The high-energy cyclotron line in 2S 1417-624 discovered with Insight-HXMT during the 2018 outburst
Q. Liu, A. Santangelo, L. D. Kong, L. Ducci, L. Ji, W. Wang, M. M., Serim, C. G\"ung\"or, Y. L. Tuo, and D. Serim

TL;DR
This paper reports the discovery of a high-energy cyclotron line at around 100 keV in the X-ray pulsar 2S 1417-624 during its 2018 outburst, revealing new insights into its magnetic field and spectral features.
Contribution
The study presents the first detection of a high-energy cyclotron resonant scattering feature in 2S 1417-624, expanding understanding of its magnetic properties and spectral behavior.
Findings
Detection of a ~100 keV CRSF with 7σ significance.
Pulse profile evolution from double to multi-peaked with flux.
CRSF energy varies from 97 to 107 keV over pulse phase.
Abstract
We report a detailed timing and spectral analysis of the X-ray pulsar 2S~1417-624 using the data from Insight-HXMT during the 2018 outburst. The pulse profiles are highly variable with respect to both unabsorbed flux and energy. A double-peaked pulse profile from the low flux evolved to a multi-peaked shape in the high-flux state. The pulse fraction is negatively correlated to the source flux in the range of (1--6) erg cm s, consistent with \textit{Rossi} X-ray Timing Explorer (RXTE) studies during the 2009 giant outburst. The energy-resolved pulse profiles around the peak outburst showed a four-peak shape in the low-energy bands and gradually evolved to triple peaks at higher energies. The continuum spectrum is well described by typical phenomenological models, such as the cut-off power law and the power law with high-energy cut-off models.…
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