Astrophysical: Cosmic background radiation

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    Planck 2013 results. II. Low Frequency Instrument data processing
    We describe the data processing pipeline of the Planck Low Frequency Instrument (LFI) data processing centre (DPC) to create and characterize full-sky maps...
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    Planck 2013 results. III. LFI systematic uncertainties
    We present the current estimate of instrumental and systematic effect uncertainties for the Planck-Low Frequency Instrument relevant to the first release of the...
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    Planck 2013 results. IV. Low Frequency Instrument beams and window functions
    This paper presents the characterization of the in-flight beams, the beam window functions, and the associated uncertainties for the Planck Low Frequency...
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    Planck 2013 results. V. LFI calibration
    We discuss the methods employed to photometrically calibrate the data acquired by the Low Frequency Instrument on Planck. Our calibration is based on a...
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    Planck 2013 results. VI. High Frequency Instrument data processing
    Wedescribe the processing of the 531 billion raw data samples from the High Frequency Instrument (HFI), which we performed to produce six temperature maps from...
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    Planck 2013 results. XII. Diffuse component separation
    Planck has produced detailed all-sky observations over nine frequency bands between 30 and 857 GHz. These observations allow robust reconstruction of the...
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    Planck 2013 results. XIV. Zodiacal emission
    The Planck satellite provides a set of all-sky maps at nine frequencies from 30 GHz to 857 GHz. Planets, minor bodies, and diffuse interplanetary dust emission...
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    Planck 2013 results. XIX. The integrated Sachs-Wolfe effect
    Based on cosmic microwave background (CMB) maps from the 2013 Planck Mission data release, this paper presents the detection of the integrated Sachs-Wolfe (ISW)...
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    Planck 2013 results. XV. CMB power spectra and likelihood
    This paper presents the Planck 2013 likelihood, a complete statistical description of the two-point correlation function of the CMB temperature fluctuations...