Processing choices change pulsar noise model preferences; the 2023 reprocessing raises solar-wind support from four to ten pulsars, with densities matching the longer DR3 data set.
As shown in Figure 2(a), an RN+DMv+SW model family dom- inates the model space under both pipelines
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Insights into the Pulsar Timing Array hypothesis space
Processing choices change pulsar noise model preferences; the 2023 reprocessing raises solar-wind support from four to ten pulsars, with densities matching the longer DR3 data set.