Published October 1, 2009
| Version v1
Journal article
IMPROVED SIMULATION OF NON-GAUSSIAN TEMPERATURE AND POLARIZATION COSMIC MICROWAVE BACKGROUND MAPS
Creators
- 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/10.1088/0067-0049/184/2/264Additional 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