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N. Kaiser, ApJ 388
1992
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P. Schneider and C. Seitz, A&A 294
1995
Earlier work this paper cites.
P. Schneider, L. van Waerbeke, B. Jain, and G. Kruse, MNRAS 296
1998
Earlier work this paper cites.
U. Seljak, ApJ 506
1998
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D. J. Bacon, A. R. Refregier, and R. S. Ellis, MNRAS 318
2000
Earlier work this paper cites.
N. Kaiser, G. Wilson, and G. A. Luppino, arXiv:astro-ph/0003338 (2000), astro-ph/0003338
2000
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D. M. Wittman, J. A. Tyson, D. Kirkman, I. Dell’Antonio, and G. Bernstein, Nature 405
2000
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L. van Waerbeke et al. , Astron. Astrophys. 358
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I. Szapudi, S. Prunet, D. Pogosyan, A. S. Szalay, and J. R. Bond, arXiv:astro-ph/0010256 (2000), astro-ph/0010256
2000
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W. Hu and M. White, ApJ 554
2001
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A. Cooray and W. Hu, ApJ 554
2001
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A. Lewis and S. Bridle, Phys. Rev. D66
2002
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R. G. Crittenden, P. Natarajan, U.-L. Pen, and T. Theuns, ApJ 568
2002
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M. Jarvis, G. Bernstein, and B. Jain, MNRAS 352
2004
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G. Chon, A. Challinor, S. Prunet, E. Hivon, and I. Szapudi, MNRAS 350
2004
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W. Hu and B. Jain, Phys. Rev. D 70
2004
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V. Springel, MNRAS 364
2005
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K. M. Górski, E. Hivon, A. J. Banday, B. D. Wandelt, F. K. Hansen, M. Reinecke, and M. Bartelmann, ApJ 622
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A. Albrecht, G. Bernstein, R. Cahn, W. L. Freedman, J. Hewitt, W. Hu, J. Huth, M. Kamionkowski, E. W. Kolb, L. Knox, J. C. Mather, S. Staggs, and N. B. Suntzeff, arXiv:astro-ph/0609591 (2006), astro-ph/0609591
2006
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J. Peacock and P. Schneider, The Messenger 125
2006
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M. Crocce, S. Pueblas, and R. Scoccimarro, MNRAS 373
2006
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L. Miller, T. D. Kitching, C. Heymans, A. F. Heavens, and L. van Waerbeke, MNRAS 382
Original
2007
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J. Hartlap, P. Simon, and P. Schneider, A&A 464
2007
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P. Schneider and M. Kilbinger, A&A 462
2007
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B. Joachimi, P. Schneider, and T. Eifler, A&A 477
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2008
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A. Albrecht, L. Amendola, G. Bernstein, D. Clowe, D. Eisenstein, L. Guzzo, C. Hirata, D. Huterer, R. Kirshner, E. Kolb, and R. Nichol, arXiv:astro-ph/0901.0721 (2009), arXiv:0901.0721 [astro-ph.IM]
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2015

Cosmic Shear Measurements with DES Science Verification Data

Becker, M. R., Troxel, M. A., MacCrann, N. et al.

Understand

We present measurements of weak gravitational lensing cosmic shear two-point statistics using Dark Energy Survey Science Verification data.

We demonstrate that our results are robust to the choice of shear measurement pipeline, either ngmix or im3shape, and robust to the choice of two-point statistic, including both real and Fourier-space statistics.
Our results pass a suite of null tests including tests for B-mode contamination and direct tests for any dependence of the two-point functions on a set of 16 observing conditions and galaxy properties, such as seeing, airmass, galaxy color, galaxy magnitude, etc.
We furthermore use a large suite of simulations to compute the covariance matrix of the cosmic shear measurements and assign statistical significance to our null tests.

Built on

N. Kaiser, ApJ 388
1992
Earlier work this paper cites.
P. Schneider and C. Seitz, A&A 294
1995
Earlier work this paper cites.
P. Schneider, L. van Waerbeke, B. Jain, and G. Kruse, MNRAS 296
1998
Earlier work this paper cites.
U. Seljak, ApJ 506
1998
Earlier work this paper cites.
D. J. Bacon, A. R. Refregier, and R. S. Ellis, MNRAS 318
2000
Earlier work this paper cites.
N. Kaiser, G. Wilson, and G. A. Luppino, arXiv:astro-ph/0003338 (2000), astro-ph/0003338
2000
Earlier work this paper cites.
D. M. Wittman, J. A. Tyson, D. Kirkman, I. Dell’Antonio, and G. Bernstein, Nature 405
2000
Earlier work this paper cites.
L. van Waerbeke et al. , Astron. Astrophys. 358
2000
Earlier work this paper cites.
I. Szapudi, S. Prunet, D. Pogosyan, A. S. Szalay, and J. R. Bond, arXiv:astro-ph/0010256 (2000), astro-ph/0010256
2000
Earlier work this paper cites.
W. Hu and M. White, ApJ 554
2001
Earlier work this paper cites.
A. Cooray and W. Hu, ApJ 554
2001
Earlier work this paper cites.
A. Lewis and S. Bridle, Phys. Rev. D66
2002
Earlier work this paper cites.
R. G. Crittenden, P. Natarajan, U.-L. Pen, and T. Theuns, ApJ 568
2002
Earlier work this paper cites.
M. Jarvis, G. Bernstein, and B. Jain, MNRAS 352
2004
Earlier work this paper cites.
G. Chon, A. Challinor, S. Prunet, E. Hivon, and I. Szapudi, MNRAS 350
2004
Earlier work this paper cites.
W. Hu and B. Jain, Phys. Rev. D 70
2004
Earlier work this paper cites.
V. Springel, MNRAS 364
2005
Earlier work this paper cites.
K. M. Górski, E. Hivon, A. J. Banday, B. D. Wandelt, F. K. Hansen, M. Reinecke, and M. Bartelmann, ApJ 622
2005
Earlier work this paper cites.
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2006
Earlier work this paper cites.
J. Peacock and P. Schneider, The Messenger 125
2006
Earlier work this paper cites.
M. Crocce, S. Pueblas, and R. Scoccimarro, MNRAS 373
2006
Earlier work this paper cites.
L. Miller, T. D. Kitching, C. Heymans, A. F. Heavens, and L. van Waerbeke, MNRAS 382
Original
2007
Earlier work this paper cites.
J. Hartlap, P. Simon, and P. Schneider, A&A 464
2007
Earlier work this paper cites.
P. Schneider and M. Kilbinger, A&A 462
2007
Earlier work this paper cites.
B. Joachimi, P. Schneider, and T. Eifler, A&A 477
Original
2008
Earlier work this paper cites.
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2009
Earlier work this paper cites.

Similar

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Original
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Cited alongside, same era.

Then

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Original
2013
Later among the works it cites.
M. Takada and W. Hu, Phys. Rev. D 87
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2013
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S. Dodelson and M. D. Schneider, Phys. Rev. D 88
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2013
Later among the works it cites.
E. M. Huff, T. Eifler, C. M. Hirata, R. Mandelbaum, D. Schlegel, and U. Seljak, MNRAS 440
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