Published October 1, 2009 | Version v1
Journal article

IMPROVED SIMULATION OF NON-GAUSSIAN TEMPERATURE AND POLARIZATION COSMIC MICROWAVE BACKGROUND MAPS

  • 1. Max-Planck-Institut fuer Astrophysik, Karl-Schwarzschild-Strasse 1, D-85748 Garching (Germany)
  • 2. Department of Physics, University of Illinois at Urbana-Champaign, 1110 W. Green Street, Urbana, IL 61801 (United States)

Description

We describe an algorithm to generate temperature and polarization maps of the cosmic microwave background (CMB) radiation containing non-Gaussianity of arbitrary local type. We apply an optimized quadrature scheme that allows us to predict and control integration accuracy, speed up the calculations, and reduce memory consumption by an order of magnitude. We generate 1000 non-Gaussian CMB temperature and polarization maps up to a multipole moment of lmax = 1024. We validate the method and code using the power spectrum and the fast cubic (bispectrum) estimator and find consistent results. The simulations are provided to the community.

Availability note (English)

Available from http://dx.doi.org/10.1088/0067-0049/184/2/264

Additional details

Identifiers

Publishing Information

Journal Title
Astrophysical Journal, Supplement Series
Journal Volume
184
Journal Issue
2
Journal Page Range
p. 264-270
ISSN
0067-0049
CODEN
APJSA2

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
41046366
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
ALGORITHMS; MAPS; POLARIZATION; RELICT RADIATION; SIMULATION
Descriptors DEC
ELECTROMAGNETIC RADIATION; MATHEMATICAL LOGIC; MICROWAVE RADIATION; RADIATIONS