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. Author manuscript; available in PMC: 2008 Dec 10.
Published in final edited form as: Icarus. 2006 Nov;185(1):39–63. doi: 10.1016/j.icarus.2006.06.001

Table 3b.

Determination of the apparent size and orientation of the asteroids observed in 2004

Date UT time Target Basic-processed
Deconvolved
Angle
(deg)
2a
(mas)
2b
(mas)
2a
(km)
2b
(km)
Angle
(deg)
2a
(mas)
2b
(mas)
2a
(km)
2b
(km)
2004-Oct-25 07:03:51 Aegle -5.1 112 92 209 171 2.1 91 77 170 143
2004-Oct-25 08:29:11 Aletheia -27.3 131 108 227 188 -23.7 122 98 211 170
2004-Oct-25 06:39:57 Andromache -235.0 109 97 137 121 -232.9 89 81 112 102
2004-Oct-25 06:53:31 Camilla 11.4 119 98 250 206 20.1 100 77 210 161
2004-Oct-25 09:44:34 Elsa -30.2 68 58 54 46 -29.6 46 42 36 33
2004-Oct-25 09:04:16 Loreley -17.9 136 111 214 174 -15.5 118 93 185 147
2004-Oct-25 06:00:38 Metis 13.0 189 161 201 172 9.5 188 152 201 162
2004-Oct-25 08:01:37 Metis2 -44.3 188 153 201 163 -44.0 190 148 203 158
2004-Oct-25 07:15:55 Palisana 9.8 99 94 98 93 51.3 83 72 82 71
2004-Oct-25 06:29:16 Sylvia -8.0 195 135 367 254 -3.9 185 115 348 217
2004-Oct-25 08:40:45 Veritas 4.8 110 92 155 129 11.7 105 81 148 115
2004-Oct-25 08:17:09 Zelinda 30.2 118 114 126 122 77.2 106 104 114 111

Notes. The measurement is performed fitting an ellipse (major-axis 2a, minor-axis 2b) on the basic-processed and the deconvolved final images. The orientation of the major-axis is given in degrees counter-clockwise from the astronomical east.