about
Planck 2013 results. I. Overview of products and scientific resultsThe Athena X-ray Integral Field Unit (X-IFU)Planck intermediate results: XXXII. The relative orientation between the magnetic field and structures traced by interstellar dustPlanck 2013 results. XVI. Cosmological parametersPlanck early results. XXII. The submillimetre properties of a sample of Galactic cold clumpsPlanck early results. XXVI. Detection with Planck and confirmation by XMM-Newton of PLCK G266.6–27.3, an exceptionally X-ray luminous and massive galaxy cluster at z ~ 1Planck 2015 results. XIII. Cosmological parametersPlanck intermediate results XXXI. Microwave survey of Galactic supernova remnantsPlanck intermediate results XXV. The Andromeda galaxy as seen by PlanckPlanck intermediate results XXIII. Galactic plane emission components derived from Planck with ancillary dataPlanck intermediate results XXX. The angular power spectrum of polarized dust emission at intermediate and high Galactic latitudesPlanck 2013 results. XXIII. Isotropy and statistics of the CMBPlanck 2015 resultsPlanck2013 results. XXVII. Doppler boosting of the CMB: Eppur si muovePlanck intermediate results XIII. Constraints on peculiar velocitiesPlanck 2015 resultsPlanck 2013 results. XXV. Searches for cosmic strings and other topological defectsThe molecular hydrogen explorer H2EXPlanck pre-launch status: The Planck missionNew constraints on modified Newtonian dynamics from galaxy clustersNon-parametric deprojection of NIKA SZ observations: Pressure distribution in thePlanck-discovered cluster PSZ1 G045.85+57.71Planck intermediate results. XVIII. The millimetre and sub-millimetre emission from planetary nebulaePlanck intermediate results. XIX. An overview of the polarized thermal emission from Galactic dustPlanck intermediate results. XX. Comparison of polarized thermal emission from Galactic dust with simulations of MHD turbulencePlanck intermediate results. XXI. Comparison of polarized thermal emission from Galactic dust at 353 GHz with interstellar polarization in the visiblePlanck intermediate results. XXII. Frequency dependence of thermal emission from Galactic dust in intensity and polarizationPlanck 2013 results. II. Low Frequency Instrument data processingPlanck 2013 results. III. LFI systematic uncertaintiesPlanck 2013 results. IV. Low Frequency Instrument beams and window functionsPlanck 2013 results. IX. HFI spectral responsePlanck 2013 results. V. LFI calibrationPlanck 2013 results. VI. High Frequency Instrument data processingPlanck 2013 results. VII. HFI time response and beamsPlanck 2013 results. VIII. HFI photometric calibration and mapmakingPlanck 2013 results. X. HFI energetic particle effects: characterization, removal, and simulationPlanck 2013 results. XI. All-sky model of thermal dust emissionPlanck 2013 results. XII. Diffuse component separationPlanck 2013 results. XIII. Galactic CO emissionPlanck 2013 results. XIV. Zodiacal emissionPlanck 2013 results. XIX. The integrated Sachs-Wolfe effect
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P50
name
Etienne Pointecouteau
@en
Etienne Pointecouteau
@nl
type
label
Etienne Pointecouteau
@en
Etienne Pointecouteau
@nl
prefLabel
Etienne Pointecouteau
@en
Etienne Pointecouteau
@nl