Unveiling the Accretion Architecture of GS 1354--64: A Broadband X-ray and Polarimetric Study of its 2025--2026 Outburst

astro-ph.HE

Submitted: 2026-10-06

Updated: 2026-10-06

Comments: Accepted for Publication in the Journal of High Energy Astrophysics (JHEAp)

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Sources

• Revisiting the 2021 Outburst of the BHC MAXI J1803-298 Using NICER, NuSTAR, and Insight-HXMT Data
• The hitchhiker's guide to the IXPE data analysis
• A clean broad iron line in GS 1354--64 as seen by XRISM
• High-Resolution Spectroscopy of X-ray Binaries
• Discovery of Strong Energy-Dependent X-ray Polarization in the Intermediate State of GS 1354-64

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