The Transiting Exoplanet Survey Satellite (TESS) will observe ~150~million stars brighter than T=16, with a photometric precision from 60~ppm to 3 percent, enabling an array of exoplanet and stellar astrophysics investigations. While NASA will provide light curves for ~400,000 targets observed at 2-min cadence, observations of most stars will only be provided as full-frame images (FFIs) at 30~min cadence. We have reduced the first two sectors of these FFIs, and present light curves for 13.8 million stars for community use. Additionally, we provide variability and periodicity metrics for more than 2.2 million stars through the Filtergraph data visualization portal. I will provide a brief description of the reduction, and a short tutorial of the public data release on Filtergraph.