Bakis, V.Eker, Z.Soydugan, F.Bilir, S.2026-02-032026-02-0320251335-18421336-0337https://doi.org/10.31577/caosp.2025.55.3.234https://hdl.handle.net/20.500.12428/34521In this study, we investigated the interrelated mass-luminosity, mass-radius, and mass-temperature relations of planet-hosting stars. The sample, which is chosen to be main-sequence systems, is divided into two metallicity regimes: one regime is below the average of all samples (z=0.017) and the other above it. Suitable figures represent the comparisons of each distinct metallicity regime.eninfo:eu-repo/semantics/openAccessstars:fundamental parametersstars:host starsArticle55323423710.31577/caosp.2025.55.3.234Q4WOS:0015091364000192-s2.0-105005874005Q4