The Jubilee ISW Project - II. Observed and simulated imprints of voids and superclusters on the cosmic microwave background

被引：45

作者：

Hotchkiss, S. ^{[1
]}

Nadathur, S. ^{[2
,3
]}

Gottloeber, S. ^{[4
]}

Iliev, I. T. ^{[1
]}

Knebe, A. ^{[5
]}

Watson, W. A. ^{[1
]}

Yepes, G. ^{[5
]}

机构：

[1] Univ Sussex, Dept Phys & Astron, Brighton BN1 9QH, E Sussex, England

[2] Univ Helsinki, Dept Phys, FI-00014 Helsinki, Finland

[3] Univ Helsinki, Helsinki Inst Phys, FI-00014 Helsinki, Finland

[4] Leibniz Inst Astrophys, D-14482 Potsdam, Germany

[5] Univ Autonoma Madrid, Dept Fis Teor, Fac Ciencias, E-28049 Madrid, Spain

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2015年 / 446卷 / 02期

基金：

芬兰科学院; 欧洲研究理事会; 澳大利亚研究理事会; 美国国家航空航天局; 美国国家科学基金会;

关键词：

methods: numerical; cosmic background radiation; dark energy; large-scale structure of Universe; BARYON ACOUSTIC-OSCILLATIONS; GALAXY SURVEY; CATALOG; CONSTRAINTS; CLUSTERS; MAP;

D O I：

10.1093/mnras/stu2072

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We examine the integrated Sachs-Wolfe (ISW) imprint of voids and superclusters on the cosmic microwave background. We first study results from the Jubilee N-body simulation. From Jubilee, we obtain the full-sky ISW signal from structures out to redshift z = 1.4 and a mock luminous red galaxy catalogue. We confirm that the expected signal in the concordance Lambda cold dark matter (Lambda CDM) model is very small and likely to always be much smaller than the anisotropies arising at the last scattering surface. Any current detections of such an imprint must, therefore, predominantly arise from something other than an ISW effect in a Lambda CDM universe. Using the simulation as a guide, we then look for the signal using a catalogue of voids and superclusters from the Sloan Digital Sky Survey. We find a result that is consistent with the Lambda CDM model, i.e. a signal consistent with zero.

引用

页码：1321 / 1334

页数：14

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