Timing noise refers to the random fluctuations in the arrival times of signals from pulsars, which can obscure precise measurements of their timing and lead to challenges in analyzing their properties. This noise can originate from various sources, including intrinsic variations in the pulsar's emission mechanism, interstellar medium effects, and instrumental inaccuracies. Understanding timing noise is crucial for improving the precision of pulsar timing measurements and for detecting gravitational waves and exoplanets.
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