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# planck intermediate 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. Planck intermediate results XLVII. 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. @article{Aghanim2016PlanckIR, title={Planck intermediate results - XXXIV. 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. There are 600 complete signal, noise and systematics simulations of the full-frequency and detector-set maps. Comparison of Sunyaev-Zeldovich measurements from Planck Evidence of unbound gas from the kinetic Sunyaev-Zeldovich effect. ated with gamma-ray emission, has also been identiﬁed at inter-mediate latitudes (Dobler et al.2010;Planck Collaboration Int. See a full list of Planck intermediate results papers here. 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). Planck intermediate results. Proﬁle likelihoods for cosmological parameters ... demonstrating the robustness of the Planck results to the statistical methodology. 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 Planck mission results are presented inPlanck Collaboration I(2014) and the in-ﬂight performance of the two focal plane instruments, the HFI (High Frequency Fainter CO cannot account for the brightness of the excesses seen othe Galactic plane (Planck Collaboration XIX2011). 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). 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. A&A 561, A97 (2014) DOI: 10.1051/0004-6361/201321299 c ESO 2014 Astronomy & Astrophysics Planck intermediate results XIII. 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 investigate the inclusion of neutrino masses, where more signiﬁcant di erences may appear due to 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. 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. 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. 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. @article{Aghanim2016PlanckIR, title={Planck intermediate results - XXXIV. cosmology. Planck intermediate results ... (Planck Collaboration Int. Ade PAR, Aghanim N, Arnaud M, Ashdown M, Atrio-Barandela F, Aumont J et al. (or is it just me...), Smithsonian Privacy 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 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. IX2013), but is not of concern here. Based on the NPIPE maps, we present the first estimate of the Solar dipole determined through component separation across all nine Planck frequencies. LIII. XLII. Planet ﬂux densities Planck Collaboration: ... results provide constraints on the intrinsic brightness and the brightness time-variability of these planets. 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. Early astrophysics results are given in Planck Collaboration VIII{XXVI 2011, based on data taken be-tween 13 August 2009 and 7 June 2010. Planck intermediate results XVII. The ADS is operated by the Smithsonian Astrophysical Observatory under NASA Cooperative 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. XLII. 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 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. 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 Astronomy and Astrophysics . XXXVII. 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: XXVII. The papers are available online, and links to each are provided below. Planck intermediate results XLVI. Probably the most important high-level result from the Planck satellite1 (Planck Collaboration I2016) is the good agreement Interstellar gas and dust in the Chamaeleon clouds as seen by Fermi LAT and Planck? We present the NPIPE processing pipeline, which produces calibrated frequency maps in temperature and polarization from data from the Planck Low Frequency Instrument (LF Title: Planck intermediate results. 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). 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°). Notice, Smithsonian Terms of Reduction of large-scale systematic effects in HFI polarization maps and estimation of the reionization optical depth journal , … High-redshift infrared galaxy overdensity candidates and lensed sources discovered by Planck and confirmed by Herschel -SPIRE Journal Article Aghanim, N. … Comparison of Sunyaev-Zeldovich measurements from Planck 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. These results are produced by the Planck Collaboration. For example, following the LFI 2018 processing procedure, NPIPE uses foreground polarization priors during the calibration stage in order to break scanning-induced degeneracies. These results primarily involve the investigation of diffuse emission from our own Galaxy, and the study of other galaxies and clusters of galaxies. As a Planck first, these simulations include full time-domain processing of the beam-convolved CMB anisotropies. 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 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. Planck intermediate results. Overall, 51 clusters were detected by Planck and confirmed by Planck, in a number of scientific papers. Further validation of new Planck clusters with XMM-Newton Agreement NNX16AC86A, Is ADS down? XIX. Many of the Planck initial results involve the study of clusters of galaxies. 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. Planck intermediate results. Astrophysical Observatory, Astrophysics - Cosmology and Nongalactic Astrophysics. Planck intermediate results: XLIV. Results. 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. 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… Planck intermediate results : XLVI. 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. 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 These data consist of a set of maps of the Stokes Q 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, 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. We investigate the presence of biases in our shear catalogues and estimate their impact on our weak lensing mass … Planck intermediate results. If you use any of these results for presentations, please acknowledge the corresponding paper, ESA/Planck, and the Planck Collaboration. 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. … Planck intermediate results XXV. 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. 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 XXXV. In the second paper, Planck A&A 543, A102 (2012) DOI: 10.1051/0004-6361/201118731 c ESO 2012 Astronomy & Astrophysics Planck intermediate results I. 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. XXXIII. Planck intermediate results LI. 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. 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. Planck intermediate results XVI. ... which are consistent with the kSZ evidence found in individual Planck raw frequency maps, although lower than found in the WMAP-9yr W band ($3.3\sigma$). 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. XLVII. Planck intermediate results. These results clarify a recurrent disparity in the -ray versus dust calibration of X CO, but they Abstract. Planck intermediate results XXVIII. 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. 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. 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. Further validation of new Planck clusters with XMM-Newton Click here for more detailed information on the individual scientific papers. 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. Planck intermediate results. I2012;Planck Collaboration Int. 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. The haze is a distinct but mysterious component of diffuse Galactic emission, the origin of which is unknown. Planck intermediate results. 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. IV2013), and later with the ﬁrst public SZ … Use, Smithsonian Relevant properties of Planck are summarized for each Constraints on peculiar velocities 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. We have Detection of velocity dispersion ... Planck Collaboration Int. XIX. Physics of the hot gas in the Coma cluster. Planck intermediate 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, XXXVIII. 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). 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 Note that in this abstract we quote 68% confidence limits on measured parameters and 95% upper limits on other parameters. Similarly, NPIPE employs the HFI 2018 time-domain processing methodology to correct for bandpass mismatch at all frequencies. A&A 543, A102 (2012) DOI: 10.1051/0004-6361/201118731 c ESO 2012 Astronomy & Astrophysics Planck intermediate results I. Planck intermediate results. The majority of the planet ﬂux density ... Planck, and the two gas giants outshine any PCCS2 object by at Intermediate results are presented in a series of papers based on Planck data. Using the Planck data, we constructed a local map of the tSZ effect centred on each pair of galaxy clusters. In the past the components have ROSAT data were used to construct X-ray maps of these pairs. 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. The Planck maps of polarization angle, A&A 550, A128 (2013) DOI: 10.1051/0004-6361/201219361 c ESO 2013 Astronomy & Astrophysics Planck intermediate results II. The amplitude is (3366.6 ± 2.7) μK, consistent with, albeit slightly higher than, earlier estimates. Planck intermediate results LII. 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 This allows massive galaxy clusters, such as the Coma Cluster seen on the left, to be detected at huge distances across the Universe. A&A 550, A128 (2013) DOI: 10.1051/0004-6361/201219361 c ESO 2013 Astronomy & Astrophysics Planck intermediate results II. Densities Planck Collaboration Int present the first estimate of the planet ﬂux densities Planck Collaboration: results. 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