Compared to results from Planck’s predecessor, WMAP, t5he results coming out of Planck have appeared in the public domain excruciatingly slowly. But here they are at last.
http://arxiv.org/pdf/1502.01582.pdf
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. This paper gives an overview of the main
characteristics of the data and the data products in the release, as well as the associated cosmological and astrophysical science results and papers.
The science products include maps of the cosmic microwave background (CMB), the thermal Sunyaev-Zeldovich effect, and diffuse foregrounds
in temperature and polarization, catalogues of compact Galactic and extragalactic sources (including separate catalogues of Sunyaev-Zeldovich
clusters and Galactic cold clumps), and extensive simulations of signals and noise used in assessing the performance of the analysis methods and
assessment of uncertainties. The likelihood code used to assess cosmological models against the Planck data are described, as well as a CMB
lensing likelihood. Scientific results include cosmological parameters deriving from CMB power spectra, gravitational lensing, and cluster counts,
as well as constraints on inflation, non-Gaussianity, primordial magnetic fields, dark energy, and modified gravity.
Papers accompanying this data and analysis release – most available on ArXiV
I. Overview of products and results (this paper)
II. Low Frequency Instrument data processing
III. LFI systematic uncertainties
IV. LFI beams and window functions
V. LFI calibration
VI. LFI maps
VII. High Frequency Instrument data processing: Time-ordered
information and beam processing
VIII. High Frequency Instrument data processing: Calibration
and maps
IX. Diffuse component separation: CMB maps
X. Diffuse component separation: Foreground maps
XI. CMB power spectra, likelihood, and consistency of cosmological parameters
XII. Simulations
XIII. Cosmological parameters
XIV. Dark energy and modified gravity
XV. Gravitational lensing
XVI. Isotropy and statistics of the CMB
XVII. Primordial non-Gaussianity
XVIII. Background geometry and topology of the Universe
XIX. Constraints on primordial magnetic fields
XX. Constraints on inflation
XXI. The integrated Sachs-Wolfe effect
XXII. A map of the thermal Sunyaev-Zeldovich effect
XXIII. The thermal Sunyaev-Zeldovich effect–cosmic infrared background correlation
XXIV. Cosmology from Sunyaev-Zeldovich cluster counts
XXV. Diffuse, low-frequency Galactic foregrounds
XXVI. The Second Planck Catalogue of Compact Sources
XXVII. The Second Planck Catalogue of Sunyaev-Zeldovich Sources
XXVIII. The Planck Catalogue of Galactic Cold Clumps