The Relativistic Binary Programme on MeerKAT: Science objectives and first results

TL;DR

This paper presents the initial results of the Relativistic Binary programme using MeerKAT, including pulsar observations, polarization data, relativistic effect measurements, and improved timing precision, advancing tests of gravity and neutron star physics.

Contribution

The paper introduces the RelBin programme, providing new polarization, dispersion, and Faraday rotation measurements, and demonstrates enhanced timing accuracy with MeerKAT for binary pulsar studies.

Findings

First Faraday rotation measures for 12 pulsars.

Successful application of RVM to binary pulsars, including the Double Pulsar.

Timing precision improved by a factor of 2-3, sometimes up to tenfold.

Abstract

We describe the ongoing Relativistic Binary programme (RelBin), a part of the MeerTime large survey project with the MeerKAT radio telescope. RelBin is primarily focused on observations of relativistic effects in binary pulsars to enable measurements of neutron star masses and tests of theories of gravity. We selected 25 pulsars as an initial high priority list of targets based on their characteristics and observational history with other telescopes. In this paper, we provide an outline of the programme, present polarisation calibrated pulse profiles for all selected pulsars as a reference catalogue along with updated dispersion measures. We report Faraday rotation measures for 24 pulsars, twelve of which have been measured for the first time. More than a third of our selected pulsars show a flat position angle swing confirming earlier observations. We demonstrate the ability of the Rotating Vector Model (RVM), fitted here to seven binary pulsars, including the Double Pulsar (PSR J0737$-$3039A), to obtain information about the orbital inclination angle. We present a high time resolution light curve of the eclipse of PSR J0737$-$3039A by the companion's magnetosphere, a high-phase resolution position angle swing for PSR J1141$-$6545, an improved detection of the Shapiro delay of PSR J1811$-$2405, and pulse scattering measurements for PSRs J1227$-$6208, J1757$-$1854, and J1811$-$1736. Finally, we demonstrate that timing observations with MeerKAT improve on existing data sets by a factor of, typically, 2-3, sometimes by an order of magnitude.