There are a series of papers coming out describing in-depth planet-forming simulations.
Paper 1 describes the simulation,
Paper 2 is about "methods to calculate population synthesis."
Paper 3 "will look for correlations between the occurrence of inner low-mass and outer giant planets."
Paper 4 "will xtend the populations synthesis to lower-mass stars (down to late-M dwarfs) and analyze the effects of stellar mass."
Paper 5 "will look at the diversity between planets in each system compared to diversity of the overall population."
Paper 6 will compare this to HARPS results.
Paper 7 will compare this to CARMENES results.
Paper 8 will compare this to Kepler results.
On arXiv tonight, the first three papers came out.
The New Generation Planetary Population Synthesis (NGPPS). I. Bern global model of planet formation and evolution, model tests, and emerging planetary systems
https://arxiv.org/abs/2007.05561The New Generation Planetary Population Synthesis (NGPPS). II. Planetary population of solar-like stars and overview of statistical results
https://arxiv.org/abs/2007.05562The New Generation Planetary Population Synthesis (NGPPS). III. Warm super-Earths and cold Jupiters: a weak occurrence correlation, but a strong architecture-composition link
https://arxiv.org/abs/2007.05563
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