Multiply eclipsing candidates from TESS satellite

The average period of the dominant pair, pair A, is 2.7 days in our sample, while for the second pair, pair B, the average period is 5.3 days. Several systems show evident eclipse timing variation (ETV) changes even from the short interval of the TESS data, indicating possible period changes and short mutual orbit. We also present evidence that the system V0871 Cen is probably a septuple-star system of architecture (Aa-Ab)-B-C-D. Most of the presented systems are adequately bright and show deep enough eclipses for observing, and therefore we call for new ground-based observations for these extremely interesting multiples.

Owing to this motivation, we have included also the ephemerides for both pairs of each system, our catalogue also contains their depths of eclipses and the light-curve shapes as extracted from the TESS data. These new ground-based observations would be very useful for further derivation of the mutual movement of both pairs on their orbit via detection of the ETVs of both pairs for example.