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Exploring cosmic origins with CORE: Survey requirements and mission design / CORE Collaboration
Future observations of cosmic microwave background (CMB) polarisation have the potential to answer some of the most fundamental questions of modern physics and cosmology. In this paper, we list the requirements for a future CMB polarisation survey addressing these scientific objectives, and discuss the design drivers of the CORE space mission proposed to ESA in answer to the "M5" call for a medium-sized mission. [...]
arXiv:1706.04516.- 2018-04-05 - 79 p. - Published in : JCAP Fulltext: PDF; Preprint: PDF;

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Planck 2015 results. IX. Diffuse component separation: CMB maps / Planck Collaboration
We present foreground-reduced CMB maps derived from the full Planck data set in both temperature and polarization. Compared to the corresponding Planck 2013 temperature sky maps, the total data volume is larger by a factor of 3.2 for frequencies between 30 and 70 GHz, and by 1.9 for frequencies between 100 and 857 GHz. [...]
arXiv:1502.05956.- 2016-09-20 - 42 p. - Published in : Astron. Astrophys. 594 (2016) A9 Fulltext: PDF; External link: Preprint

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Planck 2015. XX. Constraints on inflation / Planck Collaboration
We present the implications for cosmic inflation of the Planck measurements of the cosmic microwave background (CMB) anisotropies in both temperature and polarization based on the full Planck survey. The Planck full mission temperature data and a first release of polarization data on large angular scales measure the spectral index of curvature perturbations to be $n_\mathrm{s} = 0.968 \pm 0.006$ and tightly constrain its scale dependence to $d n_s/d \ln k =-0.003 \pm 0.007$ when combined with the Planck lensing likelihood. [...]
arXiv:1502.02114.- 2016-09-20 - 65 p. - Published in : Astron. Astrophys. 594 (2016) A20 Fulltext: PDF; External link: Preprint

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Planck 2015 results. XIV. Dark energy and modified gravity / Planck Collaboration
We study the implications of Planck data for models of dark energy (DE) and modified gravity (MG), beyond the cosmological constant scenario. We start with cases where the DE only directly affects the background evolution, considering Taylor expansions of the equation of state, principal component analysis and parameterizations related to the potential of a minimally coupled DE scalar field. [...]
arXiv:1502.01590.- 2016-09-20 - 31 p. - Published in : Astron. Astrophys. 594 (2016) A14 Fulltext: PDF; External link: Preprint

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Planck 2015 results. XIII. Cosmological parameters / Planck Collaboration
We present results based on full-mission Planck observations of temperature and polarization anisotropies of the CMB. These data are consistent with the six-parameter inflationary LCDM cosmology. [...]
arXiv:1502.01589.- 2016-09-20 - 63 p. - Published in : Astron. Astrophys. 594 (2016) A13 Fulltext: PDF; External link: Preprint

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Planck 2015 results. X. Diffuse component separation: Foreground maps / Planck Collaboration
Planck has mapped the microwave sky in nine frequency bands between 30 and 857 GHz in temperature and seven bands between 30 and 353 GHz in polarization. In this paper we consider the problem of diffuse astrophysical component separation, and process these maps within a Bayesian framework to derive a consistent set of full-sky astrophysical component maps. [...]
arXiv:1502.01588.- 2016-09-20 - 63 p. - Published in : Astron. Astrophys. 594 (2016) A10 Fulltext: PDF; External link: Preprint

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Planck 2015 results. IV. Low Frequency Instrument beams and window functions / Planck Collaboration
This paper presents the characterization of the in-flight beams, the beam window functions, and the associated uncertainties for the Planck Low Frequency Instrument (LFI). The structure of the paper is similar to that presented in the 2013 Planck release; the main differences concern the beam normalization and the delivery of the window functions to be used for polarization analysis. [...]
arXiv:1502.01584.- 2016-09-20 - 22 p. - Published in : Astron. Astrophys. 594 (2016) A4 Fulltext: PDF; External link: Preprint

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Planck 2015 results. I. Overview of products and scientific results / Planck Collaboration
The European Space Agency's Planck satellite, dedicated to studying the early Universe and its subsequent evolution, was launched 14~May 2009 and scanned the microwave and submillimetre sky continuously between 12~August 2009 and 23~October 2013. In February~2015, ESA and the Planck Collaboration released the second set of cosmology products based on data from the entire Planck mission, including both temperature and polarization, along with a set of scientific and technical papers and a web-based explanatory supplement. [...]
arXiv:1502.01582.- 2016-09-20 - 38 p. - Published in : Astron. Astrophys. 594 (2016) A1 Fulltext: PDF; External link: Preprint

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Mu2e Technical Design Report / Bartoszek, L ; Barnes, E ; Miller, J P ; Mott, J ; Palladino, A ; Quirk, J ; Roberts, B L ; Crnkovic, J ; Polychronakos, V ; Tishchenko, V et al.
The Mu2e experiment at Fermilab will search for charged lepton flavor violation via the coherent conversion process mu- N --> e- N with a sensitivity approximately four orders of magnitude better than the current world's best limits for this process. [...]
arXiv:1501.05241 ; FERMILAB-TM-2594 ; FERMILAB-DESIGN-2014-1. - 2015. - 888 p.
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Planck 2013 results. XXXI. Consistency of the Planck data / Planck Collaboration
The Planck design and scanning strategy provide many levels of redundancy that can be exploited to provide tests of internal consistency. One of the most important is the comparison of the 70 GHz (amplifier) and 100 GHz (bolometer) channels. [...]
arXiv:1508.03375.- 2014 - 27 p. - Published in : Astron. Astrophys. 571 (2014) A31 External links: EDP Sciences Free Access article; Fulltext

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