Asteroids’ physical models from combined dense and sparse photometry and scaling of the YORP effect by the observed obliquity distribution

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Volume 551 (March 2013)

A&A, 551 (2013) A67

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Table 2

List of new asteroid models derived from the Catalina Sky Survey data alone.

Asteroid		λ₁	β₁	λ₂	β₂	P	N₇₀₃	P_publ	Period reference
		[deg]	[deg]	[deg]	[deg]	[h]		[h]

2112	Ulyanov	156	48	334	65	3.04071	118	3.000	Maleszewski & Clark (2004)
2384	Schulhof	196	−60	45	−42	3.29367	121	3.294	Ditteon et al. (2002)
2617	Jiangxi	224	76	1	54	11.7730	124	11.79	Carbo et al. (2009)
3170	Dzhanibekov	217	60	21	64	6.07168	105	6.0724	Molnar et al. (2008)
4507	1990 FV	143	55	323	49	6.57933	84	6.58	Yoshida et al. (2005)
5647	1990 TZ	253	77	119	−19	6.13867	87	6.144	Bembrick & Bolt (2003)
10826	1993 SK₁₆	260	−56	60	−34	13.8327	90	13.835	Galad (2008)
19848	Yeungchuchiu	190	−68			3.45104	104	3.450	Yeung (2006)
3097	Tacitus	229	71	72	62	8.7759	99
4611	Vulkaneifel	5	−86	197	−50	3.75635	148
5461	Autumn	249	−26	79	−43	20.0929	106
5625	1991 AO₂	265	−52	97	−78	6.67411	110
5960	Wakkanai	226	−69	69	−61	4.96286	102
7201	Kuritariku	22	67	249	64	48.849	103
7632	Stanislav	234	−50	46	−45	5.29073	99
7905	Juzoitami	105	−76	226	−55	2.72744	118
13002	1982 BJ₁₃	58	−50	245	−57	3.13844	110
16009	1999 CM₈	283	44			8.3476	124
16847	Sanpoloamosciano	91	−24			8.1845	114
26792	1975 LY	226	68			79.15	140

Notes.For each asteroid, the table gives the ecliptic coordinates λ₁ and β₁ of the pole solution, the corresponding mirror solution λ₂ and β₂, the sidereal rotational period P, the number of sparse data points from the CSS N₇₀₃, and the previously published period value P_publ with the reference. The uncertainty of the sidereal rotational period corresponds to the last decimal place of P and of the pole direction to 20–40°.

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