  Automated asteroid detection routines set requirements on the number of
detections, signal-to-noise ratio, and the linearity of the expected motion in
order to balance completeness, reliability, and time delay after data
acquisition when identifying moving object tracklets. However, when the
full-frame data from a survey are archived, they can be searched later for
asteroids that were below the initial detection thresholds. We have conducted
such a search of the first three years of the reactivated NEOWISE data, looking
for near-Earth objects discovered by ground-based surveys that have previously
unreported thermal infrared data. Using these measurements, we can then perform
thermal modeling to measure the diameters and albedos of these objects. We
present new physical properties for 116 Near-Earth Objects found in this
search.
