  We present the first evidence for the binarity of four targets in the TESS
field. The temperatures are estimated by SED analysis and the orbital periods
are determined. The TESS light curves of the systems are analysed and the
orbital and the absolute parameters are derived. The targets are also compared
to well-studied binary systems with the same morphological type and their
evolutionary states are discussed. Our results indicate that the stars belong
to the class of eclipsing detached binary systems.
