Shape and spin determination of Barbarian asteroids

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Table 4

Same as Table 3, but for asteroids which were not observed during this campaign.

Asteroid	b / a	c / b	P _sid	λ ₁	β ₁	λ ₂	β ₂	η _a	D	Ref.
			[h]	[deg]	[deg]	[deg]	[deg]		[km]

234	0.90	0.88	26.474	144	−38			0.33	43.7	[1]
599			9.3240						71	[2]
606	0.82	0.92	12.2907	183	20	354	26		35.5	[3]
642			8.19						38.2	[4]
673			22.340						41.6	[5]
679	0.72	0.92	8.45602	220	32	42	−5	0.38	51.4	[6]
1284			9.55						46	[7]
2448			10.061						43	[8]

Notes. The bootstrap method was not applied to (606) because the number of dense light-curves was not sufficient.

Reference. [1] Tanga et al. (2015); [2] Debehogne et al. (1977); [3] Hanuš et al. (2011); [4] LeCrone et al. (2005); [5] Marciniak et al. (2016); [6] Marciniak et al. (2011); [7] Carreño-Carcerán et al. (2016); [8] Strabla et al. (2013).

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