Welcome
My research is focused on galaxy evolution and in particular within their halo. Due to the low surface brighntess nature of these regions, this inevitably involves methods to improve the scientific productivity of the data reduction in optical astronomical imaging (so that diffuse signal is not lost during the data processing). With the introduction of the telescope, astronomers have not been using their naked eyes for their professional research any more. Since the introduction of digital detectors and the high processing power of modern computers, today we actually "see" (detect/measure) astrophysical sources through an added "filter" of software, not directly through telescopes any more. Therefore, research in the evolution of galaxies inevitably entails deep involvement in the software that practically define your results.