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This paper investigates the potential for detecting a month-scale quasi-periodic oscillation (QPO) in the gamma-ray light curve of the blazar OP 313. The authors analyze Fermi-LAT data and find tentative evidence for a QPO, although the significance is limited by the data length. The study explores potential physical origins, suggesting a curved-jet model as a possible explanation. The work is significant because it explores a novel phenomenon in a blazar and provides a framework for future observations and analysis.
Reference

The authors find 'tentative evidence for a month-scale QPO; however, its detection significance is limited by the small number of observed cycles.'