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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.
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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.
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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.
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