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.
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