 38 43.4 ±0.3 2.29±0.13 0.43±0.15 18.32 0.12 −0.5 1.70 1.35
Hodge 06 05 42 17.65 ±0.8 −71 35 28.2 ±0.5 1.95±0.06 0.76±0.06 18.40 0.15 −0.5 2.30 —
Hodge 07 05 50 02.99 ±0.4 −67 43 06.6 ±1.0 1.77±0.05 0.75±0.07 18.33 0.06 −0.5 2.00 1.75
Hodge 11 06 14 22.89 ±0.2 −69 50 50.6 ±0.2 1.56±0.08 0.75±0.07 18.57 0.05 −1.7 13.4 —
HW 57 01 07 43.22 ±0.7 −71 52 37.5 ±0.8 0.77±0.14 −1.03±0.06 19.18 0.12 −1.3 5.3 —
IC 1641 01 09 38.82 ±0.6 −71 46 04.4 ±1.3 1.04±0.06 −1.11±0.09 18.93 0.02 −0.6 1.20 0.80
IC 1660 01 12 37.59 ±0.3 −71 45 41.4 ±0.3 1.07±0.05 −1.30±0.04 19.06 0.07 −0.2 0.11 —
IC 2146 05 37 47.37 ±0.6 −74 47 01.3 ±0.6 2.02±0.03 0.73±0.03 18.42 0.05 −0.4 2.20 2.00
KMHK 240 04 54 26.88 ±0.9 −68 14 55.1 ±0.6 2.26±0.12 −0.01±0.11 18.52 0.12 −0.5 2.10 1.90
KMHK 250 04 54 30.32 ±0.2 −69 55 15.1 ±0.4 2.01±0.09 0.01±0.08 18.51 0.11 −0.5 1.80 1.45
KMHK 291 04 55 45.26 ±0.2 −68 16 56.2 ±0.5 1.74±0.12 −0.13±0.11 18.55 0.12 −0.2 0.30 0.15
KMHK 361 04 56 37.46 ±1.4 −68 09 55.8 ±0.7 1.69±0.16 0.06±0.13 18.43 0.06 −0.3 1.35 1.00
KMHK 598 05 09 35.72 — −67 48 31.2 — 1.76±0.12 0.04±0.22 18.50 0.06 −0.2 0.15 —
KMHK 676 05 14 44.37 ±1.8 −65 20 08.5 ±0.9 1.61±0.04 0.15±0.08 18.49 0.07 −0.2 0.14 —
KMHK 987 05 30 32.71 ±0.8 −66 54 12.4 ±0.4 1.55±0.03 0.47±0.04 18.52 0.07 −0.2 0.017 —
KMHK 1073 05 33 10.75 — −71 01 21.0 — 2.10±0.07 0.54±0.06 18.34 0.11 −0.4 0.45 0.30
KMHK 1231 05 41 09.62 ±3.1 −69 54 12.4 ±0.4 1.96±0.09 0.63±0.15 18.47 0.13 −0.3 0.35 0.20
KMK 8827 05 08 54.14 — −69 00 15.2 — 1.81±0.58 −0.30±0.61 18.40 0.11 −0.2 0.20 —
KMK 8849 05 21 10.76 — −69 56 30.3 — 2.51±0.41 0.34±0.13 18.44 0.22 −0.4 0.50 0.25
Kron 1 00 21 25.78 ±1.2 −73 44 55.7 ±0.5 0.35±0.06 −1.35±0.06 18.90 0.03 −0.9 6.8 —
Kron 3 00 24 46.63 ±0.8 −72 47 37.0 ±0.2 0.53±0.02 −1.35±0.03 18.93 0.02 −0.9 5.6 —
Kron 21 00 41 24.39 ±0.3 −72 53 23.8 ±0.2 0.62±0.02 −1.53±0.03 18.84 0.06 −1.0 4.4 —
Kron 29 00 51 53.15 ±0.2 −72 57 12.2 ±0.3 0.65±0.05 −1.21±0.03 19.10 0.07 −0.4 0.25 0.12
Kron 34 00 55 33.44 ±1.5 −72 49 57.6 ±1.5 0.69±0.04 −1.25±0.04 18.90 0.12 −0.6 0.85 0.55
Lindsay 1 00 03 54.44 ±2.0 −73 28 18.7 ±1.3 0.54±0.03 −1.49±0.03 18.86 0.04 −1.2 7.2 —
Lindsay 38 00 48 49.80 ±2.5 −69 52 12.6 ±1.6 0.54±0.03 −0.86±0.03 19.22 0.01 −1.2 5.4 —
Lindsay 91 01 12 51.76 ±0.2 −73 07 07.4 ±0.5 0.76±0.07 −1.09±0.04 18.97 0.10 −0.8 4.2 —
Lindsay 113 01 49 29.69 ±4.0 −73 43 40.2 ±1.3 1.30±0.02 −1.18±0.03 18.76 0.03 −0.8 3.6 —
Lindsay 114 01 50 19.27 ±0.3 −74 21 20.5 ±0.4 1.09±0.03 −1.14±0.04 18.86 0.07 −0.4 0.04 —
NGC 121 00 26 48.94 ±0.1 −71 32 09.4 ±0.1 0.23±0.03 −1.23±0.03 19.05 0.04 −1.2 9.7 —
NGC 152 00 32 56.47 ±1.2 −73 06 59.2 ±2.2 0.41±0.03 −1.26±0.04 19.07 0.03 −0.6 1.90 1.45
NGC 265 00 47 11.82 ±0.6 −73 28 38.2 ±0.2 0.64±0.03 −1.31±0.04 19.03 0.06 −0.5 0.45 0.25
NGC 290 00 51 14.24 — −73 09 42.2 — 0.67±0.09 −1.47±0.07 18.95 0.05 −0.5 0.30 0.20
NGC 294 00 53 05.58 ±1.4 −73 22 48.7 ±3.2 0.53±0.05 −1.27±0.04 18.98 0.12 −0.7 0.70 0.45
NGC 299 00 53 24.51 ±0.2 −72 11 50.6 ±0.2 0.69±0.04 −1.25±0.02 18.99 0.06 −0.4 0.08 0.02
NGC 330 00 56 18.23 ±0.1 −72 27 32.3 ±0.1 0.75±0.03 −1.31±0.03 19.04 0.04 −0.4 0.09 0.04
NGC 339 00 57 46.56 ±0.5 −74 28 13.2 ±0.4 0.70±0.03 −1.25±0.04 18.96 0.07 −1.3 5.9 —
NGC 346 00 59 04.93 ±0.6 −72 10 37.4 ±0.4 0.70±0.04 −1.23±0.03 18.94 0.08 −0.4 0.005 —
NGC 376 01 03 52.75 ±0.7 −72 49 32.0 ±0.3 0.72±0.04 −1.31±0.03 18.98 0.07 −0.4 0.028 0.018
NGC 411 01 07 55.95 ±0.4 −71 46 04.1 ±0.4 0.87±0.08 −1.12±0.06 18.97 0.06 −0.7 1.95 1.55
NGC 416 01 07 59.17 ±0.2 −72 21 19.7 ±0.1 0.88±0.04 −1.24±0.03 18.96 0.11 −1.2 6.0 —
NGC 419 01 08 17.57 ±0.7 −72 53 03.8 ±1.0 0.77±0.06 −1.22±0.04 18.85 0.07 −0.7 2.00 1.55
NGC 422 01 09 24.48 ±6.2 −71 45 59.3 ±0.9 0.93±0.04 −1.27±0.03 18.88 0.04 −0.4 0.30 0.20
NGC 602 01 29 31.50 ±0.8 −73 33 40.8 ±0.4 0.96±0.02 −1.26±0.05 19.01 0.06 −0.2 0.005 0.002
NGC 1466 03 44 32.76 ±1.3 −71 40 15.5 ±0.3 1.72±0.06 −0.74±0.07 18.58 0.05 −1.5 13.2 —
NGC 1644 04 37 39.85 ±0.3 −66 11 56.3 ±0.5 1.80±0.02 −0.29±0.11 18.45 0.03 −0.6 1.80 1.45
NGC 1651 04 37 32.23 ±0.6 −70 35 10.8 ±0.3 2.02±0.04 −0.30±0.05 18.48 0.13 −0.6 2.20 2.05
NGC 1652 04 38 22.77 ±0.3 −68 40 19.8 ±0.2 1.87±0.06 −0.37±0.07 18.46 0.08 −0.6 2.25 —
NGC 1718 04 52 25.89 ±0.2 −67 03 06.6 ±0.4 1.85±0.03 −0.41±0.04 18.43 0.22 −0.5 2.05 1.85
NGC 1749 04 54 56.73 — −68 11 19.1 — 1.94±0.08 −0.10±0.12 18.30 0.10 −0.4 0.13 0.07
NGC 1751 04 54 11.99 ±1.1 −69 48 27.1 ±0.6 1.93±0.07 −0.09±0.10 18.52 0.15 −0.5 1.75 1.45
NGC 1755 04 55 15.56 ±0.2 −68 12 18.8 ±0.6 1.88±0.04 −0.11±0.05 18.33 0.11 −0.2 0.11 0.07
NGC 1756 04 54 49.69 ±0.7 −69 14 13.2 ±0.3 1.83±0.04 0.10±0.03 18.55 0.22 −0.4 0.20 0.15
NGC 1783 04 59 08.97 ±0.5 −65 59 13.8 ±0.2 1.64±0.04 −0.06±0.04 18.51 0.03 −0.4 1.95 1.65
NGC 1786 04 59 07.99 ±0.1 −67 44 43.9 ±0.3 1.95±0.03 0.06±0.03 18.42 0.09 −1.5 12.9 —
NGC 1793 04 59 38.74 ±0.1 −69 33 27.8 ±0.1 2.09±0.08 −0.05±0.05 18.48 0.14 −0.2 0.15 0.06
NGC 1795 04 59 47.35 ±1.1 −69 48 06.5 ±0.3 1.90±0.05 0.23±0.11 18.45 0.09 −0.4 1.85 1.50
NGC 1801 05 00 35.41 ±0.2 −69 36 49.9 ±0.7 1.90±0.05 0.05±0.04 18.39 0.12 −0.3 0.45 0.30
NGC 1805 05 02 21.78 ±0.1 −66 06 41.9 ±0.1 1.56±0.04 0.10±0.06 18.32 0.05 −0.4 0.10 0.045
NGC 1806 05 02 11.72 ±0.4 −67 59 08.0 ±0.5 1.85±0.05 −0.06±0.07 18.52 0.04 −0.4 1.90 1.60
NGC 1810 05 03 23.06 ±0.7 −66 22 56.7 ±1.4 1.72±0.05 0.07±0.04 18.45 0.04 −0.2 0.08 0.045
NGC 1818 05 04 13.43 ±0.4 −66 26 01.7 ±1.2 1.64±0.04 0.09±0.06 18.44 0.07 −0.2 0.07 0.035
NGC 1831 05 06 16.38 ±0.4 −64 55 06.1 ±0.8 1.69±0.11 −0.04±0.10 18.41 0.05 −0.3 0.90 0.70
NGC 1841 04 45 22.75 ±0.4 −83 59 55.6 ±0.6 2.05±0.02 0.00±0.03 18.34 0.13 −1.3 12.4 —
NGC 1844 05 07 30.38 ±0.9 −67 19 28.6 ±1.9 1.68±0.02 −0.03±0.03 18.47 0.07 −0.2 0.17 0.09
NGC 1846 05 07 34.15 ±0.4 −67 27 36.7 ±0.2 1.71±0.04 0.03±0.04 18.52 0.05 −0.4 1.95 1.60
NGC 1850 05 08 45.19 ±1.3 −68 45 42.0 ±1.5 2.02±0.04 0.11±0.04 18.38 0.13 −0.4 0.12 0.07
NGC 1850Ac 05 08 39.44 — −68 45 44.2 — 1.95±0.04 0.13±0.01 18.36 0.11 −0.4 0.020 0.10
NGC 1852 05 09 23.95 ±0.3 −67 46 45.6 ±0.2 1.78±0.04 0.16±0.06 18.52 0.07 −0.4 1.75 1.40
NGC 1854 05 09 19.83 ±0.5 −68 50 52.0 ±0.8 2.09±0.04 0.15±0.02 18.42 0.09 −0.2 0.15 0.09
NGC 1856 05 09 30.08 ±0.1 −69 07 43.9 ±0.3 1.88±0.05 0.20±0.05 18.32 0.17 −0.4 0.45 0.25
NGC 1858 05 10 00.07 — −68 54 15.1 — 1.87±0.04 0.25±0.03 18.46 0.12 −0.2 0.017 0.004
NGC 1866 05 13 38.65 ±0.3 −65 27 52.8 ±0.4 1.55±0.03 0.16±0.03 18.30 0.06 −0.4 0.40 0.20
NGC 1868 05 14 35.91 ±0.4 −63 57 15.1 ±0.1 1.83±0.04 0.05±0.07 18.45 0.06 −0.4 1.45 1.15
NGC 1872 05 13 11.29 ±0.8 −69 18 44.9 ±0.3 1.79±0.08 0.52±0.05 18.31 0.18 −0.4 0.60 0.40
NGC 1898 05 16 41.57 ±0.3 −69 39 24.1 ±0.1 1.98±0.05 0.35±0.05 18.60 0.06 −1.5 11.7 —
NGC 1903 05 17 22.62 ±0.3 −69 20 17.0 ±0.5 2.01±0.07 0.16±0.05 18.40 0.06 −0.2 0.15 0.10
NGC 1917 05 19 01.94 ±0.4 −69 00 05.5 ±0.5 1.65±0.11 0.57±0.09 18.36 0.05 −0.3 1.70 1.40
NGC 1928 05 20 57.49 ±1.4 −69 28 41.6 ±2.1 1.84±0.10 0.13±0.12 18.43 0.06 −1.5 13.0 —
NGC 1938 05 21 25.00 — −69 56 21.5 — 2.04±0.09 0.34±0.07 18.48 0.23 −0.3 0.15 —
NGC 1939 05 21 26.37 ±0.3 −69 56 58.4 ±1.3 2.21±0.07 0.44±0.03 18.42 0.06 −1.5 13.3 —
NGC 1943 05 22 29.36 ±0.4 −70 09 18.5 ±0.8 2.04±0.04 0.08±0.07 18.46 0.14 −0.3 0.20 0.15
NGC 1953 05 25 27.95 ±0.2 −68 50 16.1 ±0.1 1.75±0.06 0.41±0.07 18.41 0.11 −0.4 0.50 0.35
NGC 1966 05 26 45.53 — −68 49 50.9 — 1.59±0.04 0.52±0.21 18.40 0.06 −0.2 0.005 0.003
NGC 1978 05 28 44.71 ±1.2 −66 14 10.9 ±1.1 1.76±0.03 0.40±0.04 18.53 0.07 −0.5 2.50 —
NGC 1983 05 27 44.95 ±0.8 −68 59 06.5 ±0.3 1.60±0.05 0.49±0.05 18.56 0.03 0.0 0.014 —
NGC 1987 05 27 17.03 ±0.1 −70 44 11.4 ±0.2 1.94±0.06 0.46±0.04 18.43 0.07 −0.7 1.35 1.00
NGC 2002 05 30 20.82 ±0.4 −66 53 01.1 ±0.3 1.57±0.04 0.47±0.07 18.52 0.07 −0.2 0.02 —
NGC 2005 05 30 10.13 ±0.1 −69 45 10.6 ±0.2 1.88±0.04 0.56±0.04 18.44 0.09 −1.6 13.1 —
NGC 2010 05 30 33.93 ±0.8 −70 49 07.8 ±1.3 2.23±0.04 0.45±0.04 18.54 0.09 −0.2 0.12 —
NGC 2031 05 33 40.27 ±2.9 −70 59 12.6 ±1.5 2.30±0.07 0.61±0.07 18.40 0.09 −0.4 0.30 0.15
NGC 2056 05 36 33.95 ±0.2 −70 40 15.7 ±0.2 2.16±0.07 0.62±0.08 18.38 0.08 −0.4 0.45 0.30
NGC 2107 05 43 12.39 ±0.1 −70 38 24.4 ±0.2 1.96±0.10 0.83±0.11 18.37 0.16 −0.3 0.50 0.30
NGC 2108 05 43 56.54 ±0.1 −69 10 52.9 ±0.3 1.72±0.06 0.84±0.08 18.48 0.14 −0.3 1.25 1.00
NGC 2121 05 48 13.22 ±1.4 −71 28 46.9 ±0.8 1.76±0.05 0.96±0.04 18.48 0.09 −0.5 2.9 —
NGC 2154 05 57 38.22 ±0.3 −67 15 41.7 ±0.9 1.42±0.04 0.78±0.05 18.37 0.04 −0.5 2.00 1.80
NGC 2155 05 58 32.24 ±0.3 −65 28 39.7 ±0.6 1.73±0.07 0.88±0.05 18.39 0.05 −0.4 2.8 —
NGC 2156 05 57 49.88 ±1.0 −68 27 42.5 ±1.4 1.73±0.09 0.91±0.08 18.44 0.06 −0.2 0.17 0.10
NGC 2164 05 58 55.83 ±0.4 −68 30 57.6 ±0.3 1.60±0.04 0.78±0.04 18.43 0.07 −0.3 0.20 0.10
NGC 2173 05 57 58.40 ±0.2 −72 58 43.2 ±0.2 1.97±0.04 0.83±0.05 18.37 0.06 −0.4 2.05 1.70
NGC 2203 06 04 42.62 ±0.7 −75 26 16.1 ±0.5 1.93±0.03 0.88±0.03 18.38 0.07 −0.3 1.95 1.65
NGC 2209 06 08 36.19 ±0.9 −73 50 09.9 ±0.7 1.94±0.04 0.96±0.05 18.39 0.10 −0.4 1.45 1.15
NGC 2210 06 11 31.63 ±0.2 −69 07 18.7 ±0.2 1.44±0.05 1.36±0.05 18.36 0.04 −1.4 12.0 —
NGC 2213 06 10 42.13 ±0.2 −71 31 45.9 ±0.8 1.77±0.02 0.99±0.04 18.36 0.09 −0.4 1.85 1.60
NGC 2249 06 25 49.65 ±0.3 −68 55 14.2 ±0.2 1.55±0.06 1.09±0.05 18.34 0.06 −0.4 1.20 0.95
NGC 2257 06 30 12.42 ±0.3 −64 19 36.6 ±0.5 1.39±0.05 1.00±0.04 18.37 0.04 −1.4 11.8 —
OGLEclLMC390 05 21 18.91 — −69 28 33.8 — 1.99±0.21 0.60±0.29 18.44 0.10 −0.5 1.55 1.30
Reticulum 04 36 10.99 ±0.3 −58 51 45.5 ±0.5 1.95±0.05 −0.27±0.02 18.40 0.00 −1.2 11.5 —
SL 075 06 13 27.26 ±0.9 −70 41 45.0 ±0.4 1.68±0.04 1.07±0.04 18.49 0.06 −0.4 1.95 1.70

Notes.

(a)

The ages of clusters with the eMSTO are inferred by fitting the isochrone to the lower part of the eMSTO. See Sect. 2.5 for details.

(b)

The ages of clusters with the eMSTO are inferred by fitting the isochrone to the upper part of the eMSTO. See Sect. 2.5 for details.

(c)

NGC 1850A is a clump of stars located on the west side of NGC 1850 and is often considered a separate cluster (e.g., Caloi & Cassatella 1998). Based on the results of this table, NGC 1850 and NGC 1850A share similar proper motions, distance, metallicity, and age.

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