Preparing and correcting extracted BRITE observations
  Extracted BRITE lightcurves must be carefully prepared and corrected for instrumental effects before a scientific analysis can be performed. Therefore, we have created a suite of Python routines to prepare and correct the lightcurves, which is publicly available. In this paper we describe the method and successive steps performed by these routines. 
B. Buysschaert, H. Pablo, and C. Neiner
astro-ph.SR