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 ∼14,770,000 and ∼9,600,000 individual light curve segments in the Southern and Northern ecliptic hemispheres, respectively. We describe the 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 (HLSP) via doi: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.

我们展示了来自TESS全帧图像的数量有限的恒星和其他静止发光物体的光曲线，该曲线通过MIT快速查看管道（QLP）得以简化。我们的光照曲线涵盖了整个TESS的为期两年的整个任务，并且分别包括在南，北黄道半球的约14,770,000和约9,600,000个单独的光照曲线段。我们描述了用于创建光曲线的去趋势技术，并将噪声特性与理论预期进行了比较。所有QLP光曲线均可通过doi：10.17909 / t9-r086-e880（https://archive.stsci.edu/hlsp/qlp）在MAST上以高水平科学产品（HLSP）的形式获得。这是迄今为止向公众提供的最大的TESS光度法收藏。