Measuring the Clustering of tSZ-Selected Galaxy Clusters with SPT-3G

arXiv:2610.08947 · astro-ph.CO · Submitted 2026-10-06 · Read on arXiv

astro-ph.CO

Submitted: 2026-10-06

Updated: 2026-10-06

Code: https://github.com/LSSTDESC/CCL

Terminology

• Clustering — 87× in this paper · explained in 2 episodes
• Abundance — 20× in this paper · explained in 1 episode
• Calibration — 11× in this paper · explained in 7 episodes
• Accuracy — 10× in this paper · explained in 1 episode
• Consistency — 8× in this paper · explained in 3 episodes
• Robustness — 7× in this paper · explained in 5 episodes
• Weak Lensing — 4× in this paper · explained in 2 episodes
• Core — 2× in this paper · explained in 2 episodes
• Matter Power Spectrum — 2× in this paper · explained in 2 episodes
• South Pole Telescope — 2× in this paper
• Trace — 2× in this paper · explained in 2 episodes
• Adam — 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
• Redundancy — 1× in this paper · explained in 2 episodes
• Signal-to-noise ratio (SNR) — 1× in this paper · explained in 2 episodes

Sources

• Primordial Physics in the Nonlinear Universe: Revealing the oscillating halo bias from cosmological collider models
• Galaxy Clusters Selected via the Sunyaev-Zel'dovich Effect in 5 year data from the SPT-3G Main Survey
• Dark Energy Survey Year 6 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing
• Cosmic voids as a probe of the nature of dark matter: simulations and galaxy survey forecasts
• The Aemulus Project IV: Emulating Halo Bias
• The LSST Dark Energy Science Collaboration (DESC) Science Requirements Document

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