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Clusters of galaxies gravitationally lens the cosmic microwave background (CMB) radiation, resulting in a distinct imprint in the CMB on arcminute scales. Measurement of this effect offers a promising way to constrain the masses of galaxy…

宇宙学与河外天体物理 · 物理学 2018-02-28 E. J. Baxter , S. Raghunathan , T. M. Crawford , P. Fosalba , Z. Hou , G. P. Holder , Y. Omori , S. Patil , E. Rozo , T. M. C. Abbott , J. Annis , K. Aylor , A. Benoit-Lévy , B. A. Benson , E. Bertin , L. Bleem , E. Buckley-Geer , D. L. Burke , J. Carlstrom , A. Carnero Rosell , M. Carrasco Kind , J. Carretero , C. L. Chang , H-M. Cho , A. T. Crites , M. Crocce , C. E. Cunha , L. N. da Costa , C. B. D'Andrea , C. Davis , T. de Haan , S. Desai , M. A. Dobbs , S. Dodelson , J. P. Dietrich , P. Doel , A. Drlica-Wagner , J. Estrada , W. B. Everett , A. Fausti Neto , B. Flaugher , J. Frieman , J. García-Bellido , E. M. George , E. Gaztanaga , T. Giannantonio , D. Gruen , R. A. Gruendl , J. Gschwend , G. Gutierrez , N. W. Halverson , N. L. Harrington , W. G. Hartley , W. L. Holzapfel , K. Honscheid , J. D. Hrubes , B. Jain , D. J. James , M. Jarvis , T. Jeltema , L. Knox , E. Krause , K. Kuehn , S. Kuhlmann , N. Kuropatkin , O. Lahav , A. T. Lee , E. M. Leitch , T. S. Li , M. Lima , D. Luong-Van , A. Manzotti , M. March , D. P. Marrone , J. L. Marshall , P. Martini , J. J. McMahon , P. Melchior , F. Menanteau , S. S. Meyer , C. J. Miller , R. Miquel , L. M. Mocanu , J. J. Mohr , T. Natoli , B. Nord , R. L. C. Ogando , S. Padin , A. A. Plazas , C. Pryke , D. Rapetti , C. L. Reichardt , A. K. Romer , A. Roodman , J. E. Ruhl , E. Rykoff , M. Sako , E. Sanchez , J. T. Sayre , V. Scarpine , K. K. Schaffer , R. Schindler , M. Schubnell , I. Sevilla-Noarbe , E. Shirokoff , M. Smith , R. C. Smith , M. Soares-Santos , F. Z. Staniszewski , A. Stark , K. Story , E. Suchyta , G. Tarle , D. Thomas , M. A. Troxel , K. Vanderlinde , J. D. Vieira , A. R. Walker , R. Williamson , Y. Zhang , J. Zuntz

We present a method for measuring the masses of galaxy clusters using the imprint of their gravitational lensing signal on the cosmic microwave background (CMB) temperature anisotropies. The method first reconstructs the projected…

宇宙学与河外天体物理 · 物理学 2015-05-27 Jean-Baptiste Melin , James G. Bartlett

We report the first detection of gravitational lensing due to galaxy clusters using only the polarization of the cosmic microwave background (CMB). The lensing signal is obtained using a new estimator that extracts the lensing dipole…

宇宙学与河外天体物理 · 物理学 2019-11-06 S. Raghunathan , S. Patil , E. Baxter , B. A. Benson , L. E. Bleem , T. M. Crawford , G. P. Holder , T. McClintock , C. L. Reichardt , T. N. Varga , N. Whitehorn , P. A. R. Ade , S. Allam , A. J. Anderson , J. E. Austermann , S. Avila , J. S. Avva , D. Bacon , J. A. Beall , A. N. Bender , F. Bianchini , S. Bocquet , D. Brooks , D. L. Burke , J. E. Carlstrom , J. Carretero , F. J. Castander , C. L. Chang , H. C. Chiang , R. Citron , M. Costanzi , A. T. Crites , L. N. da Costa , S. Desai , H. T. Diehl , J. P. Dietrich , M. A. Dobbs , P. Doel , S. Everett , A. E. Evrard , C. Feng , B. Flaugher , P. Fosalba , J. Frieman , J. Gallicchio , J. García-Bellido , E. Gaztanaga , E. M. George , T. Giannantonio , A. Gilbert , R. A. Gruendl , J. Gschwend , N. Gupta , G. Gutierrez , T. de Haan , N. W. Halverson , N. Harrington , J. W. Henning , G. C. Hilton , D. L. Hollowood , W. L. Holzapfel , K. Honscheid , J. D. Hrubes , N. Huang , J. Hubmayr , K. D. Irwin , T. Jeltema , M. Carrasco Kind , L. Knox , N. Kuropatkin , O. Lahav , A. T. Lee , D. Li , M. Lima , A. Lowitz , M. A. G. Maia , J. L. Marshall , J. J. McMahon , P. Melchior , F. Menanteau , S. S. Meyer , R. Miquel , L. M. Mocanu , J. J. Mohr , J. Montgomery , C. Corbett Moran , A. Nadolski , T. Natoli , J. P. Nibarger , G. Noble , V. Novosad , R. L. C. Ogando , S. Padin , A. A. Plazas , C. Pryke , D. Rapetti , A. K. Romer , A. Roodman , A. Carnero Rosell , E. Rozo , J. E. Ruhl , E. S. Rykoff , B. R. Saliwanchik , E. Sanchez , J. T. Sayre , V. Scarpine , K. K. Schaffer , M. Schubnell , S. Serrano , I. Sevilla-Noarbe , C. Sievers , G. Smecher , M. Smith , M. Soares-Santos , A. A. Stark , K. T. Story , E. Suchyta , M. E. C. Swanson , G. Tarle , C. Tucker , K. Vanderlinde , T. Veach , J. De Vicente , J. D. Vieira , V. Vikram , G. Wang , W. L. K. Wu , V. Yefremenko , Y. Zhang

We detect weak gravitational lensing of the cosmic microwave background (CMB) at the location of the WISExSCOS (WxS) galaxies using the publicly available Planck lensing convergence map. By stacking the lensing convergence map at the…

宇宙学与河外天体物理 · 物理学 2018-08-15 Srinivasan Raghunathan , Federico Bianchini , Christian L. Reichardt

Galaxy cluster masses help to constrain cosmological parameters through the halo mass function. To get rid of major biases in the mass measurement, we directly probe the cluster gravitational potentials by observing their gravitational…

宇宙学与河外天体物理 · 物理学 2024-05-17 Alexandre Huchet

Clusters of galaxies are powerful cosmological probes, particularly if their masses can be determined. One possibility for mass determination is to study the cosmic microwave background (CMB) on small angular scales and observe deviations…

天体物理学 · 物理学 2009-11-10 Scott Dodelson

Large-scale $B$-mode polarization of the cosmic microwave background (CMB) is a prime target for current and future experiments in search of primordial gravitational waves (PGW). With increasingly sensitive instruments being deployed,…

The aim of this work is to study the anisotropic weak lensing signal associated with the mass distribution of massive clusters of galaxies using the Cosmic Microwave Background (CMB) data. For this purpose, we stack patches of the Planck…

宇宙学与河外天体物理 · 物理学 2023-10-09 Facundo Toscano , Heliana Luparello , Elizabeth Johana Gonzalez , Diego Garcia Lambas

Gravitational lensing can be used to directly constrain the projected density profile of galaxy clusters. We discuss possible future constraints from lensing of the CMB temperature and polarization, and compare to results from galaxy weak…

天体物理学 · 物理学 2009-11-13 Antony Lewis , Lindsay King

We present a stacked lensing analysis of 96 galaxy clusters selected by the thermal Sunyaev-Zel'dovich (SZ) effect in maps of the cosmic microwave background (CMB). We select foreground galaxy clusters with a $5\sigma$-level SZ threshold in…

We develop a Maximum Likelihood estimator (MLE) to measure the masses of galaxy clusters through the impact of gravitational lensing on the temperature and polarization anisotropies of the cosmic microwave background (CMB). We show that, at…

Large area surveys have detected significant samples of galaxy clusters that can be used to constrain cosmological parameters, provided that the masses of the clusters are measured robustly. To improve the calibration of cluster masses…

We use South Pole Telescope data from 2008 and 2009 to detect the non-Gaussian signature in the cosmic microwave background (CMB) produced by gravitational lensing and to measure the power spectrum of the projected gravitational potential.…

Cosmic Microwave Background (CMB) is a powerful probe to study the early universe and various cosmological models. Weak gravitational lensing affects the CMB by changing its power spectrum, but meanwhile, it also carries information about…

宇宙学与河外天体物理 · 物理学 2021-06-09 Chandra Shekhar Saraf
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