Extended Data Table 2 The fitting parameters for theoretical models under various conditions for different observational data

From: The origin and tidal evolution of hot Jupiters constrained by a broken age–frequency relation

  1. Standard case: (a) ‘Early’ model: initial mass and radius distributions as observed warm/cold Jupiters; initial period distribution as the result from Kepler data; (b) ‘Late’ model: initial distributions referring to Hamers et al. 2017. Case 1: Similar to Standard case but the mass distribution of ‘Early’ model as observed hot Jupiters. Case 2-4: Similar to Standard case but the period distribution of ‘Early model’ is taken as uniform in logarithmic space, the disk migration component, and high-e migration component of Nelson et al. (2017), respectively.
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