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Related papers: Stellar mass as a galaxy cluster mass proxy: appli…

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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…

Using archival X-ray observations and a log-normal population model, we estimate constraints on the intrinsic scatter in halo mass at fixed optical richness for a galaxy cluster sample identified in Dark Energy Survey Year-One (DES-Y1) data…

Estimates of cosmological parameters using galaxy clusters have the scatter in the observable at a given mass as a fundamental parameter. This work computes the amplitude of the scatter for a newly introduced mass proxy, the product of the…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-12 S. Andreon

We present the stellar mass-halo mass scaling relation for 46 X-ray selected low-mass clusters or groups detected in the XMM-BCS survey with masses $2\times10^{13}M_{\odot}\lesssim M_{500}\lesssim2.5\times10^{14}M_{\odot}$ at redshift…

Astrophysics of Galaxies · Physics 2016-02-17 I. Chiu , A. Saro , J. Mohr , S. Desai , S. Bocquet , R. Capasso , C. Gangkofner , N. Gupta , J. Liu

The cosmological constraining power of modern galaxy cluster catalogs can be improved by obtaining low-scatter mass proxy measurements for even a small fraction of sources. In the context of large upcoming surveys that will reveal the…

Cosmology and Nongalactic Astrophysics · Physics 2017-12-04 Adam B. Mantz , Steven W. Allen , R. Glenn Morris , Anja von der Linden

We measure the stacked lensing signal in the direction of galaxy clusters in the Dark Energy Survey Year 3 (DES Y3) redMaPPer sample, using cosmic microwave background (CMB) temperature data from SPT-3G, the third-generation CMB camera on…

Cosmology and Nongalactic Astrophysics · Physics 2024-06-14 B. Ansarinejad , S. Raghunathan , T. M. C. Abbott , P. A. R. Ade , M. Aguena , O. Alves , A. J. Anderson , F. Andrade-Oliveira , M. Archipley , L. Balkenhol , K. Benabed , A. N. Bender , B. A. Benson , E. Bertin , F. Bianchini , L. E. Bleem , S. Bocquet , F. R. Bouchet , D. Brooks , L. Bryant , D. L. Burke , E. Camphuis , J. E. Carlstrom , A. Carnero Rosell , J. Carretero , F. J. Castander , T. W. Cecil , C. L. Chang , P. Chaubal , P. M. Chichura , T. -L. Chou , A. Coerver , M. Costanzi , T. M. Crawford , A. Cukierman , L. N. da Costa , C. Daley , T. M. Davis , T. de Haan , S. Desai , J. De Vicente , K. R. Dibert , M. A. Dobbs , P. Doel , A. Doussot , C. Doux , D. Dutcher , W. Everett , C. Feng , K. R. Ferguson , I. Ferrero , K. Fichman , A. Foster , J. Frieman , S. Galli , A. E. Gambrel , J. García-Bellido , R. W. Gardner , E. Gaztanaga , F. Ge , G. Giannini , N. Goeckner-Wald , S. Grandis , R. A. Gruendl , R. Gualtieri , F. Guidi , 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 , F. Kéruzoré , L. Knox , M. Korman , C. -L. Kuo , A. T. Lee , S. Lee , K. Levy , A. E. Lowitz , C. Lu , A. Maniyar , J. L. Marshall , J. Mena-Fernández , F. Menanteau , R. Miquel , M. Millea , J. J. Mohr , J. Montgomery , Y. Nakato , T. Natoli , G. I. Noble , V. Novosad , R. L. C. Ogando , Y. Omori , S. Padin , A. Palmese , Z. Pan , P. Paschos , M. E. S. Pereira , A. Pieres , A. A. Plazas Malagón , K. Prabhu , W. Quan , A. Rahlin , M. Rahimi , C. L. Reichardt , K. Reil , A. K. Romer , M. Rouble , J. E. Ruhl , E. Sanchez , D. Sanchez Cid , E. Schiappucci , I. Sevilla-Noarbe , G. Smecher , M. Smith , J. A. Sobrin , A. A. Stark , J. Stephen , E. Suchyta , A. Suzuki , M. E. C. Swanson , C. Tandoi , G. Tarle , K. L. Thompson , B. Thorne , C. Trendafilova , C. Tucker , C. Umilta , J. D. Vieira , G. Wang , N. Weaverdyck , N. Whitehorn , P. Wiseman. , W. L. K. Wu , V. Yefremenko , M. R. Young , J. A. Zebrowski

We develop a framework to study the relation between the stellar mass of a galaxy and the total mass of its host dark matter halo using galaxy clustering and galaxy-galaxy lensing measurements. We model a wide range of scales, roughly from…

The amount and nature of dark energy (DE) can be tightly constrained by measuring the spatial correlation features and evolution of a sample of ~ 100,000 galaxy clusters over the redshift range 0<z < 1.5. Such an X-ray survey will discover…

We test the reliability of mass determination in clusters of galaxies by X-ray observations. The true mass in cluster models is compared to the mass derived by the X-ray emission and X-ray temperature of a model assuming hydrostatic…

Astrophysics · Physics 2016-08-30 Sabine Schindler

Using the weak gravitational lensing data from the Hyper Suprime-Cam Subaru Strategic Program (HSC survey), we study the potential of different stellar mass estimates in tracing halo mass. We consider galaxies with $\log…

We present the first weak lensing calibration of $\mu_{\star}$, a new galaxy cluster mass proxy corresponding to the total stellar mass of red and blue members, in two cluster samples selected from the SDSS Stripe 82 data: 230 redMaPPer…

We examine the relationship between the mass and x-ray gas temperature of galaxy clusters using data drawn from the literature. Simple theoretical arguments suggest that the mass of a cluster is related to the x-ray temperature as $M…

Astrophysics · Physics 2009-10-31 Donald J. Horner , Richard F. Mushotzky , Caleb A. Scharf

We present a study on the clustering of a stellar mass selected sample of 18,482 galaxies with stellar masses M*>10^10M(sun) at redshifts 0.4<z<2.0, taken from the Palomar Observatory Wide-field Infrared Survey. We examine the clustering…

Cosmology and Nongalactic Astrophysics · Physics 2011-02-15 S. Foucaud , C. J. Conselice , W. G. Hartley , K. P. Lane , S. P. Bamford , O. Almaini , K. Bundy

Stellar mass can enhance the ranking of potential hosts for compact binary coalescences identified by ground-based gravitational-wave detectors within large localisation areas containing even thousands of galaxies. Despite its benefits,…

Astrophysics of Galaxies · Physics 2025-03-27 M. Pálfi , G. Dálya , P. Raffai

Most galaxies are hosted by massive, invisible dark matter haloes, yet little is known about the scatter in the stellar mass--halo mass relation for galaxies with host halo masses $M_{h}\le 10^{11}M_{\odot}$. Using mock catalogues based on…

Astrophysics of Galaxies · Physics 2019-08-14 Magdelena Allen , Peter Behroozi , Chung-Pei Ma

We present a study on the clustering of a stellar mass selected sample of galaxies with stellar masses M*>10^10Msol at redshifts 0.4<z<2.0, taken from the Palomar Observatory Wide-field Infrared Survey. We examine the clustering properties…

Cosmology and Nongalactic Astrophysics · Physics 2016-11-25 Sebastien Foucaud , Christopher J. Conselice

We present comparison of X-ray proxies for the total cluster mass, including the spectral temperature (Tx), gas mass measured within r500 (Mg), and the new proxy, Yx, which is a simple product of Tx and Mg and is related to the total…

Astrophysics · Physics 2010-04-06 Andrey V. Kravtsov , Alexey Vikhlinin , Daisuke Nagai
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