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The Transiting Exoplanet Survey Satellite (TESS) is the first high-precisionfull-sky photometry survey in space. We present light curves from a magnitudelimited set of stars and other stationary luminous objects from the TESS FullFrame Images, as reduced by the MIT Quick Look Pipeline (QLP). Our light curvescover the full two-year TESS Primary Mission and include $\sim$ 14,770,000 and$\sim$ 9,600,000 individual light curve segments in the Southern and Northernecliptic hemispheres, respectively. We describe the photometry and detrendingtechniques we used to create the light curves, and compare the noise propertieswith theoretical expectations. All of the QLP light curves are available atMAST as a High Level Science Product via doi.org/10.17909/t9-r086-e880(https://archive.stsci.edu/hlsp/qlp). This is the largest collection of TESSphotometry available to the public to date.

Photometry of 10 Million Stars from the First Two Years of TESS Full Frame Images