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Table 5.
Some other analysed systems.
| System | Remark |
|---|---|
| OGLE LMC-ECL-02310 | Too long mutual period PAB (> 11 yr), insufficient data coverage. Long period PB. |
| OGLE LMC-ECL-15607 | Too small LITE variation for binary A, period PAB long (> 16 yr), shallow eclipses of binary B. |
| OGLE LMC-ECL-15742 | Only very small amplitude of LITE for both binaries (smaller than 0.004 d), period PAB about 7 yr. Eccentric orbit of binary B, apsidal motion of about 114 yr. |
| OGLE LMC-ECL-20932 | Too long period PAB (>22 yr). Shallow eclipses of binary B. |
| OGLE LMC-ECL-21094 | Long period PAB (>20 yr), insufficient data. Eccentric orbit of binary A, apsidal motion >150 yr. Suspected inclination change of binary B. |
| OGLE BLG-ECL-030128 | Insufficient data for analysis, mutual period PAB about 20 yr. |
| OGLE BLG-ECL-335648 | Too short suspected period PAB (≃2.4 yr), not enough data for proper analysis. |
| OGLE BLG-ECL-398110 | Mutual period PAB of about 7.4 yr, but insufficient data coverage for detailed analysis. Only shallow eclipses of binary A. |
| TYC 3929-724-1 | Detailed analysis will be published in a forthcoming separate study. |
| OGLE LMC-ECL-02156 | Inclination change of binary A. |
| OGLE LMC-ECL-16532 | Too slow LITE variation, not detected for binary B, likely because of its too long orbital period PB (≃78 d). |
| OGLE LMC-ECL-17913 | ETVs of binary A indicate a possible short period of ≃350 d, but those of binary B are too noisy. |
| OGLE LMC-ECL-21994 | Too long orbital period PAB (>20 yr), lack of data. |
| OGLE LMC-ECL-23000 | New data in contradiction with the older data. Solution possible only with an additional quadratic ephemerides term. |
Notes. The upper part comprises the systems of Group 2, while the lower part of Group 3.
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