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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…

Cosmology and Nongalactic Astrophysics · Physics 2015-10-22 J. Colin Hill

We present a method based on matched multifrequency filters for extracting cluster catalogs from Sunyaev-Zel'dovich (SZ) surveys. We evaluate its performance in terms of completeness, contamination rate and photometric recovery for three…

Astrophysics · Physics 2009-11-11 J. -B. Melin , J. G. Bartlett , J. Delabrouille

We present observations using the Small Array of the Arcminute Microkelvin Imager (AMI; 14-18 GHz) of four Abell and three MACS clusters spanning 0.171-0.686 in redshift. We detect Sunyaev-Zel'dovich (SZ) signals in five of these without…

The Planck catalogues of SZ sources, PSZ1 and PSZ2, are the largest catalogues of galaxy clusters selected through their SZ signature in the full sky. In 2013, we started a long-term observational program at Canary Island observatories with…

Cosmology and Nongalactic Astrophysics · Physics 2018-09-26 A. Streblyanska , R. Barrena , J. A. Rubino-Martin , R. F. J. van der Burg , N. Aghanim , A. Aguado-Barahona , A. Ferragamo , H. Lietzen

Using available optical and X-ray catalogues of clusters and superclusters of galaxies, we build templates of tSZ emission as they should be detected by the WMAP experiment. We compute the cross-correlation of our templates with WMAP…

Astrophysics · Physics 2009-11-07 C. Hernandez-Monteagudo , J. A. Rubino-Martin

We present a catalog of 500 galaxy cluster candidates in the SPT-Deep field: a 100 deg$^2$ field that combines data from the SPT-3G and SPTpol surveys to reach noise levels of 3.0, 2.2, and 9.0 $\mu$K-arcmin at 95, 150, and 220 GHz,…

Cosmology and Nongalactic Astrophysics · Physics 2025-03-24 K. Kornoelje , L. E. Bleem , E. S. Rykoff , T. M. C. Abbott , P. A. R. Ade , M. Aguena , O. Alves , A. J. Anderson , F. Andrade-Oliveira , B. Ansarinejad , M. Archipley , M. L. N. Ashby , J. E. Austermann , D. Bacon , L. Balkenhol , J. A. Beall , K. Benabed , A. N. Bender , B. A. Benson , F. Bianchini , S. Bocquet , F. R. Bouchet , D. Brooks , D. L. Burke , M. Calzadilla , E. Camphuis , J. E. Carlstrom , A. Carnero Rosell , J. Carretero , C. L. Chang , P. Chaubal , H. C. Chiang , P. M. Chichura , A. Chokshi , T. -L. Chou , R. Citron , A. Coerver , C. Corbett Moran , M. Costanzi , T. M. Crawford , A. T. Crites , L. N. da Costa , C. Daley , T. de Haan , J. De Vicente , S. Desai , K. R. Dibert , M. A. Dobbs , P. Doel , M. Doohan , A. Doussot , D. Dutcher , W. Everett , S. Everett , C. Feng , K. R. Ferguson , I. Ferrero , K. Fichman , B. Flaugher , B. Floyd , A. Foster , D. Friedel , J. Frieman , S. Galli , J. Gallicchio , A. E. Gambrel , J. Garc'ia-Bellido , R. W. Gardner , R. Gassis , M. Gatti , F. Ge , E. M. George , G. Giannini , N. Goeckner-Wald , S. Grandis , D. Gruen , R. A. Gruendl , R. Gualtieri , F. Guidi , Guillaume Mahler , S. Guns , N. Gupta , G. Gutierrez , N. W. Halverson , S. R. Hinton , E. Hivon , G. P. Holder , D. L. Hollowood , W. L. Holzapfel , K. Honscheid , J. C. Hood , J. D. Hrubes , A. Hryciuk , N. Huang , J. Hubmayr , K. D. Irwin , J. Mena-Fernández , D. J. James , F. Kéruzoré , A. R. Khalife , M. Klein , L. Knox , M. Korman , K. Kuehn , C. -L. Kuo , O. Lahav , A. T. Lee , S. Lee , K. Levy , D. Li , M. Lima , A. E. Lowitz , A. Lowitz , C. Lu , A. Maniyar , J. L. Marshal , J. L. Marshall , E. S. Martsen , Matthew B. Bayliss , M. McDonald , J. J. McMahon , F. Menanteau , M. Millea , R. Miquel , J. J. Mohr , J. Montgomery , J. Myles , Y. Nakato , T. Natoli , J. P. Nibarger , G. I. Noble , V. Novosad , R. L. C. Ogando , Y. Omori , A. Ouellette , S. Padin , Z. Pan , S. Patil , M. E. S. Pereira , K. A. Phadke , A. Pieres , A. A. Plazas Malag'on , A. W. Pollak , K. Prabhu , C. Pryke , W. Quan , S. Raghunathan , M. Rahimi , A. Rahlin , C. L. Reichardt , M. Rodr'iguez-Monroy , A. K. Romer , M. Rouble , J. E. Ruhl , B. R. Saliwanchik , L. Salvati , S. Samuroff , E. Sanchez , A. Saro , K. K. Schaffer , E. Schiappucci , T. Schrabback , I. Sevilla-Noarbe , C. Sievers , G. Smecher , M. Smith , J. A. Sobrin , T. Somboonpanyakul , B. Stalder , A. A. Stark , E. Suchyta , M. E. C. Swanson , C. Tandoi , G. Tarle , B. Thorne , C. To , C. Trendafilova , C. Tucker , C. Umilta , T. Veach , J. D. Vieira , M. Vincenzi , A. Vitrier , Y. Wan , G. Wang , N. Weaverdyck , J. Weller , N. Whitehorn , P. Wiseman , W. L. K. Wu , V. Yefremenko , M. R. Young , J. A. Zebrowski , Y. Zhang

We investigate the effectiveness of blind surveys for radio sources and galaxy cluster thermal Sunyaev-Zel'dovich effects (TSZEs) using the four-pair, beam-switched OCRA-f radiometer on the 32-m radio telescope in Poland. The predictions…

Cosmology and Nongalactic Astrophysics · Physics 2016-11-30 Bartosz Lew , Mark Birkinshaw , Peter Wilkinson , Andrzej Kus

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…

Cosmology and Nongalactic Astrophysics · Physics 2014-11-11 Ming Li , Raul E. Angulo , Simon D. M. White , Jens Jasche

We develop a machine learning algorithm to infer the 3D cumulative radial profiles of total and gas mass in galaxy clusters from thermal Sunyaev-Zel'dovich effect maps. We generate around 73,000 mock images along various lines of sight…

Cosmology and Nongalactic Astrophysics · Physics 2023-02-02 A. Ferragamo , D. de Andres , A. Sbriglio , W. Cui , M. De Petris , G. Yepes , R. Dupuis , M. Jarraya , I. Lahouli , F. De Luca , G. Gianfagna , E. Rasia

The Sunyaev-Zeldovich (SZ) effect is a promising tool for detecting the presence of hot gas out to the galaxy cluster peripheries. We developed a spectral imaging algorithm dedicated to the SZ observations of nearby galaxy clusters with…

Cosmology and Nongalactic Astrophysics · Physics 2016-01-26 H. Bourdin , P. Mazzotta , E. Rasia

We have constructed an all-sky catalog of optical AGNs with $z < 0.09$, based on optical spectroscopy, from the parent sample of galaxies in the 2MASS Redshift Survey (2MRS), a near-complete census of the nearby universe. Our catalog…

Astrophysics of Galaxies · Physics 2019-04-04 Ingyin Zaw , Yan-Ping Chen , Glennys R Farrar

We use mock Sunyaev-Zel'dovich effect (SZE) maps to investigate how well the Planck mission might find and characterize clusters of galaxies. We discuss different combinations of frequency maps and different methods for identifying cluster…

Astrophysics · Physics 2008-11-26 Martin White

We present weak gravitational lensing measurements of a sample of 157 clusters within the Kilo Degree Survey (KiDS), detected with a $>5\sigma$ thermal Sunyaev-Zel'dovich (SZ) signal by the Atacama Cosmology Telescope (ACT). Using a…

By cross-correlating templates constructed from the 2 Micron All Sky Survey (2MASS) Extended Source (XSC) catalogue with WMAP's first year data, we search for the thermal Sunyaev-Zel'dovich signature induced by hot gas in the local…

Astrophysics · Physics 2009-11-10 C. Hernandez-Monteagudo , R. Genova-Santos , F. Atrio-Barandela

Galaxy clusters furnish extremely rich information on the contents and structure of our universe. The potential of galaxy cluster studies to constrain dark energy, for example, motivates a number of ambitious cluster surveys. Among these,…

Astrophysics · Physics 2007-05-23 James G. Bartlett

We present measurements of the radial profiles of the mass and galaxy number density around Sunyaev-Zel'dovich-selected clusters using both weak lensing and galaxy counts. The clusters are selected from the Atacama Cosmology Telescope Data…

Cosmology and Nongalactic Astrophysics · Physics 2021-09-15 T. Shin , B. Jain , S. Adhikari , E. J. Baxter , C. Chang , S. Pandey , A. Salcedo , D. H. Weinberg , A. Amsellem , N. Battaglia , M. Belyakov , T. Dacunha , S. Goldstein , A. V. Kravtsov , T. N. Varga , T. M. C. Abbott , M. Aguena , A. Alarcon , S. Allam , A. Amon , F. Andrade-Oliveira , J. Annis , D. Bacon , K. Bechtol , M. R. Becker , G. M. Bernstein , E. Bertin , S. Bocquet , J. R. Bond , D. Brooks , E. Buckley-Geer , D. L. Burke , A. Campos , A. Carnero Rosell , M. Carrasco Kind , J. Carretero , R. Chen , A. Choi , M. Costanzi , L. N. da Costa , J. DeRose , S. Desai , J. De Vicente , M. J. Devlin , H. T. Diehl , J. P. Dietrich , S. Dodelson , P. Doel , C. Doux , A. Drlica-Wagner , K. Eckert , J. Elvin-Poole , S. Everett , S. Ferraro , I. Ferrero , A. Ferté , B. Flaugher , J. Frieman , P. A. Gallardo , M. Gatti , E. Gaztanaga , D. W. Gerdes , D. Gruen , R. A. Gruendl , G. Gutierrez , I. Harrison , W. G. Hartley , J. C. Hill , M. Hilton , S. R. Hinton , D. L. Hollowood , J. P. Hughes , D. J. James , M. Jarvis , T. Jeltema , B. J. Koopman , E. Krause , K. Kuehn , N. Kuropatkin , O. Lahav , M. Lima , M. Lokken , N. MacCrann , M. S. Madhavacheril , M. A. G. Maia , J. McCullough , J. McMahon , P. Melchior , F. Menanteau , R. Miquel , J. J. Mohr , K. Moodley , R. Morgan , J. Myles , F. Nati , A. Navarro-Alsina , M. D. Niemack , R. L. C. Ogando , L. A. Page , A. Palmese , B. Partridge , F. Paz-Chinchón , M. E. S. Pereira , A. Pieres , A. A. Plazas Malagón , J. Prat , M. Raveri , M. Rodriguez-Monroy , R. P. Rollins , A. K. Romer , E. S. Rykoff , M. Salatino , C. Sánchez , E. Sanchez , B. Santiago , V. Scarpine , A. Schillaci , L. F. Secco , S. Serrano , I. Sevilla-Noarbe , E. Sheldon , B. D. Sherwin , C. Sifón , M. Smith , M. Soares-Santos , S. T. Staggs , E. Suchyta , M. E. C. Swanson , G. Tarle , D. Thomas , C. To , M. A. Troxel , I. Tutusaus , E. M. Vavagiakis , J. Weller , E. J. Wollack , B. Yanny , B. Yin , Y. Zhang

Thanks to advances in detector technology and observing techniques, true Sunyaev-Zel'dovich (SZ) surveys will soon become a reality. This opens up a new window into the Universe, in many ways analogous to the X-ray band and inherently…

Astrophysics · Physics 2007-05-23 James G. Bartlett