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The Transient Optical Sky Survey (TOSS) is an automated, ground-basedtelescope system dedicated to searching for optical transient events. Smalltelescope tubes are mounted on a tracking, semi-equatorial frame with a singlepolar axis. Each fixed declination telescope records successive exposures whichoverlap in right ascension. Nightly observations produce time-series images offixed fields within each declination band. We describe the TOSS data pipeline,including automated routines used for image calibration, object detection andidentification, astrometry, and differential photometry. Time series of nightlyobservations are accumulated in a database for each declination band. Despitethe modest cost of the mechanical system, results from the 2009-2010 observingcampaign confirm the system's capability for producing light curves ofsatisfactory accuracy. Transients can be extracted from the individualtime-series by identifying deviations from baseline variability.

The Transient Optical Sky Survey Data Pipeline