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Due to cosmic variance we cannot learn any more about large-scale inhomogeneities from the primary cosmic microwave background (CMB) alone. More information on large scales is essential for resolving large angular scale anomalies in the…

宇宙学与河外天体物理 · 物理学 2017-03-08 Alexandra Terrana , Mary-Jean Harris , Matthew C. Johnson

While third-generation CMB experiments have allowed to release the first maps of Compton-$y$ distortion due to thermal Sunyaev-Zeldovich (SZ) effect, next-generation CMB experiments should allow us to map also the electron gas temperature,…

宇宙学与河外天体物理 · 物理学 2022-02-09 Mathieu Remazeilles

The kinematic and thermal Sunyaev-Zel'dovich (kSZ and tSZ) effects probe the abundance and thermodynamics of ionized gas in galaxies and clusters. We present a new hybrid estimator to measure the kSZ effect by combining cosmic microwave…

Sub-structures in the hot gas of galaxy clusters are related to their formation history and to the astrophysical processes at play in the intracluster medium (ICM). The thermal Sunyaev-Zel'dovich (tSZ) effect is directly sensitive to the…

The thermal Sunyaev-Zel'dovich (tSZ) effect provides a powerful probe of the thermal pressure of ionised gas in galaxy clusters and the cosmic web; constrained simulations reconstruct the mass and velocity fields of the local Universe. We…

宇宙学与河外天体物理 · 物理学 2026-01-23 Richard Stiskalek , Harry Desmond

We investigate empirical scaling relations between the thermal Sunyaev-Zeldovich effect (SZE) and cluster mass in simulated clusters of galaxies. The simulated clusters have been compiled from four different samples that differ only in…

天体物理学 · 物理学 2009-11-10 Patrick M. Motl , Eric J. Hallman , Jack O. Burns , Michael L. Norman

We consider the role of the galactic kinetic Sunyaev Zeldovich (SZ) effect as a CMB foreground. While the galactic thermal Sunyaev Zeldovich effect has previously been studied and discarded as a potential CMB foreground, we find that the…

天体物理学 · 物理学 2009-11-13 A. Waelkens , M. Maturi , T. Ensslin

Theoretical uncertainty limits our ability to extract cosmological information from baryonic fields such as the thermal Sunyaev-Zel'dovich (tSZ) effect. Being sourced by the electron pressure field, the tSZ effect depends on baryonic…

宇宙学与河外天体物理 · 物理学 2022-06-13 Leander Thiele , Miles Cranmer , William Coulton , Shirley Ho , David N. Spergel

The secondary anisotropies of the cosmic microwave background (CMB) provide a wealth of astrophysical and cosmological information. Pairing measurements of the CMB temperature map obtained by DR5 of the Atacama Cosmology Telescope (ACT)…

宇宙学与河外天体物理 · 物理学 2025-06-24 Boryana Hadzhiyska , Noah Sailer , Simone Ferraro

In this paper we probe the hot, post-shock gas component of quasar-driven winds through the thermal Sunyaev-Zel'dovich (tSZ) effect. Combining datasets from the Atacama Cosmology Telescope, the $\textit{Herschel}$ Space Observatory, and the…

We describe a fast method to simulate in a semi-analytical way consistent maps of the thermal, kinetic and polarised Sunyaev-Zel'dovich effect, featuring both cluster spatial correlations and large scale velocity flows.

天体物理学 · 物理学 2007-05-23 J. Delabrouille , J. -B. Melin , J. G. Bartlett

We propose the use of the kinetic Sunyaev-Zel'dovich (kSZ) effect to probe the circumgalactic medium (CGM), with the aid of a spectroscopic survey covering the same area of a SZ survey. One can design an optimal estimator of the kSZ effect…

宇宙学与河外天体物理 · 物理学 2016-03-23 Jiawei Shao , Taotao Fang

Secondary anisotropies of the CMB have the potential to reveal intricate details about the history of our universe between the present and recombination epochs. However, because the CMB we observe is the projected sum of a multitude of…

天体物理学 · 物理学 2009-11-10 Olivier Doré , Joseph F. Hennawi , David N. Spergel

We investigate the impact of modified theories of gravity on the kinetic Sunyaev-Zeldovich (kSZ) effect of the cosmic microwave background. We focus on a specific class of $f(R)$ models of gravity and compare their predictions for the kSZ…

宇宙学与河外天体物理 · 物理学 2016-03-23 Federico Bianchini , Alessandra Silvestri

The kinetic Sunyaev Zel'dovich (kSZ) effect, cosmic microwave background (CMB) temperature anisotropies induced by the scattering of CMB photons from free electrons, will be measured by near-term CMB experiments at high significance. By…

宇宙学与河外天体物理 · 物理学 2023-02-01 Dagoberto Contreras , Fiona McCarthy , Matthew C. Johnson

Perhaps the most controversial idea in modern cosmology is that our observable universe is contained within one bubble among many, all inhabiting the eternally inflating multiverse. One of the few way to test this idea is to look for…

宇宙学与河外天体物理 · 物理学 2015-06-01 Pengjie Zhang , Matthew C. Johnson

In this work we examine the impact of our motion with respect to the CMB rest frame on statistics of CMB maps by examining the one-, two-, three- and four- point statistics of simulated maps of the CMB and Sunyaev-Zeldovich (SZ) effects. We…

宇宙学与河外天体物理 · 物理学 2022-04-27 William R. Coulton , Sydney Feldman , Karime Maamari , Elena Pierpaoli , Siavash Yasini , Klaus Dolag

Measurements of the thermal Sunyaev-Zel'dovich (tSZ) effect have long been recognized as a powerful cosmological probe. Here we assess the importance of relativistic temperature corrections to the tSZ signal on the power spectrum analysis…

宇宙学与河外天体物理 · 物理学 2018-12-19 Mathieu Remazeilles , Boris Bolliet , Aditya Rotti , Jens Chluba

We present the first detection of the cross-correlation angular power spectrum between the thermal Sunyaev-Zel'dovich (tSZ) effect and the X-ray emission over the full sky. The tSZ effect and X-rays are produced by the same hot gas within…

宇宙学与河外天体物理 · 物理学 2017-02-01 G. Hurier , M. Douspis , N. Aghanim , E. Pointecouteau , J. M. Diego , J. F. Macias-Perez

The thermal Sunyaev-Zel'dovich (tSZ) effect is a powerful probe of cosmology. The statistical errors in the tSZ power spectrum measurements are dominated by the presence of massive clusters in a survey volume that are easy to identify on…

宇宙学与河外天体物理 · 物理学 2021-03-10 Ken Osato , Masahiro Takada
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