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Rigorous quantification of biases from unmodeled chromatic effects in PTA data

Quantify rigorously, using realistic multi-frequency pulsar timing datasets and models, the biases that unmodeled chromatic effects (such as scattering delays with radio-frequency index χ > 2) introduce into estimates of achromatic red noise and dispersion measure, extending beyond the simplified two-frequency analytical case and determining under what observational conditions these effects arise in real data.

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Background

In the appendix, the authors present a simplified analytic demonstration for two radio frequencies showing that unmodeled chromatic processes (e.g., scattering with χ > 2) can bias dispersion measure and induce spurious achromatic delays of opposite sign, potentially affecting red-noise inferences.

They note that this derivation is illustrative and may not capture the full complexity of real, multi-frequency PTA observations. A rigorous quantification under realistic conditions is needed to assess the prevalence and magnitude of such biases and to guide improved noise modeling in PTA analyses.

References

While this result is based on a simplified model of the TOA with measurements at only two radio frequencies, it is possible this effect may still arise in real data. A more rigorous quantification will be left for future work.

The NANOGrav 15 yr Data Set: Chromatic Gaussian Process Noise Models for Six Pulsars (2405.14941 - Larsen et al., 23 May 2024) in Appendix: Systematic errors from unmodeled chromatic effects