Abstract Quasiperiodic oscillations in gamma-ray burst afterglows have been suggested as probes of the central engine. Such interpretations generally assume that the observed modulation frequency directly corresponds to an intrinsic oscillation frequency of the source. We show that this assumption is not generally valid and that interpreting such features without accounting for relativistic propagation may lead to misleading inferences about the engine nature. We show that relativistic propagation effects—most importantly, integration over equal-arrival-time surfaces—act as a frequency-dependent filter that can significantly modify or suppress intrinsic variability. In the constant-Γ case, the angular kernel acts as a stationary low-pass filter that suppresses high-frequency variability without altering its frequency, whereas Blandford–McKee deceleration renders the filter time-dependent and manifests observationally as an apparent frequency drift.
Noémie Globus (Tue,) studied this question.