Simulation-based marginal likelihood for cluster strong lensing cosmology-Reference-Cited by-同舟云学术

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Simulation-based marginal likelihood for cluster strong lensing cosmology

Published:2017-09-11 Issue:2 Volume:473 Page:1736-1750
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Killedar M.^ORCID,Borgani S.,Fabjan D.,Dolag K.,Granato G.,Meneghetti M.,Planelles S.,Ragone-Figueroa C.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/473/2/1736/21515261/stx2262.pdf

Reference115 articles.

1. Weighing the Giants – III. Methods and measurements of accurate galaxy cluster weak-lensing masses

2. Arc statistics in cosmological models with dark energy

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1. The Strongest Cluster Lenses: An Analysis of the Relation between Strong Gravitational Lensing Strength and the Physical Properties of Galaxy Clusters;The Astrophysical Journal;2022-03-01

2. Core Mass Estimates in Strong Lensing Galaxy Clusters: A Comparison between Masses Obtained from Detailed Lens Models, Single-halo Lens Models, and Einstein Radii;The Astrophysical Journal;2021-10-01

3. Twenty-First-Century Statistical and Computational Challenges in Astrophysics;Annual Review of Statistics and Its Application;2021-03-07

4. A preferential attachment model for the stellar initial mass function;Electronic Journal of Statistics;2019-01-01

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