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Table 2

Spin parameters and thermophysical characteristics of asteroid models obtained in this work.

Asteroid Pole P vis. dev D pV Γ rhel Γ1AU

[h] [mag] [km] [SI units] IR [AU] [SI units]
(108) Hecuba 181 ± 2 + 42 ± 5 14.25662 ± 0.00003 0.013 0.24 35 1.08 3.18 ± 0.10 85
352 ± 1 + 39 ± 6 14.25662 ± 0.00003 0.012 70 ± 2 0.24 40 ± 30 1.10 3.18 ± 0.10 95

(202) Chryseis 94 ± 1 − 49 ± 4 23.67025 ± 0.00006 0.012 0.22 <180 0.35 2.96 ± 0.15 <405
261 ± 1 − 34 ± 4 23.67028 ± 0.00004 0.012 0.22 <180 0.36 2.96 ± 0.15 <405

(219) Thusnelda 300 ± 10 − 66 ± 10 59.7105 ± 0.0001 0.014 0.19 <120 0.80 2.24 ± 0.42 <220

(223) Rosa 22 ± 3 + 18 ± 18 20.2772 ± 0.0003 0.012 0.033 <300 0.72 2.99 ± 0.12 <680
203 ± 2 + 26 ± 15 20.2769 ± 0.0003 0.012 0.032 <300 0.78 2.99 ± 0.12 <680

(362) Havnia 14 ± 2 + 33 ± 2 16.92665 ± 0.00003 0.017 0.044 <180 0.80 2.64 ± 0.04 <370
208 ± 8 + 35 ± 4 16.92668 ± 0.00003 0.017 0.046 <200 0.67 2.64 ± 0.04 <410

(478) Tergeste 2 ± 5 − 38 ± 8 16.10308 ± 0.00004 0.019 83 ± 4 0.16 2 0.94 3.05 ± 0.10 5
216 ± 7 − 62 ± 4 16.10312 ± 0.00004 0.016 0.18 26 ± 25 0.88 3.05 ± 0.10 60

(483) Seppina 127 ± 3 + 47 ± 3 12.720968 ± 0.000004 0.019 0.16 17 0.80 3.45 ± 0.14 45
356 ± 4 + 60 ± 3 12.720977 ± 0.000002 0.019 0.16 23 0.83 3.45 ± 0.14 60

(501) Urhixidur 49 ± 40 + 84 ± 12 13.17203 ± 0.00002 0.019 0.051 4 0.53 3.20 ± 0.32 10
262 ± 24 + 66 ± 11 13.17203 ± 0.00001 0.018 0.050 13 0.53 3.20 ± 0.32 31

(537) Pauly 32 ± 3 + 43 ± 6 16.29601 ± 0.00002 0.018 0.26 11 0.70 2.96 ± 0.45 25
214 ± 4 + 60 ± 9 16.29597 ± 0.00001 0.018 46 ± 2 0.25 13 0.74 2.96 ± 0.45 29

(552) Sigelinde 8 ± 24 + 73 ± 9 17.14963 ± 0.00001 0.017 0.030 3 0.97 3.26 ± 0.09 7
189 ± 18 + 60 ± 17 17.14962 ± 0.00003 0.017 0.029 2 1.13 3.26 ± 0.09 5

(618) Elfriede 102 ± 20 + 64 ± 7 14.79565 ± 0.00002 0.015 0.047 <350 0.28 3.32 ± 0.10 <860
341 ± 13 + 49 ± 6 14.79564 ± 0.00002 0.015 0.053 <400 0.32 3.32 ± 0.10 <980

(666) Desdemona 10 ± 4 + 39 ± 5 14.60795 ± 0.00008 0.022 0.111 <70 0.83 2.79 ± 0.34 <150
174 ± 3 + 36 ± 11 14.60796 ± 0.00003 0.022 0.116 <100 0.77 2.79 ± 0.34 <215

(667) Denise 15 ± 25 − 83 ± 6 12.68499 ± 0.00003 0.024 0.051 ± 3 13 1.19 3.36 ± 0.38 32
237 ± 3 −23 ± 6 12.68497 ± 0.00003 0.025 0.051 6 1.16 3.36 ± 0.38 15

(780) Armenia 144 ± 7 − 44 ± 11 19.88453 ± 0.00007 0.014 0.042 <300 0.47 3.00 ± 0.10 <680
293 ± 3 − 23 ± 6 19.88462 ± 0.00009 0.015 0.038 ± 0.003 <250 0.63 3.00 ± 0.10 <570

(923) Herluga 218 ± 9 − 68 ± 5 29.72820 ± 0.00002 0.022 0.047 37 0.92 2.73 ± 0.40 80
334 ± 7 − 52 ± 3 29.72826 ± 0.00001 0.023 0.050 14 0.95 2.73 ± 0.40 30

(995) Sternberga 27 ± 3 − 20 ± 6 11.19511 ± 0.00012 0.019 0.22 <100 0.85 2.73 ± 0.30 <210
222 ± 4 − 26 ± 5 11.19512 ± 0.00008 0.019 0.226 <120 0.84 2.73 ± 0.30 <250

Notes. The columns contain asteroid name, J2000 ecliptic coordinates λp, βp of the spin solution, with mirror pole solution in the second row, sidereal rotation period P, and the deviation of model fit to those light curves (including fit to sparse data). The next part of the table details the radiometric solution for combined data: surface-equivalent size D, geometric albedo pV, thermal inertia Γ in J m−2 s−1∕2 K−1 (SI) units, and the reduced chi-square of the best-fit (). The last two columns give average heliocentric distance of thermal infrared observations rhel with the standard deviation, and thermal inertia normalised to 1 AU ΓAU calculated according to Eq. (1). Numbers in italics mark the pole solution of (667) Denise clearly rejected by occultation fitting.

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