3 papers
astro-ph.CO2026
Tidal alignment and tidal torquing modeling for the cosmic shear three-point correlation function and mass aperture skewness
Rafael C. H. Gomes, Kyle Miller, Sunao Sugiyama +3
We present a model for the intrinsic alignment contamination of the shear three-point correlation function and skewness of the mass aperture statistic using the tidal alignment and…
astro-ph.CO2025
Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum
Kyle Miller, Surhud More, Bhuvnesh Jain
Upcoming weak-lensing surveys will probe the matter distribution at a few percent level on nonlinear scales () where baryonic feedback from galaxy formation…
astro-ph.IM2024
Galaxy cluster profiles: A Gaussian mixture model approach to halo miscentering
Matthew Currie, Kyle Miller, Tae-Hyeon Shin +2
Measurements of the galaxy density and weak-lensing profiles of galaxy clusters typically rely on an assumed cluster center, which is taken to be the brightest cluster galaxy or ot…