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The Spacewatch Project1 (McMillan et al. 2007) uses ground-based optical telescopes to detect Near-Earth Objects (NEOs) to faint limiting magnitudes, and specializes in following up NEOs as they recede from Earth and get fainter after discovery. Followup tracking is needed to consolidate knowledge of the orbits of NEOs during their discovery apparitions because return apparitions can be several years away, and survey programs can not always revisit their own discoveries. Spacewatch is being groomed for quick response to the needs of upcoming missions that will discover NEOs in unprecedented numbers. Potential improvements range from relatively inexpensive upgrades of electronics and software to more ambitious new detectors, new optics, and use of larger telescopes. Telescopes available to Spacewatch on Kitt Peak mountain in Arizona range from 0.9-meter to 4-meters in diameter, capable of recovering 140-meter diameter NEOs as far away as an Astronomical Unit. Formal agreements between Spacewatch and the Wide-field Infrared Survey Explorer (WISE) mission and between Spacewatch and the Panoramic Survey Telescope and Rapid Response System (Pan-STARRS) attest to those projects ' needs for Spacewatch services