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Table 2
Comparison between our CITPM models and independent results.
| Asteroid | λ | β | D | pV | Γ | References | ||
| [deg] | [deg] | [km] | J m-2 s-0.5 K-1 | |||||
|
|
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| 21 | Lutetia | 56 | − 7 | 101 ± 4 | 0.19–0.23 | 30–60 | CITPM (3σ errors) | |
| 52.2 ± 0.4 | − 7.8 ± 0.4 | 98 ± 2 | 0.19 ± 0.01 | Sierks et al. (2011) | ||||
| 95.97 | <10 | O’Rourke et al. (2012) | ||||||
| <30 | Keihm et al. (2012) | |||||||
| 98.3 ± 5.9 | 0.208 ± 0.025 | <100 | Mueller et al. (2006) | |||||
|
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| 220 | Stephania | 24 (or 224) | − 60 (or − 59) | 32–34 | 0.075 ± 0.015 | 5–75 | CITPM | |
| 26 (or 223) | − 50 (or − 62) | Hanuš et al. (2013b) | ||||||
| 31.738 ± 0.219 | 0.069 ± 0.016 | Masiero et al. (2014) | ||||||
|
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| 306 | Unitas | 82 | − 30 | 48.7 ± 0.7 | 0.21–0.27 | 10–100 | CITPM | |
| 79 | − 35 | 49 ± 5 | Ďurech et al. (2007, 2011) | |||||
| 55–56 | 0.14–0.15 | 100–260 | Delbo & Tanga (2009) | |||||
| 47.2 ± 0.13 | 0.201 ± 0.013 | Masiero et al. (2014) | ||||||
|
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| 2867 | Šteins | 142 | − 83 | 5.6–6.2 | 0.4–0.5 | 70–370 | CITPM | |
| 94 | − 85 ± 5 | 5.26 ± 0.26 | Jorda et al. (2012) | |||||
| 0.39 ± 0.02 | Spjuth et al. (2012) | |||||||
| 210 ± 30 | Leyrat et al. (2011) | |||||||
Notes. The physical parameters are the ecliptic longitude λ and latitude β of the spin axis direction, the volume-equivalent diameter D, the geometric albedo pV, and the thermal inertia of the surface Γ.
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