Study on the mapping of dark matter clustering from real space to redshift space
Yi Zheng, Yong-Seon Song (KASI)

TL;DR
This paper develops a systematic approach to accurately model the mapping of dark matter clustering from real to redshift space, effectively handling non-linearities and velocity effects to match observed power spectra.
Contribution
It introduces a new perturbative mapping formula that separates and controls systematics, validated with simulations up to small scales.
Findings
Gaussian FoG function with one parameter is effective
Mapping formula accurately reproduces 2D power spectrum up to k~0.2h/Mpc
Systematics are controlled by direct measurement and polynomial expansion
Abstract
The mapping of dark matter clustering from real space to redshift space introduces the anisotropic property to the measured density power spectrum in redshift space, known as the redshift space distortion effect. The mapping formula is intrinsically non-linear, which is complicated by the higher order polynomials due to indefinite cross correlations between the density and velocity fields, and the Finger-of-God effect due to the randomness of the peculiar velocity field. Whilst the full higher order polynomials remain unknown, the other systematics can be controlled consistently within the same order truncation in the expansion of the mapping formula, as shown in this paper. The systematic due to the unknown non-linear density and velocity fields is removed by separately measuring all terms in the expansion directly using simulations. The uncertainty caused by the velocity randomness is…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsAstronomical Observations and Instrumentation · CCD and CMOS Imaging Sensors · Image Processing Techniques and Applications
