no code implementations • 27 Jan 2022 • A. Leleu, J. -B. Delisle, R. Mardling, S. Udry, G. Chatel, Y. Alibert, P. Eggenberger
In particular, we show that in Kepler-1972, not taking into account planet-planet interactions yields an error of $\sim 30\%$ on the radii of planets b and c, in addition to generating in-transit scatter, which leads to mistake KOI3184. 02 for a false positive.
no code implementations • 12 Nov 2021 • A. Leleu, G. Chatel, S. Udry, Y. Alibert, J. -B. Delisle, R. Mardling
Here we introduce a detection method that is robust to large TTVs, and illustrate its use by recovering and confirming a pair of resonant super-Earths with ten-hour TTVs around Kepler-1705.