MoLUSC: A Mock Local Universe Survey Constructor
Author(s) -
T. Sousbie,
H. M. Courtois,
Greg L. Bryan,
Julien Devriendt
Publication year - 2008
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/526507
Subject(s) - dark matter , galaxy , redshift , sky , transformation (genetics) , computer science , scale (ratio) , astrophysics , physics , biochemistry , chemistry , quantum mechanics , gene
This paper presents MoLUSC, a new method for generating mock galaxy catalogsfrom a large scale ($\approx 1000^3$ Mpc$^3$) dark matter simulation, thatrequires only modest CPU time and memory allocation. The method uses asmall-scale ($\approx 256^3$ Mpc$^3$) dark matter simulation on which the\galics semi-analytic code has been run in order to define the transformationfrom dark matter density to galaxy density transformation using a probabilistictreatment. MoLUSC is then applied to a large-scale dark matter simulation inorder to produce a realistic distribution of galaxies and their associatedspectra. This permits the fast generation of large-scale mock surveys usingrelatively low-resolution simulations. We describe various tests which havebeen conducted to validate the method, and demonstrate a first application togenerate a mock Sloan Digital Sky Survey redshift survey.Comment: submitted to Ap
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