Built on

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1983
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U. Seljak, The Astrophysical Journal, Volume 482, Issue 1, pp. 6-16. 482
1996
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M. Kamionkowski, A. Kosowsky, and A. Stebbins, Physical Review D 55
1997
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J.-L. Vergely, R. F. Ferrero, D. Egret, and J. Koeppen, Astronomy and Astrophysics (1998), URL http://adsabs.harvard.edu/abs/1998A{%}26A...340..543V
1998
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R. H. Hildebrand, J. L. Dotson, C. D. Dowell, D. A. Schleuning, and J. E. Vaillancourt, The Astrophysical Journal 516
1999
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B. Draine, Annual Review of Astronomy and Astrophysics 41
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K. M. Gorski, E. Hivon, A. J. Banday, B. D. Wandelt, F. K. Hansen, M. Reinecke, and M. Bartelmann, The Astrophysical Journal 622
2005
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A. Lazarian, Journal of Quantitative Spectroscopy and Radiative Transfer 106
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2007
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M. Jurić, Ž. Ivezić, A. Brooks, R. H. Lupton, D. Schlegel, D. Finkbeiner, N. Padmanabhan, N. Bond, B. Sesar, C. M. Rockosi, et al., The Astrophysical Journal 673
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M. Compiègne, L. Verstraete, A. Jones, J.-P. Bernard, F. Boulanger, N. Flagey, J. Le Bourlot, D. Paradis, and N. Ysard, Astronomy & Astrophysics 525
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2010
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B. T. Draine and B. Hensley, The Astrophysical Journal 757
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2012
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K. Abazajian, K. Arnold, J. Austermann, B. Benson, C. Bischoff, J. Bock, J. Bond, J. Borrill, E. Calabrese, J. Carlstrom, et al., Astroparticle Physics 63
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2015
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2016

Line-of-Sight Extrapolation Noise in Dust Polarization

Poh, Jason, Dodelson, Scott

Understand

The B-modes of polarization at frequencies ranging from 50-1000 GHz are produced by Galactic dust, lensing of primordial E-modes in the cosmic microwave background (CMB) by intervening large scale structure, and possibly by primordial B-modes in the CMB imprinted by gravitational waves produced during inflation.

The conventional method used to separate the dust component of the signal is to assume that the signal at high frequencies (e.g., 350 GHz) is due solely to dust and then extrapolate the signal down to lower frequency (e.g., 150 GHz) using the measured scaling of the polarized dust signal amplitude with frequency.
For typical Galactic thermal dust temperatures of about 20K, these frequencies are not fully in the Rayleigh-Jeans limit.
Therefore, deviations in the dust cloud temperatures from cloud to cloud will lead to different scaling factors for clouds of different temperatures.

Built on

R. H. Hildebrand, Quarterly Journal of the Royal Astronomical Society 24
1983
Earlier work this paper cites.
U. Seljak, The Astrophysical Journal, Volume 482, Issue 1, pp. 6-16. 482
1996
Earlier work this paper cites.
M. Kamionkowski, A. Kosowsky, and A. Stebbins, Physical Review D 55
1997
Earlier work this paper cites.
J.-L. Vergely, R. F. Ferrero, D. Egret, and J. Koeppen, Astronomy and Astrophysics (1998), URL http://adsabs.harvard.edu/abs/1998A{%}26A...340..543V
1998
Earlier work this paper cites.
R. H. Hildebrand, J. L. Dotson, C. D. Dowell, D. A. Schleuning, and J. E. Vaillancourt, The Astrophysical Journal 516
1999
Earlier work this paper cites.
B. Draine, Annual Review of Astronomy and Astrophysics 41
2003
Earlier work this paper cites.
K. M. Gorski, E. Hivon, A. J. Banday, B. D. Wandelt, F. K. Hansen, M. Reinecke, and M. Bartelmann, The Astrophysical Journal 622
2005
Earlier work this paper cites.
A. Lazarian, Journal of Quantitative Spectroscopy and Radiative Transfer 106
Original
2007
Earlier work this paper cites.
M. Jurić, Ž. Ivezić, A. Brooks, R. H. Lupton, D. Schlegel, D. Finkbeiner, N. Padmanabhan, N. Bond, B. Sesar, C. M. Rockosi, et al., The Astrophysical Journal 673
2008
Earlier work this paper cites.
M. Compiègne, L. Verstraete, A. Jones, J.-P. Bernard, F. Boulanger, N. Flagey, J. Le Bourlot, D. Paradis, and N. Ysard, Astronomy & Astrophysics 525
Original
2010
Earlier work this paper cites.
B. T. Draine and B. Hensley, The Astrophysical Journal 757
Original
2012
Earlier work this paper cites.

Similar

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Original
2012
Cited alongside, same era.
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Original
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Cited alongside, same era.
B. T. Draine and B. Hensley, The Astrophysical Journal 765
Original
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Original
2014
Cited alongside, same era.
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Then

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Original
2015
Later among the works it cites.
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2014

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