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This repository contains high-level reduced data products from our publication "Constraints on wide-band radiative changes after a glitch in PSR J1452-6036" (Jankowski et al. 2021, MNRAS). We share the best-fitting pulsar timing ephemeris from our Markov chain Monte Carlo analysis, the input arrival times, and the resulting corner plot. Please consult the paper for further information.
pulsars, pulsar timing, radiation mechanisms: non-thermal, ephemerides, methods: data analysis
pulsars, pulsar timing, radiation mechanisms: non-thermal, ephemerides, methods: data analysis
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