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The Second Radio Synchrotron Background Workshop: Conference Summary and Report / Singal, J. (Richmond U.) ; Fornengo, N. (INFN, Turin) ; Regis, M. (INFN, Turin) ; Bernardi, G. (Bologna, Ist. Radioastronomia ; Rhodes U. ; South African Astron. Observ.) ; Bordenave, D. (Virginia U., Astron. Dept. ; NRAO, Charlottesville) ; Branchini, E. (Rome III U. ; Genoa U. ; INFN, Genoa) ; Cappelluti, N. (Miami U.) ; Caputo, A. (Tel Aviv U. ; Weizmann Inst. ; CERN) ; Carucci, I.P. (INFN, Turin) ; Chluba, J. (Jodrell Bank ; U. Manchester (main)) et al.
We summarize the second radio synchrotron background workshop, which took place June 15-17, 2022 in Barolo, Italy. This meeting was convened because available measurements of the diffuse radio zero level continue to suggest that it is several times higher than can be attributed to known Galactic and extragalactic sources and processes, rendering it the least well understood electromagnetic background at present and a major outstanding question in astrophysics. [...]
arXiv:2211.16547; FERMILAB-CONF-22-918-PPD.- 2023-03-20 - 33 p.
- Published in : Publ. Astron. Soc. Pac. Fulltext: 2211.16547 - PDF; 10ce9d7a5eecef56fdbdcc4e7e2aca33 - PDF; Publication - PDF; Fulltext from Publisher: PDF; External link: Fermilab Library Server
In : 2nd Radio Synchrotron Background Conference, Barolo, Italy, 14 - 18 Jun 2022, pp.036001

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Planck 2018 results. I. Overview and the cosmological legacy of Planck / Planck Collaboration
The European Space Agency's Planck satellite, which was dedicated to studying the early Universe and its subsequent evolution, was launched on 14 May 2009. It scanned the microwave and submillimetre sky continuously between 12 August 2009 and 23 October 2013, producing deep, high-resolution, all-sky maps in nine frequency bands from 30 to 857GHz. [...]
arXiv:1807.06205.- 2020-09-01 - 56 p. - Published in : Astron. Astrophys. 641 (2020) A1 Fulltext: 1807.06205 - PDF; arXiv:1807.06205 - PDF;

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Planck 2015 results. XXVI. The Second Planck Catalogue of Compact Sources / Planck Collaboration
The Second Planck Catalogue of Compact Sources is a catalogue of sources detected in single-frequency maps from the full duration of the Planck mission and supersedes previous versions of the Planck compact source catalogues. It consists of compact sources, both Galactic and extragalactic, detected over the entire sky. [...]
arXiv:1507.02058.- 2016-09-20 - 39 p. - Published in : Astron. Astrophys. 594 (2016) A26 Fulltext: PDF; External link: Preprint

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Planck 2015 results. XXV. Diffuse low-frequency Galactic foregrounds / Planck Collaboration
(abridged) We discuss the Galactic foreground emission between 20 and 100GHz based on observations by Planck/WMAP. The Commander component-separation tool has been used to separate the various astrophysical processes in total intensity. [...]
arXiv:1506.06660.- 2016-09-20 - 45 p. - Published in : Astron. Astrophys. 594 (2016) A25 Fulltext: PDF; External link: Preprint

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Planck 2015 results. V. LFI calibration / Planck Collaboration
We present a description of the pipeline used to calibrate the Planck Low Frequency Instrument (LFI) timelines into thermodynamic temperatures for the Planck 2015 data release, covering 4 years of uninterrupted operations. As in the 2013 data release, our calibrator is provided by the spin-synchronous modulation of the CMB dipole, exploiting both the orbital and solar components. [...]
arXiv:1505.08022.- 2016-09-20 - 24 p. - Published in : Astron. Astrophys. 594 (2016) A5 Fulltext: PDF; External link: Preprint

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Planck 2015 results. XIX. Constraints on primordial magnetic fields / Planck Collaboration
We predict and investigate four types of imprint of a stochastic background of primordial magnetic fields (PMFs) on the cosmic microwave background (CMB) anisotropies: the impact of PMFs on the CMB spectra; the effect on CMB polarization induced by Faraday rotation; magnetically-induced non-Gaussianities; and the magnetically-induced breaking of statistical isotropy. Overall, Planck data constrain the amplitude of PMFs to less than a few nanogauss. [...]
arXiv:1502.01594.- 2016-09-20 - 27 p. - Published in : Astron. Astrophys. 594 (2016) A19 Fulltext: PDF; External link: Preprint

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Planck 2015 results. XIII. Cosmological parameters / Planck Collaboration
We present results based on full-mission Planck observations of temperature and polarization anisotropies of the CMB. These data are consistent with the six-parameter inflationary LCDM cosmology. [...]
arXiv:1502.01589.- 2016-09-20 - 63 p. - Published in : Astron. Astrophys. 594 (2016) A13 Fulltext: PDF; External link: Preprint

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Planck 2015 results. X. Diffuse component separation: Foreground maps / Planck Collaboration
Planck has mapped the microwave sky in nine frequency bands between 30 and 857 GHz in temperature and seven bands between 30 and 353 GHz in polarization. In this paper we consider the problem of diffuse astrophysical component separation, and process these maps within a Bayesian framework to derive a consistent set of full-sky astrophysical component maps. [...]
arXiv:1502.01588.- 2016-09-20 - 63 p. - Published in : Astron. Astrophys. 594 (2016) A10 Fulltext: PDF; External link: Preprint

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Planck 2015 results. VIII. High Frequency Instrument data processing: Calibration and maps / Planck Collaboration
This paper describes the processing applied to the Planck High Frequency Instrument (HFI) cleaned, time-ordered information to produce photometrically calibrated maps in temperature and (for the first time) in polarization. The data from the 2.5 year full mission include almost five independent full-sky surveys. [...]
arXiv:1502.01587.- 2016-09-20 - 27 p. - Published in : Astron. Astrophys. 594 (2016) A8 Fulltext: PDF; External link: Preprint

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Planck 2015 results. VII. HFI TOI and beam processing / Planck Collaboration
The Planck High Frequency Instrument (HFI) has observed the full sky at six frequencies (100, 143, 217, 353, 545, and 857 GHz) in intensity and at four frequencies in linear polarization (100, 143, 217, and 353 GHz). In order to obtain sky maps, the time-ordered information (TOI) containing the detector and pointing samples must be processed and the angular response must be assessed. [...]
arXiv:1502.01586.- 2016-09-20 - 30 p. - Published in : Astron. Astrophys. 594 (2016) A7 Fulltext: PDF; External link: Preprint

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See also: similar author names
52	Leahy, J P
1	Leahy, J Patrick
6	Leahy, J V
1	Leahy, John V

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