SPT-3G 2019-2022 flaring star lightcurves

Associated data with https://arxiv.org/abs/2401.13525: Flaring Stars in a Non-targeted mm-wave Survey with SPT-3G

We present lightcurves of flaring stars detected by the South Pole Telescope (SPT) from 2019 through 2022. There are two datasets: four year lightcurves of single-observation (long cadence) data as well as ~30 minute lightcurves of single-scan (short cadence) data during flaring peaks. SPT-3G is the third generation camera on the SPT, and observes at three bands centered at 95, 150, and 220 GHz. The main SPT-3G observing field covers a 1500-square-degree region of the sky from 20h40m0s to 3h20m0s in right ascension and -42 to -70 degrees in declination.

A full description of the data, and associated catalog, can be found at https://pole.uchicago.edu/public/data/tandoi24/