Monthly Notices of the Royal Astronomical Society· 2026Q1
The FLAMINGO Project: Exploring the X-ray–cosmic-shear cross-correlation as a probe of large-scale structure
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- Q1SCImago
- 2026year
Short summary
The FLAMINGO simulations show that the cross-correlation between X-ray emission and cosmic shear is most sensitive to gas in galaxy haloes between 10^14 and 10^15 solar masses, offering a new way to probe baryonic feedback effects on large-scale structure.
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