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We describe our custom processing of the entire Wide-field Infrared SurveyExplorer (WISE) 12 micron imaging data set, and present a high-resolution,full-sky map of diffuse Galactic dust emission that is free of compact sourcesand other contaminating artifacts. The principal distinctions between ourresulting co-added images and the WISE Atlas stacks are our removal of compactsources, including their associated electronic and optical artifacts, and ourpreservation of spatial modes larger than 1.5 degrees. We provide access to theresulting full-sky map via a set of 430 12.5 degree by 12.5 degree mosaics.These stacks have been smoothed to 15" resolution and are accompanied bycorresponding coverage maps, artifact images, and bit-masks for point sources,resolved compact sources, and other defects. When combined appropriately withother mid-infrared and far-infrared data sets, we expect our WISE 12 micronco-adds to form the basis for a full-sky dust extinction map with angularresolution several times better than Schlegel et al. (1998).

A Full-sky, High-resolution Atlas of Galactic 12 micron Dust Emission with WISE