These results are produced by the Planck Collaboration. We investigate the presence of biases in our shear catalogues and estimate their impact on our weak lensing mass … Abstract. Interstellar gas and dust in the Chamaeleon clouds as seen by Fermi LAT and Planck? The majority of the planet flux density ... Planck, and the two gas giants outshine any PCCS2 object by at 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. 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). Astronomy and Astrophysics . XXXV. The papers are available online, and links to each are provided below. Planck intermediate results. Title: Planck intermediate results. 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. Notice, Smithsonian Terms of 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 Planck intermediate results. Planck intermediate results: XXVII. Planck intermediate results. There are 600 complete signal, noise and systematics simulations of the full-frequency and detector-set maps. Planck intermediate results LI. Structure of the Galactic magnetic field from dust polarization maps of the southern Galactic cap Structure of the Galactic magnetic field from dust polarization maps of the southern Galactic cap 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. @article{Aghanim2016PlanckIR, title={Planck intermediate results - XXXIV. 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. 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. Evidence of unbound gas from the kinetic Sunyaev-Zeldovich effect. 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, Physics of the hot gas in the Coma cluster. Planck intermediate results : XLVI. XXXVIII. Planck intermediate results: XLIV. 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 XVI. 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. I2012;Planck Collaboration Int. 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. After modelling and subtracting the tSZ effect and X-ray emission for each cluster in the pair, we studied the residuals on both the SZ and X-ray maps. Planet flux densities Planck Collaboration: ... results provide constraints on the intrinsic brightness and the brightness time-variability of these planets. Planck intermediate results XXV. The amplitude is (3366.6 ± 2.7) μK, consistent with, albeit slightly higher than, earlier estimates. We investigate the inclusion of neutrino masses, where more significant di erences may appear due to See a full list of Planck intermediate results papers here. 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. 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, XLVII. By combining the Planck data with observations from NASA’s WMAP satellite astronomers suspect that the haze is due to emission from unusually high energy electrons moving through the Galaxy’s magnetic field. Relevant properties of Planck are summarized for each Using the Planck data, we constructed a local map of the tSZ effect centred on each pair of galaxy clusters. LIII. A&A 543, A102 (2012) DOI: 10.1051/0004-6361/201118731 c ESO 2012 Astronomy & Astrophysics Planck intermediate results I. These data consist of a set of maps of the Stokes Q We have Further validation of new Planck clusters with XMM-Newton 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. 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. 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. In addition, NPIPE introduces several improvements, including, but not limited to: inclusion of the 8% of data collected during repointing manoeuvres; smoothing of the LFI reference load data streams; in-flight estimation of detector polarization parameters; and construction of maximally independent detector-set split maps. A&A 550, A128 (2013) DOI: 10.1051/0004-6361/201219361 c ESO 2013 Astronomy & Astrophysics Planck intermediate results II. Early astrophysics results are given in Planck Collaboration VIII{XXVI 2011, based on data taken be-tween 13 August 2009 and 7 June 2010. 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. Planck intermediate results. 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 Planck intermediate results XLVI. 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. 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. A&A 543, A102 (2012) DOI: 10.1051/0004-6361/201118731 c ESO 2012 Astronomy & Astrophysics Planck intermediate results I. Similarly, NPIPE employs the HFI 2018 time-domain processing methodology to correct for bandpass mismatch at all frequencies. Fainter CO cannot account for the brightness of the excesses seen othe Galactic plane (Planck Collaboration XIX2011). cosmology. These results clarify a recurrent disparity in the -ray versus dust calibration of X CO, but they Use, Smithsonian Intermediate results are presented in a series of papers based on Planck data. 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 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, Planck intermediate results ... (Planck Collaboration Int. Comparison of Sunyaev-Zeldovich measurements from Planck A&A 550, A128 (2013) DOI: 10.1051/0004-6361/201219361 c ESO 2013 Astronomy & Astrophysics Planck intermediate results II. 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. @article{Aghanim2016PlanckIR, title={Planck intermediate results - XXXIV. Profile likelihoods for cosmological parameters ... demonstrating the robustness of the Planck results to the statistical methodology. 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. Further validation of new Planck clusters with XMM-Newton The Planck maps of polarization angle, Based on the NPIPE maps, we present the first estimate of the Solar dipole determined through component separation across all nine Planck frequencies. XXXVII. As a Planck first, these simulations include full time-domain processing of the beam-convolved CMB anisotropies. 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. ated with gamma-ray emission, has also been identified at inter-mediate latitudes (Dobler et al.2010;Planck Collaboration Int. Agreement NNX16AC86A, Is ADS down? XLII. 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 Constraints on peculiar velocities Many of the Planck initial results involve the study of clusters of galaxies. Reduction of large-scale systematic effects in HFI polarization maps and estimation of the reionization optical depth journal , … XIX. In the past the components have Click here for more detailed information on the individual scientific papers. Planck intermediate results LII. 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