Direct shear times kSZ correlation: controlling baryons without modeling galaxies

arXiv:2607.29091 · astro-ph.CO · Submitted 2026-07-31 · Read on arXiv

Anoma Ganguly, Emmanuel Schaan, Elisabeth Krause, Tim Eifler

astro-ph.CO

Submitted: 2026-07-31

Comments: Comments welcome

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

Weak Lensing — 20× in this paper · explained in 2 episodes
Matter Power Spectrum — 18× in this paper · explained in 2 episodes
Baryonic Feedback — 15× in this paper · explained in 3 episodes
Atacama Cosmology Telescope — 9× in this paper
Anisotropy — 4× in this paper · explained in 3 episodes
AGN — 3× in this paper · explained in 1 episode
Accuracy — 3× in this paper · explained in 1 episode
Adam — 3× in this paper · explained in 2 episodes
Trace — 3× in this paper · explained in 2 episodes
AGN Feedback — 2× in this paper · explained in 1 episode
Abundance — 2× in this paper · explained in 1 episode
Benchmark — 2× in this paper · explained in 2 episodes
LSST Dark Energy Science Collaboration — 2× in this paper
Simons Observatory — 2× in this paper
Bernardeau Nishimichi Taruya — 1× in this paper
Bispectrum — 1× in this paper · explained in 3 episodes
Clustering — 1× in this paper · explained in 2 episodes
Cosmic Microwave Background — 1× in this paper
Gravitational Lensing — 1× in this paper · explained in 2 episodes
Non-Gaussianity — 1× in this paper · explained in 2 episodes
Primordial non-Gaussianity — 1× in this paper · explained in 2 episodes
Signal-to-noise ratio (SNR) — 1× in this paper · explained in 2 episodes

Sources

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