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Volumn 329, Issue 5994, 2010, Pages 924-927

Cosmological constraints from strong gravitational lensing in clusters of galaxies

Author keywords

[No Author keywords available]

Indexed keywords

ANISOTROPY; COSMOLOGY; EXPERIMENTAL STUDY; X-RAY DIFFRACTION;

EID: 77955873677     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1185759     Document Type: Article
Times cited : (212)

References (43)
  • 1
  • 8
    • 77955871884 scopus 로고    scopus 로고
    • ArXiv e-prints
    • N. Kaiser, G. Wilson, G. A. Luppino, ArXiv e-prints; http:// arxiv.org/abs/astro-ph/0003338 (2000).
    • (2000)
    • Kaiser, N.1    Wilson, G.2    Luppino, G.A.3
  • 34
    • 77955885804 scopus 로고    scopus 로고
    • ArXiv e-prints
    • S. H. Suyu et al., ArXiv e-prints; http://arxiv.org/abs/ 0910.2773 (2009).
    • (2009)
    • Suyu, S.H.1
  • 37
    • 77955864877 scopus 로고    scopus 로고
    • note
    • Filaments aligned at finite inclinations behind the cluster (thus breaking azimuthal symmetry) do yield larger deviations between the projected and multiplane models compared with the symmetric case. For the nonsymmetric case, the deviations are typically on the same level as the errors due to scatter in the cluster galaxy properties. These deviations are still subdominant to the effects of uncorrelated line-of-sight halos.
  • 43
    • 77955877842 scopus 로고    scopus 로고
    • E.J. and J.-P.K. acknowledge fruitful discussions with D. Coe, L. Koopmans, L. Moustakas, and M. Auger. The authors are thankful for computational resources from Institut du Développement et des Ressources en Informatique Scientifique CNRS, Jet Propulsion Laboratory, and J.-C. Bourret. E.J. acknowledges a NASA postdoctoral fellowship, and P.N. acknowledges a Radcliffe Fellowship and a Guggenheim Fellowship. J.-P.K., M.L., and C.S. acknowledge support from CNRS, and M.L. thanks Centre National d'Études Spatiales and Ville de Marseille. The authors thank A. Vikhlinin for providing data on cosmological constraints from x-ray clusters to combine with our strong lensing results.
    • E.J. and J.-P.K. acknowledge fruitful discussions with D. Coe, L. Koopmans, L. Moustakas, and M. Auger. The authors are thankful for computational resources from Institut du Développement et des Ressources en Informatique Scientifique CNRS, Jet Propulsion Laboratory, and J.-C. Bourret. E.J. acknowledges a NASA postdoctoral fellowship, and P.N. acknowledges a Radcliffe Fellowship and a Guggenheim Fellowship. J.-P.K., M.L., and C.S. acknowledge support from CNRS, and M.L. thanks Centre National d'Études Spatiales and Ville de Marseille. The authors thank A. Vikhlinin for providing data on cosmological constraints from x-ray clusters to combine with our strong lensing results.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.