Cited by 604Cosmology and Gravitation TheoriesGalaxies: Formation, Evolution, PhenomenaDark Matter and Cosmic Phenomena

Cosmology with cosmic shear observations: a review

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Kilbinger, Martin·2015·Reports on Progress in Physics

Abstract

Cosmic shear is the distortion of images of distant galaxies due to weak gravitational lensing by the large-scale structure in the Universe. Such images are coherently deformed by the tidal field of matter inhomogeneities along the line of sight. By measuring galaxy shape correlations, we can study the properties and evolution of structure on large scales as well as the geometry of the Universe. Thus, cosmic shear has become a powerful probe into the nature of dark matter and the origin of the current accelerated expansion of the Universe. Over the last years, cosmic shear has evolved into a reliable and robust cosmological probe, providing measurements of the expansion history of the Universe and the growth of its structure. We review here the principles of weak gravitational lensing and show how cosmic shear is interpreted in a cosmological context. Then we give an overview of weak-lensing measurements, and present the main observational cosmic-shear results since it was discovered 15 years ago, as well as the implications for cosmology. We then conclude with an outlook on the various future surveys and missions, for which cosmic shear is one of the main science drivers, and discuss promising new weak cosmological lensing techniques for future observations.

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  • Weak lensing maps mass distribution versus redshift and traces cosmic expansion and structure growth.

    “WL techniques can be used to map the distribution of mass as a function of redshift and thereby trace the history of both the expansion of the universe and the growth of structure”

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Research works printed but not linked: 10

  1. Anderson T W 2003 An Introduction to Multivariate Statistical Analysis 3rd edn (New York: Wiley)
  2. Coles P and Lucchin F 1996 Cosmology: The Origin and Evolution of Cosmic Structure (New York: Wiley)
  3. Harvey D et al 2014 Astron. Comput. 5 35-44 · DOI
  4. Kaiser N, Squires G, Fahlman G and Woods D 1994 Clusters of galaxies, Proc. of the XIVth Moriond Astrophysics Meeting (Méribel, France, 12-19 March 1994) p 269
  5. Meyers J E and Burchat P R S 2014 (ArXiv:1409.6273) · arXiv
  6. Miyazaki S et al 2012 Society of Photo-Optical Instrumentation Engineers (SPIE) Conf. Series vol 8446
  7. Peebles P J E 1980 The Large-Scale Structure of the Universe (Princeton, NJ: Princeton University Press)
  8. Schneider M D S et al 2014 (ArXiv e-prints)
  9. Schneider P, Ehlers J and Falco E E 1992 Gravitational Lenses (Berlin: Springer)
  10. Schneider P, Kochanek C S and Wambsganss J 2006 Gravitational Lensing: Strong, Weak and Micro (Berlin: Springer)

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Authors
Kilbinger, M.
Affiliations
Laboratoire AIM
Corresponding author
Kilbinger, Martin
Venue
Reports on Progress in Physics
Published
2015-07-01
Volume
78
Issue
8
Pages
086901
ISSN
  • 0034-4885 (ISSN-L)
  • 1361-6633
OpenAlex
W1922448784
Cited by
604
References
432
Citations by year
2026: 48 · 2025: 55 · 2024: 54 · 2023: 40 · 2022: 59 · 2021: 64 · 2020: 69 · 2019: 70 · 2018: 69 · 2017: 31 · 2016: 33 · 2015: 11
FWCI
3.87
Type
journal article
Language
en
Open access
Locations
  • Reports on Progress in Physics (publishedVersion)
  • arXiv (Cornell University) (publishedVersion)
  • PubMed (publishedVersion)
  • arXiv (Cornell University)
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
  • Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Dark Matter and Cosmic Phenomena
Keywords
cosmic shear, weak gravitational lensing, large-scale structure, dark matter, cosmic expansion history, structure growth, cosmic geometry
MeSH terms
Astronomy, Forecasting, Gravitation, Models, Theoretical, Galaxies, Optical Phenomena

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