相关论文: Identification of galaxy clusters in cosmic microw…

Prospects for measuring the relative velocities of galaxy clusters in photometric surveys using the kinetic Sunyaev-Zel'dovich Effect

We consider the prospects for measuring the pairwise kinetic Sunyaev-Zel'dovich (kSZ) signal from galaxy clusters discovered in large photometric surveys such as the Dark Energy Survey (DES). We project that the DES cluster sample will, in…

宇宙学与河外天体物理 · 物理学 2015-06-12 Ryan Keisler , Fabian Schmidt

Sunyaev Zel'dovich observations of a statistically complete sample of galaxy clusters with OCRA-p

We present 30 GHz Sunyaev Zel'dovich observations of a statistically complete sample of galaxy clusters with OCRA-p. The clusters are the 18 most X-ray luminous clusters at z > 0.2 in the ROSAT Brightest Cluster Sample. We correct for…

宇宙学与河外天体物理 · 物理学 2015-05-28 Katy Lancaster , Mark Birkinshaw , Marcin P. Gawronski , Richard Battye , Ian Browne , Richard Davis , Paul Giles , Roman Feiler , Andrzej Kus , Bartosz Lew , Stuart Lowe , Ben Maughan , Abdulaziz Mohammad , Bogna Pazderska , Eugeniusz Pazderski , Mike Peel , Boud Roukema , Peter Wilkinson

Fundamental Physics from Future Weak-Lensing Calibrated Sunyaev-Zel'dovich Galaxy Cluster Counts

Future high-resolution measurements of the cosmic microwave background (CMB) will produce catalogs of tens of thousands of galaxy clusters through the thermal Sunyaev-Zel'dovich (tSZ) effect. We forecast how well different configurations of…

宇宙学与河外天体物理 · 物理学 2018-01-01 Mathew Madhavacheril , Nicholas Battaglia , Hironao Miyatake

The Sunyaev-Zel'dovich Effect and Large-Scale Structure

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

Planck 2013 results. XX. Cosmology from Sunyaev-Zeldovich cluster counts

We present constraints on cosmological parameters using number counts as a function of redshift for a sub-sample of 189 galaxy clusters from the Planck SZ (PSZ) catalogue. The PSZ is selected through the signature of the Sunyaev--Zeldovich…

宇宙学与河外天体物理 · 物理学 2015-06-15 Planck Collaboration , P. A. R. Ade , N. Aghanim , C. Armitage-Caplan , M. Arnaud , M. Ashdown , F. Atrio-Barandela , J. Aumont , C. Baccigalupi , A. J. Banday , R. B. Barreiro , R. Barrena , J. G. Bartlett , E. Battaner , R. Battye , K. Benabed , A. Benoît , A. Benoit-Lévy , J. -P. Bernard , M. Bersanelli , P. Bielewicz , I. Bikmaev , A. Blanchard , J. Bobin , J. J. Bock , H. Böhringer , A. Bonaldi , J. R. Bond , J. Borrill , F. R. Bouchet , H. Bourdin , M. Bridges , M. L. Brown , M. Bucher , R. Burenin , C. Burigana , R. C. Butler , J. -F. Cardoso , P. Carvalho , A. Catalano , A. Challinor , A. Chamballu , R. -R. Chary , L. -Y Chiang , H. C. Chiang , G. Chon , P. R. Christensen , S. Church , D. L. Clements , S. Colombi , L. P. L. Colombo , F. Couchot , A. Coulais , B. P. Crill , A. Curto , F. Cuttaia , A. Da Silva , H. Dahle , L. Danese , R. D. Davies , R. J. Davis , P. de Bernardis , A. de Rosa , G. de Zotti , J. Delabrouille , J. -M. Delouis , J. Démoclès , F. -X. Désert , C. Dickinson , J. M. Diego , K. Dolag , H. Dole , S. Donzelli , O. Doré , M. Douspis , X. Dupac , G. Efstathiou , T. A. Enßlin , H. K. Eriksen , F. Finelli , I. Flores-Cacho , O. Forni , M. Frailis , E. Franceschi , S. Fromenteau , S. Galeotta , K. Ganga , R. T. Génova-Santos , M. Giard , G. Giardino , Y. Giraud-Héraud , J. González-Nuevo , K. M. Górski , S. Gratton , A. Gregorio , A. Gruppuso , F. K. Hansen , D. Hanson , D. Harrison , S. Henrot-Versillé , C. Hernández-Monteagudo , D. Herranz , S. R. Hildebrandt , E. Hivon , M. Hobson , W. A. Holmes , A. Hornstrup , W. Hovest , K. M. Huffenberger , G. Hurier , T. R. Jaffe , A. H. Jaffe , W. C. Jones , M. Juvela , E. Keihänen , R. Keskitalo , I. Khamitov , T. S. Kisner , R. Kneissl , J. Knoche , L. Knox , M. Kunz , H. Kurki-Suonio , G. Lagache , A. Lähteenmäki , J. -M. Lamarre , A. Lasenby , R. J. Laureijs , C. R. Lawrence , J. P. Leahy , R. Leonardi , J. León-Tavares , J. Lesgourgues , A. Liddle , M. Liguori , P. B. Lilje , M. Linden-Vørnle , M. López-Caniego , P. M. Lubin , J. F. Macías-Pérez , B. Maffei , D. Maino , N. Mandolesi , A. Marcos-Caballero , M. Maris , D. J. Marshall , P. G. Martin , E. Martínez-González , S. Masi , S. Matarrese , F. Matthai , P. Mazzotta , P. R. Meinhold , A. Melchiorri , J. -B. Melin , L. Mendes , A. Mennella , M. Migliaccio , S. Mitra , M. -A. Miville-Deschênes , A. Moneti , L. Montier , G. Morgante , D. Mortlock , A. Moss , D. Munshi , P. Naselsky , F. Nati , P. Natoli , C. B. Netterfield , H. U. Nørgaard-Nielsen , F. Noviello , D. Novikov , I. Novikov , S. Osborne , C. A. Oxborrow , F. Paci , L. Pagano , F. Pajot , D. Paoletti , B. Partridge , F. Pasian , G. Patanchon , O. Perdereau , L. Perotto , F. Perrotta , F. Piacentini , M. Piat , E. Pierpaoli , D. Pietrobon , S. Plaszczynski , E. Pointecouteau , G. Polenta , N. Ponthieu , L. Popa , T. Poutanen , G. W. Pratt , G. Prézeau , S. Prunet , J. -L. Puget , J. P. Rachen , R. Rebolo , M. Reinecke , M. Remazeilles , C. Renault , S. Ricciardi , T. Riller , I. Ristorcelli , G. Rocha , M. Roman , C. Rosset , G. Roudier , M. Rowan-Robinson , J. A. Rubiño-Martín , B. Rusholme , M. Sandri , D. Santos , G. Savini , D. Scott , M. D. Seiffert , E. P. S. Shellard , L. D. Spencer , J. -L. Starck , V. Stolyarov , R. Stompor , R. Sudiwala , R. Sunyaev , F. Sureau , D. Sutton , A. -S. Suur-Uski , J. -F. Sygnet , J. A. Tauber , D. Tavagnacco , L. Terenzi , L. Toffolatti , M. Tomasi , M. Tristram , M. Tucci , J. Tuovinen , M. Türler , G. Umana , L. Valenziano , J. Valiviita , B. Van Tent , P. Vielva , F. Villa , N. Vittorio , L. A. Wade , B. D. Wandelt , J. Weller , M. White , S. D. M. White , D. Yvon , A. Zacchei , A. Zonca

An SZ-selected sample of the most massive galaxy clusters in the 2500-square-degree South Pole Telescope survey

The South Pole Telescope (SPT) is currently surveying 2500 deg^2 of the southern sky to detect massive galaxy clusters out to the epoch of their formation using the Sunyaev-Zel'dovich (SZ) effect. This paper presents a catalog of the 26…

宇宙学与河外天体物理 · 物理学 2015-05-20 R. Williamson , B. A. Benson , F. W. High , K. Vanderlinde , P. A. R. Ade , K. A. Aird , K. Andersson , R. Armstrong , M. L. N. Ashby , M. Bautz , G. Bazin , E. Bertin , L. E. Bleem , M. Bonamente , M. Brodwin , J. E. Carlstrom , C. L. Chang , S. C. Chapman , A. Clocchiatti , T. M. Crawford , A. T. Crites , T. de Haan , S. Desai , M. A. Dobbs , J. P. Dudley , G. G. Fazio , R. J. Foley , W. R. Forman , G. Garmire , E. M. George , M. D. Gladders , A. H. Gonzalez , N. W. Halverson , G. P. Holder , W. L. Holzapfel , S. Hoover , J. D. Hrubes , C. Jones , M. Joy , R. Keisler , L. Knox , A. T. Lee , E. M. Leitch , M. Lueker , D. Luong-Van , D. P. Marrone , J. J. McMahon , J. Mehl , S. S. Meyer , J. J. Mohr , T. E. Montroy , S. S. Murray , S. Padin , T. Plagge , C. Pryke , C. L. Reichardt , A. Rest , J. Ruel , J. E. Ruhl , B. R. Saliwanchik , A. Saro , K. K. Schaffer , L. Shaw , E. Shirokoff , J. Song , H. G. Spieler , B. Stalder , S. A. Stanford , Z. Staniszewski , A. A. Stark , K. Story , C. W. Stubbs , J. D. Vieira , A. Vikhlinin , A. Zenteno

Measuring the Thermal Sunyaev-Zel'dovich Effect Through the Cross Correlation of Planck and WMAP Maps with ROSAT Galaxy Cluster Catalogs

We measure a significant correlation between the thermal Sunyaev-Zel'dovich effect in the Planck and WMAP maps and an X-ray cluster map based on ROSAT. We use the 100, 143 and 343 GHz Planck maps and the WMAP 94 GHz map to obtain this…

宇宙学与河外天体物理 · 物理学 2014-02-14 Amir Hajian , Nicholas Battaglia , David N. Spergel , J. Richard Bond , Christoph Pfrommer , Jonathan L. Sievers

SPT-SZ MCMF: An extension of the SPT-SZ catalog over the DES region

We present an extension to a Sunyaev-Zel'dovich Effect (SZE) selected cluster catalog based on observations from the South Pole Telescope (SPT); this catalog extends to lower signal-to-noise than the previous SPT-SZ catalog and therefore…

宇宙学与河外天体物理 · 物理学 2023-10-05 M. Klein , J. J. Mohr , S. Bocquet , M. Aguena , S. W. Allen , O. Alves , B. Ansarinejad , M. L. N. Ashby , D. Bacon , M. Bayliss , B. A. Benson , L. E. Bleem , M. Brodwin , D. Brooks , E. Bulbul , D. L. Burke , R. E. A. Canning , J. E. Carlstrom , A. Carnero Rosell , J. Carretero , C. L. Chang , C. Conselice , M. Costanzi , A. T. Crites , L. N. da Costa , M. E. S. Pereira , T. M. Davis , J. De Vicente , S. Desai , T. de Haan , M. A. Dobbs , P. Doel , I. Ferrero , A. M. Flores , J. Frieman , E. M. George , G. Giannini , M. D. Gladders , A. H. Gonzalez , S. Grandis , D. Gruen , R. A. Gruendl , G. Gutierrez , N. W. Halverson , S. R. Hinton , G. P. Holder , D. L. Hollowood , W. L. Holzapfel , K. Honscheid , J. D. Hrubes , N. Huang , D. J. James , G. Khullar , K. Kim , L. Knox , R. Kraft , F. Kéruzoré , A. T. Lee , D. Luong-Van , G. Mahler , A. Mantz , D. P. Marrone , J. L. Marshall , M. McDonald , J. J. McMahon , J. Mena-Fernández , F. Menanteau , S. S. Meyer , R. Miquel , J. Myles , S. Padin , A. Pieres , A. A. Plazas Malagón , C. Pryke , C. L. Reichardt , K. Reil , J. Roberson , A. K. Romer , C. Romero , J. E. Ruhl , B. R. Saliwanchik , L. Salvati , E. Sanchez , A. Saro , K. K. Schaffer , T. Schrabback , M. Schubnell , I. Sevilla-Noarbe , K. Sharon , E. Shirokoff , M. Smith , T. Somboonpanyakul , B. Stalder , S. A. Stanford , A. A. Stark , V. Strazzullo , E. Suchyta , M. E. C. Swanson , G. Tarle , C. To , K. Vanderlinde , J. D. Vieira , A. von der Linden , N. Weaverdyck , R. Williamson , P. Wiseman , M. Young

The Sunyaev-Zeldovich Background

The cosmic background due to the Sunyaev-Zeldovich (SZ) effect is expected to be the largest signal at mm and cm wavelengths at a resolution of a few arcminutes. We investigate some simple statistics of SZ maps and their scaling with the…

天体物理学 · 物理学 2009-11-13 Gilbert Holder , Ian G. McCarthy , Arif Babul

The Planck Sunyaev-Zel'dovich vs. the X-ray View of the Coma Cluster

The Planck collaboration has recently published precise and resolved measurements of the Sunyaev-Zel'dovich effect in Abell 1656 (the Coma cluster of galaxies), so directly gauging the electron pressure profile in the intracluster plasma.…

宇宙学与河外天体物理 · 物理学 2015-06-12 R. Fusco-Femiano , A. Lapi , A. Cavaliere

Sunyaev--Zel'dovich profile fitting with joint AMI-Planck analysis

We develop a Bayesian method of analysing Sunyaev-Zel'dovich measurements of galaxy clusters obtained from the Arcminute Microkelvin Imager (AMI) radio interferometer system and from the Planck satellite, using a joint likelihood function…

宇宙学与河外天体物理 · 物理学 2020-02-11 Yvette C. Perrott , Kamran Javid , Pedro Carvalho , Patrick J. Elwood , Michael P. Hobson , Anthony N. Lasenby , Malak Olamaie , Richard D. E. Saunders

Evidence for relativistic Sunyaev-Zeldovich effect in Planck CMB maps with an average electron-gas temperature of $T_{\rm e}\simeq 5$ keV

Stacking the public Planck CMB temperature maps (NILC, SMICA, SEVEM, Commander) on galaxy clusters from Planck catalogues reveals substantial residual contamination from thermal Sunyaev-Zeldovich (tSZ) emission. Unexpectedly, stacking…

宇宙学与河外天体物理 · 物理学 2025-03-05 Mathieu Remazeilles , Jens Chluba

Constraining the Baryon Abundance with the Kinematic Sunyaev-Zel'dovich Effect: Projected-Field Detection Using Planck, WMAP, and unWISE

The kinematic Sunyaev-Zel'dovich (kSZ) effect -- the Doppler boosting of cosmic microwave background (CMB) photons scattering off free electrons with non-zero line-of-sight velocity -- is an excellent probe of the distribution of baryons in…

宇宙学与河外天体物理 · 物理学 2021-08-25 Aleksandra Kusiak , Boris Bolliet , Simone Ferraro , J. Colin Hill , Alex Krolewski

Sunyaev-Zel'dovich Cluster Profiles Measured with the South Pole Telescope

We present Sunyaev-Zel'dovich measurements of 15 massive X-ray selected galaxy clusters obtained with the South Pole Telescope. The Sunyaev-Zel'dovich (SZ) cluster signals are measured at 150 GHz, and concurrent 220 GHz data are used to…

宇宙学与河外天体物理 · 物理学 2014-11-20 T. Plagge , B. A. Benson , P. A. R. Ade , K. A. Aird , L. E. Bleem , J. E. Carlstrom , C. L. Chang , H. -M. Cho , T. M. Crawford , A. T. Crites , T. de Haan , M. A. Dobbs , E. M. George , N. R. Hall , N. W. Halverson , G. P. Holder , W. L. Holzapfel , J. D. Hrubes , M. Joy , R. Keisler , L. Knox , A. T. Lee , E. M. Leitch , M. Lueker , D. Marrone , J. J. McMahon , J. Mehl , S. S. Meyer , J. J. Mohr , T. E. Montroy , S. Padin , C. Pryke , C. L. Reichardt , J. E. Ruhl , K. K. Schaffer , L. Shaw , E. Shirokoff , H. G. Spieler , B. Stalder , Z. Staniszewski , A. A. Stark , K. Vanderlinde , J. D. Vieira , R. Williamson , O. Zahn

A Measurement of Gas Temperatures in Galaxy Clusters using the Relativistic Sunyaev-Zeldovich Effect

The hot gas in clusters of galaxies creates a distinctive spectral distortion in the cosmic microwave background (CMB) via the Sunyaev-Zeldovich (SZ) effect. To first order, the shape of the spectral distortion is fixed, but relativistic…

宇宙学与河外天体物理 · 物理学 2019-03-13 Adam D. Hincks , Ricardo Génova-Santos , Gemma Luzzi , Elia Stefano Battistelli

Joint signal extraction from galaxy clusters in X-ray and SZ surveys: A matched-filter approach

The hot ionized gas of the intra-cluster medium emits thermal radiation in the X-ray band and also distorts the cosmic microwave radiation through the Sunyaev-Zel'dovich (SZ) effect. Combining these two complementary sources of information…

宇宙学与河外天体物理 · 物理学 2016-06-08 Paula Tarrío , Jean-Baptiste Melin , Monique Arnaud , Gabriel W. Pratt

Measurement of the pairwise kinematic Sunyaev-Zeldovich effect with Planck and BOSS data

We present a new measurement of the kinetic Sunyaev-Zeldovich effect (kSZ) using Planck cosmic microwave background (CMB) and Baryon Oscillation Spectroscopic Survey (BOSS) data. Using the `LowZ North/South' galaxy catalogue from BOSS DR12,…

宇宙学与河外天体物理 · 物理学 2018-01-24 Yi-Chao Li , Yin-Zhe Ma , Mathieu Remazeilles , Kavilan Moodley

SZ cluster science with the Planck HFI experiment

In the near future the Planck satellite will gather impressive information about the anisotropies of the cosmic microwave background and about the galaxy clusters which perturb that signal. We will here review the ability of Planck to…

天体物理学 · 物理学 2007-05-23 Steen H. Hansen

Cosmological constraints from Planck galaxy clusters with CMB lensing mass bias calibration

We present a new cosmological analysis of the galaxy clusters in the Planck MMF3 cosmology sample with a cosmic microwave background (CMB) lensing calibration of the cluster masses. As demonstrated by Planck, galaxy clusters detected via…

宇宙学与河外天体物理 · 物理学 2019-08-22 Íñigo Zubeldia , Anthony Challinor

Cosmology with Sunyaev-Zeldovich observations from space

In order to assess the potential of future microwave anisotropy space experiments for detecting clusters by their Sunyaev-Zeldovich (SZ) thermal effect, we have simulated maps of the large scale distribution of their Compton parameter $y$…

天体物理学 · 物理学 2007-05-23 N. Aghanim , A. De Luca , F. R. Bouchet , G. Gispert , J. L. Puget