These are the simulated lightcurves for a synthetic sample of short-cadence solar-like oscillators as they might be observed by the Transiting Exoplanet Survey Satellite (TESS), as presented by Ball et al. (2018), "A synthetic sample of short-cadence solar-like oscillators for TESS". Each zip file contains the FITS lightcurves and mode data for stars observed in one sector, starting in the southern ecliptic hemisphere. The CSV file contains a selection of data contained in the FITS headers. For more detail, read the paper on arXiv. Note that the FITS headers incorrectly report the units of the white noise level as \(\mathrm{ppm}\) rather than \(\mathrm{ppm}\cdot\mathrm{hr}^{1/2}\). The white noise level excludes any systematic component, which should be added in quadrature if desired.