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相关论文: Constraining cosmology with thermal Sunyaev-Zel'do…

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In this paper, we explain how moments of the thermal Sunyaev-Zel'dovich (tSZ) effect can constrain both cosmological parameters and the astrophysics of the intracluster medium (ICM). As the tSZ signal is strongly non-Gaussian, higher…

宇宙学与河外天体物理 · 物理学 2013-05-30 J. Colin Hill , Blake D. Sherwin

The thermal Sunyaev-Zel'dovich (tSZ) effect is the inverse-Compton scattering of cosmic microwave background (CMB) photons off hot, ionized electrons, primarily located in galaxy groups and clusters. Recent years have seen immense…

宇宙学与河外天体物理 · 物理学 2015-10-22 J. Colin Hill

We explore the significance of noise from thermal Sunyaev-Zel{'}dovich (tSZ) signals for cluster detection using cosmic microwave background (CMB) surveys. The noise arises both from neighboring objects and also from haloes below the…

宇宙学与河外天体物理 · 物理学 2022-03-30 Srinivasan Raghunathan

Thermal Sunyaev-Zeldovich (tSZ) power spectrum is one of the most sensitive methods to constrain cosmological parameters, scaling as the amplitude $\sigma_8^8$. It is determined by the integral over the halo mass function multiplied by the…

宇宙学与河外天体物理 · 物理学 2017-05-31 Benjamin Horowitz , Uroš Seljak

Upcoming millimeter experiments that probe the cosmic microwave background (CMB) will observe tens of thousands of galaxy clusters through the thermal Sunyaev-Zeldovich (tSZ) effect. tSZ selected clusters are powerful probes of cosmological…

宇宙学与河外天体物理 · 物理学 2019-10-02 Dylan Cromer , Nicholas Battaglia , Mathew S. Madhavacheril

The thermal Sunyaev-Zel'dovich (tSZ) effect is one of the primary tools for finding and characterizing galaxy clusters. Several ground-based experiments are either underway or are being planned for mapping wide areas of the sky at $\sim…

宇宙学与河外天体物理 · 物理学 2020-03-24 Nikhel Gupta , Cristiano Porciani , Kaustuv Basu

At high angular frequencies, beyond the damping tail of the primary power spectrum, the dominant contribution to the power spectrum of cosmic microwave background (CMB) temperature fluctuations is the thermal Sunyaev-Zel'dovich (tSZ)…

宇宙学与河外天体物理 · 物理学 2013-05-06 Dipak Munshi , Shahab Joudaki , Joseph Smidt , Peter Coles , Scott T. Kay

We propose a new analysis of small scale CMB data by introducing the cosmological dependency of the foreground signals, focusing first on the thermal Sunyaev-Zel'dovich (tSZ) power spectrum, derived from the halo model. We analyse the…

宇宙学与河外天体物理 · 物理学 2022-03-22 Marian Douspis , Laura Salvati , Adélie Gorce , Nabila Aghanim

Thermal Sunyaev-Zel'dovich effect is one of the recent probes of cosmology and large scale structures. We update constraints on cosmological parameters from galaxy clusters observed by the Planck satellite in a first attempt to combine…

宇宙学与河外天体物理 · 物理学 2018-06-06 Laura Salvati , Marian Douspis , Nabila Aghanim

The thermal Sunyaev-Zel'dovich (tSZ) effect induces a Compton-$y$ distortion in cosmic microwave background (CMB) temperature maps that is sensitive to a line of sight integral of the ionized gas pressure. By correlating the positions of…

宇宙学与河外天体物理 · 物理学 2020-02-26 S. Pandey , E. J. Baxter , J. C. Hill

Recent detections of the cross-correlation of the thermal Sunyaev-Zel'dovich (tSZ) effect and weak gravitational lensing (WL) enable unique studies of cluster astrophysics and cosmology. In this work, we present constraints on the amplitude…

宇宙学与河外天体物理 · 物理学 2018-01-25 Ken Osato , Samuel Flender , Daisuke Nagai , Masato Shirasaki , Naoki Yoshida

At high angular frequencies the thermal Sunyaev-Zel'dovich (tSZ) effect constitutes the dominant signal in the CMB sky. The tSZ effect is caused by large scale pressure fluctuations in the baryonic distribution in the Universe so its…

宇宙学与河外天体物理 · 物理学 2012-01-11 Dipak Munshi , Joseph Smidt , Shahab Joudaki , Peter Coles

Non-Gaussian statistics of late-time cosmological fields contain information beyond that captured in the power spectrum. Here we focus on one such example: the one-point probability distribution function (PDF) of the thermal…

宇宙学与河外天体物理 · 物理学 2019-05-15 Leander Thiele , J. Colin Hill , Kendrick M. Smith

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

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

(Abridged) The amplitude of the thermal Sunyaev Zel'dovich effect (tSZ) power spectrum is extremely sensitive to the abundance of galaxy clusters and therefore to fundamental cosmological parameters that control their growth, such as…

宇宙学与河外天体物理 · 物理学 2015-06-18 Ian G. McCarthy , Amandine M. C. Le Brun , Joop Schaye , Gilbert P. Holder

Combinations of galaxy surveys and cosmic microwave background secondaries, such as the thermal Sunyaev Zeldovich (tSZ) effect, are increasingly being used to jointly constrain cosmology and astrophysical properties of the gas within and…

宇宙学与河外天体物理 · 物理学 2025-10-10 M. Lokken , J. R. Bond , R. Hložek , N. J. Carlson , Z. Li , A. van Engelen

The power spectrum of unresolved thermal Sunyaev-Zeldovich (tSZ) clusters is extremely sensitive to the amplitude of the matter fluctuations. This paper present an analysis of the tSZ power spectrum using temperature power spectra of the…

宇宙学与河外天体物理 · 物理学 2025-05-16 George Efstathiou , Fiona McCarthy

The thermal Sunyaev-Zel'dovich (tSZ) effect is a spectral distortion of the cosmic microwave background (CMB) resulting from inverse Compton scattering of CMB photons with electrons in the medium of galaxy clusters. The spectrum of the tSZ…

宇宙学与河外天体物理 · 物理学 2023-05-18 David Zegeye , Thomas Crawford , Wayne Hu

The Sunyaev-Zel'dovich (SZ) effect from clusters of galaxies should yield a significant signal in cosmic microwave background(CMB) experiments at small angular scales ($\ell \ga 1000$). Experiments with sufficient frequency coverage should…

天体物理学 · 物理学 2007-05-23 Gilbert P. Holder , John E. Carlstrom
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