Abstract
We present times of minima for an eclipsing binary V405 Dra of EW type. We used the MAVKA software to derive times of minima from observations conducted by one of the authors (Pyatnytskyy) (18 minima), from TESS data (816 minima), and from ASAS-SN, SuperWASP, and NSVS observations (15 minima). The O-C diagram built using the mentioned times of minima shows a complex period variation in the system.
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