Astronomers using the WEBT telescope network discovered a 433-day optical oscillation in quasar 3C 454.3, one of the most persistent QPOs ever detected.
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Bright blazar reveals 433-day optical quasi-periodic oscillation across nine years

433 days QPO period
19 years Observation span
0.86 Redshift
0.5–2.3 Billion solar masses SMBH mass
Optical QPO Period 433-day
Observations Analyzed 19 years
Solar Masses (SMBH) 0.5–2.3 billion