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- W2149351844 abstract "We present two large cosmological N-body simulations, called Horizon Run 2 (HR2) and Horizon Run 3 (HR3), made using <TEX>$6000^3$</TEX> = 216 billions and <TEX>$7210^3$</TEX> = 374 billion particles, spanning a volume of <TEX>$(7.200;h^{-1}Gpc)^3$</TEX> and <TEX>$(10.815;h^{-1}Gpc)^3$</TEX>, respectively. These simulations improve on our previous Horizon Run 1 (HR1) up to a factor of 4.4 in volume, and range from 2600 to over 8800 times the volume of the Millennium Run. In addition, they achieve a considerably finer mass resolution, down to <TEX>$1.25{times}10^{11}h^{-1}M_{odot}$</TEX>, allowing to resolve galaxy-size halos with mean particle separations of <TEX>$1.2h^{-1}$</TEX>Mpc and <TEX>$1.5h^{-1}$</TEX>Mpc, respectively. We have measured the power spectrum, correlation function, mass function and basic halo properties with percent level accuracy, and verified that they correctly reproduce the CDM theoretical expectations, in excellent agreement with linear perturbation theory. Our unprecedentedly large-volume N-body simulations can be used for a variety of studies in cosmology and astrophysics, ranging from large-scale structure topology, baryon acoustic oscillations, dark energy and the characterization of the expansion history of the Universe, till galaxy formation science - in connection with the new SDSS-III. To this end, we made a total of 35 all-sky mock surveys along the past light cone out to z = 0.7 (8 from the HR2 and 27 from the HR3), to simulate the BOSS geometry. The simulations and mock surveys are already publicly available at http://astro.kias.re.kr/Horizon-Run23/." @default.
- W2149351844 created "2016-06-24" @default.
- W2149351844 creator A5015908436 @default.
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- W2149351844 creator A5038397546 @default.
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- W2149351844 creator A5081806003 @default.
- W2149351844 date "2011-12-31" @default.
- W2149351844 modified "2023-10-17" @default.
- W2149351844 title "THE NEW HORIZON RUN COSMOLOGICAL N-BODY SIMULATIONS" @default.
- W2149351844 cites W1853767801 @default.
- W2149351844 cites W1894431533 @default.
- W2149351844 cites W1963811565 @default.
- W2149351844 cites W1964637103 @default.
- W2149351844 cites W1968752888 @default.
- W2149351844 cites W1973368884 @default.
- W2149351844 cites W1974823277 @default.
- W2149351844 cites W1977025542 @default.
- W2149351844 cites W1977522608 @default.
- W2149351844 cites W1982197353 @default.
- W2149351844 cites W1985559124 @default.
- W2149351844 cites W1993101312 @default.
- W2149351844 cites W1994006347 @default.
- W2149351844 cites W1995518004 @default.
- W2149351844 cites W1999367759 @default.
- W2149351844 cites W2007116814 @default.
- W2149351844 cites W2013644708 @default.
- W2149351844 cites W2016527243 @default.
- W2149351844 cites W2019473452 @default.
- W2149351844 cites W2029234737 @default.
- W2149351844 cites W2032469582 @default.
- W2149351844 cites W2039521251 @default.
- W2149351844 cites W2040357020 @default.
- W2149351844 cites W2042255966 @default.
- W2149351844 cites W2042707894 @default.
- W2149351844 cites W2045182341 @default.
- W2149351844 cites W2048616258 @default.
- W2149351844 cites W2049867118 @default.
- W2149351844 cites W2050197233 @default.
- W2149351844 cites W2062867710 @default.
- W2149351844 cites W2064645772 @default.
- W2149351844 cites W2065743072 @default.
- W2149351844 cites W2073832139 @default.
- W2149351844 cites W2075280515 @default.
- W2149351844 cites W2075387088 @default.
- W2149351844 cites W2075492061 @default.
- W2149351844 cites W2075841342 @default.
- W2149351844 cites W2077217166 @default.
- W2149351844 cites W2080820021 @default.
- W2149351844 cites W2082820126 @default.
- W2149351844 cites W2087432755 @default.
- W2149351844 cites W2088731601 @default.
- W2149351844 cites W2090319734 @default.
- W2149351844 cites W2091059059 @default.
- W2149351844 cites W2093615713 @default.
- W2149351844 cites W2096373963 @default.
- W2149351844 cites W2101568531 @default.
- W2149351844 cites W2110563485 @default.
- W2149351844 cites W2113869105 @default.
- W2149351844 cites W2118265220 @default.
- W2149351844 cites W2134287871 @default.
- W2149351844 cites W2135403967 @default.
- W2149351844 cites W2135497511 @default.
- W2149351844 cites W2141709306 @default.
- W2149351844 cites W2143513913 @default.
- W2149351844 cites W2144942952 @default.
- W2149351844 cites W2145844833 @default.
- W2149351844 cites W2147875900 @default.
- W2149351844 cites W2154542873 @default.
- W2149351844 cites W2157917411 @default.
- W2149351844 cites W2160253850 @default.
- W2149351844 cites W2162550289 @default.
- W2149351844 cites W2165724299 @default.
- W2149351844 cites W2167641424 @default.
- W2149351844 cites W2169866137 @default.
- W2149351844 cites W2170689655 @default.
- W2149351844 cites W2951915383 @default.
- W2149351844 cites W3099213746 @default.
- W2149351844 cites W3099582894 @default.
- W2149351844 cites W3100110286 @default.
- W2149351844 cites W3100175138 @default.
- W2149351844 cites W3100250662 @default.
- W2149351844 cites W3100636306 @default.
- W2149351844 cites W3101569155 @default.
- W2149351844 cites W3102003231 @default.
- W2149351844 cites W3103054202 @default.
- W2149351844 cites W3103877238 @default.
- W2149351844 cites W3104049539 @default.
- W2149351844 cites W3105469218 @default.
- W2149351844 cites W3105889752 @default.
- W2149351844 cites W3106274511 @default.
- W2149351844 cites W3106305664 @default.
- W2149351844 cites W3121565996 @default.
- W2149351844 cites W4301956287 @default.
- W2149351844 doi "https://doi.org/10.5303/jkas.2011.44.6.217" @default.
- W2149351844 hasPublicationYear "2011" @default.
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