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J. R. Bond, A. H. Jaffe, and L. Knox, Phys. Rev. D 57
1998
Earlier work this paper cites.
M. Tegmark, A. J. S. Hamilton, M. A. Strauss, M. S. Vogeley, and A. S. Szalay, ApJ 499
1998
Earlier work this paper cites.
T. Di Matteo, R. Perna, T. Abel, and M. J. Rees, Astrophys. J. 564
2002
Earlier work this paper cites.
S. P. Oh and K. J. Mack, Mon. Not. R. Astron. Soc. 346
2003
Earlier work this paper cites.
M. F. Morales and J. Hewitt, ApJ 615
2004
Earlier work this paper cites.
M. G. Santos, A. Cooray, and L. Knox, Astrophys. J. 625
2005
Earlier work this paper cites.
S. R. Furlanetto, S. P. Oh, and F. H. Briggs, Phys. Rep. 433
2006
Earlier work this paper cites.
M. McQuinn, O. Zahn, M. Zaldarriaga, L. Hernquist, and S. R. Furlanetto, ApJ 653
2006
Earlier work this paper cites.
X. Wang, M. Tegmark, M. G. Santos, and L. Knox, Astrophys. J. 650
2006
Earlier work this paper cites.
J. D. Bowman, M. F. Morales, and J. N. Hewitt, ApJ 661
2007
Earlier work this paper cites.
Y. Mao, M. Tegmark, M. McQuinn, M. Zaldarriaga, and O. Zahn, Phys. Rev. D 78
Original
2008
Earlier work this paper cites.
L. Gleser, A. Nusser, and A. J. Benson, Mon. Not. R. Astron. Soc. 391
Original
2008
Earlier work this paper cites.
A. de Oliveira-Costa, M. Tegmark, B. M. Gaensler, J. Jonas, T. L. Landecker, and P. Reich, Mon. Not. R. Astron. Soc. 388
Original
2008
Earlier work this paper cites.
J. D. Bowman, M. F. Morales, and J. N. Hewitt, Astrophys. J. 695
Original
2009
Earlier work this paper cites.
G. Harker, S. Zaroubi, G. Bernardi, M. A. Brentjens, A. G. de Bruyn, B. Ciardi, V. Jelić, L. V. E. Koopmans, P. Labropoulos, G. Mellema, A. Offringa, V. N. Pandey, J. Schaye, R. M. Thomas, and S. Yatawatta, Mon. Not. R. Astron. Soc. 397
Original
2009
Earlier work this paper cites.
M. F. Morales and M. Matejek, Mon. Not. R. Astron. Soc. 400
Original
2009
Earlier work this paper cites.
R. Barkana, Mon. Not. R. Astron. Soc. 397
Original
2009
Earlier work this paper cites.
M. F. Morales and J. S. B. Wyithe, Annu. Rev. Astron. Astrophys. 48
Original
2010
Earlier work this paper cites.

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2014

The Epoch of Reionization Window: I. Mathematical Formalism

Liu, Adrian, Parsons, Aaron R., Trott, Cathryn M.

Understand

The 21 cm line provides a powerful probe of astrophysics and cosmology at high redshifts, but unlocking the potential of this probe requires the robust mitigation of foreground contaminants that are typically several orders of magnitude brighter than the cosmological signal.

Recent simulations and observations have shown that the smooth spectral structure of foregrounds combines with instrument chromaticity to contaminate a "wedge"-shaped region in cylindrical Fourier space.
While previous efforts have explored the suppression of foregrounds within this wedge, as well as the avoidance of this highly contaminated region, all such efforts have neglected a rigorous examination of the error statistics associated with the wedge.
Using a quadratic estimator formalism applied to the interferometric measurement equation, we provide a framework for such a rigorous analysis (incorporating a fully covariant treatment of errors).