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/本数据集关联于arXiv预印本https://arxiv.org/abs/2401.13525，主题为《基于SPT-3G的非靶向毫米波巡天（Non-targeted mm-wave Survey）中的耀变恒星（Flaring Stars）》。 本数据集收录了2019年至2022年间由南极望远镜（South Pole Telescope，SPT）探测到的耀变恒星的光变曲线（lightcurves），包含两类数据：覆盖四年时长的单次观测长采样周期（long cadence）光变曲线，以及耀变峰值时段内单次扫描的短采样周期（short cadence）约30分钟光变曲线。 SPT-3G是南极望远镜的第三代成像相机，工作在中心频率为95 GHz、150 GHz与220 GHz的三个波段。其主要观测天区覆盖1500平方度的天空区域，赤经（right ascension）范围为20h40m0s至3h20m0s，赤纬（declination）范围为-42°至-70°。 本数据集的完整说明与配套星表可通过链接https://pole.uchicago.edu/public/data/tandoi24/ 获取。