Variability of Stellar Sources

我的项目集中在恒星源的可变性上。我目前正在使用GAIA DR1和2MASS数据集来搜索爆发变量，特别是猎户座FU。同时，我还使用了UKIRT在白矮星的J， H和K波段的光度数据，这些数据被采集了多个时代，以搜索白矮星周围的红外变异性。这有助于确定30%的白矮星是如何被金属污染的。从长远来看，我将继续寻找并试图了解白矮星在光学和近红外波长上的变异性。

My project is focused on the variability of stellar sources. I am currently using the GAIA DR1 and 2MASS data sets to search for eruptive variables, specifically FU Orionis. In conjunction I am also using UKIRT photometric data in the J, H and K bands of white dwarfs which was taken over multiple epochs to search for infrared variability around the white dwarfs. This could help to identify how 30% of white dwarfs become polluted with metals. Long term, I will continue to search for and try to understand the variability of white dwarfs in both optical and near-infrared wavelengths.