New periods are reported for NSV 575 and NSV 014, the period of NSV 489 is corrected from O-C analysis, and NSV 014 is reclassified as a likely low-amplitude pulsator.
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Determination of Light Curve Parameters of Poorly Studied Eclipsing Variables Using Data from Tess and Other Sky Surveys
New periods are reported for NSV 575 and NSV 014, the period of NSV 489 is corrected from O-C analysis, and NSV 014 is reclassified as a likely low-amplitude pulsator.