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¹Physics Division, Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA
²Berkeley Center for Cosmological Physics, Department of Physics, University of California, Berkeley, California 94720, USA
³Institute of Astronomy, Madingley Road, Cambridge, CB3 0HA, United Kingdom
⁴Kavli Institute for Cosmology Cambridge, Madingley Road, Cambridge, CB3 0HA, United Kingdom

^*Contact author: boryanah@alumni.princeton.edu

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Articles Citing

Missing baryons recovered: A measurement of the gas fraction in galaxies and groups with the kinematic Sunyaev-Zel’dovich effect and CMB lensing

Novel Kinetic Sunyaev-Zel’dovich Estimator for Electron-Electron Correlations

Precision kinematic Sunyaev-Zel’dovich measurements across halo mass and redshift with DESI DR2 and ACT DR6. I. Luminous red galaxies

Precision kinematic Sunyaev-Zel’dovich measurements across halo mass and redshift with DESI DR2 and ACT DR6. II. Bright galaxy survey and emission-line galaxies

Probing cosmic velocities with the pairwise kinematic Sunyaev-Zel’dovich signal in DESI Bright Galaxy Sample DR1 and ACT DR6

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The kinetic Sunyaev Zeldovich effect as a benchmark for AGN feedback models in hydrodynamical simulations: insights from DESI + ACT

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The FLAMINGO simulations data release

Quantifying the Impact of Selection Effects on FRB DM–z Relation Cosmological Inference

Probing Baryonic Feedback and Cosmology with the 3 × 2-point Statistic of Fast Radio Bursts and Galaxies

Backlighting the Universe with Fast Radio Bursts: An Anthology of Dispersion Measure Cross Correlations with Tracers of Large-scale Structure and Baryonic Matter

Joint X-Ray, Kinetic Sunyaev–Zeldovich, and Weak Lensing Measurements: Toward a Consensus Picture of Efficient Gas Expulsion from Groups and Clusters

The SRG/eROSITA All-Sky Survey

What’s missing in AGN feedback: Lessons learnt from Magneticum, IllustrisTNG, and Simba

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