Growth after the streaming instability - From planetesimal accretion to pebble accretion

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Table 1

Simulations set-up in Sects. 3.1–3.3.

Name	Initial planetesimal size	Inclination	m_p (M_⊕)	a_p (AU)

run_md_test	Mono-size	No	4.0	0.1
run_md_1	Mono-size	Yes	0.004	2.7
run_md_2	Mono-size	Yes	0.009	2.7
run_md_3	Mono-size	Yes	0.02	2.6
run_pd_1	Poly-size	Yes	1.3	1.7
run_pd_2	Poly-size	Yes	1.6	1.5
run_pd_3	Poly-size	Yes	1.4	1.8
run_sp_1	One embryo + small planetesimals	Yes	1.3	1.8
run_sp_2	One embryo + small planetesimals	Yes	1.4	1.6
run_sp_3	One embryo + small planetesimals	Yes	1.3	1.7

Notes. The mass and semimajor axis of the most massive planet are given at t = 1 Myr.

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