The Timing Evolution of the Magnetar Swift J1818.0-1607 During a Period of Reduced Activity
Moaz Abdelmaguid, Paulo C. C. Freire, Joseph D. Gelfand, Yogesh Maan, Samayra Straal, J. A. J. Alford

TL;DR
This study monitors the magnetar Swift J1818.0-1607 over 60 days, revealing a mode switch in pulse profile and updated estimates of its age and magnetic field, highlighting short-term spin-down variations.
Contribution
It provides the first detailed timing and profile evolution analysis of Swift J1818.0-1607 during a reduced activity phase, updating its age and magnetic field estimates.
Findings
Pulse profile changed from double to single peak.
Spin-down rate decreased during the observation period.
Estimated age is about 2500 years, with a magnetic field of 10^14 G.
Abstract
We report results from an observational campaign of the radio-loud magnetar Swift J1818.0-1607 using the Green Bank Telescope (GBT) at 2.0 GHz, which began in November 2021 during a period of reduced activity approximately 20 months after its March 2020 outburst. Over the 60-day duration reported here, the integrated pulse profile remained consistently stable, exhibiting a single, narrow peak with with a small precursor component and no evidence of a postcursor one. This pulse profile is in sharp contrast to the double-peaked morphology observed during an observing campaign approximately 120 days preceding ours. Along with this change in the integrated pulse profile shape, we also measure a slower spin-down rate compared to the end of that preceding campaign. Together, these differences suggest that a mode-switching event likely occurred between the end of that campaign and the start of…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Astrophysical Phenomena and Observations · Gamma-ray bursts and supernovae
