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CERN Document Server 2,047 records found  1 - 10próximoend  jump to record: Search took 1.59 seconds. 
1.
(100)
Tests of a particle flow algorithm with CALICE test beam data / CALICE Collaboration
The studies presented in this paper provide a first experimental test of the Particle Flow Algorithm (PFA) concept using data recorded in high granularity calorimeters. Pairs of overlaid pion showers from CALICE 2007 test beam data are reconstructed by the PandoraPFA program developed to implement PFA for a future lepton collider. [...]
arXiv:1105.3417; CALICE-PUB-2011-002; CALICE-CAN-2010-007; CALICE Analysis Note CAN-024; CALICE Analysis Note CAN-024a.- 2011 - 12 p. - Published in : JINST 6 (2011) P07005 Addendum CAN-024a: PDF; CALICE Note: PDF; Fulltext: PDF; External link: Preprint
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2.
(91)
Tracking within Hadronic Showers in the CALICE SDHCAL prototype using a Hough Transform Technique / CALICE Collaboration
The high granularity of the CALICE Semi-Digital Hadronic CALorimeter (SDHCAL) provides the capability to reveal the track segments present in hadronic showers. These segments are then used as a tool to probe the behaviour of the active layers in situ, to better reconstruct the energy of these hadronic showers and also to distinguish them from electromagnetic ones. [...]
arXiv:1702.08082; CALICE-PUB-2017-001.- 2017-05-12 - 21 p. - Published in : JINST 12 (2017) P05009 Fulltext: PDF;
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3.
(45)
First results of the CALICE SDHCAL technological prototype / CALICE Collaboration
The CALICE Semi-Digital Hadronic Calorimeter (SDHCAL) prototype, built in 2011, was exposed to beams of hadrons, electrons and muons in two short periods in 2012 on two different beam lines of the CERN SPS. The prototype with its 48 active layers, made of Glass Resistive Plate Chambers and their embedded readout electronics, was run in triggerless and power-pulsing mode [...]
arXiv:1602.02276; CALICE-PUB-2016-001.- 2016-04-01 - 36 p. - Published in : JINST 11 (2016) P04001 Fulltext: PDF; External link: Preprint
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4.
(16)
Cover not available Handbook of LHC Higgs Cross Sections: 2. Differential Distributions / Dittmaier, S.
This Report summarises the results of the second year's activities of the LHC Higgs Cross Section Working Group [...]
arXiv:1201.3084 ; CERN-2012-002 CERN-2012-002. - Geneva : CERN, 2012. - 275 p.


ebook
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5.
(12)
Physics Behind Precision / Azzi, P. (ed.) (INFN, Padua) ; Azzurri, P. (INFN, Pisa) ; Biswas, S. (Korea Inst. Advanced Study, Seoul) ; Blekman, F. (ed.) (Brussels U., IIHE) ; Corcella, G. (Frascati) ; De Curtis, S. (Florence U. ; INFN, Florence) ; Erler, J. (Mexico U.) ; Foppiani, N. (Pisa, Scuola Normale Superiore) ; Helenius, I. (Lund U., Dept. Theor. Phys.) ; Jadach, S. (Cracow, INP) et al.
This document provides a writeup of contributions to the FCC-ee mini-workshop on "Physics behind precision" held at CERN, on 2-3 February 2016..
arXiv:1703.01626. - 2017. - 44 p.
Preprint
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6.
(11)
Les Houches 2011: Physics at TeV Colliders New Physics Working Group Report / Brooijmans, G. (Columbia U.) ; Gripaios, B. (Cambridge U.) ; Moortgat, F. (Zurich, ETH) ; Santiago, J. (CAFPE, Granada ; Granada U., Theor. Phys. Astrophys.) ; Skands, P. (CERN) ; Albornoz Vásquez, D. (Paris, Inst. Astrophys.) ; Allanach, B.C. (Cambridge U., DAMTP) ; Alloul, A. (Strasbourg, IPHC ; Strasbourg, IReS) ; Arbey, A. (CERN ; Lyon, IPN ; Lyon Observ.) ; Azatov, A. (INFN, Rome ; Rome U.) et al.
We present the activities of the 'New Physics' working group for the 'Physics at TeV Colliders' workshop (Les Houches, France, 30 May-17 June, 2011). Our report includes new agreements on formats for interfaces between computational tools, new tool developments, important signatures for searches at the LHC, recommendations for presentation of LHC search results, as well as additional phenomenological studies..
arXiv:1203.1488; FERMILAB-CONF-12-924-T.- 2012 - 243 p. - Published in : , pp. 221-463 Fermilab Library: PDF; Fulltext: PDF; External link: Fermilab Library
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7.
(10)
Planck 2015 results. XXI. The integrated Sachs-Wolfe effect / Planck Collaboration
This paper presents a study of the ISW effect from the Planck 2015 temperature and polarization data release. The CMB is cross-correlated with different LSS tracers: the NVSS, SDSS and WISE catalogues, and the Planck 2015 convergence lensing map. [...]
arXiv:1502.01595.- 2016-09-20 - 30 p. - Published in : Astron. Astrophys. 594 (2016) A21 Fulltext: PDF; External link: Preprint
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8.
(10)
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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9.
(9)
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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10.
(9)
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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