The large-scale polarization of the microwave foreground
Authors:
- Angélica de Oliveira-CostaAOAngélica de Oliveira-Costa
- Max TegmarkMTMax Tegmark
- Christopher O’dEllCOChristopher O’dEll
- Brian KeatingBKBrian Keating
- Peter TimbiePTPeter Timbie
- George EfstathiouGEGeorge Efstathiou
- George SmootGSGeorge Smoot
- 1 December 2003
- journal article
- Published by Elsevier in New Astronomy Reviews
- Vol. 47 (11-12) , 1117-1121
Abstract
No abstract availableKeywords
All Related Versions
This publication has 23 references indexed in Scilit:
- The power-law behaviours of angular spectra of polarized Galactic synchrotronNew Astronomy, 2002
- Towards a model of full-sky Galactic synchrotron intensity and linear polarisation: A re-analysis of the Parkes dataAstronomy & Astrophysics, 2002
- A multifrequency analysis of the polarized diffuse galactic radio emission at degree scalesAIP Conference Proceedings, 2002
- The angular power spectrum of radio emission at 2.3 GHzAstronomy & Astrophysics, 2001
- Radical Compression of Cosmic Microwave Background DataThe Astrophysical Journal, 2000
- Polarization pursuers’ guidePhysical Review D, 2000
- Foregrounds and CMB experimentsNew Astronomy, 1999
- Polarized radio emission over the southern Galactic plane at 2.4 GHzMonthly Notices of the Royal Astronomical Society, 1997
- CMB anisotropies: Total angular momentum methodPhysical Review D, 1997
- Fluctuations in the galactic synchrotron radiation - I. Implications for searches for fluctuations of cosmological originMonthly Notices of the Royal Astronomical Society, 1991