Spins and shapes of 11 near-Earth asteroids observed within the NEOROCKS project

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Table A.2

Overview of the modeling results.

Asteroid		# of solutions for period / pole	Psid [h]	best-fit λ; β[°]	uncertainty radius [°]	best-fit ϵ[°]	a/b; a/c	Reference
(5189)	1990 UQ	1 / 1	6.65738 ± 0.00002	224; −85	13	179	1.61; 2.67	Sect. 4.1
(6569)	Ondaatje	1 / 1	5.960234 ± 0.000004	214;−72	10	173	1.94; 2.02	Sect. 4.2
(7025)	1993 QA	2/2	2.506168 ± 0.000001	13;−71	13	151	1.10; 1.37	Sect. 4.3
			2.506299 ± 0.000001*	339; −77	12	160	1.27; 1.32	Sect. 4.3
(7482)	1994 PC1	256/-	${2.602}_{- 0.007}^{+ 0.005}$ $2.602_{ - 0.007}^{ + 0.005}$					Sect. 4.12
(8566)	1996 EN	1 / 1	4.8440 ± 0.0001	112; −84	19	137	1.03; 1.12	Sect. 4.4
(22099)	2000 EX₁₀₆	16/-	${6.333}_{- 0.006}^{+ 0.003}$ $6.333_{ - 0.006}^{ + 0.003}$					Sect. 4.12
(66251)	1999 GJ₂	11 /-	${2.4622}_{- 0.0005}^{+ 0.0003}$ $2.4622_{ - 0.0005}^{ + 0.0003}$		β<10		1.01–1.09;	Sect. 4.5
							1.07–1.49
(86450)	2000 CK₃₃	1/1	6.60564 ± 0.00002	208;−68	15	174	1.99; 2.25	Sect. 4.6
(98943)	2001 CC₂₁	1/1	5.021522 ±0.000003	259; +84	8	7	1.59; 2.15	Sect. 4.7
(137199)	1999 KX₄	1/3	2.769675 ± 0.000008	92; −60*	18	142	1.05; 1.41	Sect. 4.8
				202; −14	8	120		Sect. 4.8
				150; −35	6	136		Sect. 4.8
(170891)	2004 TY₁₆	78/-	${2.791}_{- 0.001}^{+ 0.004}$ $2.791_{ - 0.001}^{ + 0.004}$					Sect. 4.12
(276786)	2004 KD₁	2/2	5.017051 ±0.000003	202; +56	8	25	1.20; 1.49	Sect. 4.9
			5.018636 ±0.000003*	304; −59	22	153	1.75; 2.03	Sect. 4.9
(329437)	2002 OA₂₂	12/-	2.6204 ± 0.0009					Sect. 4.12
(495615)	2015 PQ₂₉₁	2/2	13.7413 ± 0.0007*	151;+45	33	11	1.48; 1.58	Sect. 4.10
			13.7518 ±0.0007	126; +33	21	26	1.42; 2.16	Sect. 4.10
(506459)	2002 AL₁₄	83/-	${2.3081}_{- 0.0003}^{+ 0.0018}$ $2.3081_{ - 0.0003}^{ + 0.0018}$					Sect. 4.12
(512245)	2016 AU₈	1 / 1	4.50541 ± 0.00004	75; −86	18	173	1.25; 2.15	Sect. 4.11
	2013 BO₇₆	172/-	5.11 ±0.01					Sect. 4.12

globally best-fit solution

period and pole direction uncertainties are reported at the 3σ confidence level a/b,a/c represent axis ratios of surface-fit ellipsoids

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