This paper presents new photometric observations of eclipsing binary systems and new eclipsing candidates. We used SILICUPS software to derive 47 minima timings with corresponding realistic uncertainties. We also introduce three variable star candidates, ATO J320.1286+51.7924, ATO J337.0231+56.7537, and 2MASS J04570945+2419256, for further and more detailed study.
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Martin Kolář (2024) studied this question.
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