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Similar

H.-J. Seo, J. Eckel, D. J. Eisenstein, K. Mehta, M. Metchnik, N. Padmanabhan et al., High-Precision Predictions for the Acoustic Scale in the Nonlinear Regime , Astrophys. J. 720
2010
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K. T. Mehta, H.-J. Seo, J. Eckel, D. J. Eisenstein, M. Metchnik, P. Pinto et al., GALAXY BIAS AND ITS EFFECTS ON THE BARYON ACOUSTIC OSCILLATION MEASUREMENTS , Astrophys. J. 734
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2011
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N. McCullagh and A. S. Szalay, Nonlinear Behavior of Baryon Acoustic Oscillations from the Zel’dovich Approximation Using a Non-Fourier Perturbation Approach , Astrophys. J. 752
Original
2012
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S. Tassev and M. Zaldarriaga, Towards an optimal reconstruction of baryon oscillations , J. Cosmol. Astropart. Phys. 10
Original
2012
Cited alongside, same era.

Then

M. White, Reconstruction within the Zeldovich approximation , Mon. Not. R. Astron. Soc. 450
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2015
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É. Aubourg, S. Bailey, J. E. Bautista, F. Beutler, V. Bhardwaj, D. Bizyaev et al., Cosmological implications of baryon acoustic oscillation measurements , Phys. Rev. D 92
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2015
Later among the works it cites.
M. Schmittfull, Y. Feng, F. Beutler, B. Sherwin and M. Y. Chu, Eulerian BAO reconstructions and N -point statistics , Phys. Rev. D 92
Original
2015
Later among the works it cites.
P. Bull, P. G. Ferreira, P. Patel and M. G. Santos, LATE-TIME COSMOLOGY WITH 21 cm INTENSITY MAPPING EXPERIMENTS , Astrophys. J. 803
Original
2015
Later among the works it cites.
S. Tassev, D. J. Eisenstein, B. D. Wandelt and M. Zaldarriaga, sCOLA: The N-body COLA Method Extended to the Spatial Domain , ArXiv e-prints (Feb., 2015) , [ 1502.07751 ]

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2016

Baryon Acoustic Oscillations reconstruction with pixels

Obuljen, Andrej, Villaescusa-Navarro, Francisco, Castorina, Emanuele et al.

Understand

Gravitational non-linear evolution induces a shift in the position of the baryon acoustic oscillations (BAO) peak together with a damping and broadening of its shape that bias and degrades the accuracy with which the position of the peak can be determined.

BAO reconstruction is a technique developed to undo part of the effect of non-linearities.
We present and analyse a reconstruction method that consists of displacing pixels instead of galaxies and whose implementation is easier than the standard reconstruction method.
We show that this method is equivalent to the standard reconstruction technique in the limit where the number of pixels becomes very large.