Binary pulsars can be used to probe Galactic potential gradients through calculating their line-of-sight accelerations. We present the first data release of direct line-of-sight acceleration measurements for 29 binary pulsars. We validate these data with a local acceleration model, and compare our results to those from earlier works. We find evidence for an acceleration gradient in agreement with these values, with our results indicating a local disk density of ${\rho }_{\mathrm{d}}={\mathrm{0.040}}_{-\mathrm{0.020}}^{+\mathrm{0.020}}{M}_{\odot }{\mathrm{pc}}^{-3}$. We also find evidence for unmodeled noise of unknown origin in our dataset.

• Received 28 July 2023
• Accepted 1 May 2024

DOI:https://doi.org/10.1103/PhysRevD.109.123015