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Table 5

NEAs with existing precoveries for which a new reduction will be helpful (see text).

Asteroid Year of Additional arc Number of Current σȧ Expected σȧ Expected σȧ ȧ max / σ ȧ
1st precovery precoveries (1′′) (300 mas)
(years) (10-4 au/My)

162421 2000ET70 1977 23.050 2 16.8 1.7 0.7 8.04
4179 Toutatis 1934 42.292 2 0.4 0.4 0.3 4.43
138175 2000EE104 1999 0.923 5 11.6 5.8 4.5 3.46
7350 1993VA 1963 22.563 3 7.7 2.0 1.5 2.37
66400 1999LT7 1987 12.134 2 19.1 7.0 4.5 2.29
5797 Bivoj 1953 26.253 1 4.3 3.6 3.4 2.28
350751 2002AW 1991 10.776 2 72.9 24.2 9.8 2.01
1999FA 1978 19.855 1 127.7 10.3 9.7 1.96
87024 2000JS66 1979 21.328 2 32.4 11.0 4.8 1.54
2004SV55 1983 20.997 5 576.5 4.7 3.9 1.31
7341 1991VK 1981 9.886 1 3.3 3.2 2.4 1.27
1943 Anteros 1968 4.767 2 1.9 1.9 1.7 1.05
5604 1992FE 1976 8.983 2 10.0 5.5 3.5 1.01
4450 Pan 1937 50.631 2 10.8 4.7 3.7 1.01

Notes. The year of the first precovery, the additional extended arc, the number of available precoveries, and the current and expected drift uncertainty obtained for various precision of precoveries, are presented.

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