@article{article_723779, title={Photometric solutions for three eclipsing binary systems: SY Sge, V688 Aql, and CY Ari}, journal={Turkish Journal of Astronomy and Astrophysics}, volume={1}, pages={1–7}, year={2020}, author={Gökay, H.gökhan and Öztürk Çetni, Derya and Terzioğlu, Zahide and Özdemir, Sacit and Çoker, Deniz and Garner, Ceren}, keywords={eclipsing binaries, fundamental parameters, photometry}, abstract={<p> <span style="font-size:12px;">We present a detailed light curve analysis of three eclipsing binaries, consisted of two Algol type systems, SY Sge and V688 </span> <span style="font-size:12px;">Aql, and one W UMa type system, CY Ari, observed at the Ankara University Observatory. The light curves constructed  </span> <span style="font-size:12px;">in Johnson BVRI pass-bands were simultaneously analysed on the basis of Roche Geometry. Fourier coefficients method </span> <span style="font-size:12px;">was applied on the light curve of W UMa type system to estimate a set of initial system parameters. Moreover, since  </span> <span style="font-size:12px;">there is not any radial velocity measurement of the systems, a q-search test was applied for all three systems to reach a </span> <span style="font-size:12px;">minimized $\chi^2$. Combining system parameters with photometric mass ratio allows us to obtain absolute parameters of the  </span> <span style="font-size:12px;">systems which leads to locate the systems on theoretical HR diagram and to estimate their evolutionary status. </span> </p>}, number={3}, publisher={Türk Astronomi Derneği}