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Cosmic shear is considered one of the most powerful methods for studying the properties of Dark Energy in the Universe.
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Schneider, P. & Kilbinger, M. 2007, A&A, 462, 841
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Joachimi, B. & Schneider, P. 2008, A&A, 488, 829
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Joachimi, B., Schneider, P., & Eifler, T. 2008, A&A, 477, 43
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2004
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Schneider, P., Kilbinger, M., & Lombardi, M. 2005, A&A, 431, 9
2005
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Albrecht, A., Bernstein, G., Cahn, R., et al. 2006, astro-ph/0609591
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Jing, Y. P., Zhang, P., Lin, W. P., Gao, L., & Springel, V. 2006, ApJ, 640, L119
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Kilbinger, M., Schneider, P., & Eifler, T. 2006, A&A, 457, 15
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Schneider, P., Kochanek, C. S., & Wambsganss, J. 2006, Gravitational Lensing: Strong, Weak and Micro (Springer-Verlag Berlin)
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2008
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Bassett, B. A., Fantaye, Y., Hlozek, R., & Kotze, J. 2009, astro-ph/0906.0993
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Eifler, T., Schneider, P., & Hartlap, J. 2009, A&A, 502, 721
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Hilbert, S., Hartlap, J., White, S. D. M., & Schneider, P. 2009, A&A, 499, 31
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Joachimi, B. & Bridle, S. L. 2009, astro-ph/0911.2454
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Schrabback, T., Hartlap, J., Joachimi, B., et al. 2009, astro-ph/0911.0053
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Eifler, T., Schneider, P., & Krause, E. 2010, A&A, 510, A260000+
2010
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Fu, L. & Kilbinger, M. 2010, MNRAS, 401, 1264
2010
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