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A model for polarized microwave foreground emission from interstellar dust

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Title: A model for polarized microwave foreground emission from interstellar dust
Authors: O'Dea, DT
Clark, CN
Contaldi, CR
MacTavish, CJ
Item Type: Journal Article
Abstract: The upcoming generation of cosmic microwave background experiments face a major challenge in detecting the weak cosmic B-mode signature predicted as a product of primordial gravitational waves. To achieve the required sensitivity these experiments must have impressive control of systematic effects and detailed understanding of the foreground emission that will influence the signal. In this paper, we present templates of the intensity and polarization of emission from one of the main Galactic foregrounds, interstellar dust. These are produced using a model which includes a three-dimensional description of the Galactic magnetic field, examining both large and small scales. We also include in the model the details of the dust density, grain alignment and the intrinsic polarization of the emission from an individual grain. We present here Stokes parameter template maps at 150 GHz and provide an online repository (http://www.imperial.ac.uk/people/c.contaldi/fgpol) for these and additional maps at frequencies that will be targeted by upcoming experiments such as EBEX, Spider and SPTpol.
Issue Date: 1-Jan-2012
Date of Acceptance: 16-Sep-2011
URI: http://hdl.handle.net/10044/1/93829
DOI: 10.1111/j.1365-2966.2011.19851.x
ISSN: 0035-8711
Publisher: Royal Astronomical Society
Start Page: 1795
End Page: 1803
Journal / Book Title: Monthly Notices of the Royal Astronomical Society
Volume: 419
Issue: 2
Copyright Statement: © 2011 The Authors Monthly Notices of the Royal Astronomical Society © 2011 RAS. This is a pre-copy-editing, author-produced version of an article accepted for publication in Monthly Notices of the Royal Astronomical Society, following peer review. The definitive publisher-authenticated version D. T. O’Dea, C. N. Clark, C. R. Contaldi, C. J. MacTavish, A model for polarized microwave foreground emission from interstellar dust, Monthly Notices of the Royal Astronomical Society, Volume 419, Issue 2, January 2012, Pages 1795–1803 is available online at: https://doi.org/10.1111/j.1365-2966.2011.19851.x
Sponsor/Funder: Science and Technology Facilities Council (STFC)
Science and Technology Facilities Council (STFC)
Funder's Grant Number: PP/E002129/1
ST/G000743/1
Keywords: Science & Technology
Physical Sciences
Astronomy & Astrophysics
gravitational waves
polarization
galaxies: magnetic fields
PROBE WMAP OBSERVATIONS
GALACTIC MAGNETIC-FIELD
BACKGROUND-RADIATION
POWER SPECTRA
OBSERVATIONAL CONSTRAINTS
COMPONENT SEPARATION
2003 FLIGHT
TEMPERATURE
PLANE
DENSITY
Science & Technology
Physical Sciences
Astronomy & Astrophysics
gravitational waves
polarization
galaxies: magnetic fields
PROBE WMAP OBSERVATIONS
GALACTIC MAGNETIC-FIELD
BACKGROUND-RADIATION
POWER SPECTRA
OBSERVATIONAL CONSTRAINTS
COMPONENT SEPARATION
2003 FLIGHT
TEMPERATURE
PLANE
DENSITY
astro-ph.CO
astro-ph.CO
astro-ph.GA
0201 Astronomical and Space Sciences
Astronomy & Astrophysics
Publication Status: Published
Online Publication Date: 2011-09-16
Appears in Collections:Physics
Theoretical Physics