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The characterization of the Galactic foregrounds has been shown to be the main obstacle in the challenging quest to detect primordial B-modes in the polarized microwave sky.
Armitage-Caplan, C., Dunkley, J., Eriksen, H. K., & Dickinson, C., Impact on the tensor-to-scalar ratio of incorrect Galactic foreground modelling. 2012, MNRAS, 424, 1914, 1203.0152
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Górski, K. M., Hivon, E., Banday, A. J., et al., HEALPix: A Framework for High-Resolution Discretization and Fast Analysis of Data Distributed on the Sphere. 2005, ApJ, 622, 759, astro-ph/0409513
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Tristram, M., Macías-Pérez, J. F., Renault, C., & Santos, D., XSPECT, estimation of the angular power spectrum by computing cross-power spectra with analytical error bars. 2005, MNRAS, 358, 833, astro-ph/0405575
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Eriksen, H. K., Dickinson, C., Lawrence, C. R., et al., Cosmic Microwave Background Component Separation by Parameter Estimation. 2006, ApJ, 641, 665, astro-ph/0508268
2006
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Eriksen, H. K., Jewell, J. B., Dickinson, C., et al., Joint Bayesian Component Separation and CMB Power Spectrum Estimation. 2008, ApJ, 676, 10, 0709.1058
2008
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Delabrouille, J., Betoule, M., Melin, J.-B., et al., The pre-launch Planck Sky Model: a model of sky emission at submillimetre to centimetre wavelengths. 2013, A&A, 553, A96, 1207.3675
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Planck Collaboration XI, Planck
2014
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Planck Collaboration Int. XVII, Planck
2014
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2014
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BICEP2 and Keck Array Collaborations, BICEP2 / Keck Array VI: Improved Constraints On Cosmology and Foregrounds When Adding 95 GHz Data From Keck Array. 2015, ArXiv e-prints, 1510.09217
2015
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BICEP2/Keck Array and Planck Collaborations, Joint Analysis of BICEP2/Keck Array and Planck Data. 2015, Phys. Rev. Lett., 114, 101301, 1502.00612
2015
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Choi, S. K. & Page, L. A., Polarized galactic synchrotron and dust emission and their correlation. 2015, J. Cosmology Astropart. Phys., 12, 020, 1509.05934
2015
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Clark, S. E., Hill, J. C., Peek, J. E. G., Putman, M. E., & Babler, B. L., Neutral Hydrogen Structures Trace Dust Polarization Angle: Implications for Cosmic Microwave Background Foregrounds. 2015, Physical Review Letters, 115, 241302, 1508.07005
2015
Cited alongside, same era.
Creminelli, P., López Nacir, D., Simonović, M., Trevisan, G., & Zaldarriaga, M., Detecting primordial B-modes after Planck. 2015, J. Cosmology Astropart. Phys., 11, 31, 1502.01983
2015
Cited alongside, same era.
Errard, J., Feeney, S. M., Peiris, H. V., & Jaffe, A. H., Robust forecasts on fundamental physics from the foreground-obscured, gravitationally-lensed CMB polarization. 2015, ArXiv e-prints, 1509.06770
2015
Cited alongside, same era.
Krachmalnicoff, N., Baccigalupi, C., Aumont, J., Bersanelli, M., & Mennella, A., Characterization of foreground emission at degree angular scale for CMB B-modes observations. Thermal Dust and Synchrotron signal from Planck and WMAP data. 2015, ArXiv e-prints, 1511.00532
2015
Kalberla, P. M. W., Kerp, J., Haud, U., et al., Cold Milky Way Hi gas in filaments. 2016, ArXiv e-prints, 1602.07604
2016
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2016
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2016
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2016
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2016
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2016
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Martin, P. G., Blagrave, K. P. M., Lockman, F. J., et al., GHIGLS: H I Mapping at Intermediate Galactic Latitude Using the Green Bank Telescope. 2015, ApJ, 809, 153, 1504.07723
2015
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2015
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2015
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2015
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2015
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Remazeilles, M., Dickinson, C., Eriksen, H. K. K., & Wehus, I. K., Sensitivity and foreground modelling for large-scale CMB B-mode polarization satellite missions. 2015, ArXiv e-prints, 1509.04714
2015
Cited alongside, same era.
Tassis, K. & Pavlidou, V., Searching for inflationary B modes: can dust emission properties be extrapolated from 350 GHz to 150 GHz? 2015, MNRAS, 451, L90, 1410.8136
2015
Cited alongside, same era.
Errard, J., Feeney, S. M., Peiris, H. V., & Jaffe, A. H., Robust forecasts on fundamental physics from the foreground-obscured, gravitationally-lensed CMB polarization. 2016, J. Cosmology Astropart. Phys., 3, 052, 1509.06770
2016
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2016
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