The variable star (Zayed-V3) was discovered in the constellation called (Camelopardalis), it is of the type of DSCT, the spectral type of the star is A0, and the Mag. range is 8.27 V (Johnson V) by TESS .and shows variations in its brightness period 64.92 minutes.
Sallam explained that the stars were photographed using an Astronomical Observatory with a diameter of 0.6 meters, using a specialized astronomical camera at a cooling temperature of minus 30 degrees Celsius, an optical filter (Johnson V) and an optical filter (Sloan r) to provide accurate optical readings of the observed stars in order to be able to complete The process of discovery, registration and official recognition.
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