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Planck Collaboration:, P. A. R. Ade, M. I. R. Alves, G. Aniano, C. Armitage-Caplan, M. Arnaud, F. Atrio-Barandela, J. Aumont, C. Baccigalupi, A. J. Banday
Robust forecasts on fundamental physics from the foreground-obscured, gravitationally-lensed CMB polarization
Josquin Errard, Stephen M. Feeney, Hiranya V. Peiris and Andrew H. Jaffe Journal of Cosmology and Astroparticle Physics 2016(03) 052 (2016) https://doi.org/10.1088/1475-7516/2016/03/052
Radiative feedback and cosmic molecular gas: the role of different radiative sources
Umberto Maio, Margarita Petkova, Gabriella De Lucia and Stefano Borgani Monthly Notices of the Royal Astronomical Society 460(4) 3733 (2016) https://doi.org/10.1093/mnras/stw1196
New constraints on modelling the random magnetic field of the MW
MAPS OF THE MAGELLANIC CLOUDS FROM COMBINED SOUTH POLE TELESCOPE AND PLANCK DATA
T. M. Crawford, R. Chown, G. P. Holder, K. A. Aird, B. A. Benson, L. E. Bleem, J. E. Carlstrom, C. L. Chang, H-M. Cho, A. T. Crites, T. de Haan, M. A. Dobbs, E. M. George, N. W. Halverson, N. L. Harrington, W. L. Holzapfel, Z. Hou, J. D. Hrubes, R. Keisler, L. Knox, A. T. Lee, E. M. Leitch, D. Luong-Van, D. P. Marrone, J. J. McMahon, et al. The Astrophysical Journal Supplement Series 227(2) 23 (2016) https://doi.org/10.3847/1538-4365/227/2/23
PILOT: a balloon-borne experiment to measure the polarized FIR emission of dust grains in the interstellar medium
Cosmic infrared background anisotropies as a window into primordial non-Gaussianity
Marco Tucci, Vincent Desjacques and Martin Kunz Monthly Notices of the Royal Astronomical Society 463(2) 2046 (2016) https://doi.org/10.1093/mnras/stw2086
FOREGROUND BIAS FROM PARAMETRIC MODELS OF FAR-IR DUST EMISSION
Sensitivity and foreground modelling for large-scale cosmic microwave background B-mode polarization satellite missions
M. Remazeilles, C. Dickinson, H. K. K. Eriksen and I. K. Wehus Monthly Notices of the Royal Astronomical Society 458(2) 2032 (2016) https://doi.org/10.1093/mnras/stw441
Searching for inflationary B modes: can dust emission properties be extrapolated from 350 GHz to 150 GHz?
Konstantinos Tassis and Vasiliki Pavlidou Monthly Notices of the Royal Astronomical Society: Letters 451(1) L90 (2015) https://doi.org/10.1093/mnrasl/slv077
Planckintermediate results. XXI. Comparison of polarized thermal emission from Galactic dust at 353 GHz with interstellar polarization in the visible
Paolo Creminelli, Diana López Nacir, Marko Simonović, Gabriele Trevisan and Matias Zaldarriaga Journal of Cosmology and Astroparticle Physics 2015(11) 031 (2015) https://doi.org/10.1088/1475-7516/2015/11/031