From planetesimals to dwarf planets by pebble accretion

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Table 2

List of model runs and posterior values for the MCMC simulations.

Model	log₁₀ σ	log₁₀ τ_s	log₁₀ τ₂	f₂	m_brk [10²⁰ g]	m_imf (m_⊕)	m_peb (m_⊕)	C_τσ	ln 𝒫
`lami-1p`	$- {2.78}_{- 0.38}^{+ 0.40}$ $\[-2.78_{-0.38}^{+0.40}\]$	$- {1.70}_{- 1.22}^{+ 1.15}$ $\[-1.70_{-1.22}^{+1.15}\]$			${8.90}_{- 1.96}^{+ 2.12}$ $\[8.90_{-1.96}^{+2.12}\]$	${11.61}_{- 1.08}^{+ 1.00}$ $\[11.61_{-1.08}^{+1.00}\]$	${5.22}_{- 2.25}^{+ 4.09}$ $\[5.22_{-2.25}^{+4.09}\]$	$- {10.05}_{- 0.12}^{+ 0.11}$ $\[-10.05_{-0.12}^{+0.11}\]$	−86.64
`turb-1p`	$- {2.56}_{- 0.49}^{+ 0.41}$ $\[-2.56_{-0.49}^{+0.41}\]$	$- {2.12}_{- 1.27}^{+ 1.46}$ $\[-2.12_{-1.27}^{+1.46}\]$			${6.69}_{- 1.49}^{+ 1.96}$ $\[6.69_{-1.49}^{+1.96}\]$	${11.39}_{- 2.12}^{+ 1.24}$ $\[11.39_{-2.12}^{+1.24}\]$	${7.60}_{- 3.61}^{+ 5.45}$ $\[7.60_{-3.61}^{+5.45}\]$	$- {9.81}_{- 0.13}^{+ 0.13}$ $\[-9.81_{-0.13}^{+0.13}\]$	−86.14
`lami-2p`	$- {2.92}_{- 0.30}^{+ 0.43}$ $\[-2.92_{-0.30}^{+0.43}\]$	$- {1.88}_{- 1.36}^{+ 1.27}$ $\[-1.88_{-1.36}^{+1.27}\]$	$- {1.96}_{- 1.33}^{+ 1.32}$ $\[-1.96_{-1.33}^{+1.32}\]$	${0.14}_{- 0.10}^{+ 0.11}$ $\[0.14_{-0.10}^{+0.11}\]$	${8.14}_{- 2.36}^{+ 2.20}$ $\[8.14_{-2.36}^{+2.20}\]$	${11.61}_{- 1.09}^{+ 1.02}$ $\[11.61_{-1.09}^{+1.02}\]$	${5.60}_{- 2.47}^{+ 4.48}$ $\[5.60_{-2.47}^{+4.48}\]$	$- {10.12}_{- 1.74}^{+ 0.15}$ $\[-10.12_{-1.74}^{+0.15}\]$	−86.10
`turb-2p`	$- {2.84}_{- 0.30}^{+ 0.52}$ $\[-2.84_{-0.30}^{+0.52}\]$	$- {1.88}_{- 1.48}^{+ 1.32}$ $\[-1.88_{-1.48}^{+1.32}\]$	$- {2.30}_{- 1.19}^{+ 1.58}$ $\[-2.30_{-1.19}^{+1.58}\]$	${0.15}_{- 0.10}^{+ 0.10}$ $\[0.155_{-0.10}^{+0.10}\]$	${6.21}_{- 1.57}^{+ 1.86}$ $\[6.21_{-1.57}^{+1.86}\]$	${11.66}_{- 1.34}^{+ 1.14}$ $\[11.66_{-1.34}^{+1.14}\]$	${7.10}_{- 3.28}^{+ 5.30}$ $\[7.10_{-3.28}^{+5.30}\]$	$- {9.86}_{- 0.62}^{+ 0.16}$ $\[-9.86_{-0.62}^{+0.16}\]$	−85.96

Notes. See Table 1 for the parameters and Equation (15) for C_τσ. The lower and upper values indicate the 16% and 84% posterior ranges. The last column gives the maximum likelihood of the sample.

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