All Tables

Table 1: Observing geometry and modeling assumptions (H and G are from Tedesco 1992).
Table 2: Observations of 21 Lutetia. Times are those of mid exposure on June 24, 2004 and are not light-time corrected. Filter "V'' denotes an Apogee measurement; numbers denote the central wavelength (in $\mu$ m) of the MIRSI filter used.
Table 3: NEATM fits to the available thermal-infrared data: the MIRSI data as given in Table 2, and the five IRAS sightings (Tedesco 1992). No attempt at lightcurve-correction was made.
Table 4: NEATM diameters and albedos of Lutetia for the two data sets.
Table 5: Summary of diameter and albedo determinations for Lutetia. Values in parentheses are calculated by the authors on the basis of Eq. (3) and H=7.35. NEATM results are quoted with 15 and 30% uncertainty in diameter and albedo, respectively; TPM results with 10% uncertainty in diameter and 20% uncertainty in albedo (see Sects. 3.2.2 and 3.3.2).