Table A.1
Volume-equivalent diameter estimates of (6) Hebe gathered from the literature.
| Diameter (D, km) | Method | Reference | ||
|
|
||||
| 1 | 215.00 ± 21.50 | STM | Morrison (1974) | |
| 2 | 201.00 ± 20 × 10 | STM | Morrison (1977) | |
| 3 | 186.00 ± 9.00 | Occ | Taylor & Dunham (1978) | |
| 4 | 190.40 ± 7 × 10 | Occ | Dunham & Mallen (1979) | |
| 5 | 185.18 ± 2.90 | STM | Tedesco et al. (2004) | |
| 6 | 180.42 ± 8.50 | STM | Ryan & Woodward (2010) | |
| 7 | 214.49 ± 10.25 | NEATM | Ryan & Woodward (2010) | |
| 8 | 180.00 ± 40.00 | LC+Occ | Durech et al. (2011) | |
| 10 | 197.14 ± 1.83 | STM | Usui et al. (2011) | |
| 11 | 185.00 ± 10.68 | NEATM | Masiero et al. (2011) | |
| 12 | 165.00 ± 21.00 | LC+AO | Hanuš et al. (2013) | |
| 13 | 195.64 ± 5.44 | NEATM | Masiero et al. (2014) | |
|
|
||||
| 191.5 ± 8.3 | Mean value∗ | |||
| 193 ± 6 | ADAM (SPHERE only) | This paper | ||
| 196 ± 6 | ADAM (all AO) | This paper | ||
| 198 ± 4/2 | TPM | This paper | ||
Notes. STM: Standard Thermal Model, NEATM: Near-Earth Asteroid Thermal Model, LC: light curve, Occ: stellar occultation, AO: adaptative optics imaging, LC+Occ: light curve-based 3-D model scaled using an occultation, LC+AO: light curve-based 3D model scaled using adaptative optics images.
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