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Table 1

Spin parameters and sizes of asteroid models obtained in this work.

Asteroid Pole P Observing span Napp Nlc D D RMS
λp(°) βp(°) (h) (yr) (km) (km)
(70) Panopaea 42 ± 5 +27 ± 3 15.80440 ± 0.00002 1980-2019 7 122 128 ± 7 7
240 ± 6 +26 ± 4 15.80439 ± 0.00001 7
(275) Sapientia 85 ± 11 -10 ± 18 14.93045 ± 0.00005 1998-2018 7 38 6
264 ± 4 -1 ± 20 14.93045 ± 0.00005 6
(275) Sapientia (ADAM) 82 ± 8 -11 ± 17 14.93044 ± 0.00005 1998-2018 7 38 100 ± 1 -
260 ± 7 -2 ± 20 14.93044 ± 0.00005 100 ± 1 -
(286) Iclea 31 ± 5 +13 ± 4 15.36120 ± 0.00004 2002-2019 9 52 2
196 ± 5 +44 ± 7 15.36114 ± 0.0007 3
(326) Tamara 79 ± 1 -3 ± 3 14.46130 ± 0.0005 1981-2019 9 69 5
242 ± 1 -36 ± 3 14.46136 ± 0.0004 81 ± 9 9
(412) Elisabetha 3 ± 20 + 17 ± 7 19.65610 ± 0.00003 1990-2021 7 77 119 ± 9 9
191 ± 23 +52 ± 8 19.65618 ± 0.00004 4
(426) Hippo 62 ± 55 -49 ± 20 67.5038 ± 0.0005 1993-2021 7 103 6
223 ± 80 -89 ± 17 67.5041 ± 0.0005 122 ± 4 4
(439) Ohio 308 ± 50 -61 ± 7 37.46726 ± 0.00005 1984-2022 10 66 2
(464) Megaira 47 ± 2 + 16 ± 5 12.878572 ± 0.000002 1979-2020 9 85 3
236 ± 5 +38 ± 10 12.878572 ± 0.000002 2
(464) Megaira (ADAM) 45 ± 3 + 13 ± 5 12.878573 ± 0.000001 1979-2020 9 85 75 ± 1 -
234 ± 4 +34 ± 14 12.878573 ± 0.000001 79 ± 1 -
(476) Hedwig 49 ± 4 +60 ± 7 27.2403 ± 0.0006 1982 - 2018 6 58 6
218 ± 4 +36 ± 4 27.2404 ± 0.0005 122 ± 10 10
(524) Fidelio 52 ± 50 +76 ± 6 14.171031 ± 0.000005 2005-2019 6 31 66 ± 5 5
186 ± 25 +54 ± 10 14.171042 ± 0.000005 67 ± 3 3
(530) Turandot 42 ± 3 +28 ± 5 19.95240 ± 0.00009 1986-2019 8 62 89 ± 11 11
226 ± 9 +54 ± 10 19.95231 ± 0.000009 89 ± 6 6
(530) Turandot (ADAM) 39 ± 6 +31 ± 11 19.95239 ± 0.00009 1986-2019 8 62 89 ± 2 -
223 ± 9 +60 ± 9 19.95232 ± 0.000009 89 ± 2 -
(551) Ortrud 149 ± 35 -63 ± 9 -66 ± 8 17.41924 ± 0.00003 2006-2021 7 88 85 ± 11 11
305 ± 30 17.41921 ± 0.00002 86 ± 10 10
(566) Stereoskopia 164 ± 15 -2 ± 2 12.08466 ± 0.00006 1990-2022 6 35 148 ± 8 8
338 ± 9 -13 ± 2 12.08463 ± 0.00003 148 ± 11 11
(657) Gunlod 127 ± 25 +61 ± 6 15.92872 ± 0.00003 1984-2022 6 47 37 ± 3 3
252 ± 50 +51 ± 20 15.92870 ± 0.00004 1984-2022 6 47 1
(738) Alagasta 67 ± 7 -47 ± 5 -41 ± 8 +39 ± 2 17.8888 ± 0.0005 2015-2020 5 41 56 ± 6 6
246 ± 10 17.8889 ± 0.0006 54 ± 4 4
(806) Gyldenia 34 ± 12 16.85695 ± 0.00003 2010-2021 8 63 57 ± 8 8
235 ± 15 +42 ± 5 16.85699 ± 0.00007 55 ± 4 4

Notes. The columns contain asteroid name, J2000 ecliptic coordinates λρ, βp of the spin axis solution, and the sidereal rotation period P, with the mirror pole solution in the second row. The following columns provide the main characteristics of the light-curve dataset (same for both pole solutions): observing span in calendar years, number of apparitions (Napp) and number of light curves (Nlc.) The last two columns give volume-equivalent diameter D and its RMS residual from the stellar occultation fitting. Boldface highlights the solution preferred by means of occultation fits. See Sect. 4 for the discussion on diameter uncertainties.

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