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Wayne State University's Dan Zowada Memorial Observatory is a fully robotic0.5m telescope and imaging system located under the dark skies of New Mexico.The observatory is particularly suited to time domain astronomy: theobservation of variable objects, such as tidal disruption events, supernovae,and active galactic nuclei. We have developed a software suite for imagereduction, alignment and stacking, and calculation of absolute photometry inthe Sloan filters used at the telescope. Our pipeline also performs imagesubtraction to enable photometry of objects embedded in bright backgrounds suchas galaxies. The 5 sigma detection limit of the Zowada Observatory forintegration of 16 x 90 second exposures is 19.0 magnitude in g-band, 18.1magnitude in r-band, 17.9 magnitude in i-band, and 16.6 magnitude in z-band.For a 3 sigma detection limit, measurements may be performed with greateruncertainties as deep as 19.9, 19.1. 18.9 and 17.5 magnitude in griz bands,respectively.

Wayne State Universitys Dan Zowada Memorial Observatory: Characterization and Pipeline of a 0.5 Meter Robotic Telescope