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Halo Nonlinear Reconstruction
Yu, Yu1; Zhu, Hong-Ming2,3; Pen, Ue-Li4,5,6,7
2017-10-01
Source PublicationASTROPHYSICAL JOURNAL
Volume847Issue:2
AbstractWe apply the nonlinear reconstruction method to simulated halo fields. For halo number density 2.77 X 10(-2) (h(-1)Mpc)(-3)at z = 0, corresponding to the SDSS main sample density, we find that the scale where the noise saturates the linear signal is improved to k greater than or similar to 0.36 h Mpc(-1), which is a factor of 2.29 improvement in scale, or 12 in number of linear modes. The improvement is less for higher redshift or lower halo density. We expect this to substantially improve the BAO accuracy of dense, low-redshift surveys, including the SDSS main sample, 6dFGS and 21 cm intensity mapping initiatives.
SubtypeArticle
KeywordLarge-scale Structure Of Universe
WOS HeadingsScience & Technology ; Physical Sciences
Funding OrganizationNational Science Foundation of China(11403071) ; National Science Foundation of China(11403071) ; Canada Foundation for Innovation under the Compute Canada ; Canada Foundation for Innovation under the Compute Canada ; Government of Ontario ; Government of Ontario ; Ontario Research Fund Research Excellence ; Ontario Research Fund Research Excellence ; University of Toronto ; University of Toronto ; David Dunlap family ; David Dunlap family ; Government of Canada through Industry Canada ; Government of Canada through Industry Canada ; Province of Ontario through the Ministry of Research Innovation ; Province of Ontario through the Ministry of Research Innovation ; National Science Foundation of China(11403071) ; National Science Foundation of China(11403071) ; Canada Foundation for Innovation under the Compute Canada ; Canada Foundation for Innovation under the Compute Canada ; Government of Ontario ; Government of Ontario ; Ontario Research Fund Research Excellence ; Ontario Research Fund Research Excellence ; University of Toronto ; University of Toronto ; David Dunlap family ; David Dunlap family ; Government of Canada through Industry Canada ; Government of Canada through Industry Canada ; Province of Ontario through the Ministry of Research Innovation ; Province of Ontario through the Ministry of Research Innovation
DOI10.3847/1538-4357/aa89e7
WOS KeywordBARYON ACOUSTIC-OSCILLATIONS ; MATTER POWER SPECTRUM ; DISTANCE MEASUREMENTS ; INFORMATION-CONTENT ; GALAXY SAMPLE ; I. ; ALGORITHM ; Z=0.35 ; SCALE
Indexed BySCI
Language英语
Funding OrganizationNational Science Foundation of China(11403071) ; National Science Foundation of China(11403071) ; Canada Foundation for Innovation under the Compute Canada ; Canada Foundation for Innovation under the Compute Canada ; Government of Ontario ; Government of Ontario ; Ontario Research Fund Research Excellence ; Ontario Research Fund Research Excellence ; University of Toronto ; University of Toronto ; David Dunlap family ; David Dunlap family ; Government of Canada through Industry Canada ; Government of Canada through Industry Canada ; Province of Ontario through the Ministry of Research Innovation ; Province of Ontario through the Ministry of Research Innovation ; National Science Foundation of China(11403071) ; National Science Foundation of China(11403071) ; Canada Foundation for Innovation under the Compute Canada ; Canada Foundation for Innovation under the Compute Canada ; Government of Ontario ; Government of Ontario ; Ontario Research Fund Research Excellence ; Ontario Research Fund Research Excellence ; University of Toronto ; University of Toronto ; David Dunlap family ; David Dunlap family ; Government of Canada through Industry Canada ; Government of Canada through Industry Canada ; Province of Ontario through the Ministry of Research Innovation ; Province of Ontario through the Ministry of Research Innovation
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000416699000001
Citation statistics
Cited Times:8[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/20291
Collection星系宇宙学研究部
Affiliation1.Chinese Acad Sci, Shanghai Astron Observ, Key Lab Res Galaxies & Cosmol, 80 Nandan Rd, Shanghai 200030, Peoples R China
2.Chinese Acad Sci, Natl Astron Observatories, Key Lab Computat Astrophys, 20A Datun Rd, Beijing 100012, Peoples R China
3.Univ Chinese Acad Sci, Beijing 100049, Peoples R China
4.Univ Toronto, Canadian Inst Theoret Astrophys, 60 St George St, Toronto, ON M5S 3H8, Canada
5.Univ Toronto, Dunlap Inst Astron & Astrophys, 50 St George St, Toronto, ON M5S 3H4, Canada
6.Canadian Inst Adv Res, CIFAR Program Gravitat & Cosmol, Toronto, ON M5G 1Z8, Canada
7.Perimeter Inst Theoret Phys, 31 Caroline St North, Waterloo, ON N2L 2Y5, Canada
Recommended Citation
GB/T 7714
Yu, Yu,Zhu, Hong-Ming,Pen, Ue-Li. Halo Nonlinear Reconstruction[J]. ASTROPHYSICAL JOURNAL,2017,847(2).
APA Yu, Yu,Zhu, Hong-Ming,&Pen, Ue-Li.(2017).Halo Nonlinear Reconstruction.ASTROPHYSICAL JOURNAL,847(2).
MLA Yu, Yu,et al."Halo Nonlinear Reconstruction".ASTROPHYSICAL JOURNAL 847.2(2017).
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