An All Sky Cirrus Confusion Noise Map for WIRE

The Wide Field Infrared Explorer (WIRE) is an infrared space observatory being developed inder NASA's small explorer program for launch inlate 1998 (Schember, et al. 1996). WIRE's main function will be to produce a sky survey at wavelengths of 12 and 25(micro), covering several tens of square degrees at a sensitivity of 0.2mJy, 5(standard deviation)at 25(micro)m, and several hundred square degrees at a sensitivity of 0.7 mJy, 5(standard deviation) at 25(micro)m to study starburst galaxies and search for luminous protogalaxies.