Study of the 2024 major Vela glitch at the Argentine Institute of Radioastronomy
Ezequiel Zubieta, Ryan Missel, Susana B. Araujo Furlan, Carlos O. Lousto, Federico Garc\'ia, Santiago del Palacio, Guillermo Gancio, Jorge A. Combi, Linwei Wang

TL;DR
This paper presents a detailed analysis of the 2024 major glitch in the Vela pulsar, including precise timing, pulse statistical properties, and recovery behavior, using radio observations and advanced data analysis techniques.
Contribution
The study provides the first detailed characterization of the Vela pulsar's 2024 glitch, combining pulsar timing with machine learning methods to analyze pulse properties.
Findings
Identified two recovery timescales of approximately 3 and 17 days.
Established a correlation between pulse amplitude and width.
Found no significant qualitative changes in pulse properties before and after the glitch.
Abstract
We report here on new results of the systematic monitoring of southern glitching pulsars at the Argentine Institute of Radioastronomy. In particular, we study in this work the new major glitch in the Vela pulsar (PSR J08354510) that occurred on 2024 April 29. We aim to thoroughly characterise the rotational behaviour of the Vela pulsar around its last major glitch and investigate the statistical properties of its individual pulses around the glitch. We characterise the rotational behaviour of the pulsar around the glitch through the pulsar timing technique. We measured the glitch parameters by fitting timing residuals to the data collected during the days surrounding the event. In addition, we study Vela individual pulses during the days of observation just before and after the glitch. We selected nine days of observations around the major glitch on 2024 April 29 and studied their…
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