In-depth study of moderately young but extremely red, very dusty substellar companion HD 206893B

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Table F.1

Properties of dusty, peculiar, and possibly young dwarfs later than L4 considered in our study.

Source name	Spectral type	Cand. member	Mass	Ref.
			(M_Jup)

2MASS J11193254-1137466	L7	TWA	4.3–7.6	1, 2
2MASS J17081563+2557474	L5	...	...	1
WISEP J004701.06+680352.1	L7	AB Dor	~18	3, 4
PSO J318.5338-22.8603	L7	β Pic	8.3 ± 0.5	5, 6
ULAS J222711-004547	L7	...	...	7
WISE J174102.78-464225.5	L7	β Pic or AB Dor	4-21	8
WISE J020625.27+264023.6	L8	...	...	9, 22
WISE J164715.57+563208.3	L9	Argus	4–5	9, 10
2MASS J00011217+1535355	L4	AB Dor	25.3 ± 1.0	11, 12, 13
2MASS J21543454-1055308	L4	Argus?	...	14, 22
2MASS J22064498-4217208	L4	AB Dor	23.1 ± 6.4	15
2MASS J23433470-3646021	L3–L6	AB Dor	...	12
2MASS J03552337+113343	L5	AB Dor	13–30	16, 17, 18
2MASS J21481628+4003593	L6	Argus?	...	10, 15, 19, 22
2MASSW J2244316+204343	L6	AB Dor	11–12	15, 20
2MASS J05012406-0010452	L4	Columba		12, 21

Reference. 1 – Kellogg et al. (2015), 2 – Kellogg et al. (2016), 3 – Gizis et al. (2012), 4 – Gizis et al. (2015), 5 – Liu et al. (2013), 6 – Allers et al. (2016), 7 – Marocco et al. (2014), 8 – Schneider et al. (2014), 9 – Kirkpatrick et al. (2011), 10 – Gagné et al. (2014b), 11 – Knapp et al. (2004), 12 – Gagné et al. (2015b), 13 – Gagné et al. (2015c), 14 – Gagné et al. (2014a), 15 – Faherty et al. (2016), 16 – Reid et al. (2006), 17 – Cruz et al. (2009), 18 – Faherty et al. (2013), 19 – Looper et al. (2008), 20 – McLean et al. (2003), 21 – Casewell et al. (2008), 22 – Liu et al. (2016).

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