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Table 2:

Determinations of the geometric albedo of 21 Lutetia.

Author 		Method Albedo
Tedesco & Veeder (1992) Thermal 0.221 $\pm$ 0.02
Zellner & Gradie (1976) Pol. (h) 0.10
Lupishko & Mohamed (1996) Pol. 0.10
Magri et al. (1999) Radar 0.19 $\pm$ 0.07
Mueller et al. (2006) Thermal 0.208 $\pm$ 0.025
Gil-Hutton (2007) Pol. ( $P_{\rm min}$) 0.11 $\pm$ 0.01
Gil-Hutton (2007) Pol. (h) 0.20 $\pm$ 0.04
Carvano et al. (2008) Thermal 0.13 $\pm$ 0.03
Shepard et al. (2008) Radio 0.24 $\pm$ 0.07
Weaver et al. (2010) Vis + 3D model 0.16 $\pm$ 0.02
Belskaya et al. (2010) Pol. (h) 0.13/0.16 $\pm$ 0.02*
This work Vis + 3D model 0.18 $\pm$ 0.02

Notes. * $p_{V} = 0.13 \pm 0.02$ when using the calibration based on albedos of meteorites (Zellner & Gradie 1976) and pV = 0.16 $\pm$ 0.02 when using the calibration based on IRAS albedos (Cellino et al. 1999).


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