Catalogue of ISO LWS observations of asteroids | Astronomy & Astrophysics (A&A)

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Table 4:

Object specific TPM input parameters. The $\lambda _{\rm ecl}$ and $\beta _{\rm ecl}$ values are the ecliptic coordinates of the spin vector direction, with $\beta _{\rm ecl}$ counted from the equator.
Object	[H, G]	$P_{\rm sid}$ [h]	$\lambda _{\rm ecl}$ , $\beta _{\rm ecl}$	Source of shape & spin vector
(1) Ceres	[3.28, 0.05]¹	9.074184	331.51 $^\circ$ , +77.88 $^\circ$	HST observations⁴
(2) Pallas	[4.13, 0.16]²	7.813225	34.80 $^\circ$ , -11.75 $^\circ$	Lightcurve inversion techniques^5,6
(4) Vesta	[3.20, 0.34]³	5.342129	319.45 $^\circ$ , +59.23 $^\circ$	HST observations⁷
(10) Hygiea	[5.43, 0.07]²	27.623265	117.01 $^\circ$ , -28.53 $^\circ$	Lightcurve inversion techniques⁸

¹ Lagerkvist et al. (1992); ² Lagerkvist et al. (2001); ³ Müller & Lagerros (1998); ⁴ Thomas et al. (2005); ⁵ M. Kaasalainen, priv. comm. 22/Sep./2005; ⁶ Torppa et al. (2003); ⁷ Thomas et al. (1997); ⁸ M. Kaasalainen, priv. comm. 31/Jan./2006;

Source LaTeX | All tables | In the text

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