Create appropriate LSST PhoSim data to use for an example of processing such data. The dataset need not be large in spatial extent (perhaps a raft, or even a single CCD), but should include the following properties:

• single area of sky (though with arbitrary rotation), consistent with selected FPA spatial extent
• at least 3 passbands
• Reasonable spread in brightness (saturation limit, down to single-visit depth)
• include stars with representative colors; including galaxies is optional
• span a reasonable range in time (perhaps a year)

The above properties would result in a dataset that could be used to illustrate a variety of processing and visualization demonstrations.

It may be possible to use an existing lsstSim dataset (even if not all of the above criteria are met), and a published catalog to begin building the demonstration.