Fetching the paper…
Reading the bibliography…
Cosmic shear is one of the most powerful probes of Dark Energy, targeted by several current and future galaxy surveys.
1903
Earlier work this paper cites.
1904
Earlier work this paper cites.
1905
Earlier work this paper cites.
1905
Earlier work this paper cites.
1906
Earlier work this paper cites.
C. García-García, D. Alonso and E. Bellini, Disconnected pseudo-C l
1906
Earlier work this paper cites.
1909
Earlier work this paper cites.
1911
Earlier work this paper cites.
1912
Earlier work this paper cites.
P. J. E. Peebles, Statistical Analysis of Catalogs of Extragalactic Objects. I. Theory , ApJ 185
1973
Earlier work this paper cites.
D. C. Wells, E. W. Greisen and R. H. Harten, FITS - a Flexible Image Transport System , A&AS 44
1981
Earlier work this paper cites.
D. Scott, M. Srednicki and M. White, “Sample Variance” in Small-Scale Cosmic Microwave Background Anisotropy Experiments , ApJ 421
1994
Earlier work this paper cites.
N. Kaiser, G. Squires and T. Broadhurst, A Method for Weak Lensing Observations , ApJ 449
1995
Earlier work this paper cites.
M. Tegmark, How to measure CMB power spectra without losing information , Phys. Rev. D 55
1997
Earlier work this paper cites.
J. R. Bond, A. H. Jaffe and L. Knox, Estimating the power spectrum of the cosmic microwave background , Phys. Rev. D 57
1998
Earlier work this paper cites.
S. P. Oh, D. N. Spergel and G. Hinshaw, An Efficient Technique to Determine the Power Spectrum from Cosmic Microwave Background Sky Maps , ApJ 510
1999
Earlier work this paper cites.
D. J. Bacon, A. R. Refregier and R. S. Ellis, Detection of weak gravitational lensing by large-scale structure , MNRAS 318
2000
Earlier work this paper cites.
N. Kaiser, G. Wilson and G. A. Luppino, Large-Scale Cosmic Shear Measurements , arXiv e-prints (2000) astro [ astro-ph/0003338 ]
2000
Earlier work this paper cites.
L. Van Waerbeke, Y. Mellier, T. Erben, J. C. Cuilland re, F. Bernardeau, R. Maoli et al., Detection of correlated galaxy ellipticities from CFHT data: first evidence for gravitational lensing by large-scale structures , A&A 358
2000
Earlier work this paper cites.
D. M. Wittman, J. A. Tyson, D. Kirkman, I. Dell’Antonio and G. Bernstein, Detection of weak gravitational lensing distortions of distant galaxies by cosmic dark matter at large scales , Nature 405
2000
Earlier work this paper cites.
A. Heavens, A. Refregier and C. Heymans, Intrinsic correlation of galaxy shapes: implications for weak lensing measurements , MNRAS 319
2000
Earlier work this paper cites.
R. A. C. Croft and C. A. Metzler, Weak-Lensing Surveys and the Intrinsic Correlation of Galaxy Ellipticities , ApJ 545
2000
Earlier work this paper cites.
N. Benítez, Bayesian Photometric Redshift Estimation , ApJ 536
2000
Earlier work this paper cites.
A. Cooray and W. Hu, Power Spectrum Covariance of Weak Gravitational Lensing , ApJ 554
2001
Earlier work this paper cites.
M. Bartelmann and P. Schneider, Weak gravitational lensing , Phys. Rep. 340
2001
Earlier work this paper cites.
O. Doré, L. Knox and A. Peel, CMB power spectrum estimation via hierarchical decomposition , Phys. Rev. D 64
2001
Earlier work this paper cites.
P. Schneider, L. van Waerbeke, M. Kilbinger and Y. Mellier, Analysis of two-point statistics of cosmic shear. I. Estimators and covariances , A&A 396
2002
Earlier work this paper cites.
E. Hivon, K. M. Górski, C. B. Netterfield, B. P. Crill, S. Prunet and F. Hansen, MASTER of the Cosmic Microwave Background Anisotropy Power Spectrum: A Fast Method for Statistical Analysis of Large and Complex Cosmic Microwave Background Data Sets , ApJ 567
2002
Earlier work this paper cites.
G. M. Bernstein and M. Jarvis, Shapes and Shears, Stars and Smears: Optimal Measurements for Weak Lensing , AJ 123
2002
Earlier work this paper cites.
A. Cooray and W. Hu, Second-Order Corrections to Weak Lensing by Large-Scale Structure , ApJ 574
2002
Earlier work this paper cites.
U.-L. Pen, Fast power spectrum estimation , MNRAS 346
2003
Earlier work this paper cites.
C. Hirata and U. Seljak, Shear calibration biases in weak-lensing surveys , MNRAS 343
2003
Earlier work this paper cites.
2004
Earlier work this paper cites.
J. Jewell, S. Levin and C. H. Anderson, Application of Monte Carlo Algorithms to the Bayesian Analysis of the Cosmic Microwave Background , ApJ 609
2004
Earlier work this paper cites.
G. Efstathiou, Myths and truths concerning estimation of power spectra: the case for a hybrid estimator , MNRAS 349
2004
Cited alongside, same era.
M. L. Brown, P. G. Castro and A. N. Taylor, Cosmic microwave background temperature and polarization pseudo-C l
2005
Cited alongside, same era.
K. M. Górski, E. Hivon, A. J. Banday, B. D. Wand elt, F. K. Hansen, M. Reinecke et al., HEALPix: A Framework for High-Resolution Discretization and Fast Analysis of Data Distributed on the Sphere , ApJ 622
2005
Cited alongside, same era.
A. Albrecht, G. Bernstein, R. Cahn, W. L. Freedman, J. Hewitt, W. Hu et al., Report of the Dark Energy Task Force , arXiv e-prints (2006) astro [ astro-ph/0609591 ]
2006
Cited alongside, same era.
2016
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
alphaXiv searches the wider corpus for related work and actual follow-ups.
alphaXiv is searching for related work…
2006
Cited alongside, same era.
T. E. Oliphant, A guide to NumPy , vol. 1. Trelgol Publishing USA, 2006
2006
Cited alongside, same era.
2007
Cited alongside, same era.
2007
Cited alongside, same era.
J. D. Hunter, Matplotlib: A 2d graphics environment , Computing in Science & Engineering 9
2007
Cited alongside, same era.
2008
Cited alongside, same era.
2009
Cited alongside, same era.
2009
Cited alongside, same era.
2017
Later among the works it cites.
2017
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2019
Later among the works it cites.
D. Alonso, J. Sanchez, A. Slosar and LSST Dark Energy Science Collaboration, A unified pseudo-C ℓ
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
A. Zonca, L. Singer, D. Lenz, M. Reinecke, C. Rosset, E. Hivon et al., healpy: equal area pixelization and spherical harmonics transforms for data on the sphere in python , Journal of Open Source Software 4
2019
Later among the works it cites.
10.5281/zenodo.4010767
J. Zuntz, D. Alonso, A. Slosar, A. Broussard, T. McClintock, H. Miyatake et al., Sacc: Save all correlations and covariances , Sept., 2020 · 2020
Closest in time.
P. Virtanen, R. Gommers, T. E. Oliphant, M. Haberland, T. Reddy, D. Cournapeau et al., SciPy 1.0: Fundamental Algorithms for Scientific Computing in Python , Nature Methods 17
2020
Closest in time.