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Main Authors: Baker, Daniel, Pen, Ue-Li
Format: Preprint
Published: 2025
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Online Access:https://arxiv.org/abs/2508.15270
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author Baker, Daniel
Pen, Ue-Li
author_facet Baker, Daniel
Pen, Ue-Li
contents Understanding the evolution of pulsar dispersion measures is vital to high precision timing experiments, as well as astrometric experiments to determine pulsar positions and proper motions. In this work, we present a novel approach to measuring dispersion measure gradients using pulsar scintillometry. This approach makes use of the multipath propagation through the interstellar medium to simultaneously probe dispersion measures along multiple sight lines from a single observation. Using existing data of PSR B0834+06, we are able to measure gradients of $9.7\pm0.3\times10^{-6}~\rm{pc}~\rm{cm}^{-3}~\rm{mas}^{-1}$.
format Preprint
id arxiv_https___arxiv_org_abs_2508_15270
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Single Epoch Measurements of Dispersion Measure Gradients Towards PSR B0834+06
Baker, Daniel
Pen, Ue-Li
High Energy Astrophysical Phenomena
Instrumentation and Methods for Astrophysics
Understanding the evolution of pulsar dispersion measures is vital to high precision timing experiments, as well as astrometric experiments to determine pulsar positions and proper motions. In this work, we present a novel approach to measuring dispersion measure gradients using pulsar scintillometry. This approach makes use of the multipath propagation through the interstellar medium to simultaneously probe dispersion measures along multiple sight lines from a single observation. Using existing data of PSR B0834+06, we are able to measure gradients of $9.7\pm0.3\times10^{-6}~\rm{pc}~\rm{cm}^{-3}~\rm{mas}^{-1}$.
title Single Epoch Measurements of Dispersion Measure Gradients Towards PSR B0834+06
topic High Energy Astrophysical Phenomena
Instrumentation and Methods for Astrophysics
url https://arxiv.org/abs/2508.15270