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Fig. B.17


Asteroid (538) Friederike. From top to bottom: observation to model ratios versus wavelength, heliocentric distance, rotational phase, and phase angle for model AM 1 (the AM 2 model on all data did not provide an acceptable fit and was rejected). Right: χ2 versus thermal inertia curves for model AM1 (top), and AM2 (bottom) using WISE W3 and W4 data only.

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