Variable stars in the SuperWASP all sky survey

SuperWASP全天空测光巡天（Pollecht et al. 2006）是最成功的凌日系外行星地面搜索，发现了超过150个热彗星。在10年的运行中，它还产生了超过3000万个高节奏光变曲线的档案，包括超过5000亿个明亮恒星的单独测量。近年来，我们已经利用这个光度档案来解决恒星演化的各个方面，重点是食双星和恒星多样性（Lohr et al. 2012; 2013 a; 2013 b; 2014 a; 2014 b; 2015 a; 2015 b）和恒星脉动（Norton et al. 2016; Holdsworth et al. 2014; Smalley et al. 2011; 2017，Greer et al. 2017）。

The SuperWASP all sky photometric survey (Pollacco et al. 2006) is the most successful ground-based search for transiting exoplanets, having discovered >150 hot Jupiters. In 10 years of operation, it has also produced an archive of more than 30 million high cadence lightcurves comprising over 500 billion individual measurements of bright stars. In recent years we have exploited this photometric archive to address aspects of stellar evolution, focussing on eclipsing binaries and stellar multiplicity (Lohr et al. 2012; 2013a; 2013b; 2014a; 2014b; 2015a; 2015b) and on stellar pulsations (Norton et al. 2016; Holdsworth et al. 2014; Smalley et al. 2011; 2017, Greer et al. 2017).