Beyond the 3rd moment: a practical study of using lensing convergence CDFs for cosmology with DES Y3
Beyond the 3rd moment: a practical study of using lensing convergence CDFs for cosmology with DES Y3
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超越第三矩:使用透镜会聚 CDF 与 DES Y3 进行宇宙学的实际研究
DOI:
10.1093/mnras/stad3118
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发表时间:
2023
影响因子:
4.8
通讯作者:
Anbajagane D
中科院分区:
文献类型:
--
作者:
Anbajagane D
Widefield surveys probe clustered scalar fields – such as galaxy counts, lensing potential, etc. – which are sensitive to different cosmological and astrophysical processes. Constraining such processes depends on the statistics that summarize the field. We explore the cumulative distribution function (CDF) as a summary of the galaxy lensing convergence field. Using a suite ofN-body light-cone simulations, we show the CDFs’ constraining power is modestly better than the second and third moments, as CDFs approximately capture information from all moments. We study the practical aspects of applying CDFs to data, using the Dark Energy Survey (DES Y3) data as an example, and compute the impact of different systematics on the CDFs. The contributions from the point spread function and reduced shear approximation areof the total signal. Source clustering effects and baryon imprints contribute 1–10 per cent. Enforcing scale cuts to limit systematics-driven biases in parameter constraints degrade these constraints a noticeable amount, and this degradation is similar for the CDFs and the moments. We detect correlations between the observed convergence field and the shape noise field at 13σ. The non-Gaussian correlations in the noise field must be modelled accurately to use the CDFs, or other statistics sensitive to all moments, as a rigorous cosmology tool.