Relevant properties of Planck are summarized for each Planck constraints on reionization history Planck Collaboration: R. Adam67, ... data solely from CMB anisotropies, the low value suggested by combining Planck 2015 results with other data sets, and also reduces the uncertain-ties. Reduction of large-scale systematic effects in HFI polarization maps and estimation of the reionization optical depth Planck Collaboration: N. Aghanim53, M. Ashdown63;6, J. Aumont53, C. Baccigalupi75, M. Ballardini29;45;48, A. J. Banday85;9, R. B. Barreiro58, For component-separation purposes, important improvements include: maps that retain the CMB Solar dipole, allowing for high-precision relative calibration in higher-level analyses; well-defined single-detector maps, allowing for robust CO extraction; and HFI temperature maps between 217 and 857 GHz that are binned into 0'.9 pixels (Nside = 4096), ensuring that the full angular information in the data is represented in the maps even at the highest Planck resolutions. Early astrophysics results are given in Planck Collaboration VIII{XXVI 2011, based on data taken be-tween 13 August 2009 and 7 June 2010. The aim of this paper is to study the inner Galaxy where the four emission components at radio and millimetre wavelengths peak in a narrow latitude band. Planck constraints on reionization history Planck Collaboration: R. Adam67, ... with data solely from CMB anisotropies, the low value suggested by combining Planck 2015 results with other data sets, and also reduces the uncertainties. PDF | On Jan 1, 2013, P. A. R. Ade and others published Planck intermediate results | Find, read and cite all the research you need on ResearchGate I2012;Planck Collaboration Int. Constraints on peculiar velocities Since 2010, the Planck Collaboration has undertaken an exten-sive follow-up programme to confirm SZ cluster candidates, first from intermediate versions of the Planck SZ catalogue (Planck Collaboration IX2011;Planck Collaboration Int. Fainter CO cannot account for the brightness of the excesses seen othe Galactic plane (Planck Collaboration XIX2011). Planck intermediate results LII. Signature of the magnetic field geometry of interstellar filaments in dust polarization maps ... Planck1 has produced the first all-sky map of the po-larized emission from dust at sub-mm wavelengths (Planck Collaboration I2015). Planck intermediate results XLVI. The amplitude is (3366.6 ± 2.7) μK, consistent with, albeit slightly higher than, earlier estimates. Intermediate as-trophysics results are being presented in a series of pa-pers based on data taken between 13 August 2009 and 27 November 2010. XXXV. @article{Aghanim2016PlanckIR, title={Planck intermediate results - XXXIV. A&A 550, A128 (2013) DOI: 10.1051/0004-6361/201219361 c ESO 2013 Astronomy & Astrophysics Planck intermediate results II. Based on the NPIPE maps, we present the first estimate of the Solar dipole determined through component separation across all nine Planck frequencies. High-redshift infrared galaxy overdensity candidates and lensed sources discovered by Planck and confirmed by Herschel -SPIRE Journal Article Aghanim, N. … The net effect of these improvements is lower levels of noise and systematics in both frequency and component maps at essentially all angular scales, as well as notably improved internal consistency between the various frequency channels. The clusters contain huge amounts of very hot gas, and as the light from the cosmic microwave background passes through the gas on its way to Earth it is energised – an effect known as the Sunyaev-Zel’dovich effect. In the past the components have Planck intermediate results: X. XXII2015; Planck Collaboration X ... not allow us to derive significant results in the framework adopted for this study and consequently the other channels are not used. We present the NPIPE processing pipeline, which produces calibrated frequency maps in temperature and polarization from data from the Planck Low Frequency Instrument (LF IX2013), but is not of concern here. From the large-scale polarization data, we derive an updated estimate of the optical depth of reionization of τ = 0.051 ± 0.006, which appears robust with respect to data and sky cuts. Interstellar gas and dust in the Chamaeleon clouds as seen by Fermi LAT and Planck? Note that in this abstract we quote 68% confidence limits on measured parameters and 95% upper limits on other parameters. (or is it just me...), Smithsonian Privacy The Planck maps of polarization angle, Click here for more detailed information on the individual scientific papers. See a full list of Planck intermediate results papers here. A&A 561, A97 (2014) DOI: 10.1051/0004-6361/201321299 c ESO 2014 Astronomy & Astrophysics Planck intermediate results XIII. Using Planck data combined with the Meta Catalogue of X-ray detected Clusters of galaxies (MCXC), we address the study of peculiar motions by searching for evidence of the kinetic Sunyaev-Zeldovich effect (kSZ). The release of NPIPE maps and simulations is accompanied with a complete suite of raw and processed time-ordered data and the software, scripts, auxiliary data, and parameter files needed to improve further on the analysis and to run matching simulations. Profile likelihoods for cosmological parameters ... demonstrating the robustness of the Planck results to the statistical methodology. Planck intermediate results XXVIII. We investigate the inclusion of neutrino masses, where more significant di erences may appear due to Planck intermediate results LI. Planck intermediate results: XLIV. We introduce results from the Wendelstein Weak Lensing (WWL) pathfinder project, in which we have observed three intermediate-redshift Planck clusters of galaxies with the new 30 arcmin × 30 arcmin wide field imager at the 2 m Fraunhofer Telescope at Wendelstein Observatory. We present further results from the ongoing XMM-Newton validation follow-up of Planck cluster candidates, detailing X-ray observations of eleven candidates detected at a signal-to-noise ratio of 4.5 < S/N < 5.3 in the same 10-month survey maps used in the construction of the Early SZ sample. A&A 543, A102 (2012) DOI: 10.1051/0004-6361/201118731 c ESO 2012 Astronomy & Astrophysics Planck intermediate results I. Intermediate Science Results Between the initial release of results in January 2011, and the release of the first full-sky maps planned for early 2013, the Planck Collaboration has produced a number of intermediate science results. Probing the role of the ... Planck Collaboration: Probing the role of the magnetic field in the formation of structure in molecular clouds ... ization morphology can be interpreted as the result of dynam-ically important magnetic fields. Comparison of Sunyaev-Zeldovich measurements from Planck ated with gamma-ray emission, has also been identified at inter-mediate latitudes (Dobler et al.2010;Planck Collaboration Int. XXXVII. Agreement NNX16AC86A, Is ADS down? These results are produced by the Planck Collaboration. Results using Planck and XMM-Newton measurements have shown that galaxy clusters come in all sorts of shapes and sizes, and that common assumptions may not be valid. We have The haze can’t be accounted for by previously know sources, and a new mechanism for cosmic-ray acceleration in the centre of our Galaxy is implied. Using data from the Planck satellite, we study the statistical properties of interstellar dust polarization at high Galactic latitudes around the south pole (b < -60°). We conclude that independent time variations of the fine structure constant and of the mass of the electron are constrained by Planck to = = (3:6 3:7) 10 3 and m e=m Many of the Planck initial results involve the study of clusters of galaxies. Overall, 51 clusters were detected by Planck and confirmed by Planck, in a number of scientific papers. These results clarify a recurrent disparity in the -ray versus dust calibration of X CO, but they As a Planck first, these simulations include full time-domain processing of the beam-convolved CMB anisotropies. Emission of dust in the diffuse interstellar medium from the far-infrared to microwave frequencies Planck Collaboration: A. Abergel56,P.A.R.Ade79, N. Aghanim56,M.I.R.Alves56,G.Aniano56,M.Arnaud68, M. Ashdown65,7, J. Aumont56, We present further results from the ongoing XMM-Newton validation follow-up of Planck cluster candidates, detailing X-ray observations of eleven candidates detected at a signal-to-noise ratio of 4.5 < S/N < 5.3 in the same 10-month survey maps used in the construction of the Early SZ sample. We present the NPIPE processing pipeline, which produces calibrated frequency maps in temperature and polarization from data from the Planck Low Frequency Instrument (LFI) and High Frequency Instrument (HFI) using high-performance computers. Intermediate Science Results Between the initial release of results in January 2011, and the release of the first full-sky maps planned for early 2013, the Planck Collaboration has produced a number of intermediate science results. Planck intermediate results XLVII. Using the Planck data, we constructed a local map of the tSZ effect centred on each pair of galaxy clusters. Reduction of large-scale systematic effects in HFI polarization maps and estimation of the reionization optical depth journal , … The characterisation of the physical properties of the three components has allowed us to build a template model to extract the total SZ signal of this system with Planck data. Evidence of unbound gas from the kinetic Sunyaev-Zeldovich effect. A&A 543, A102 (2012) DOI: 10.1051/0004-6361/201118731 c ESO 2012 Astronomy & Astrophysics Planck intermediate results I. … E- and B-modes of dust polarization from the magnetized filamentary structure of the interstellar medium Planck Collaboration: P. A. R. Ade81, N. Aghanim55, M. Arnaud69, M. Ashdown66;5, J. Aumont55, C. Baccigalupi80, A. J. Banday89;9, Planet flux densities Planck Collaboration: ... results provide constraints on the intrinsic brightness and the brightness time-variability of these planets. 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