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Table 2

List of new asteroid models derived from the Catalina Sky Survey data alone.

Asteroid λ1 β1 λ2 β2 P N703 Ppubl Period reference
[deg] [deg] [deg] [deg] [h] [h]

2112 Ulyanov 156 48 334 65 3.04071 118 3.000 Maleszewski & Clark (2004)
2384 Schulhof 196 −60 45 −42 3.29367 121 3.294 Ditteon et al. (2002)
2617 Jiangxi 224 76 1 54 11.7730 124 11.79 Carbo et al. (2009)
3170 Dzhanibekov 217 60 21 64 6.07168 105 6.0724 Molnar et al. (2008)
4507 1990 FV 143 55 323 49 6.57933 84 6.58 Yoshida et al. (2005)
5647 1990 TZ 253 77 119 −19 6.13867 87 6.144 Bembrick & Bolt (2003)
10826 1993 SK16 260 −56 60 −34 13.8327 90 13.835 Galad (2008)
19848 Yeungchuchiu 190 −68 3.45104 104 3.450 Yeung (2006)
3097 Tacitus 229 71 72 62 8.7759 99
4611 Vulkaneifel 5 −86 197 −50 3.75635 148
5461 Autumn 249 −26 79 −43 20.0929 106
5625 1991 AO2 265 −52 97 −78 6.67411 110
5960 Wakkanai 226 −69 69 −61 4.96286 102
7201 Kuritariku 22 67 249 64 48.849 103
7632 Stanislav 234 −50 46 −45 5.29073 99
7905 Juzoitami 105 −76 226 −55 2.72744 118
13002 1982 BJ13 58 −50 245 −57 3.13844 110
16009 1999 CM8 283 44 8.3476 124
16847 Sanpoloamosciano 91 −24 8.1845 114
26792 1975 LY 226 68 79.15 140

Notes.For each asteroid, the table gives the ecliptic coordinates λ1 and β1 of the pole solution, the corresponding mirror solution λ2 and β2, the sidereal rotational period P, the number of sparse data points from the CSS N703, and the previously published period value Ppubl with the reference. The uncertainty of the sidereal rotational period corresponds to the last decimal place of P and of the pole direction to 20–40°.

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