Properties of slowly rotating asteroids from the Convex Inversion Thermophysical Model

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Table 4

Previously published spin parameters for targets studied here.

Asteroid	Pole		P	Reference
			[h]
(108) Hecuba	79 ± 1	+13 ± 11	–	Blanco & Riccioli (1998)
	259 ± 7	−6 ± 7	–	Blanco & Riccioli (1998)

(219) Thusnelda	253 ± 4	− 69 ± 4	59.712 ± 0.002	Ďurech et al. (2020)

(362) Havnia	96		16.918773	Wang et al. (2015)
	273		16.918935	Wang et al. (2015)

(478) Tergeste	2 ± 2	− 42 ± 3	16.10308 ± 0.00003	Marciniak et al. (2018)
	216 ± 6	− 56 ± 4	16.10308 ± 0.00003	Marciniak et al. (2018)

(483) Seppina	–	+ 42 ± 20	12.72081 ± 0.00006	Ďurech et al. (2020)

(537) Pauly	290 ± 31	+ 40 ± 31	–	Blanco et al. (2000)
	31 ± 12	+ 32 ± 10	16.2961 ± 0.0005	Hanuš et al. (2016)
	211 ± 16	+ 51 ± 10	16.2961 ± 0.0005	Hanuš et al. (2016)

(552) Sigelinde	–	+ 48 ± 19	17.1494 ± 0.0002	Ďurech et al. (2020)

(618) Elfriede	113 ± 3	+ 54 ± 3	14.7952 ± 0.0001	Ďurech et al. (2020)
	323 ± 1	+25 ± 3	14.7952 ± 0.0001	Ďurech et al. (2020)

(666) Desdemona	–	+ 12 ± 22	14.6080 ± 0.0002	Ďurech et al. (2020)

(667) Denise	40 ± 6	− 86 ± 3	12.6848 ± 0.0002	Ďurech et al. (2020)

(923) Herluga	188 ± 5	− 60 ± 5	29.7282 ± 0.0007	Ďurech et al. (2020)

Notes. The columns contain asteroid name, J2000ecliptic coordinates λ_p, β_p of the spin solution, sidereal rotation period P, and the reference. Values in italics denote solutions substantially differing from the ones obtained in the current paper.

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