The spectrum of flux for a synchrotron source, such as an Active Galactic Nucleus (AGN), exhibits a decline at low frequencies, raising questions about the underlying mechanisms. The discussion seeks to clarify what constitutes "low frequency," specifically whether it refers to infrared, visible, X-ray, or gamma-ray ranges. Participants are encouraged to explore the implications of this drop-off in flux and its significance in astrophysical contexts. The provided links may offer additional insights into the topic. Understanding the nature of low-frequency emissions is crucial for comprehending synchrotron radiation behavior.