Table A.1
Properties of the 30 identified binary systems with well-constrained orbits.
ID | RA | Decl | F606W | m1 | min. m2 | P | K | e | Comment |
---|---|---|---|---|---|---|---|---|---|
[deg] | [deg] | [mag] | [M⊙] | [M⊙] | [d] | [km/s] | |||
1358 | 5.9975 | −72.1090 | 16.92 | 0.78 | 0.47 | 66.25 ±0.03 | ![]() |
0.13 ±0.05 | |
22875 | 6.0072 | −72.1080 | 18.16 | 0.73 | 0.39 | 5.17 ±0.01 | ![]() |
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|
26528 | 5.9889 | −72.0966 | 17.94 | 0.75 | 0.16 | ![]() |
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|
29053 | 5.9744 | −72.1069 | 18.46 | 0.72 | 0.11 | 17.44 ±0.01 | ![]() |
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|
29629 | 5.9718 | −72.0959 | 17.10 | 0.78 | 0.17 | 7.25 ±0.01 | ![]() |
![]() |
|
30718 | 5.9659 | −72.0993 | 18.20 | 0.73 | 0.32 | 41.40 ±0.02 | ![]() |
0.37 ±0.08 | |
51235 | 6.0438 | −72.0850 | 15.70 | 0.80 | 0.36 | ![]() |
![]() |
![]() |
|
53591 | 6.0357 | −72.0931 | 16.97 | 0.78 | 0.47 | 4.90 ±0.01 | 50.8 ±3.2 | ![]() |
WF4-V04, ELO, X-ray |
55706 | 6.0294 | −72.0852 | 16.35 | 1.2 | 0.52 | ![]() |
25.3 ±3.0 | ![]() |
BSS |
57067 | 6.0268 | −72.0813 | 16.31 | 1.2 | 0.49 | 2.70 ±0.01 | ![]() |
![]() |
BSS, ELO |
61863 | 6.0127 | −72.0840 | 14.21 | 0.82 | 0.15 | ![]() |
![]() |
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bimodal |
61968 | 6.0114 | −72.0937 | 17.74 | 0.75 | 0.38 | 6.27 ±0.01 | 40.0 ±2.7 | ![]() |
|
63549 | 6.0069 | −72.0905 | 16.65 | 1.2 | 0.3 | ![]() |
![]() |
![]() |
BSS |
65419 | 6.0021 | −72.0868 | 16.94 | 0.77 | 0.72 | ![]() |
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![]() |
white dwarf cand., bimodal |
68514 | 5.9910 | −72.0814 | 16.96 | 0.78 | 0.35 | 4.16 ±0.01 | ![]() |
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|
70896 | 5.9811 | −72.0835 | 13.53 | 0.82 | 0.35 | ![]() |
![]() |
0.34 ±0.06 | |
98813 | 6.0306 | −72.0804 | 15.49 | 0.81 | 0.10 | 33.61 ±0.03 | 7.9 ±0.9 | ![]() |
bimodal |
104622 | 6.0138 | −72.0798 | 16.34 | 1.2 | 0.42 | 22.66 ±0.01 | 23.4 ±2.5 | ![]() |
BSS, bimodal |
106521 | 6.0083 | −72.0780 | 13.96 | 0.83 | 0.20 | ![]() |
![]() |
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|
106958 | 6.0070 | −72.0736 | 16.73 | 1.2 | 0.44 | ![]() |
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BSS, bimodal |
107261 | 6.0065 | −72.0734 | 16.21 | 0.79 | 0.33 | ![]() |
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|
110506 | 5.9949 | −72.0799 | 16.76 | 0.77 | 0.36 | 8.94 ±0.01 | 33.9 ±1.6 | ![]() |
SSG, X-ray, ELO |
112447 | 5.9877 | −72.0738 | 12.49 | 0.80 | 0.27 | ![]() |
11.9 ±0.6 | ![]() |
|
129292 | 6.0766 | −72.0601 | 14.73 | 0.82 | 0.17 | ![]() |
![]() |
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bimodal |
132746 | 6.0573 | −72.0596 | 17.19 | 0.74 | 0.14 | ![]() |
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![]() |
SSG, WF2-V32, bimodal |
132812 | 6.0570 | −72.0549 | 18.29 | 0.72 | 0.23 | ![]() |
![]() |
![]() |
|
133593 | 6.0512 | −72.0623 | 17.10 | 0.78 | 0.43 | 16.71 ±0.01 | 31.7 ±1.7 | ![]() |
|
155735 | 6.0718 | −72.0508 | 17.02 | 0.76 | 0.39 | 6.77 ±0.01 | ![]() |
![]() |
SSG, ELO |
1004589 | 5.9146 | −72.0806 | 17.17 | 0.84 | 0.44 | 35.18 ±0.03 | ![]() |
0.32 ±0.04 | |
1009837 | 5.9084 | −72.0830 | 17.84 | 0.88 | 0.49 | ![]() |
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Notes. The Keplerian parameters were calculated using UltraNest. The columns list the ACS source ID, the right ascension and declination coordinates, the apparent visual magnitude in the F606W filter, the estimated primary and (minimum) companion stellar masses, the period, the RV semi-amplitude, and the eccentricity. Stars showing an excess in Hα are marked as emission line objects (ELO) and binaries with bimodal posterior distributions are indicated in the notes column.
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