  The Transiting Exoplanet Survey Satellite (TESS) is the first high-precision
full-sky photometry survey in space. We present light curves from a magnitude
limited set of stars and other stationary luminous objects from the TESS Full
Frame Images, as reduced by the MIT Quick Look Pipeline (QLP). Our light curves
cover 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 Northern
ecliptic hemispheres, respectively. We describe the photometry and detrending
techniques we used to create the light curves, and compare the noise properties
with theoretical expectations. All of the QLP light curves are available at
MAST 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 TESS
photometry available to the public to date.
