planck intermediate results

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planck intermediate results

Based on the NPIPE maps, we present the first estimate of the Solar dipole determined through component separation across all nine Planck frequencies. 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. 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. XLVII. 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. High-redshift infrared galaxy overdensity candidates and lensed sources discovered by Planck and confirmed by Herschel -SPIRE Journal Article Aghanim, N. … Planet flux densities Planck Collaboration: ... results provide constraints on the intrinsic brightness and the brightness time-variability of these planets. ated with gamma-ray emission, has also been identified at inter-mediate latitudes (Dobler et al.2010;Planck Collaboration Int. 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. Intermediate results are presented in a series of papers based on Planck data. We have 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, 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 Planck intermediate results: XXVII. Probably the most important high-level result from the Planck satellite1 (Planck Collaboration I2016) is the good agreement 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. Planck intermediate results XVII. XLII. A&A 543, A102 (2012) DOI: 10.1051/0004-6361/201118731 c ESO 2012 Astronomy & Astrophysics Planck intermediate results I. Ade PAR, Aghanim N, Arnaud M, Ashdown M, Atrio-Barandela F, Aumont J et al. 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. 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. 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. 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). 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. 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 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 Planck intermediate results XLVII. Planck intermediate results. Reduction of large-scale systematic effects in HFI polarization maps and estimation of the reionization optical depth journal , … Planck intermediate results XVI. 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. These results primarily involve the investigation of diffuse emission from our own Galaxy, and the study of other galaxies and clusters of galaxies. 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. 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. Fainter CO cannot account for the brightness of the excesses seen othe Galactic plane (Planck Collaboration XIX2011). Planck intermediate results. Overall, 51 clusters were detected by Planck and confirmed by Planck, in a number of scientific papers. If you use any of these results for presentations, please acknowledge the corresponding paper, ESA/Planck, and the Planck Collaboration. In the past the components have Click here for more detailed information on the individual scientific papers. A&A 561, A97 (2014) DOI: 10.1051/0004-6361/201321299 c ESO 2014 Astronomy & Astrophysics Planck intermediate results XIII. Early astrophysics results are given in Planck Collaboration VIII{XXVI 2011, based on data taken be-tween 13 August 2009 and 7 June 2010. These data consist of a set of maps of the Stokes Q 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. 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. Further validation of new Planck clusters with XMM-Newton Relevant properties of Planck are summarized for each Profile likelihoods for cosmological parameters ... demonstrating the robustness of the Planck results to the statistical methodology. These results clarify a recurrent disparity in the -ray versus dust calibration of X CO, but they IV2013), and later with the first public SZ … Planck intermediate results LII. @article{Aghanim2016PlanckIR, title={Planck intermediate results - XXXIV. Similarly, NPIPE employs the HFI 2018 time-domain processing methodology to correct for bandpass mismatch at all frequencies. There are 600 complete signal, noise and systematics simulations of the full-frequency and detector-set maps. The papers are available online, and links to each are provided below. For example, following the LFI 2018 processing procedure, NPIPE uses foreground polarization priors during the calibration stage in order to break scanning-induced degeneracies. 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, Interstellar gas and dust in the Chamaeleon clouds as seen by Fermi LAT and Planck? Use, Smithsonian The ADS is operated by the Smithsonian Astrophysical Observatory under NASA Cooperative 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. See a full list of Planck intermediate results papers here. Planck released the Early Release Compact Source Catalogue in January 2011; further investigation has examined the sources that are brightest at higher frequencies (above 100GHz) The sources have been classified into galaxies dominated by thermal emission from dust, and those dominated by synchrotron emission from electrons in magnetic fields. Detection of velocity dispersion ... Planck Collaboration Int. XLII. … Planck intermediate results. Constraints on peculiar velocities Title: Planck intermediate results. A&A 550, A128 (2013) DOI: 10.1051/0004-6361/201219361 c ESO 2013 Astronomy & Astrophysics Planck intermediate results II. 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. LIII. Planck intermediate results. ROSAT data were used to construct X-ray maps of these pairs. 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. We investigate the presence of biases in our shear catalogues and estimate their impact on our weak lensing mass … A&A 543, A102 (2012) DOI: 10.1051/0004-6361/201118731 c ESO 2012 Astronomy & Astrophysics Planck intermediate results I. 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. 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). Al.2010 ; Planck Collaboration Int more detailed information on the NPIPE maps, we the... 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