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The Sunyaev-Zel'dovich effect is a powerful tool for cosmology that can be used to measure the radial peculiar velocities of galaxy clusters, and thus to test, and constrain, theories of structure formation and evolution. This requires, in…

天体物理学 · 物理学 2009-11-06 N. Aghanim , K. M. Górski , J. -L. Puget

In recent years, observations of the Sunyaev-Zeldovich (SZ) effect have had significant cosmological implications and have begun to serve as a powerful and independent probe of the warm and hot gas that pervades the Universe. As a few…

The Sunyaev-Zel'dovich effect provides a useful probe of cosmology and structure formation in the Universe. Recent years have seen rapid progress in both quality and quantity of its measurements. In this review, we overview cosmological and…

宇宙学与河外天体物理 · 物理学 2014-07-02 Tetsu Kitayama

This brief, general review the Sunyaev-Zeldovich (S-Z) effect includes a description of the calculation of the total intensity change and polarization components, a discussion of the basic properties of the S-Z power spectrum and cluster…

天体物理学 · 物理学 2008-11-26 Y. Rephaeli , S. Sadeh , M. Shimon

Modern interferometers routinely provide radio-astronomical images down to subarcsecond resolution. However, interferometers filter out spatial scales larger than those sampled by the shortest baselines, which affects the measurement of…

(Abriged version) The Sunyaev-Zel'dovich (SZ) effect of galaxy clusters is a tool to measure three quantities: Compton parameter, electron temperature, and cluster peculiar velocity. However, a major problem is non-removed contamination by…

天体物理学 · 物理学 2009-11-10 Nabila Aghanim , Steen H. Hansen , Guilaine Lagache

Interferometric observations of the Sunyaev-Zel'dovich Effect (SZE) toward clusters of galaxies provide sensitive cosmological probes. We present results from 1 cm observations (at BIMA and OVRO) of a large, intermediate redshift cluster…

天体物理学 · 物理学 2009-10-31 J. J. Mohr , J. E. Carlstrom , G. P. Holder , W. L. Holzapfel , M. K. Joy , E. M. Leitch , E. D. Reese

I discuss galaxy cluster surveys based on the Sunyaev--Zel'dovich effect and their relevance for cosmological studies. The unique aspects of cluster selection by this method are emphasized and certain issues of surveying are addressed.…

天体物理学 · 物理学 2007-05-23 J. G. Bartlett

The ionosphere is the main driver of a series of systematic effects that limit our ability to explore the low frequency (<1 GHz) sky with radio interferometers. Its effects become increasingly important towards lower frequencies and are…

天体物理仪器与方法 · 物理学 2018-08-08 F. de Gasperin , M. Mevius , D. A. Rafferty , H. T. Intema , R. A. Fallows

We study the prospects for extracting detailed statistical properties of the Sunyaev-Zel'dovich (SZ) effect associated with large scale structure using upcoming multifrequency CMB experiments. The greatest obstacle to detecting the…

天体物理学 · 物理学 2009-10-07 Asantha Cooray , Wayne Hu , Max Tegmark

This chapter aims to provide a review of the basics of 21 cm interferometric observations and its methodologies. A summary of the main concepts of radio interferometry and their connection with the 21 cm observables - power spectra and…

天体物理仪器与方法 · 物理学 2019-09-27 G. Bernardi

The Sunyaev-Zel'dovich (SZ) effect of galaxy clusters is characterized by three parameters: Compton parameter, electron temperature and cluster peculiar velocity. In the present study we consider the problem of extracting these parameters…

天体物理学 · 物理学 2009-11-07 Nabila Aghanim , Steen H. Hansen , Sergio Pastor , Dmitry V. Semikoz

The well known Sunyaev-Zel'dovich (SZ) effect is reexamined using a Doppler shift type mechanism arising from the scattering of photons by electrons in an optically thin gas. The results are in excellent agreement with the observational…

天体物理学 · 物理学 2007-05-23 A. Sandoval-Villalbazo , L. S. Garcia-Colin

The Sunyaev-Zel'dovich effect causes a change in the apparent brightness of the Cosmic Microwave Background Radiation towards a cluster of galaxies or any other reservoir of hot plasma. Measurements of the effect provide distinctly…

天体物理学 · 物理学 2008-11-26 M. Birkinshaw

We investigate the prospects for observing a specific spectral distortion of the cosmic microwave background, which occurs due to the anisotropy of the radiation when it is scattered by hot plasma of galaxy clusters. Detection of this…

宇宙学与河外天体物理 · 物理学 2025-12-09 D. I. Novikov , A. O. Mihalchenko , A. M. Osipova , K. O. Parfenov , S. V. Pilipenko

The Sunyaev-Zel'dovich effect is a small spectral distortion of the spectrum of the cosmic microwave background (CMB) radiation. This slight distortion is described by the Bose-Einstein (mu-type) distribution with non-zero chemical…

综合物理 · 物理学 2018-10-17 Anatoliy I Fisenko , Vladimir F Lemberg

In this paper we propose generalizations of the Sokolov-Ternov and Unruh effects, and discuss the possibility to measure them on different experiments.

高能物理 - 唯象学 · 物理学 2025-12-22 Emil T. Akhmedov , Kirill Gubarev

Comptonization of the cosmic microwave background (CMB) radiation by hot gas in clusters of galaxies - the Sunyaev-Zeldovich (S-Z) effect - is of great astrophysical and cosmological significance. In recent years observations of the effect…

天体物理学 · 物理学 2007-05-23 Yoel Rephaeli

The Sunyaev-Zel'dovich (SZ) effect is a powerful tool for studying clusters of galaxies and cosmology. Large mm-wave telescopes are now routinely detecting and mapping the SZ effect in a number of clusters, measure their comptonisation…

An observing campaign was devoted to the search for the Sunyaev-Zeldovich (S-Z) effect towards X-ray ROSAT Clusters in the millimetric spectral domain. A double channel (1.2 and 2 {\it mm}) photometer was installed at the focus of the 15m…

天体物理学 · 物理学 2007-05-23 P. Andreani , G. Dall'Oglio , L. Pizzo , L. Martinis , P. Shaver , H. Boehringer , R. Lemke , L. -A. Nyman , R. Booth , N. Whyborn
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