The MeerKAT Pulsar Timing Array: first data release
Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 519:3 (2022) 3976-3991
Authors:
MT Miles, RM Shannon, M Bailes, DJ Reardon, MJ Keith, AD Cameron, A Parthasarathy, M Shamohammadi, R Spiewak, W van聽Straten, S Buchner, F Camilo, M Geyer, A Karastergiou, M Kramer, M Serylak, G Theureau, V Venkatraman聽Krishnan
Abstract:
ABSTRACT
We present the first 2.5聽yr of data from the MeerKAT Pulsar Timing Array (MPTA), part of MeerTime, a MeerKAT Large Survey Project. The MPTA aims to precisely measure pulse arrival times from an ensemble of 88 pulsars visible from the Southern hemisphere, with the goal of contributing to the search, detection, and study of nanohertz-frequency gravitational waves as part of the International Pulsar Timing Array. This project makes use of the MeerKAT telescope and operates with a typical observing cadence of 2 weeks using the L-band receiver that records data from 856 to 1712聽MHz. We provide a comprehensive description of the observing system, software, and pipelines used and developed for the MeerTime project. The data products made available as part of this data release are from the 78 pulsars that had at least 30 observations between the start of the MeerTime programme in February 2019 and October 2021. These include both sub-banded and band-averaged arrival times and the initial timing ephemerides, noise models, and the frequency-dependent standard templates (portraits) used to derive pulse arrival times. After accounting for detected noise processes in the data, the frequency-averaged residuals of 67 of the pulsars achieved a root-mean-square residual precision of $\lt 1 \, \mu \rm {s}$. We also present a novel recovery of the clock correction waveform solely from pulsar timing residuals and an exploration into preliminary findings of interest to the international pulsar timing community. The arrival times, standards, and full Stokes parameter-calibrated pulsar timing archives are publicly available.
