Spin rates of V-type asteroids | Astronomy & Astrophysics (A&A)

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Table A.4

As in Table A.2, but for the low inclination population.

Asteroid	Synodic period	U-code	Diameter	Class,	a	e	sin(i)
No.	(LCDB) (h)	(LCDB)	(km)	references	(au)
1914	6.331	2	9.6	V^(2,5,12)	2.406	0.139	0.0848
2247	4.4974	−	4.4	V^(2,12,16)	2.449	0.090	0.1017
2442	11.453	2	8.3	V^(1,2,12,14), J^(8,18)	2.388	0.097	0.0944
2566	4.451	3	7.8	V^(1,13,14,15)	2.450	0.104	0.0771
2653	5.5228	3	9.9	V^(1,13,15)	2.444	0.114	0.0888
2704	2.6382	3	5.2	V^(1,2,12,13)	2.385	0.117	0.0889
2763	7.8	3	7.5	V^{(1,3,9,11,13,15,17)}, S⁽¹⁹⁾	2.404	0.179	0.0756
2823	2.6262	−	5.4	V^(2,4,12,15)	2.326	0.175	0.0726
3331	7.5888	−	4.4	V	2.418	0.112	0.0624
3849	2.778	2	5.8	V^{(1,2,6,12,13)}	2.474	0.065	0.0940
3867	28.035	2	5.4	V	2.351	0.136	0.0954
4188	2.58	3−	6.6	V^{(1,2,12,13,14,15)}	2.335	0.111	0.0986
4796	3.5086	3	5.7	V^{(1,2,7,12,13,15)}	2.355	0.141	0.0538
7798	3.8724	−	5.0	V	2.479	0.131	0.0800
7899	85.658	2	3.9	V	2.343	0.114	0.0937
8645	7.616	3−	5.1	V^(2,7,12)	2.431	0.041	0.0885
9223	3.758	2	4.5	V^(2,6,12)	2.301	0.080	0.0699
11149	12.85	3−	3.5	V	2.442	0.079	0.1035
15481	5.01	2	4.7	V	2.383	0.107	0.0784
15630	8.064	2	3.6	V^(2,6,12,17)	2.326	0.146	0.0818
27192	5.5741	−	3.2	V	2.323	0.119	0.097
29337	4.5096	3	4.2	V	2.468	0.189	0.1025
47417	11.71	2−	4.6	V	2.400	0.090	0.0990
56570	3.22	2	2.4	V^(2,11,12)	2.378	0.096	0.0721
82125	2.554	2	1.8	V	2.414	0.092	0.0976
118567	6.741	2	1.3	V	2.318	0.093	0.1026
151036	4.974	2	1.9	V	2.448	0.124	0.0957

Notes. In bold we flag asteroids for which we determined or confirmed periods in this article.

References.⁽¹⁾ Neese (2010), ⁽²⁾ Hasselmann et al. (2012), ⁽³⁾ Duffard et al. (2004), ⁽⁴⁾ Moskovitz et al. (2008b), ⁽⁵⁾ Alvarez-Candal et al. (2006), ⁽⁶⁾Hardersen et al. (2018), ⁽⁷⁾Hasegawa et al. (2014), ⁽⁸⁾Xu et al. (1995), ⁽⁹⁾Spahr et al. (1997), ⁽¹⁰⁾Roig & Gil-Hutton (2006), ⁽¹¹⁾Licandro et al. (2017), ⁽¹²⁾Carvano et al. (2010), ⁽¹³⁾Bus & Binzel (2002), ⁽¹⁴⁾DeMeo et al. (2009), ⁽¹⁵⁾Moskovitz et al. (2010), ⁽¹⁶⁾Hicks et al. (2014), ⁽¹⁷⁾Popescu et al. (2018), ⁽¹⁸⁾Binzel & Xu (1993), ⁽¹⁹⁾Erasmus et al. (2019).

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