The code for two sessions of demos are in:
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Lightcurves -- Examining a set of variable star, supernova, and AGN light curves sampled at the LSST cadence and with realistic LSST uncertainties.
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ProcessCcd -- Using the LSST stack to process one DECam image to obtain a calibrated image and a catalog of detected objects.
Slides for the talk "Getting Started with LSST" by Jonathan Sick are available at https://doi.org/10.5281/zenodo.200418.