The timing and spectral properties of the 2022 outburst of SGR J1935+2154 observed with NICER
Fu Yu-Cong, Lin Lin, Ge Ming-Yu, Enoto Teruaki, Hu Chin-Ping, Younes, George, G\"o\u{g}\"u\c{s} Ersin, and Malacaria Christian

TL;DR
This study analyzes the timing and spectral properties of the 2022 outburst of SGR J1935+2154 using NICER data, revealing connections between X-ray activity, glitches, and radio bursts, and providing insights into the magnetar's behavior.
Contribution
It presents detailed timing and spectral analysis of the 2022 outburst, highlighting the relationship between glitches, phase jumps, and multi-wavelength emissions in SGR J1935+2154.
Findings
X-ray flux decays exponentially during the outburst.
A phase jump of 0.16±0.03 is related to a glitch.
Spectra fit with blackbody plus power law, with the non-thermal component dropping over time.
Abstract
The magnetar SGR J1935+2154 entered a new active episode on October 10, 2022, with X-ray bursts and enhanced persistent emission. At the tail of high burst rate interval, lasting several hours, radio bursts were detected, revealing the connection between the X-ray activities and radio emissions. We analyzed observations of SGR J1935+2154 for nearly three months, using data from Neutron Star Interior Composition Explorer (NICER). We report the timing and spectral results following the onset of this outburst. In general, the X-ray flux of the persistent emission decays exponentially. While a flare is evident on the light curve, a fast radio burst (FRB) was detected immediately following the peak of this flare. We found a phase jump of pulse profile, with a deviation of phase, which is related to the glitch. The spectra are well fit with the combination of a blackbody and a…
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