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We present ugriz light curves for 146 spectroscopically confirmed orspectroscopically probable Type Ia supernovae from the 2005 season of theSDSS-II Supernova survey. The light curves have been constructed using aphotometric technique that we call scene modelling, which is described indetail here; the major feature is that supernova brightnesses are extractedfrom a stack of images without spatial resampling or convolution of the imagedata. This procedure produces accurate photometry along with accurate estimatesof the statistical uncertainty, and can be used to derive photometry taken withmultiple telescopes. We discuss various tests of this technique thatdemonstrate its capabilities. We also describe the methodology used for thecalibration of the photometry, and present calibrated magnitudes and fluxes forall of the spectroscopic SNe Ia from the 2005 season.

The Sloan Digital Sky Survey-II: Photometry and Supernova Ia Light Curves from the 2005 data