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

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Table A.5

As in Table A.2, but for the inner other population.

Asteroid	Synodic period	U-code	Diameter	Class,	a	e	sin(i)
No.	(LCDB) (h)	(LCDB)	(km)	references	(au)
854	37.56	3	7.8	V^(2,3,12)	2.368	0.164	0.1124
2432	3.206	3−	7.4	V	2.352	0.129	0.1158
2851	5.414	3−	8.8	V^(1,13,14,15)	2.478	0.123	0.1348
3536	5.79	3	3.2	V^{(1,22,26,31,35)}	2.343	0.077	0.1156
3900	5.324	3	5.0	V^{(1,7,10,11,13,17)}	2.371	0.113	0.1224
4383	3.4069	3	6.5	V^(2,7,9,12)	2.425	0.055	0.1095
5150	5.1953	3	5.4	V	2.477	0.138	0.1076
5524	8.416	3	19.9	V	2.366	0.059	0.1194
5599	3.6195	3	6.4	V^(2,12,16)	2.419	0.155	0.1264
5875	5.551	3	7.5	V^{(2,6,11,12,17)}	2.379	0.067	0.1246
6680	6.722	3	4.5	V	2.322	0.095	0.1408
6976	4.025	3	5.5	V	2.333	0.119	0.1303
7484	6.237	2	4.0	V	2.405	0.071	0.1114
9368	2.9183	3	4.3	V^(2,5,12)	2.310	0.163	0.1289
9652	4.385	2	6.0	V	2.418	0.197	0.1196
18641	5.2461	3	3.7	V	2.357	0.097	0.1344
25327	6.716	3	4.4	V⁽⁴⁾	2.434	0.186	0.2187
25542	10.55227	2	2.7	V	2.443	0.116	0.1224
35062	19.08	2	3.2	V^{(2,4,11,12,17)}	2.370	0.285	0.1755
42979	3.498	2	2.0	V	2.400	0.110	0.1198
53533	5.674	2	2.4	V	2.419	0.137	0.1082
54584	2.92	3-	3.2	V	2.342	0.123	0.1431

References. ⁽¹⁾ Neese (2010), ⁽²⁾ Hasselmann et al. (2012), ⁽³⁾Birlan et al. (2011), ⁽⁴⁾Solontoi et al. (2012), ⁽⁵⁾Hardersen et al. (2018), ⁽⁶⁾Hardersen et al. (2015), ⁽⁷⁾Hasegawa et al. (2014), ⁽⁸⁾Xu et al. (1995), ⁽⁹⁾Pajuelo et al. (2018), ⁽¹⁰⁾Spahr et al. (1997), ⁽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).

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