천문학회보 (The Bulletin of The Korean Astronomical Society)
- 제42권2호
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- Pages.55.1-55.1
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- 2017
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- 1226-2692(pISSN)
HectoMAP and Horizon Run 4: Over- and Under-dense Large-scale Structures in the Real and Simulated Universe
- Hwang, Ho Seong (Quantum Universe Center, Korea Institute for Advanced Study) ;
- Geller, M.J. (Smithsonian Astrophysical Observatory) ;
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Park, Changbom
(School of Physics, Korea Institute for Advanced Study) ;
- Fabricant, D.G. (Smithsonian Astrophysical Observatory) ;
- Kurtz, M.J. (Smithsonian Astrophysical Observatory) ;
- Rines, K.J. (Western Washington University) ;
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Kim, Juhan
(Center for Advanced Computation, Korea Institute for Advanced Study) ;
- Diaferio, A. (Universita degli Studi di Torino/Istituto Nazionale di Fisica Nucleare) ;
- Zahid, H.J. (Smithsonian Astrophysical Observatory) ;
- Berlind, P. (Smithsonian Astrophysical Observatory) ;
- Calkins, M. (Smithsonian Astrophysical Observatory) ;
- Tokarz, S. (Smithsonian Astrophysical Observatory) ;
- Moran, S. (Smithsonian Astrophysical Observatory)
- 발행 : 2017.10.10
초록
HectoMAP is a dense redshift survey of red galaxies covering a 53 square degree strip of the northern sky, and Horizon Run 4 is one of the densest and largest cosmological simulations based on the standard Lambda cold dark matter model. We use HectoMAP and Horizon Run 4 to compare the physical properties of observed large-scale structures with simulated ones in the redshift range 0.22
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