z-logo
open-access-imgOpen Access
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

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here
Accelerating Research

Address

John Eccles House
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom