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We develop and test a new statistical method to measure the kinematic Sunyaev-Zel'dovich (kSZ) effect. A sample of independently detected clusters is combined with the cosmic flow field predicted from a galaxy redshift survey in order to…

宇宙学与河外天体物理 · 物理学 2014-11-11 Ming Li , Raul E. Angulo , Simon D. M. White , Jens Jasche

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

Measurements of secondary cosmic microwave background (CMB) anisotropies, such as the Sunyaev-Zel'dovich (SZ) effect, will enable new tests of neutrino and dark sector properties. The kinetic SZ (kSZ) effect is produced by cosmological…

宇宙学与河外天体物理 · 物理学 2023-03-07 Gerrit S. Farren , Daniel Grin , Andrew H. Jaffe , Renée Hložek , David J. E. Marsh

The peculiar motions of massive halos probe the distribution of matter in the universe, the gravitational potential, and the history of cosmic structure growth. The kinematic Sunyaev-Zeldovich (kSZ) effect offers a robust observational…

宇宙学与河外天体物理 · 物理学 2025-10-24 Patricio A. Gallardo , Yulin Gong , Boryana Hadzhiyska , Yun-Hsin Hsu

We propose a method of searching for radio sources exhibiting the Sunyaev-Zeldovich effect in the multi-frequency emission maps from the Planck mission data using a convolutional neural network. A catalog for recognizing radio sources is…

宇宙学与河外天体物理 · 物理学 2021-04-22 O. V. Verkhodanov , A. P. Topchieva , A. D. Oronovskaya , S. A. Bazrov , D. A. Shorin

The CMB temperature-redshift relation, T_CMB(z)=T_0(1+z), is a key prediction of the standard cosmology, but is violated in many non standard models. Constraining possible deviations to this law is an effective way to test the LambdaCDM…

宇宙学与河外天体物理 · 物理学 2015-09-16 G. Luzzi , R. T. Génova-Santos , C. J. A. P. Martins , M. De Petris , L. Lamagna

The interaction of the cosmic microwave background (CMB) with the hot gas in clusters of galaxies, the so-called Sunyaev--Zel'dovich (SZ) effect, is a very useful tool that allows us to determine the physical conditions in such clusters and…

宇宙学与河外天体物理 · 物理学 2017-05-24 M. Lopez-Corredoira , C. M. Gutierrez , R. T. Genova-Santos

[ABRIDGED] Inhomogeneous reionization acts as a source of arcminute-scale anisotropies in the cosmic microwave background (CMB), the most important of which is the kinetic Sunyaev-Zel'dovich (kSZ) effect. Observational efforts with the…

宇宙学与河外天体物理 · 物理学 2015-06-03 Andrei Mesinger , Matthew McQuinn , David Spergel

The thermal Sunyaev-Zel'dovich (tSZ) effect measures the line-of-sight projection of the thermal pressure of free electrons and lacks any redshift information. By cross correlating the tSZ effect with an external cosmological tracer we can…

宇宙学与河外天体物理 · 物理学 2014-06-11 Geraint Pratten , Dipak Munshi

Observational cosmology has become an important laboratory for testing General Relativity, with searches for modified gravity forming a significant portion of the science case for existing and future surveys. In this paper, we illustrate…

宇宙学与河外天体物理 · 物理学 2019-10-23 Zhen Pan , Matthew C. Johnson

In this review we present a comprehensive discussion of peculiar velocity field measured recently on very large scales with a novel method using X-ray galaxy clusters as tracers. The measurement is based on the kinematic component of the…

宇宙学与河外天体物理 · 物理学 2012-02-06 A. Kashlinsky , F. Atrio-Barandela , H. Ebeling

A new generation of CMB experiments will soon make sensitive high resolution maps of the microwave sky. At angular scales less than $\sim$10 arcminutes, most CMB anisotropies are generated at z $< 1000$, rather than at the surface of last…

天体物理学 · 物理学 2011-02-11 Mario A. Riquelme , David N. Spergel

The thermal Sunyaev-Zel'dovich (tSZ) effect, the inverse-Compton scattering of cosmic microwave background (CMB) photons off high-energy electrons, is a powerful probe of hot, ionized gas in the Universe. It is often measured via…

宇宙学与河外天体物理 · 物理学 2025-08-15 Kristen M. Surrao , Shivam Pandey , J. Colin Hill , Eric J. Baxter

The imaging of galaxy clusters through the Sunyaev--Zel'dovich effect is a valuable tool to probe the thermal pressure of the intra-cluster gas, especially in the outermost regions where X-ray observations suffer from photon statistics. For…

宇宙学与河外天体物理 · 物理学 2019-10-09 Anna Silvia Baldi , Hervé Bourdin , Pasquale Mazzotta , Dominique Eckert , Stefano Ettori , Massimo Gaspari , Mauro Roncarelli

The cosmic microwave background (CMB) photons that scatter off free electrons in the large-scale structure induce a linear polarization pattern proportional to the remote CMB temperature quadrupole observed in the electrons' rest frame. The…

宇宙学与河外天体物理 · 物理学 2022-10-12 Selim C. Hotinli , Gilbert P. Holder , Matthew C. Johnson , Marc Kamionkowski

Upcoming cosmic shear analyses will precisely measure the cosmic matter distribution at low redshifts. At these redshifts, the matter distribution is affected by galaxy formation physics, primarily baryonic feedback from star formation and…

宇宙学与河外天体物理 · 物理学 2024-02-02 Chun-Hao To , Shivam Pandey , Elisabeth Krause , Nihar Dalal , Dhayaa Anbajagane , David H. Weinberg

The thermal Sunyaev$-$Zel'dovich (SZ) effect offers a unique probe of the hot and diffuse universe that could help close the missing baryon problem. Traditional extractions of the SZ effect, however, exhibit systematic noise that may lead…

天体物理仪器与方法 · 物理学 2025-09-09 Cameron T. Pratt , Zhijie Qu , Joel N. Bregman

A generic search is presented for the associated production of a Z boson or a photon with an additional unspecified massive particle X, pp $\to$ pp + Z/$\gamma$ + X, in proton-tagged events from proton-proton collisions at $\sqrt{s}$ = 13…

高能物理 - 实验 · 物理学 2023-09-22 CMS Collaboration , TOTEM Collaboration