This is the 4th discovery of a Variable Star System from Avogadro Observatory, working in team with Alessandro Marchini, Riccardo Papini and Fabio Salvaggio of the Siena University Observatory. On May 2016 the UCAC4 373-082585 was studied and its variability nature as a HADS was discovered. The HADS (High Amplitude δ Scuti stars) are radial pulsators showing asymmetric light curves (steep ascending branches) and amplitudes >0.15 mag.
The Light Curve of UCAC4 373-082585 is the following:
This is the variable VSX page.