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Density-reconstruction sharpens the baryon acoustic oscillations signal by undoing some of the smoothing incurred by nonlinear structure formation.
1903
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D. J. Eisenstein, H.-J. Seo and M. White, On the Robustness of the Acoustic Scale in the Low-Redshift Clustering of Matter , ApJ 664
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2010
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2011
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2012
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S. Tassev and M. Zaldarriaga, Towards an optimal reconstruction of baryon oscillations , JCAP 10
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2016
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2016
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2012
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2013
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2013
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2013
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2013
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2014
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M. Vargas-Magaña, S. Ho, X. Xu, A. G. Sánchez, R. O’Connell, D. J. Eisenstein et al., The clustering of Galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: potential systematics in fitting of baryon acoustic feature , MNRAS 445
2014
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M. White, The Zel’dovich approximation , MNRAS 439
2014
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2017
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2017
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Y. Yu, H.-M. Zhu and U.-L. Pen, Halo Nonlinear Reconstruction , ApJ 847
2017
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2017
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2017
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2018
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2018
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2018
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R. Hada and D. J. Eisenstein, An iterative reconstruction of cosmological initial density fields , MNRAS (2018)
2018
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2018
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E. Castorina and M. White, Beyond the plane-parallel approximation for redshift surveys , MNRAS 476
2018
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2018
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2018
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2018
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2018
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2018
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M. M. Abidi and T. Baldauf, Cubic halo bias in Eulerian and Lagrangian space , JCAP 2018
2018
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