315 results found
Ade PAR, Aghanim N, Arnaud M, et al., 2016, Planck intermediate results XXXVI. Optical identification and redshifts of Planck SZ sources with telescopes at the Canary Islands observatories, ASTRONOMY & ASTROPHYSICS, Vol: 586, ISSN: 1432-0746
Ade PAR, Aghanim N, Arnaud M, et al., 2016, Planck 2015 results XXIV. Cosmology from Sunyaev-Zeldovich cluster counts, ASTRONOMY & ASTROPHYSICS, Vol: 594, ISSN: 1432-0746
Ade PAR, Aghanim N, Arnaud M, et al., 2016, Planck 2015 results XII. Full focal plane simulations, ASTRONOMY & ASTROPHYSICS, Vol: 594, ISSN: 1432-0746
Ade PAR, Aghanim N, Arnaud M, et al., 2016, Planck 2015 results XXI. The integrated Sachs-Wolfe effect, ASTRONOMY & ASTROPHYSICS, Vol: 594, ISSN: 1432-0746
Ade PAR, Aghanim N, Arnaud M, et al., 2016, Planck 2015 results XVIII. Background geometry and topology of the Universe, Astronomy & Astrophysics, Vol: 594, Pages: A18-A18, ISSN: 0004-6361
Maps of cosmic microwave background (CMB) temperature and polarization from the 2015 release of Planck data provide the highestquality full-sky view of the surface of last scattering available to date. This enables us to detect possible departures from a globally isotropic cosmology. We present the first searches using CMB polarization for correlations induced by a possible non-trivial topology with a fundamental domain that intersects, or nearly intersects, the last-scattering surface (at comoving distance χrec), both via a direct scan for matched circular patterns at the intersections and by an optimal likelihood calculation for specific topologies. We specialize to flat spaces with cubic toroidal (T3) and slab (T1) topologies, finding that explicit searches for the latter are sensitive to other topologies with antipodal symmetry. These searches yield no detection of a compact topology with a scale below the diameter of the last-scattering surface. The limits on the radius ℛi of the largest sphere inscribed in the fundamental domain (at log-likelihood ratio Δlnℒ > −5 relative to a simply-connected flat Planck best-fit model) are: ℛi > 0.97 χrec for the T3 cubic torus; and ℛi > 0.56 χrec for the T1 slab. The limit for the T3 cubic torus from the matched-circles search is numerically equivalent, ℛi > 0.97 χrec at 99% confidence level from polarization data alone. We also perform a Bayesian search for an anisotropic global Bianchi VIIh geometry. In the non-physical setting, where the Bianchi cosmology is decoupled from the standard cosmology, Planck temperature data favour the inclusion of a Bianchi component with a Bayes factor of at least 2.3 units of log-evidence. However, the cosmological parameters that generate this pattern are in strong disagreement with those found from CMB anisotropy data alone. Fitting the induced polarization pattern for this model to the Planck data requires an amplitude of −0.10 ± 0.04
Ade PAR, Aghanim N, Arnaud M, et al., 2016, Planck 2015 results XIV. Dark energy and modified gravity, ASTRONOMY & ASTROPHYSICS, Vol: 594, ISSN: 1432-0746
Ade PAR, Aghanim N, Arnaud M, et al., 2016, Planck intermediate results XL. The Sunyaev-Zeldovich signal from the Virgo cluster, ASTRONOMY & ASTROPHYSICS, Vol: 596, ISSN: 1432-0746
Ade PAR, Aghanim N, Arnaud M, et al., 2016, Planck 2015 results XXIII. The thermal Sunyaev-Zeldovich effect-cosmic infrared background correlation, ASTRONOMY & ASTROPHYSICS, Vol: 594, ISSN: 1432-0746
Ade PAR, Aghanim N, Arnaud M, et al., 2016, Planck intermediate results XXXIX. The Planck list of high-redshift source candidates, Publisher: EDP SCIENCES S A
Ade PAR, Aghanim N, Ashdown M, et al., 2016, Planck 2015 results II. Low Frequency Instrument data processings, ASTRONOMY & ASTROPHYSICS, Vol: 594, ISSN: 1432-0746
Ade PAR, Aghanim N, Ashdown M, et al., 2016, Planck intermediate results XLI. A map of lensing-induced B-modes, ASTRONOMY & ASTROPHYSICS, Vol: 596, ISSN: 1432-0746
Ade PAR, Aghanim N, Ashdown M, et al., 2016, Planck 2015 results IV. Low Frequency Instrument beams and window functions, ASTRONOMY & ASTROPHYSICS, Vol: 594, ISSN: 1432-0746
Ade PAR, Aumont J, Baccigalupi C, et al., 2016, Planck 2015 results III. LFI systematic uncertainties, ASTRONOMY & ASTROPHYSICS, Vol: 594, ISSN: 1432-0746
Aghanim N, Alves MIR, Arnaud M, et al., 2016, Planck intermediate results XXXIV. The magnetic field structure in the Rosette Nebula, ASTRONOMY & ASTROPHYSICS, Vol: 586, ISSN: 1432-0746
Aghanim N, Alves MIR, Arzoumanian D, et al., 2016, Planck intermediate results XLIV. Structure of the Galactic magnetic field from dust polarization maps of the southern Galactic cap, ASTRONOMY & ASTROPHYSICS, Vol: 596, ISSN: 1432-0746
Aghanim N, Arnaud M, Ashdown M, et al., 2016, Planck 2015 results XXII. A map of the thermal Sunyaev-Zeldovich effect, ASTRONOMY & ASTROPHYSICS, Vol: 594, ISSN: 1432-0746
Aghanim N, Arnaud M, Ashdown M, et al., 2016, Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters, Astronomy & Astrophysics, Vol: 594, ISSN: 0004-6361
This paper presents the Planck 2015 likelihoods, statistical descriptions of the 2-point correlationfunctions of the cosmic microwave background (CMB) temperature and polarization fluctuations that account for relevant uncertainties, both instrumental and astrophysical in nature. They are based on the same hybrid approach used for the previous release, i.e., a pixel-based likelihood at low multipoles (ℓ< 30) and a Gaussian approximation to the distribution of cross-power spectra at higher multipoles. The main improvements are the use of more and better processed data and of Planck polarization information, along with more detailed models of foregrounds and instrumental uncertainties. The increased redundancy brought by more than doubling the amount of data analysed enables further consistency checks and enhanced immunity to systematic effects. It also improves the constraining power of Planck, in particular with regard to small-scale foreground properties. Progress in the modelling of foreground emission enables the retention of a larger fraction of the sky to determine the properties of the CMB, which also contributes to the enhanced precision of the spectra. Improvements in data processing and instrumental modelling further reduce uncertainties. Extensive tests establish the robustness and accuracy of the likelihood results, from temperature alone, from polarization alone, and from their combination. For temperature, we also perform a full likelihood analysis of realistic end-to-end simulations of the instrumental response to the sky, which were fed into the actual data processing pipeline; this does not reveal biases from residual low-level instrumental systematics. Even with the increase in precision and robustness, the ΛCDM cosmological model continues to offer a very good fit to the Planck data. The slope of the primordial scalar fluctuations, ns, is confirmed smaller than unity at more than 5σ from Planck alone. We further validate the robustn
Aghanim N, Ashdown M, Aumont J, et al., 2016, Planck intermediate results XLVI. Reduction of large-scale systematic effects in HFI polarization maps and estimation of the reionization optical depth, ASTRONOMY & ASTROPHYSICS, Vol: 596, ISSN: 1432-0746
Aghanim N, Ashdown M, Aumont J, et al., 2016, Planck intermediate results XLVIII. Disentangling Galactic dust emission and cosmic infrared background anisotropies, ASTRONOMY & ASTROPHYSICS, Vol: 596, ISSN: 1432-0746
Aghanim N, Ashdown M, Aumont J, et al., 2016, Planck intermediate results XLIX. Parity-violation constraints from polarization data, ASTRONOMY & ASTROPHYSICS, Vol: 596, ISSN: 1432-0746
Alsing J, Heavens A, Jaffe AH, et al., 2016, Hierarchical cosmic shear power spectrum inference, MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, Vol: 455, Pages: 4452-4466, ISSN: 0035-8711
Arnaud M, Ashdown M, Atrio-Barandela F, et al., 2016, Planck intermediate results XXXI. Microwave survey of Galactic supernova remnants, ASTRONOMY & ASTROPHYSICS, Vol: 586, ISSN: 1432-0746
Bao C, Baccigalupi C, Gold B, et al., 2016, MAXIMUM LIKELIHOOD FOREGROUND CLEANING FOR COSMIC MICROWAVE BACKGROUND POLARIMETERS IN THE PRESENCE OF SYSTEMATIC EFFECTS, Astrophysical Journal, Vol: 819, ISSN: 0004-637X
© 2016. The American Astronomical Society. All rights reserved. We extend a general maximum likelihood foreground estimation for cosmic microwave background (CMB) polarization data to include estimation of instrumental systematic effects. We focus on two particular effects: frequency band measurement uncertainty and instrumentally induced frequency dependent polarization rotation. We assess the bias induced on the estimation of the B-mode polarization signal by these two systematic effects in the presence of instrumental noise and uncertainties in the polarization and spectral index of Galactic dust. Degeneracies between uncertainties in the band and polarization angle calibration measurements and in the dust spectral index and polarization increase the uncertainty in the extracted CMB B-mode power, and may give rise to a biased estimate. We provide a quantitative assessment of the potential bias and increased uncertainty in an example experimental configuration. For example, we find that with 10% polarized dust, a tensor to scalar ratio of r = 0.05, and the instrumental configuration of the E and B experiment balloon payload, the estimated CMB B-mode power spectrum is recovered without bias when the frequency band measurement has 5% uncertainty or less, and the polarization angle calibration has an uncertainty of up to 4°.
Bao C, Gold B, Baccigalupi C, et al., 2016, Erratum: THE IMPACT of the SPECTRAL RESPONSE of AN ACHROMATIC HALF-WAVE PLATE on the MEASUREMENT of the COSMIC MICROWAVE BACKGROUND POLARIZATION (Astrophysical Journal (2012) 747 (97)), Astrophysical Journal, Vol: 818, ISSN: 0004-637X
Collaboration P, Adam R, Ade PAR, et al., 2016, Planck 2015 results. I. Overview of products and scientific results
The European Space Agency's Planck satellite, dedicated to studying the earlyUniverse and its subsequent evolution, was launched 14~May 2009 and scanned themicrowave and submillimetre sky continuously between 12~August 2009 and23~October 2013. In February~2015, ESA and the Planck Collaboration releasedthe second set of cosmology products based on data from the entire Planckmission, including both temperature and polarization, along with a set ofscientific and technical papers and a web-based explanatory supplement. Thispaper gives an overview of the main characteristics of the data and the dataproducts in the release, as well as the associated cosmological andastrophysical science results and papers. The science products include maps ofthe cosmic microwave background (CMB), the thermal Sunyaev-Zeldovich effect,and diffuse foregrounds in temperature and polarization, catalogues of compactGalactic and extragalactic sources (including separate catalogues ofSunyaev-Zeldovich clusters and Galactic cold clumps), and extensive simulationsof signals and noise used in assessing the performance of the analysis methodsand assessment of uncertainties. The likelihood code used to assesscosmological models against the Planck data are described, as well as a CMBlensing likelihood. Scientific results include cosmological parameters derivingfrom CMB power spectra, gravitational lensing, and cluster counts, as well asconstraints on inflation, non-Gaussianity, primordial magnetic fields, darkenergy, and modified gravity.
Collaboration P, Adam R, Ade PAR, et al., 2016, Planck 2015 results. VII. HFI TOI and beam processing, A, Vol: 594
The Planck High Frequency Instrument (HFI) has observed the full sky at sixfrequencies (100, 143, 217, 353, 545, and 857 GHz) in intensity and at fourfrequencies in linear polarization (100, 143, 217, and 353 GHz). In order toobtain sky maps, the time-ordered information (TOI) containing the detector andpointing samples must be processed and the angular response must be assessed.The full mission TOI is included in the Planck 2015 release. This paperdescribes the HFI TOI and beam processing for the 2015 release. HFI calibrationand map-making are described in a companion paper. The main pipeline has beenmodified since the last release (2013 nominal mission in intensity only), byincluding a correction for the non-linearity of the warm readout and byimproving the model of the bolometer time response. The beam processing is anessential tool that derives the angular response used in all the Planck sciencepapers and we report an improvement in the effective beam window functionuncertainty of more than a factor 10 relative to the 2013 release. Noisecorrelations introduced by pipeline filtering function are assessed usingdedicated simulations. Angular cross-power spectra using datasets that aredecorrelated in time are immune to the main systematic effects.
Collaboration P, Ade PAR, Aghanim N, et al., 2016, Planck 2015 results. XXVI. The Second Planck Catalogue of Compact Sources, Astronomy & Astrophysics, Vol: 594, ISSN: 1432-0746
The Second Planck Catalogue of Compact Sources is a catalogue of sourcesdetected in single-frequency maps from the full duration of the Planck missionand supersedes previous versions of the Planck compact source catalogues. Itconsists of compact sources, both Galactic and extragalactic, detected over theentire sky. Compact sources detected in the lower frequency channels areassigned to the PCCS2, while at higher frequencies they are assigned to one oftwo sub-catalogues, the PCCS2 or PCCS2E, depending on their location on thesky. The first of these catalogues covers most of the sky and allows the userto produce subsamples at higher reliabilities than the target 80% integralreliability of the catalogue. The PCCS2E contains sources detected in skyregions where the diffuse emission makes it difficult to quantify thereliability of the detections. Both the PCCS2 and PCCS2E include polarizationmeasurements, in the form of polarized flux densities, or upper limits, andorientation angles for all seven polarization-sensitive Planck channels. Theimproved data-processing of the full-mission maps and their reduced noiselevels allow us to increase the number of objects in the catalogue, improvingits completeness for the target 80 % reliability as compared with the previousversions, the PCCS and ERCSC catalogues.
This data is extracted from the Web of Science and reproduced under a licence from Thomson Reuters. You may not copy or re-distribute this data in whole or in part without the written consent of the Science business of Thomson Reuters.