Table 3: Orbital elements and some pysical parameters for other members and candidates of the EL61-group a.
Object a e i q $\Delta\upsilon_{\min}$ $\delta v_{\min}$ S' Refb
1996 TO66 43.283 0.121 27.4 38.051 24.2 15.0 2.38 $\pm$ 2.04 (5)
2005 RR43 43.115 0.138 28.6 37.175 111.2 58.0 -0.4 $\pm$ 2.0 (3)
2003 TX300 43.216 0.125 25.8 37.821 107.5 68.4 1 $\pm$ 2.00 (1)
2002 GH32 42.185 0.086 26.6 38.541 141.9 79.3 35.25 $\pm$ 10.21 (5)
2003 EL61 43.240 0.192 28.2 34.931 323.5   0.0 $\pm$ 2.0 (4)
1999 OY3 42.185 0.086 26.6 3 8.541 292.8 96.6 -2.62 $\pm$ 3.39 (5)
2005 FY9 45.543 0.158 29.0 38.333 141.2 118.0 8.9 $\pm$ 1.0 (2)
1998 HL151 40.930 0.091 28.0 37.224 142.5 136.4 9.83 $\pm$ 21.1 (5)
1998 WT31 45.821 0.180 28.7 37.581 233.3 139.8 5.57 $\pm$ 5.61 (5)
2000 CG105 46.280 0.038 28.0 44.533   149.0 2.58 $\pm$ 17.72 (5)
1999 RY215 45.228 0.236 22.2 34.554 - 183.0 4.54 $\pm$ 6.65 (5)
1999 KR16 49.206 0.309 24.8 34.001 - 242.9 44.74 $\pm$ 3.21 (5)
a a: semi-major axis [AU]; e: eccentricity; i: inclination [$^{\circ}$]; q: perihelion distance [AU]; $\Delta v_{\min}$ and $\delta v_{\min}$ [m s-1] quantities computed by Ragozzine & Brown (2007); S': the spectral slope.
b References are for the measured spectral gradient: (1) Licandro et al. (2006b), (2) Licandro et al. (2006a), (3) Pinilla-Alonso et al. (2007),(4) Pinilla-Alonso et al. (2008) and (5) Ragozzine & Brown (2007) and references therein.


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