Overall, 51 clusters were detected by Planck and confirmed by Planck, in a number of scientific papers. A&A 561, A97 (2014) DOI: 10.1051/0004-6361/201321299 c ESO 2014 Astronomy & Astrophysics Planck intermediate results XIII. 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: XXVII. These results primarily involve the investigation of diffuse emission from our own Galaxy, and the study of other galaxies and clusters of galaxies. Fainter CO cannot account for the brightness of the excesses seen othe Galactic plane (Planck Collaboration XIX2011). Planck intermediate results LII. Planck intermediate results. Planck intermediate results. From the Planck temperature data combined with Planck lensing, for this cosmology we find a Hubble constant, H 0 = (67.8 ± 0.9) km s -1 Mpc -1, a matter density parameter Ω m = 0.308 ± 0.012, and a tilted scalar spectral index with n s = 0.968 ± 0.006, consistent with the 2013 analysis. The majority of the planet flux density ... Planck, and the two gas giants outshine any PCCS2 object by at The haze is a distinct but mysterious component of diffuse Galactic emission, the origin of which is unknown. LIII. The Planck maps of polarization angle, Relevant properties of Planck are summarized for each We investigate the inclusion of neutrino masses, where more significant di erences may appear due to We have The results provide more information on the general populations of these two types of sources: Using precise full-sky observations from Planck, and subtracting the emission from known sources, Planck has identified and characterised the emission from the “Galactic Haze” at microwave wavelengths. In the past the components have Planck intermediate results ... (Planck Collaboration Int. A&A 550, A128 (2013) DOI: 10.1051/0004-6361/201219361 c ESO 2013 Astronomy & Astrophysics Planck intermediate results II. Large-scale Galactic magnetic fields Planck Collaboration: ... Planck data The results presented in this paper are based on the 2015 data release2 described in Planck Collaboration I (2016), Planck Collaboration II (2016), and Planck Collaboration XXXV. Reduction of large-scale systematic effects in HFI polarization maps and estimation of the reionization optical depth journal , … This allows massive galaxy clusters, such as the Coma Cluster seen on the left, to be detected at huge distances across the Universe. XIII (2014) we focused on con-straining the monopole and dipole of the peculiar veloc-ity field, which gives constraints on the large-scale inho-mogeneity of the Universe. The Planck mission results are presented inPlanck Collaboration I(2014) and the in-flight performance of the two focal plane instruments, the HFI (High Frequency XLVII. Note that in this abstract we quote 68% confidence limits on measured parameters and 95% upper limits on other parameters. 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. Early astrophysics results are given in Planck Collaboration VIII{XXVI 2011, based on data taken be-tween 13 August 2009 and 7 June 2010. Agreement NNX16AC86A, Is ADS down? XXXVII. A&A 550, A128 (2013) DOI: 10.1051/0004-6361/201219361 c ESO 2013 Astronomy & Astrophysics Planck intermediate results II. 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. Ade PAR, Aghanim N, Arnaud M, Ashdown M, Atrio-Barandela F, Aumont J et al. 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. Interstellar gas and dust in the Chamaeleon clouds as seen by Fermi LAT and Planck? If you use any of these results for presentations, please acknowledge the corresponding paper, ESA/Planck, and the Planck Collaboration. and the cosmological parameters, in order to compare the limits obtained from Planck and WMAP and to determine the constraining power gained by including other cosmological probes. 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°). @article{Aghanim2016PlanckIR, title={Planck intermediate results - XXXIV. 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 Comparison of Sunyaev-Zeldovich measurements from Planck Planck intermediate results: X. 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. 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. 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, (or is it just me...), Smithsonian Privacy Planck intermediate results. IX2013), but is not of concern here. Physics of the hot gas in the Coma cluster. Planck intermediate results. XXXVIII. The amplitude is (3366.6 ± 2.7) μK, consistent with, albeit slightly higher than, earlier estimates. We present the NPIPE processing pipeline, which produces calibrated frequency maps in temperature and polarization from data from the Planck Low Frequency Instrument (LF Planck intermediate results XLVII. Astrophysical Observatory, Astrophysics - Cosmology and Nongalactic Astrophysics. 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. See a full list of Planck intermediate results papers here. Planck intermediate results. 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 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. According to the Planck data, little CO emission has been missed outside the boundaries of the present 2.6 mm surveys, down to a sensitivity of 1 or 2Kkms1 (Planck Collaboration XIII2014). 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. ... which are consistent with the kSZ evidence found in individual Planck raw frequency maps, although lower than found in the WMAP-9yr W band ($3.3\sigma$). The Andromeda galaxy as seen by Planck Planck Collaboration: P. A. R. Ade82, N. Aghanim55, M. Arnaud69, M. Ashdown65;6, J. Aumont55, C. Baccigalupi81, A. J. Banday90;10, R. B. Barreiro61, N. Bartolo28;62, E. Battaner91;92, R. Battye64, K. Benabed56;89… 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. We present the results from a deep XMM-Newton re-observation of PLCKG214.6+37.0, part of a multi-wavelength programme to investigate Planck discovered superclusters. Detection of velocity dispersion ... Planck Collaboration Int. NPIPE represents a natural evolution of previous Planck analysis efforts, and combines some of the most powerful features of the separate LFI and HFI analysis pipelines. 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, XLII. cosmology. Planck measurements have shown that galaxy clusters come in all sorts of shapes and sizes, and discovered the first ever seen triple-system of galaxy clusters. 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 In the second paper, Planck Planck intermediate results XVI. 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. These data consist of a set of maps of the Stokes Q Results. A&A 543, A102 (2012) DOI: 10.1051/0004-6361/201118731 c ESO 2012 Astronomy & Astrophysics Planck intermediate results I. Astronomy and Astrophysics . Abstract. Using the Planck data, we constructed a local map of the tSZ effect centred on each pair of galaxy clusters. 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. Intermediate results are presented in a series of papers based on Planck data. A&A 543, A102 (2012) DOI: 10.1051/0004-6361/201118731 c ESO 2012 Astronomy & Astrophysics Planck intermediate results I. Planck intermediate results. 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 investigate the presence of biases in our shear catalogues and estimate their impact on our weak lensing mass … 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. Planck intermediate results XVII. It is roughly centered on the Galactic centre, and also seems to lie in the same place as gamma ray “bubbles” detected by NASA’s Fermi satellite. Planck intermediate results LI. The papers are available online, and links to each are provided below. Profile likelihoods for cosmological parameters ... demonstrating the robustness of the Planck results to the statistical methodology. Planck intermediate results XXVIII. Planck intermediate results: XLIV. As a Planck first, these simulations include full time-domain processing of the beam-convolved CMB anisotropies. Planck intermediate results. 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