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We present preliminary diameters and albedos for 13511 MBAs that wereobserved during the 3-Band Cryo phase of the WISE survey (after the outercryogen tank was exhausted) and as part of the NEOWISE Post-Cryo Survey (afterthe inner cryogen tank was exhausted). With a reduced or complete loss ofsensitivity in the two long wavelength channels of WISE, the uncertainty in ourfitted diameters and albedos is increased to ~20% for diameter and ~40% foralbedo. Diameter fits using only the 3.4 and 4.6 um channels are shown to bedependent on the literature optical H absolute magnitudes. These data allow usto increase the number of size estimates for large MBAs which have beenidentified as members of dynamical families. We present thermal fits for 14asteroids previously identified as the parents of a dynamical family that werenot observed during the fully cryogenic mission.

Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-Cryogenic Observations of Main Belt Asteroids