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Table 1

Number of dense light curves Nlc, sparse data points Nsp, and IRAS and WISE observations.

Asteroid N lc N sp IRAS WISE reduced
12 μm 25 μm 60 μm 100 μm 11 μm 22 μm

21 Lutetiaa 59 5 5 5 9 0.80
220 Stephania 397 2 2 2 11 11 0.58
306 Unitas 15 386 11 11 11 10 13 0.68
2867 Šteins 21 614 12 12 0.77

Notes. The goodness of fit to the thermal data is expressed by the reduced .

(a)

For Lutetia, we did not use sparse data because 20 of the set of 59 dense light curves were calibrated. The IR data set also contained data from the Spitzer and Herschel telescopes.

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