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Analysis of an iterative reconstruction method in comparison of the standard reconstruction method

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arxiv 2311.09531 v2 pith:EODV5KDG submitted 2023-11-16 astro-ph.CO astro-ph.IM

Analysis of an iterative reconstruction method in comparison of the standard reconstruction method

classification astro-ph.CO astro-ph.IM
keywords algorithmreconstructionsmoothingdensitymethodfielditerativespace
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We present a detailed analysis of a new, iterative density reconstruction algorithm. This algorithm uses a decreasing smoothing scale to better reconstruct the density field in Lagrangian space. We implement this algorithm to run on the Quijote simulations, and extend it to (a) include a smoothing kernel that smoothly goes from anisotropic to isotropic, and (b) a variant that does not correct for redshift space distortions. We compare the performance of this algorithm with the standard reconstruction method. Our examinations of the methods include cross-correlation of the reconstructed density field with the linear density field, reconstructed two-point functions, and BAO parameter fitting. We also examine the impact of various parameters, such as smoothing scale, anisotropic smoothing, tracer type/bias, and the inclusion of second order perturbation theory. We find that the two reconstruction algorithms are comparable in most of the areas we examine. In particular, both algorithms give consistent fittings of BAO parameters. The fits are robust over a range of smoothing scales. We find the iterative algorithm is significantly better at removing redshift space distortions. The new algorithm will be a promising method to be employed in the ongoing and future large-scale structure surveys.

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