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Model Dependence of XRISM Black Hole Spin Constraints in Cyg X-1

  • Authors: Andrzej A. Zdziarski, Swadesh Chand, Michał Szanecki, Gulab Dewangan, Barbara De Marco

Andrzej A. Zdziarski et al 2026 The Astrophysical Journal Letters 1005 .

  • Provider: AAS Journals

Caption: Figure 3.

The rms(E) in the 0.01–1 Hz frequency range for NICER (red) and XRISM Resolve (blue). For comparison, the black symbols show the rms(E) from NICER in the soft spectral state (A. A. Zdziarski et al. 2024). We see similar trends in soft X-rays, with broad peaks around 1 keV, although the soft-state rms is much lower. Above that, we observe a decrease with energy in the hard state and an increase in the soft state, while both converge in the Fe K energy region.

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