http://arxiv.org/abs/2211.17035
We report the discovery and confirmation of the planetary system TOI-1288. This late G dwarf harbours two planets: TOI-1288 b and TOI-1288 c. We combine TESS space-borne and ground-based transit photometry with HARPS-N and HIRES high-precision Doppler measurements, which we use to constrain the masses of both planets in the system and the radius of planet b. TOI-1288~b has a period of $2.699835^{+0.000004}{-0.000003}$ d, a radius of $5.24 \pm 0.09$ R$\oplus$, and a mass of $42 \pm 3$ M$\oplus$, making this planet a hot transiting super-Neptune situated right in the Neptunian desert. This desert refers to a paucity of Neptune-sized planets on short period orbits. Our 2.4-year-long Doppler monitoring of TOI-1288 revealed the presence of a Saturn-mass planet on a moderately eccentric orbit ($0.13^{+0.07}{-0.09}$) with a minimum mass of $84 \pm 7$ M$\oplus$ and a period of $443^{+11}{-13}$ d. The 5 sectors worth of TESS data do not cover our expected mid-transit time for TOI-1288 c, and we do not detect a transit for this planet in these sectors.
E. Knudstrup, D. Gandolfi, G. Nowak, et. al.
Thu, 1 Dec 22
15/85
Comments: 16 pages, 17 figures, under review MNRAS