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数据集来搜索喷发变量，特别是FU Orionis。同时，我还使用UKIRT测光数据在J，H和K波段的白色矮星，这是采取了多个时代，以寻找红外线变化周围的白色矮星。这可能有助于确定30%的白色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色矮星在光学和近红外波长上的变化。

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.