High-cadence Timing of Binary Pulsars with CHIME

Abstract

Abstract We performed near-daily observations of the binary pulsars PSR J0218+4232, PSR J1518+4904, and PSR J2023+2853 with the Canadian Hydrogen Intensity Mapping Experiment (CHIME). For the first time, we detected the Shapiro time delay in all three pulsar binary systems, using only 2–4 yr of CHIME/Pulsar timing data. We measured the pulsar masses to be 1.49 − 0.20 + 0.23 M ⊙, 1.470 − 0.034 + 0.030 M ⊙, and 1.50 − 0.38 + 0.49 M ⊙, respectively. The companion mass to PSR J0218+4232 was found to be 0.179 − 0.016 + 0.018 M ⊙. We constrained the mass of the neutron star companion of PSR J1518+4904 to be 1.248 − 0.029 + 0.035 M ⊙, using the observed apsidal motion as a constraint on the mass estimation. The binary companion to PSR J2023+2853 was found to have a mass of 0.93 − 0.14 + 0.17 M ⊙; in the context of the near-circular orbit, this mass estimate suggests that the companion to PSR J2023+2853 is likely a high-mass white dwarf. By comparing the timing model obtained for PSR J0218+4232 with previous observations, we found a significant change in the observed orbital period of the system of P b ̇ = 0.14 ( 2 ) × 10 − 12 ; we determined that this variation arises from “Shklovskii acceleration” due to the relative motion of the binary system, and used this measurement to estimate a distance of d = (6.7 ± 1.0) kpc to PSR J0218+4232. This work demonstrates the capability of high-cadence observations, enabled by the CHIME/Pulsar system, to detect and refine general-relativistic effects of binary pulsars over short observing timescales.