scholarly journals Bounds on graviton mass using weak lensing and SZ effect in galaxy clusters

2018 ◽  
Vol 781 ◽  
pp. 220-226 ◽  
Author(s):  
Akshay Rana ◽  
Deepak Jain ◽  
Shobhit Mahajan ◽  
Amitabha Mukherjee
2014 ◽  
Vol 439 (1) ◽  
pp. 2-27 ◽  
Author(s):  
Anja von der Linden ◽  
Mark T. Allen ◽  
Douglas E. Applegate ◽  
Patrick L. Kelly ◽  
Steven W. Allen ◽  
...  

Author(s):  
Arthur B. Congdon ◽  
Charles R. Keeton
Keyword(s):  

2007 ◽  
Author(s):  
Erin S. Sheldon ◽  
David E. Johnston ◽  
Ryan Scranton ◽  
Ben P. Koester ◽  
Timothy A. McKay ◽  
...  

2019 ◽  
Vol 485 (1) ◽  
pp. 69-87 ◽  
Author(s):  
C Stern ◽  
J P Dietrich ◽  
S Bocquet ◽  
D Applegate ◽  
J J Mohr ◽  
...  

2009 ◽  
Vol 703 (2) ◽  
pp. 2232-2248 ◽  
Author(s):  
Erin S. Sheldon ◽  
David E. Johnston ◽  
Morad Masjedi ◽  
Timothy A. McKay ◽  
Michael R. Blanton ◽  
...  

2016 ◽  
Vol 460 (4) ◽  
pp. 3913-3924 ◽  
Author(s):  
Masato Shirasaki ◽  
Daisuke Nagai ◽  
Erwin T. Lau

2020 ◽  
Vol 497 (1) ◽  
pp. 894-905
Author(s):  
Mauro Sereno ◽  
Stefano Ettori ◽  
Giorgio F Lesci ◽  
Federico Marulli ◽  
Matteo Maturi ◽  
...  

ABSTRACT Unbiased and precise mass calibration of galaxy clusters is crucial to fully exploit galaxy clusters as cosmological probes. Stacking of weak lensing (WL) signal allows us to measure observable–mass relations down to less massive haloes without extrapolation. We propose a Bayesian inference method to constrain the intrinsic scatter of the mass proxy in stacked analyses. The scatter of the stacked data is rescaled with respect to the individual scatter based on the number of binned clusters. We apply this method to the galaxy clusters detected with the AMICO (Adaptive Matched Identifier of Clustered Objects) algorithm in the third data release of the Kilo-Degree Survey. The results confirm the optical richness as a low-scatter mass proxy. Based on the optical richness and the calibrated WL mass–richness relation, mass of individual objects down to $\sim\! 10^{13}\, \mathrm{M}_\odot$ can be estimated with a precision of ∼20 per cent.


2020 ◽  
Vol 28 (1) ◽  
Author(s):  
Keiichi Umetsu

AbstractWeak gravitational lensing of background galaxies provides a direct probe of the projected matter distribution in and around galaxy clusters. Here, we present a self-contained pedagogical review of cluster–galaxy weak lensing, covering a range of topics relevant to its cosmological and astrophysical applications. We begin by reviewing the theoretical foundations of gravitational lensing from first principles, with a special attention to the basics and advanced techniques of weak gravitational lensing. We summarize and discuss key findings from recent cluster–galaxy weak-lensing studies on both observational and theoretical grounds, with a focus on cluster mass profiles, the concentration–mass relation, the splashback radius, and implications from extensive mass-calibration efforts for cluster cosmology.


2015 ◽  
Vol 447 (4) ◽  
pp. 3044-3059 ◽  
Author(s):  
P. A. Giles ◽  
B. J. Maughan ◽  
T. Hamana ◽  
S. Miyazaki ◽  
M. Birkinshaw ◽  
...  
Keyword(s):  

2012 ◽  
Vol 383 ◽  
pp. 012011
Author(s):  
Iacopo Bartalucci ◽  
Ilaria Formicola ◽  
Rossella Martino

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