A possible detection of gas rotation in galaxy groups via the kinetic Sunyaev-Zeldovich effect
astro-ph.CO, astro-ph.GA
Submitted: 2026-03-15
Updated: 2026-10-09
Terminology
Sources
- Component separation with flexible models. Application to the separation of astrophysical emissions
- Data Release 1 of the Dark Energy Spectroscopic Instrument
- Evidence of galaxy cluster rotation in the cosmic microwave background
- Evidence for large baryonic feedback at low and intermediate redshifts from kinematic Sunyaev-Zel'dovich observations with ACT and DESI photometric galaxies
- Missing baryons recovered: a measurement of the gas fraction in galaxies and groups with the kinematic Sunyaev-Zel'dovich effect and CMB lensing
- Velocity Reconstruction from KSZ: Measuring $f_{NL}$ with ACT and DESILS
- KSZ Velocity Reconstruction with ACT and DESI-LS using a Tomographic QML Power Spectrum Estimator
- Detection of pairwise kinetic Sunyaev-Zel'dovich effect with DESI galaxy groups and Planck in Fourier space
- Mass dependence of halo baryon fractions from the kinetic Sunyaev-Zeldovich effect
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