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CERN Document Server 20 elementer funnet  1 - 10neste  gå til element: Søket tok 1.29 sekunder. 
1.
A Next-Generation Liquid Xenon Observatory for Dark Matter and Neutrino Physics / Aalbers, J. (SLAC ; KIPAC, Menlo Park) ; AbdusSalam, S.S. (Shahid Beheshti U.) ; Abe, K. (Kamioka Observ. ; Tokyo U., IPMU) ; Aerne, V. (Zurich U.) ; Agostini, F. (U. Bologna, DIFA ; INFN, Bologna) ; Maouloud, S. Ahmed (Paris U., VI-VII) ; Akerib, D.S. (SLAC ; KIPAC, Menlo Park) ; Akimov, D.Yu. (Moscow Phys. Eng. Inst.) ; Akshat, J. (Purdue U.) ; Musalhi, A.K. Al (Oxford U.) et al.
The nature of dark matter and properties of neutrinos are among the most pressing issues in contemporary particle physics. The dual-phase xenon time-projection chamber is the leading technology to cover the available parameter space for Weakly Interacting Massive Particles (WIMPs), while featuring extensive sensitivity to many alternative dark matter candidates. [...]
arXiv:2203.02309; INT-PUB-22-003; FERMILAB-PUB-22-112-PPD-QIS-T.- 2022-12-15 - 77 p. - Published in : J. Phys. G 50 (2023) 013001 Fulltext: 2203.02309 - PDF; jt - PDF; Fulltext from Publisher: PDF; External link: Fermilab Library Server
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2.
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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3.
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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4.
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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5.
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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6.
Planck 2015 results. IV. Low Frequency Instrument beams and window functions / Planck Collaboration
This paper presents the characterization of the in-flight beams, the beam window functions, and the associated uncertainties for the Planck Low Frequency Instrument (LFI). The structure of the paper is similar to that presented in the 2013 Planck release; the main differences concern the beam normalization and the delivery of the window functions to be used for polarization analysis. [...]
arXiv:1502.01584.- 2016-09-20 - 22 p. - Published in : Astron. Astrophys. 594 (2016) A4 Fulltext: PDF; External link: Preprint
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7.
Planck 2015 results. I. Overview of products and scientific results / Planck Collaboration
The European Space Agency's Planck satellite, dedicated to studying the early Universe and its subsequent evolution, was launched 14~May 2009 and scanned the microwave and submillimetre sky continuously between 12~August 2009 and 23~October 2013. In February~2015, ESA and the Planck Collaboration released the second set of cosmology products based on data from the entire Planck mission, including both temperature and polarization, along with a set of scientific and technical papers and a web-based explanatory supplement. [...]
arXiv:1502.01582.- 2016-09-20 - 38 p. - Published in : Astron. Astrophys. 594 (2016) A1 Fulltext: PDF; External link: Preprint
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8.
Planck intermediate results. XXX. The angular power spectrum of polarized dust emission at intermediate and high Galactic latitudes / Planck Collaboration
The polarized thermal emission from Galactic dust is the main foreground present in measurements of the polarization of the cosmic microwave background (CMB) at frequencies above 100GHz. We exploit the Planck HFI polarization data from 100 to 353GHz to measure the dust angular power spectra $C_\ell^{EE,BB}$ over the range $40<\ell<600$. [...]
arXiv:1409.5738.- 2016-02-09 - 25 p. - Published in : Astron. Astrophys. 586 (2016) A133 Fulltext: PDF; External link: Nature article
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9.
BSMBench: a flexible and scalable supercomputer benchmark from computational particle physics / Bennett, Ed (Swansea U.) ; Lucini, Biagio (Swansea U.) ; Del Debbio, Luigi (U. Edinburgh, Higgs Ctr. Theor. Phys.) ; Jordan, Kirk (IBM, Cambridge) ; Patella, Agostino (CERN) ; Pica, Claudio (Southern Denmark U., CP3-Origins ; U. Southern Denmark, Odense, DIAS) ; Rago, Antonio (Plymouth U. ; Plymouth U., Math. Stat. Dept.)
Benchmarking plays a central role in the evaluation of High Performance Computing architectures. Several benchmarks have been designed that allow users to stress various components of supercomputers. [...]
arXiv:1401.3733; CP3-ORIGINS-2014-001; DIAS-2014-1; CP3-ORIGINS-2014-001; DNRF90; DIAS-2014-1.- 2016-09-15 - 6 p. - Published in : 10.1109/HPCSim.2016.7568421 Fulltext: PDF; External link: Preprint
In : International Conference on High Performance Computing and Simulation, Innsbruck, Austria, 18 - 22 Jul 2016, pp.834-839
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10.
The Polarized Radiation Imaging and Spectroscopy Mission / PRISM Collaboration
PRISM (Polarized Radiation Imaging and Spectroscopy Mission) was proposed to ESA in May 2013 as a large-class mission for investigating within the framework of the ESA Cosmic Vision program a set of important scientific questions that require high resolution, high sensitivity, full-sky observations of the sky emission at wavelengths ranging from millimeter-wave to the far-infrared. PRISM's main objective is to explore the distant universe, probing cosmic history from very early times until now as well as the structures, distribution of matter, and velocity flows throughout our Hubble volume [...]
arXiv:1310.1554.- 2014-02-05 - 55 p. - Published in : JCAP 02 (2014) 006 Fulltext: PDF; External link: Preprint
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CERN Document Server : 20 elementer funnet   1 - 10neste  gå til element:
Se også: lignende forfatternavn
39 Watson, R
50 Watson, R A
1 Watson, R B
1 Watson, R E
1 Watson, R G
1 Watson, R H
3 Watson, R L
1 Watson, R M
1 Watson, Richann
4 Watson, Richard
1 Watson, Richard A
1 Watson, Richard Thomas
1 Watson, Richard W
2 Watson, Robert
6 Watson, Robert A
1 Watson, Robert N M
1 Watson, Robert N.M.
1 Watson, Robert T
1 Watson, Ronald
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