All Tables

• Table 1: Log of photometric observations of IU Aur. Johnson UBVand BVR filters were used at Ankara University Observatory (AUO) and at Çanakkale Onsekiz Mart University Observatory (ÇOMUO), respectively.
• Table 2: New minimum times of IU Aur observed at AUO and ÇOMUO. Secondary minimum was not used in calculation of third body orbit.
• Table 3: Simultaneous MORO solution of the UBV light curves of the eclipsing system IU Aur; for comparison, a previous solution is also presented in the third column.
• Table 4: Third-body orbital parameters.
• Table 5: Absolute dimensions of IU Aur according to the new photometric solution of Table 3.