Uncovering the true periods of the young sub-Neptunes orbiting TOI-2076
Context. TOI-2076 is a transiting three-planet system of sub-Neptunes orbiting a bright (G = 8.9 mag), young (340 ± 80 Myr) K-type star. Although a validated planetary system, the orbits of the two outer planets were unconstrained as only two non-consecutive transits were seen in TESS photometry. This left 11 and 7 possible period aliases for each
Osborn, H. P. et al.
Fecha de publicación:
8
2022