Short and Long-term Observations of X-ray Binaries with Neutron Star Components

New long and short-term photometric variations of the selected high-mass (HMXB) and low-mass (LMXB) X-ray binaries with neutron star components are studied in this study. We obtained new observations of the systems during 2015-2021 with B, V, R and I filters at TUBITAK National Observatory (TUG) with 60cm and 100cm telescopes. We analyzed the new observation sets, we obtained by combining all available datasets in the literature. In addition to optical datasets, observations obtained with X-ray telescopes were also used in the analysis. Using these datasets, we got new periods for selected binary systems and multiple periods for some systems.