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We present a detection of the splashback feature around galaxy clusters selected using their Sunyaev-Zel'dovich (SZ) signal. Recent measurements of the splashback feature around optically selected galaxy clusters have found that the…

Cosmology and Nongalactic Astrophysics · Physics 2019-05-27 T. Shin , S. Adhikari , E. J. Baxter , C. Chang , B. Jain , N. Battaglia , L. Bleem , S. Bocquet , J. DeRose , D. Gruen , M. Hilton , A. Kravtsov , T. McClintock , E. Rozo , E. S. Rykoff , T. N. Varga , R. H. Wechsler , H. Wu , S. Aiola , S. Allam , K. Bechtol , B. A. Benson , E. Bertin , J. R. Bond , M. Brodwin , D. Brooks , E. Buckley-Geer , D. L. Burke , J. E. Carlstrom , A. Carnero Rosell , M. Carrasco Kind , J. Carretero , F. J. Castander , S. K. Choi , C. E. Cunha , T. M. Crawford , L. N. da Costa , J. De Vicente , S. Desai , M. J. Devlin , J. P. Dietrich , P. Doel , J. Dunkley , T. F. Eifler , A. E. Evrard , B. Flaugher , P. Fosalba , P. A. Gallardo , J. García-Bellido , E. Gaztanaga , D. W. Gerdes , M. Gralla , R. A. Gruendl , J. Gschwend , N. Gupta , G. Gutierrez , W. G. Hartley , J. C. Hill , S. P. Ho , D. L. Hollowood , K. Honscheid , B. Hoyle , K. Huffenberger , J. P. Hughes , D. J. James , T. Jeltema , A. G. Kim , E. Krause , K. Kuehn , O. Lahav , M. Lima , M. S. Madhavacheril , M. A. G. Maia , J. L. Marshall , L. Maurin , J. McMahon , F. Menanteau , C. J. Miller , R. Miquel , J. J. Mohr , S. Naess , F. Nati , L. Newburgh , M. D. Niemack , R. L. C. Ogando , L. A. Page B. Partridge , S. Patil , A. A. Plazas , D. Rapetti , C. L. Reichardt , A. K. Romer , E. Sanchez , V. Scarpine , R. Schindler , S. Serrano , M. Smith , R. C. Smith , M. Soares-Santos , F. Sobreira , S. T. Staggs , A. Stark , G. Stein , E. Suchyta , M. E. C. Swanson , G. Tarle , D. Thomas , A. van Engelen , E. J. Wollack , Z. Xu , Z. Zhang

Evolution in the mass function of galaxy clusters sensitively traces both the expansion history of the Universe and cosmological structure formation. Robust cluster mass determinations are a key ingredient for a reliable measurement of this…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-03 Holger Israel , Thomas Erben , Thomas H. Reiprich , Alexey Vikhlinin , Craig L. Sarazin , Peter Schneider

The combination of galaxy-galaxy weak lensing and galaxy clustering is a powerful probe of the cosmological model, and exploration of how to best model and extract this information from the signals is essential. We present the measurement…

We infer the mean optical depth of a sample of optically-selected galaxy clusters from the Dark Energy Survey (DES) via the pairwise kinematic Sunyaev-Zel'dovich (kSZ) effect. The pairwise kSZ signal between pairs of clusters drawn from the…

Cosmology and Nongalactic Astrophysics · Physics 2023-06-21 E. Schiappucci , F. Bianchini , M. Aguena , M. Archipley , L. Balkenhol , L. E. Bleem , P. Chaubal , T. M. Crawford , S. Grandis , Y. Omori , C. L. Reichardt , E. Rozo , E. S. Rykoff , C. To , T. M. C. Abbott , P. A. R. Ade , O. Alves , A. J. Anderson , F. Andrade-Oliveira , J. Annis , J. S. Avva , D. Bacon , K. Benabed , A. N. Bender , B. A. Benson , G. M. Bernstein , E. Bertin , S. Bocquet , F. R. Bouchet , D. Brooks , D. L. Burke , J. E. Carlstrom , A. Carnero Rosell , M. Carrasco Kind , J. Carretero , T. W. Cecil , C. L. Chang , P. M. Chichura , T. -L. Chou , M. Costanzi , A. Cukierman , L. N. da Costa , C. Daley , T. de Haan , S. Desai , K. R. Dibert , H. T. Diehl , M. A. Dobbs , P. Doel , C. Doux , D. Dutcher , S. Everett , W. Everett , C. Feng , K. R. Ferguson , I. Ferrero , A. Ferté , B. Flaugher , A. Foster , J. Frieman , S. Galli , A. E. Gambrel , J. García-Bellido , R. W. Gardner , M. Gatti , T. Giannantonio , N. Goeckner-Wald , D. Gruen , R. Gualtieri , S. Guns , G. Gutierrez , N. W. Halverson , S. R. Hinton , E. Hivon , G. P. Holder , D. L. Hollowood , W. L. Holzapfel , K. Honscheid , J. C. Hood , N. Huang , D. J. James , L. Knox , M. Korman , K. Kuehn , C. -L. Kuo , O. Lahav , A. T. Lee , C. Lidman , M. Lima , A. E. Lowitz , C. Lu , M. March , J. Mena-Fernández , F. Menanteau , M. Millea , R. Miquel , J. J. Mohr , J. Montgomery , J. Muir , T. Natoli , G. I. Noble , V. Novosad , R. L. C. Ogando , S. Padin , Z. Pan , F. Paz-Chinchón , M. E. S. Pereira , A. Pieres , A. A. Plazas Malagón , K. Prabhu , J. Prat , W. Quan , A. Rahlin , M. Raveri , M. Rodriguez-Monroy , A. K. Romer , M. Rouble , J. E. Ruhl , E. Sanchez , V. Scarpine , M. Schubnell , G. Smecher , M. Smith , M. Soares-Santos , J. A. Sobrin , E. Suchyta , A. Suzuki , G. Tarle , D. Thomas , K. L. Thompson , B. Thorne , C. Tucker , C. Umilta , J. D. Vieira , M. Vincenzi , G. Wang , N. Weaverdyck , J. Weller , N. Whitehorn , W. L. K. Wu , V. Yefremenko , M. R. Young

The recent discovery of a large number of galaxy clusters using the Sunyaev-Zel'dovich (SZ) effect has opened a new era on the study of the most massive clusters in the Universe. Multi-wavelength analyses are required to understand the…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-15 Cristóbal Sifón , Felipe Menanteau , John P. Hughes , Mauricio Carrasco , L. Felipe Barrientos

We search for signatures of cosmological shocks in gas pressure profiles of galaxy clusters using the cluster catalogs from three surveys: the Dark Energy Survey (DES) Year 3, the South Pole Telescope (SPT) SZ survey, and the Atacama…

Astrophysics of Galaxies · Physics 2023-12-14 D. Anbajagane , C. Chang , E. J. Baxter , S. Charney , M. Lokken , M. Aguena , S. Allam , O. Alves , A. Amon , R. An , F. Andrade-Oliveira , D. Bacon , N. Battaglia , K. Bechtol , M. R. Becker , B. A. Benson , G. M. Bernstein , L. Bleem , S. Bocquet , J. R. Bond , D. Brooks , A. Carnero Rosell , M. Carrasco Kind , R. Chen , A. Choi , M. Costanzi , T. M. Crawford , M. Crocce , L. N. da Costa , M. E. S. Pereira , T. M. Davis , J. De Vicente , S. Desai , M. J. Devlin , H. T. Diehl , P. Doel , C. Doux , A. Drlica-Wagner , J. Elvin-Poole , I. Ferrero , A. Ferte , B. Flaugher , P. Fosalba , D. Friedel , J. Frieman , J. Garcia-Bellido , M. Gatti , G. Giannini , S. Grandis , D. Gruen , R. A. Gruendl , G. Gutierrez , I. Harrison , J. C. Hill , M. Hilton , S. R. Hinton , D. L. Hollowood , K. Honscheid , B. Jain , D. J. James , M. Jarvis , K. Kuehn , M. Lin , N. MacCrann , J. L. Marshall , J. McCullough , J. J. McMahon , J. Mena-Fernandez , F. Menanteau , R. Miquel , K. Moodley , T. Mroczkowski , J. Myles , S. Naess , A. Navarro-Alsina , R. L. C. Ogando , L. A. Page , A. Palmese , S. Pandey , B. Patridge , A. Pieres , A. A. Plazas Malagon , A. Porredon , J. Prat , C. Reichardt , K. Reil , M. Rodriguez-Monroy , R. P. Rollins , A. K. Romer , E. S. Rykoff , E. Sanchez , C. Sanchez , D. Sanchez Cid , E. Schaan , M. Schubnell , L. F. Secco , I. Sevilla-Noarbe , E. Sheldon , T. Shin , C. Sifon , M. Smith , S. T. Staggs , E. Suchyta , M. E. C. Swanson , G. Tarle , C. To , M. A. Troxel , I. Tutusaus , E. M. Vavagiakis , N. Weaverdyck , J. Weller , P. Wiseman , E. J. Wollack , B. Yanny

We present galaxy cluster mass-richness relations found in the Sloan Digital Sky Survey Stripe 82 co-add using clusters found using a Voronoi tessellation cluster finder. These relations were found using stacked weak lensing shear observed…

Cosmology and Nongalactic Astrophysics · Physics 2015-07-14 Matthew P. Wiesner , Huan Lin , Marcelle Soares-Santos

We present results of weak lensing cluster counts obtained from 11 sq.deg SuprimeCam data. Although the area is much smaller than previous work dealing with weak lensing peak statistics, the number density of galaxies usable for weak…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-17 Takashi Hamana , Junya Sakurai , Michitaro Koike , Lance Miller

The South Pole Telescope (SPT) is a 10 meter telescope operating at mm wavelengths. It has recently completed a three-band survey covering 2500 sq. degrees. One of the survey's main goals is to detect galaxy clusters using Sunyaev-Zeldovich…

We measure the weak lensing shear around galaxy troughs, i.e. the radial alignment of background galaxies relative to underdensities in projections of the foreground galaxy field over a wide range of redshift in Science Verification data…

Cross-correlation analysis of the thermal Sunyaev-Zel'dovich (tSZ) effect and weak gravitational lensing (WL) provides a powerful probe of cosmology and astrophysics of the intra-cluster medium. We present the measurement of the…

Cosmology and Nongalactic Astrophysics · Physics 2020-01-22 Ken Osato , Masato Shirasaki , Hironao Miyatake , Daisuke Nagai , Naoki Yoshida , Masamune Oguri , Ryuichi Takahashi

Intrinsic variations of the projected density profiles of clusters of galaxies at fixed mass are a source of uncertainty for cluster weak lensing. We present a semi-analytical model to account for this effect, based on a combination of…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-23 D. Gruen , S. Seitz , M. R. Becker , O. Friedrich , A. Mana

Context. The large-scale mass distribution around dark matter haloes hosting galaxy clusters provides sensitive cosmological information. Aims. In this work, we make use of a large photometric galaxy cluster sample, constructed from the…

We compare X-ray and weak-lensing masses for four galaxy clusters that comprise the top-ranked shear-selected cluster system in the Deep Lens Survey. The weak-lensing observations of this system, which is associated with A781, are from the…

In light of the tension in cosmological constraints reported by the Planck team between their SZ-selected cluster counts and Cosmic Microwave Background (CMB) temperature anisotropies, we compare the Planck cluster mass estimates with…

We report the first investigation of cool-core properties of galaxy clusters selected via their Sunyaev--Zel'dovich (SZ) effect. We use 13 galaxy clusters uniformly selected from 178 deg^2 observed with the South Pole Telescope (SPT) and…

The clustering of galaxy clusters is a powerful cosmological tool, which can help to break degeneracies between parameters when combined with other cosmological observables. We aim to demonstrate its potential in constraining cosmological…

Cosmology and Nongalactic Astrophysics · Physics 2024-02-16 Alessandra Fumagalli , Matteo Costanzi , Alexandro Saro , Tiago Castro , Stefano Borgani

The galaxy phase-space distribution in galaxy clusters provides insights into the formation and evolution of cluster galaxies, and it can also be used to measure cluster mass profiles. We present a dynamical study based on $\sim$3000…

We present the weak lensing mass calibration of the stellar mass based $\mu_{\star}$ mass proxy for redMaPPer galaxy clusters in the Dark Energy Survey Year 1. For the first time we are able to perform a calibration of $\mu_{\star}$ at high…

When extracting the weak lensing shear signal, one may employ either locally normalized or globally normalized shear estimators. The former is the standard approach when estimating cluster masses, while the latter is the more common method…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-19 Eduardo Rozo , Hao-Yi Wu , Fabian Schmidt