Author ORCID Identifier
https://orcid.org/0000-0002-4828-0262
https://orcid.org/0000-0002-1797-3277
https://orcid.org/0000-0001-7697-7422
N/A
N/A
Document Type
Article
Publication Date
2015
Abstract
Light travel time changes due to gravitational waves (GWs) may be detected within the next decade through precision timing of millisecond pulsars. Removal of frequency-dependent interstellar medium (ISM) delays due to dispersion and scattering is a key issue in the detection process. Current timing algorithms routinely correct pulse times of arrival (TOAs) for time-variable delays due to cold plasma dispersion. However, none of the major pulsar timing groups correct for delays due to scattering from multi-path propagation in the ISM. Scattering introduces a frequency-dependent phase change in the signal that results in pulse broadening and arrival time delays. Any method to correct the TOA for interstellar propagation effects must be based on multi-frequency measurements that can effectively separate dispersion and scattering delay terms from frequency-independent perturbations such as those due to a GW. Cyclic spectroscopy, first described in an astronomical context by Demorest (2011), is a potentially powerful tool to assist in this multi-frequency decomposition. As a step toward a more comprehensive ISM propagation delay correction, we demonstrate through a simulation that we can accurately recover impulse response functions (IRFs), such as those that would be introduced by multi-path scattering, with a realistic signal-to-noise ratio (S/N). We demonstrate that timing precision is improved when scatter-corrected TOAs are used, under the assumptions of a high S/N and highly scattered signal. We also show that the effect of pulse-to-pulse "jitter" is not a serious problem for IRF reconstruction, at least for jitter levels comparable to those observed in several bright pulsars.
Digital Commons Citation
Palliyaguru, Nipuni; Stinebring, Daniel; McLaughlin, Maura; Demorest, Paul; and Jones, Glenn, "Correcting For Interstellar Scattering Delay In High-Precision Pulsar Timing: Simulation Results" (2015). Faculty & Staff Scholarship. 495.
https://researchrepository.wvu.edu/faculty_publications/495
Source Citation
Palliyaguru, Nipuni., Stinebring, Daniel., Mclaughlin, Maura., Demorest, Paul., & Jones, Glenn.(2015). Correcting For Interstellar Scattering Delay In High-Precision Pulsar Timing: Simulation Results. The Astrophysical Journal, 815(2), 89. http://doi.org/10.1088/0004-637X/815/2/89