Table 3.
Other detections of the triples.
| Object | This work (a) | Gaia DR3 orbits (a)(b) | Other |
|---|---|---|---|
| (Pout, eout, ωout) | (Pout, eout, ωout) | ||
| TIC 133771812 | 243.87 d; 0.217; 195° | ... | ... |
| TIC 176713425 | 52.57 d; 0.412; 95.2° | ... | ... |
| TIC 185615681 | 55.86 d; 0.098; 309° | ... | Rowan et al. (2023) |
| TIC 287756035 | 368 d; 0.235; 53.7° | ... | ... |
| TIC 321978218 | 57.51 d; 0.258; 123° | 57.52 d; 0.28; 116° | ... |
| TIC 323486857 | 41.36 d; 0.007; 241° | 41.35 d; 0.045; 180° | ... |
| TIC 650024463 | 107.88 d; 0.323; 351° | ... | ... |
Notes. Three of the seven triply eclipsing systems were spotted in prior broad surveys, but no quantitative analysis of the system parameters (especially of the constituent stars) was undertaken. Two of them have outer orbits reported by Gaia, but no third body eclipses were reported by Gaia. One of the systems, TIC 185615681, was included in the Rowan et al. (2023) list of mutlistellar systems tabulated from ASAS-SN data, and studied for the apsidal motion of its inner binary by Zasche (2012) and Kim et al. (2018), as well as for RVs by Duerbeck & Rucinski (2007).
Where available, we show for each source, the period, eccentricity, and argument of periastron of the outer orbit, separated by semicolons.
The Gaia orbital solutions are both spectroscopic; Babusiaux et al. (2023), Gaia Collaboration (2023).
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