Discovery of 4 warm giants

With a mass of 2.02+/-0.13M_J_ and a radius of 0.96^+0.05^_-0.06_R_J_, TOI-5027 b orbits its host star in an eccentric orbit with e=0.385^+0.025^_-0.026_ every 10.24368+/-0.00001 days. TOI-2328 b is a Saturn-like planet with a mass of 0.16+/-0.02M_J_ and a radius of 0.89^+0.04^_-0.05_R_J_, orbiting its host star in a nearly circular orbit with e=0.057^+0.046^_-0.029_ at an orbital period of 17.10197+/-0.00001 days. All four planets have orbital periods above 10 days, and our planet interior structure models are consistent with a rocky-icy core with a H/He envelope, providing evidence supporting the core-accretion model of planet formation for this kind of planets.