CERN Accelerating science

002153377 001__ 2153377
002153377 005__ 20220810144839.0
002153377 0248_ $$aoai:cds.cern.ch:2153377$$pcerncds:CERN$$pcerncds:CERN:FULLTEXT$$pcerncds:FULLTEXT
002153377 0247_ $$2DOI$$a10.1103/PhysRevC.94.054908
002153377 035__ $$9arXiv$$aoai:arXiv.org:1605.07569
002153377 035__ $$9Inspire$$a1465513
002153377 037__ $$9arXiv$$aarXiv:1605.07569$$cnucl-ex
002153377 037__ $$aCERN-EP-2016-127
002153377 041__ $$aeng
002153377 084__ $$2CERN Library$$aEP-2016-127
002153377 088__ $$9CERN-EP-DRAFT-ALICE-2016-011
002153377 088__ $$aCERN-EP-2016-127
002153377 100__ $$aAdam, Jaroslav$$iINSPIRE-00360890$$uPrague, Tech. U.$$vFaculty of Nuclear Sciences and Physical Engineering, Czech Technical University in Prague , Prague, Czech Republic
002153377 245__ $$aD-meson production in $p$–Pb collisions at $\sqrt{s_{\rm NN}}=5.02$ TeV and in $pp$ collisions at $\sqrt{s}=7$ TeV
002153377 269__ $$aGeneva$$bCERN$$c16 May 2016
002153377 260__ $$c2016-11-23
002153377 300__ $$a31 p
002153377 506__ $$dcds-edboard-alice@cern.ch
002153377 506__ $$malice-member [CERN]
002153377 506__ $$mcds-ph-ep-publications-referee [CERN]
002153377 500__ $$9arXiv$$a43 pages, 17 captioned figures, 3 tables, authors from page 37, published version, figures at http://aliceinfo.cern.ch/ArtSubmission/node/2711
002153377 520__ $$aThe production cross sections of the prompt charmed mesons D$^0$, D$^+$, D$^{*+}$ and D$_{\rm s}^+$ were measured at mid-rapidity in p-Pb collisions at a centre-of-mass energy per nucleon pair $\sqrt{s_{\rm NN}}=5.02$ TeV with the ALICE detector at the LHC. D mesons were reconstruct ed from their decays D$^0\rightarrow {\rm K}^-\pi^+$, D$^+\rightarrow {\rm K}^-\pi^+\pi^+$, D$^{*+}\rightarrow {\rm D}^0\pi^+$, D$_s^+\rightarrow\phi\pi^+\rightarrow {\rm K}^-{\rm K}^+\pi^+$, and their charge conjugates. The $p_{\rm T}$-differential production cross sections were measured at mid-rapidity in the transverse momentum interval $1<p_{\rm T}<24$ GeV/$c$ for D$^0$, D$^+$ and D$^{*+}$ mesons and in $2<p_{\rm T}<12$ GeV/$c$ for $D_s^+$ mesons, using an analysis method based on the selection of decay topologies displaced from the interaction vertex. The production cross sections of the D$^0$, D$^+$ and D$^{*+}$ mesons were also measured in three $p_{\rm T}$ intervals as a function of the rapidity $y_{\rm cms}$ in the centre-of-mass system in $-1.26<y_{\rm cms}<0.34$. In addition, the prompt D$^0$ production cross section was measured in pp collisions at $\sqrt{s}=7$ TeV and p-Pb collisions at $\sqrt{s_{\rm NN}}=5.02$ TeV down to $p_{\rm T}=0$ using an analysis technique that is based on the estimation and subtraction of the combinatorial background, without reconstruction of the D$^0$ decay vertex. The nuclear modification factor $R_{\rm pPb}(p_{\rm T})$, defined as the ratio of the $p_{\rm T}$-differential D-meson cross section in p-Pb collisions and that in pp collisions scaled by the mass number of the Pb nucleus, was calculated for the four D-meson species and found to be compatible with unity within experimental uncertainties. The results are compared to theoretical calculations that include cold-nuclear-matter effects and to transport model calculations incorporating the interactions of charm quarks with an expanding deconfined medium.
002153377 520__ $$9HEPDATA$$hCERN-LHC.  The production cross sections of the prompt charmed mesons D$^0$, D$^+$, D$^{*+}$ and D$_s$ were measured at mid-rapidity in p-Pb collisions at a centre-of-mass energy per nucleon pair $\sqrt{s_{\rm NN}}=5.02$ TeV with the ALICE detector at the LHC. D mesons were reconstructed from their decays D$^0\rightarrow{\rm K}^-\pi^+$, D$^+\rightarrow{\rm K}^-\pi^+\pi^+$, D$^{*+}\rightarrow D^0\pi^+$, D$_s^+\rightarrow\phi\pi^+\rightarrow{\rm K}^-{\rm K}^+\pi^+$, and their charge conjugates. The $p_{\rm T}$-differential production cross sections were measured at mid-rapidity in the interval $1&lt;p_{\rm T}&lt;24$ GeV/$c$ for D$^0$, D$^+$ and D$^{*+}$ mesons and in $2&lt;p_{\rm T}&lt;12$ GeV/$c$ for D$_s$ mesons, using an analysis method based on the selection of decay topologies displaced from the interaction vertex. The production cross sections of the D$^0$, D$^+$ and D$^{*+}$ mesons were also measured in three $p_{\rm T}$ intervals as a function of the rapidity $y_{\rm cms}$ in the centre-of-mass system in $-1.26&lt;y_{\rm cms}&lt;0.34$. In addition, the prompt D$^0$ cross section was measured in pp collisions at $\sqrt{s}=7$ TeV and p-Pb collisions at $\sqrt{s_{\rm NN}}=5.02$ TeV down to $p_{\rm T}=0$ using an analysis technique that is based on the estimation and subtraction of the combinatorial background, without reconstruction of the D$^0$ decay vertex. The nuclear modification factor $R_{\rm pPb}(p_{\rm T})$, defined as the ratio of the $p_{\rm T}$-differential D-meson cross section in p-Pb collisions and that in pp collisions scaled by the mass number of the Pb nucleus, was calculated for the four D-meson species and found to be compatible with unity within experimental uncertainties. The results are compared to theoretical calculations that include cold-nuclear-matter effects and to transport model calculations incorporating the interactions of charm quarks with an expanding deconfined medium.
002153377 520__ $$9APS$$aBackground: In the context of the investigation of the quark gluon plasma produced in heavy-ion collisions, hadrons containing heavy (charm or beauty) quarks play a special role for the characterization of the hot and dense medium created in the interaction. The measurement of the production of charm and beauty hadrons in proton–proton collisions, besides providing the necessary reference for the studies in heavy-ion reactions, constitutes an important test of perturbative quantum chromodynamics (pQCD) calculations. Heavy-flavor production in proton–nucleus collisions is sensitive to the various effects related to the presence of nuclei in the colliding system, commonly denoted cold-nuclear-matter effects. Most of these effects are expected to modify open-charm production at low transverse momenta (pT) and, so far, no measurement of D-meson production down to zero transverse momentum was available at mid-rapidity at the energies attained at the CERN Large Hadron Collider (LHC). Purpose: The measurements of the production cross sections of promptly produced charmed mesons in p-Pb collisions at the LHC down to pT=0 and the comparison to the results from pp interactions are aimed at the assessment of cold-nuclear-matter effects on open-charm production, which is crucial for the interpretation of the results from Pb-Pb collisions. Methods: The prompt charmed mesons D0,D+,D*+, and Ds+ were measured at mid-rapidity in p-Pb collisions at a center-of-mass energy per nucleon pair sNN=5.02 TeV with the ALICE detector at the LHC. D mesons were reconstructed from their decays D0→K−π+,D+→K−π+π+, D*+→D0π+,Ds+→ϕπ+→K−K+π+, and their charge conjugates, using an analysis method based on the selection of decay topologies displaced from the interaction vertex. In addition, the prompt D0 production cross section was measured in pp collisions at s=7 TeV and p-Pb collisions at sNN=5.02 TeV down to pT=0 using an analysis technique that is based on the estimation and subtraction of the combinatorial background, without reconstruction of the D0 decay vertex. Results: The production cross section in pp collisions is described within uncertainties by different implementations of pQCD calculations down to pT=0. This allowed also a determination of the total cc¯ production cross section in pp collisions, which is more precise than previous ALICE measurements because it is not affected by uncertainties owing to the extrapolation to pT=0. The nuclear modification factor RpPb(pT), defined as the ratio of the pT-differential D meson cross section in p-Pb collisions and that in pp collisions scaled by the mass number of the Pb nucleus, was calculated for the four D-meson species and found to be compatible with unity within uncertainties. The results are compared to theoretical calculations that include cold-nuclear-matter effects and to transport model calculations incorporating the interactions of charm quarks with an expanding deconfined medium. Conclusions: These measurements add experimental evidence that the modification of the D-meson transverse momentum distributions observed in Pb–Pb collisions with respect to pp interactions is due to strong final-state effects induced by the interactions of the charm quarks with the hot and dense partonic medium created in ultrarelativistic heavy-ion collisions. The current precision of the measurement does not allow us to draw conclusions on the role of the different cold-nuclear-matter effects and on the possible presence of additional hot-medium effects in p-Pb collisions. However, the analysis technique without decay-vertex reconstruction, applied on future larger data samples, should provide access to the physics-rich range down to pT=0.
002153377 520__ $$9arXiv$$aThe production cross sections of the prompt charmed mesons D$^0$, D$^+$, D$^{*+}$ and D$_s$ were measured at mid-rapidity in p-Pb collisions at a centre-of-mass energy per nucleon pair $\sqrt{s_{\rm NN}}=5.02$ TeV with the ALICE detector at the LHC. D mesons were reconstructed from their decays D$^0\rightarrow{\rm K}^-\pi^+$, D$^+\rightarrow{\rm K}^-\pi^+\pi^+$, D$^{*+}\rightarrow D^0\pi^+$, D$_s^+\rightarrow\phi\pi^+\rightarrow{\rm K}^-{\rm K}^+\pi^+$, and their charge conjugates. The $p_{\rm T}$-differential production cross sections were measured at mid-rapidity in the interval $1<p_{\rm T}<24$ GeV/$c$ for D$^0$, D$^+$ and D$^{*+}$ mesons and in $2<p_{\rm T}<12$ GeV/$c$ for D$_s$ mesons, using an analysis method based on the selection of decay topologies displaced from the interaction vertex. The production cross sections of the D$^0$, D$^+$ and D$^{*+}$ mesons were also measured in three $p_{\rm T}$ intervals as a function of the rapidity $y_{\rm cms}$ in the centre-of-mass system in $-1.26<y_{\rm cms}<0.34$. In addition, the prompt D$^0$ cross section was measured in pp collisions at $\sqrt{s}=7$ TeV and p-Pb collisions at $\sqrt{s_{\rm NN}}=5.02$ TeV down to $p_{\rm T}=0$ using an analysis technique that is based on the estimation and subtraction of the combinatorial background, without reconstruction of the D$^0$ decay vertex. The nuclear modification factor $R_{\rm pPb}(p_{\rm T})$, defined as the ratio of the $p_{\rm T}$-differential D-meson cross section in p-Pb collisions and that in pp collisions scaled by the mass number of the Pb nucleus, was calculated for the four D-meson species and found to be compatible with unity within experimental uncertainties. The results are compared to theoretical calculations that include cold-nuclear-matter effects and to transport model calculations incorporating the interactions of charm quarks with an expanding deconfined medium.
002153377 540__ $$3preprint$$aCC-BY-4.0
002153377 540__ $$3publication$$aCC-BY-3.0
002153377 542__ $$3preprint$$dCERN$$g2016
002153377 542__ $$3publication$$dCERN$$g2016
002153377 562__ $$cPublic comments
002153377 595__ $$aautomerged
002153377 595__ $$aCERN-EP
002153377 65017 $$2SzGeCERN$$aNuclear Physics - Experiment
002153377 65027 $$2arXiv$$aParticle Physics - Experiment
002153377 6531_ $$9CERN$$aflavor physics
002153377 6531_ $$9CERN$$arelativistic heavy ion physics
002153377 6531_ $$9CERN$$aheavy quark production
002153377 6531_ $$9CERN$$aquark deconfinement
002153377 6531_ $$9CERN$$aexperimental results
002153377 693__ $$aCERN LHC$$eALICE
002153377 695__ $$9LANL EDS$$anucl-ex
002153377 695__ $$9LANL EDS$$ahep-ex
002153377 690C_ $$aCERN
002153377 690C_ $$aARTICLE
002153377 690C_ $$aALICE_Papers
002153377 700__ $$aAdamova, Dagmar$$iINSPIRE-00261412$$uRez, Nucl. Phys. Inst.
002153377 700__ $$aAggarwal, Madan Mohan$$iINSPIRE-00180711$$uPanjab U.
002153377 700__ $$aAglieri Rinella, Gianluca$$iINSPIRE-00249866$$uCERN
002153377 700__ $$aAgnello, Michelangelo$$iINSPIRE-00360901$$uTurin Polytechnic$$uINFN, Turin
002153377 700__ $$aAgrawal, Neelima$$iINSPIRE-00381545$$uIndian Inst. Tech., Mumbai
002153377 700__ $$aAhammed, Zubayer$$iINSPIRE-00180720$$uCalcutta, VECC
002153377 700__ $$aAhmad, Shakeel$$iINSPIRE-00560210$$uAligarh Muslim U.
002153377 700__ $$aAhn, Sang Un$$iINSPIRE-00254695$$uKISTI, Daejeon
002153377 700__ $$aAiola, Salvatore$$iINSPIRE-00381830$$uYale U.
002153377 700__ $$aAkindinov, Alexander$$iINSPIRE-00061314$$uMoscow, ITEP
002153377 700__ $$aAlam, Sk Noor$$iINSPIRE-00415748$$uCalcutta, VECC
002153377 700__ $$aSilva De Albuquerque, Danilo$$iINSPIRE-00560229$$uCampinas State U.
002153377 700__ $$aAleksandrov, Dmitry$$iINSPIRE-00158344$$uKurchatov Inst., Moscow
002153377 700__ $$aAlessandro, Bruno$$iINSPIRE-00250010$$uINFN, Turin
002153377 700__ $$aAlexandre, Didier$$iINSPIRE-00381902$$uBirmingham U.
002153377 700__ $$aAlfaro Molina, Jose Ruben$$iINSPIRE-00249844$$uMexico U.
002153377 700__ $$aAlici, Andrea$$iINSPIRE-00249832$$uEnrico Fermi Ctr., Rome$$uINFN, Bologna
002153377 700__ $$aAlkin, Anton$$iINSPIRE-00245838$$uBITP, Kiev
002153377 700__ $$aAlme, Johan$$iINSPIRE-00249819$$uBergen U.$$uBergen Coll. Higher Educ.
002153377 700__ $$aAlt, Torsten$$iINSPIRE-00249807$$uFrankfurt U., FIAS
002153377 700__ $$aAltinpinar, Sedat$$iINSPIRE-00247365$$uBergen U.
002153377 700__ $$aAltsybeev, Igor$$iINSPIRE-00307325$$uSt. Petersburg State U.
002153377 700__ $$aAlves Garcia Prado, Caio$$iINSPIRE-00382006$$uSao Paulo U.
002153377 700__ $$aAndrei, Cristian$$iINSPIRE-00249783$$uBucharest, IFIN-HH
002153377 700__ $$aAndronic, Anton$$iINSPIRE-00261430$$uDarmstadt, EMMI
002153377 700__ $$aAnguelov, Venelin$$iINSPIRE-00244018$$uHeidelberg U.
002153377 700__ $$aAnticic, Tome$$iINSPIRE-00062373$$uBoskovic Inst., Zagreb
002153377 700__ $$aAntinori, Federico$$iINSPIRE-00175367$$uINFN, Padua
002153377 700__ $$aAntonioli, Pietro$$iINSPIRE-00058331$$uINFN, Bologna
002153377 700__ $$aAphecetche, Laurent Bernard$$iINSPIRE-00058998$$uSUBATECH, Nantes
002153377 700__ $$aAppelshaeuser, Harald$$iINSPIRE-00250020$$uFrankfurt U., Inst. Kernphys.
002153377 700__ $$aArcelli, Silvia$$iINSPIRE-00250042$$uBologna U.$$uINFN, Bologna
002153377 700__ $$aArnaldi, Roberta$$iINSPIRE-00261446$$uINFN, Turin
002153377 700__ $$aArnold, Oliver Werner$$iINSPIRE-00537106$$uMunich, Tech. U., Universe$$uTech. U., Munich (main)
002153377 700__ $$aArsene, Ionut Cristian$$iINSPIRE-00261457$$uOslo U.
002153377 700__ $$aArslandok, Mesut$$iINSPIRE-00245664$$uFrankfurt U., Inst. Kernphys.
002153377 700__ $$aAudurier, Benjamin$$iINSPIRE-00522415$$uSUBATECH, Nantes
002153377 700__ $$aAugustinus, Andre$$iINSPIRE-00261469$$uCERN
002153377 700__ $$aAverbeck, Ralf Peter$$iINSPIRE-00063377$$uDarmstadt, EMMI
002153377 700__ $$aAzmi, Mohd Danish$$iINSPIRE-00249731$$uAligarh Muslim U.
002153377 700__ $$aBadala, Angela$$iINSPIRE-00249728$$uINFN, Catania
002153377 700__ $$aBaek, Yong Wook$$iINSPIRE-00249716$$uKonkuk U.
002153377 700__ $$aBagnasco, Stefano$$iINSPIRE-00028794$$uINFN, Turin
002153377 700__ $$aBailhache, Raphaelle Marie$$iINSPIRE-00247346$$uFrankfurt U., Inst. Kernphys.
002153377 700__ $$aBala, Renu$$iINSPIRE-00261473$$uJammu U.
002153377 700__ $$aBalasubramanian, Supraja$$iINSPIRE-00548311$$uYale U.
002153377 700__ $$aBaldisseri, Alberto$$iINSPIRE-00064101$$uIRFU, Saclay
002153377 700__ $$aBaral, Rama Chandra$$iINSPIRE-00289153$$uBhubaneswar, Inst. Phys.
002153377 700__ $$aBarbano, Anastasia Maria$$iINSPIRE-00506685$$uTurin U.$$uINFN, Turin
002153377 700__ $$aBarbera, Roberto$$iINSPIRE-00250052$$uCatania U.$$uINFN, Catania
002153377 700__ $$aBarile, Francesco$$iINSPIRE-00249702$$uBari U.$$uINFN, Bari
002153377 700__ $$aBarnafoldi, Gergely Gabor$$iINSPIRE-00261490$$uWigner RCP, Budapest
002153377 700__ $$aBarnby, Lee Stuart$$iINSPIRE-00064600$$uBirmingham U.$$uCERN
002153377 700__ $$aRamillien Barret, Valerie$$iINSPIRE-00261503$$uClermont-Ferrand U.
002153377 700__ $$aBartalini, Paolo$$iINSPIRE-00064862$$uHua-Zhong Normal U.
002153377 700__ $$aBarth, Klaus$$iINSPIRE-00522252$$uCERN
002153377 700__ $$aBartke, Jerzy Gustaw$$iINSPIRE-00254910$$uCracow, INP
002153377 700__ $$aBartsch, Esther$$iINSPIRE-00506794$$uFrankfurt U., Inst. Kernphys.
002153377 700__ $$aBasile, Maurizio$$iINSPIRE-00172080$$uBologna U.$$uINFN, Bologna
002153377 700__ $$aBastid, Nicole$$iINSPIRE-00065071$$uClermont-Ferrand U.
002153377 700__ $$aBasu, Sumit$$iINSPIRE-00360931$$uCalcutta, VECC
002153377 700__ $$aBathen, Bastian$$iINSPIRE-00249684$$uMunster U.
002153377 700__ $$aBatigne, Guillaume$$iINSPIRE-00057450$$uSUBATECH, Nantes
002153377 700__ $$aBatista Camejo, Arianna$$iINSPIRE-00415862$$uClermont-Ferrand U.
002153377 700__ $$aBatyunya, Boris$$iINSPIRE-00180230$$uDubna, JINR
002153377 700__ $$aBatzing, Paul Christoph$$iINSPIRE-00382071$$uOslo U.
002153377 700__ $$aBearden, Ian Gardner$$iINSPIRE-00261515$$uBohr Inst.
002153377 700__ $$aBeck, Hans$$iINSPIRE-00261523$$uFrankfurt U., Inst. Kernphys.$$uHeidelberg U.
002153377 700__ $$aBedda, Cristina$$iINSPIRE-00382119$$uINFN, Turin
002153377 700__ $$aBehera, Nirbhay Kumar$$iINSPIRE-00299673$$uInha U.
002153377 700__ $$aBelikov, Iouri$$iINSPIRE-00250068$$uStrasbourg, IPHC
002153377 700__ $$aBellini, Francesca$$iINSPIRE-00244351$$uBologna U.$$uINFN, Bologna
002153377 700__ $$aBello Martinez, Hector$$iINSPIRE-00506861$$uPuebla U., Mexico
002153377 700__ $$aBellwied, Rene$$iINSPIRE-00180735$$uHouston U.
002153377 700__ $$aBelmont Iii, Ronald John$$iINSPIRE-00254969$$uWayne State U.
002153377 700__ $$aBelmont Moreno, Ernesto$$iINSPIRE-00249679$$uMexico U.
002153377 700__ $$aEspinoza Beltran, Lucina Gabriela$$iINSPIRE-00563992$$uSinaloa U.
002153377 700__ $$aBelyaev, Vladimir$$iINSPIRE-00386131$$uMoscow Phys. Eng. Inst.
002153377 700__ $$aBencedi, Gyula$$iINSPIRE-00360943$$uWigner RCP, Budapest
002153377 700__ $$aBeole, Stefania$$iINSPIRE-00261543$$uTurin U.$$uINFN, Turin
002153377 700__ $$aBerceanu, Ionela$$iINSPIRE-00261556$$uBucharest, IFIN-HH
002153377 700__ $$aBercuci, Alexandru$$iINSPIRE-00261560$$uBucharest, IFIN-HH
002153377 700__ $$aBerdnikov, Yaroslav$$iINSPIRE-00066204$$uSt. Petersburg, INP
002153377 700__ $$aBerenyi, Daniel$$iINSPIRE-00245794$$uWigner RCP, Budapest
002153377 700__ $$aBertens, Redmer Alexander$$iINSPIRE-00382235$$uUtrecht U.
002153377 700__ $$aBerzano, Dario$$iINSPIRE-00245123$$uCERN
002153377 700__ $$aBetev, Latchezar$$iINSPIRE-00250085$$uCERN
002153377 700__ $$aBhasin, Anju$$iINSPIRE-00180740$$uJammu U.
002153377 700__ $$aBhat, Inayat Rasool$$iINSPIRE-00415990$$uJammu U.
002153377 700__ $$aBhati, Ashok Kumar$$iINSPIRE-00180755$$uPanjab U.
002153377 700__ $$aBhattacharjee, Buddhadeb$$iINSPIRE-00385476$$uGauhati U.
002153377 700__ $$aBhom, Jihyun$$iINSPIRE-00287624$$uCracow, INP
002153377 700__ $$aBianchi, Livio$$iINSPIRE-00254651$$uHouston U.
002153377 700__ $$aBianchi, Nicola$$iINSPIRE-00139110$$uFrascati
002153377 700__ $$aBianchin, Chiara$$iINSPIRE-00247334$$uWayne State U.
002153377 700__ $$aBielcik, Jaroslav$$iINSPIRE-00180768$$uPrague, Tech. U.
002153377 700__ $$aBielcikova, Jana$$iINSPIRE-00180776$$uRez, Nucl. Phys. Inst.
002153377 700__ $$aBilandzic, Ante$$iINSPIRE-00261580$$uBohr Inst.$$uMunich, Tech. U., Universe$$uTech. U., Munich (main)
002153377 700__ $$aBiro, Gabor$$iINSPIRE-00548333$$uWigner RCP, Budapest
002153377 700__ $$aBiswas, Rathijit$$iINSPIRE-00522421$$uBose Inst., Kolkata$$uCAPSS, Kolkata
002153377 700__ $$aBiswas, Saikat$$iINSPIRE-00525263$$uBose Inst., Kolkata$$uCAPSS, Kolkata$$uBhubaneswar, NISER
002153377 700__ $$aBjelogrlic, Sandro$$iINSPIRE-00360967$$uUtrecht U.
002153377 700__ $$aBlair, Justin Thomas$$iINSPIRE-00531266$$uTexas U.
002153377 700__ $$aBlau, Dmitry$$iINSPIRE-00247320$$uKurchatov Inst., Moscow
002153377 700__ $$aBlume, Christoph$$iINSPIRE-00067666$$uFrankfurt U., Inst. Kernphys.
002153377 700__ $$aBock, Friederike$$iINSPIRE-00246175$$uLBL, Berkeley$$uHeidelberg U.
002153377 700__ $$aBogdanov, Alexey$$iINSPIRE-00261637$$uMoscow Phys. Eng. Inst.
002153377 700__ $$aBoggild, Hans$$iINSPIRE-00067837$$uBohr Inst.
002153377 700__ $$aBoldizsar, Laszlo$$iINSPIRE-00307799$$uWigner RCP, Budapest
002153377 700__ $$aBombara, Marek$$iINSPIRE-00261642$$uKosice U.
002153377 700__ $$aBonora, Matthias$$iINSPIRE-00563828$$uCERN
002153377 700__ $$aBook, Julian Heinz$$iINSPIRE-00261651$$uFrankfurt U., Inst. Kernphys.
002153377 700__ $$aBorel, Herve$$iINSPIRE-00068253$$uIRFU, Saclay
002153377 700__ $$aBorissov, Alexander$$iINSPIRE-00254729$$uPusan Natl. U.
002153377 700__ $$aBorri, Marcello$$iINSPIRE-00286268$$uLiverpool U.$$uDaresbury
002153377 700__ $$aBossu, Francesco$$iINSPIRE-00249614$$uiThemba LABS
002153377 700__ $$aBotta, Elena$$iINSPIRE-00250108$$uTurin U.$$uINFN, Turin
002153377 700__ $$aBourjau, Christian$$iINSPIRE-00537054$$uBohr Inst.
002153377 700__ $$aBraun-Munzinger, Peter$$iINSPIRE-00069060$$uDarmstadt, EMMI
002153377 700__ $$aBregant, Marco$$iINSPIRE-00261672$$uSao Paulo U.
002153377 700__ $$aBreitner, Timo Gunther$$iINSPIRE-00249589$$uGoethe U., Frankfurt, Inst. Inform.
002153377 700__ $$aBroker, Theo Alexander$$iINSPIRE-00382350$$uFrankfurt U., Inst. Kernphys.
002153377 700__ $$aBrowning, Tyler Allen$$iINSPIRE-00360979$$uPurdue U.
002153377 700__ $$aBroz, Michal$$iINSPIRE-00246094$$uPrague, Tech. U.
002153377 700__ $$aBrucken, Erik Jens$$iINSPIRE-00019412$$uHelsinki Inst. of Phys.
002153377 700__ $$aBruna, Elena$$iINSPIRE-00181319$$uINFN, Turin
002153377 700__ $$aBruno, Giuseppe Eugenio$$iINSPIRE-00314938$$uBari U.$$uINFN, Bari
002153377 700__ $$aBudnikov, Dmitry$$iINSPIRE-00249577$$uRFNC-VNIIEF, Sarov
002153377 700__ $$aBuesching, Henner$$iINSPIRE-00241182$$uFrankfurt U., Inst. Kernphys.
002153377 700__ $$aBufalino, Stefania$$iINSPIRE-00289290$$uTurin Polytechnic$$uCERN
002153377 700__ $$aBuncic, Predrag$$iINSPIRE-00178263$$uCERN
002153377 700__ $$aBusch, Oliver$$iINSPIRE-00261698$$uTsukuba U.
002153377 700__ $$aButhelezi, Edith Zinhle$$iINSPIRE-00261702$$uiThemba LABS
002153377 700__ $$aBashir Butt, Jamila$$iINSPIRE-00040297$$uCOMSATS, Islamabad
002153377 700__ $$aBuxton, Jesse Thomas$$iINSPIRE-00507048$$uOhio State U.
002153377 700__ $$aCabala, Jan$$iINSPIRE-00560262$$uKosice Tech. U.
002153377 700__ $$aCaffarri, Davide$$iINSPIRE-00249565$$uCERN
002153377 700__ $$aCai, Xu$$iINSPIRE-00198777$$uHua-Zhong Normal U.
002153377 700__ $$aCaines, Helen Louise$$iINSPIRE-00177317$$uYale U.
002153377 700__ $$aCalero Diaz, Liliet$$iINSPIRE-00416093$$uFrascati
002153377 700__ $$aCaliva, Alberto$$iINSPIRE-00382423$$uUtrecht U.
002153377 700__ $$aCalvo Villar, Ernesto$$iINSPIRE-00248154$$uLima, Pont. U. Catolica
002153377 700__ $$aCamerini, Paolo$$iINSPIRE-00070739$$uTrieste U.$$uINFN, Trieste
002153377 700__ $$aCarena, Francesco$$iINSPIRE-00289308$$uCERN
002153377 700__ $$aCarena, Wisla$$iINSPIRE-00186542$$uCERN
002153377 700__ $$aCarnesecchi, Francesca$$iINSPIRE-00531272$$uBologna U.$$uINFN, Bologna
002153377 700__ $$aCastillo Castellanos, Javier Ernesto$$iINSPIRE-00247261$$uIRFU, Saclay
002153377 700__ $$aCastro, Andrew John$$iINSPIRE-00507151$$uTennessee U.
002153377 700__ $$aCasula, Ester Anna Rita$$iINSPIRE-00360992$$uCagliari U.$$uINFN, Cagliari
002153377 700__ $$aCeballos Sanchez, Cesar$$iINSPIRE-00361004$$uHavana, CEADEN
002153377 700__ $$aCepila, Jan$$iINSPIRE-00245437$$uPrague, Tech. U.
002153377 700__ $$aCerello, Piergiorgio$$iINSPIRE-00071926$$uINFN, Turin
002153377 700__ $$aCerkala, Jakub$$iINSPIRE-00522395$$uKosice Tech. U.
002153377 700__ $$aChang, Beomsu$$iINSPIRE-00241230$$uJyvaskyla U.
002153377 700__ $$aChapeland, Sylvain$$iINSPIRE-00249510$$uCERN
002153377 700__ $$aChartier, Marielle$$iINSPIRE-00385460$$uLiverpool U.
002153377 700__ $$aCharvet, Jean-Luc Fernand$$iINSPIRE-00241253$$uIRFU, Saclay
002153377 700__ $$aChattopadhyay, Subhasis$$iINSPIRE-00180920$$uCalcutta, VECC
002153377 700__ $$aChattopadhyay, Sukalyan$$iINSPIRE-00207158$$uSaha Inst.
002153377 700__ $$aChauvin, Alex$$iINSPIRE-00548342$$uTech. U., Munich (main)$$uMunich, Tech. U., Universe
002153377 700__ $$aChelnokov, Volodymyr$$iINSPIRE-00389106$$uBITP, Kiev
002153377 700__ $$aCherney, Michael Gerard$$iINSPIRE-00184613$$uCreighton U.
002153377 700__ $$aCheshkov, Cvetan Valeriev$$iINSPIRE-00261739$$uLyon, IPN
002153377 700__ $$aCheynis, Brigitte$$iINSPIRE-00250110$$uLyon, IPN
002153377 700__ $$aChibante Barroso, Vasco Miguel$$iINSPIRE-00249506$$uCERN
002153377 700__ $$aDobrigkeit Chinellato, David$$iINSPIRE-00254605$$uCampinas State U.
002153377 700__ $$aCho, Soyeon$$iINSPIRE-00537064$$uInha U.
002153377 700__ $$aChochula, Peter$$iINSPIRE-00186177$$uCERN
002153377 700__ $$aChoi, Kyungeon$$iINSPIRE-00180982$$uPusan Natl. U.
002153377 700__ $$aChojnacki, Marek$$iINSPIRE-00244445$$uBohr Inst.
002153377 700__ $$aChoudhury, Subikash$$iINSPIRE-00361022$$uCalcutta, VECC
002153377 700__ $$aChristakoglou, Panagiotis$$iINSPIRE-00261752$$uNIKHEF, Amsterdam
002153377 700__ $$aChristensen, Christian Holm$$iINSPIRE-00228862$$uBohr Inst.
002153377 700__ $$aChristiansen, Peter$$iINSPIRE-00254597$$uLund U.
002153377 700__ $$aChujo, Tatsuya$$iINSPIRE-00073415$$uTsukuba U.
002153377 700__ $$aChung, Suh-Urk$$iINSPIRE-00073470$$uPusan Natl. U.
002153377 700__ $$aCicalo, Corrado$$iINSPIRE-00289316$$uINFN, Cagliari
002153377 700__ $$aCifarelli, Luisa$$iINSPIRE-00172106$$uEnrico Fermi Ctr., Rome$$uBologna U.$$uINFN, Bologna
002153377 700__ $$aCindolo, Federico$$iINSPIRE-00073552$$uINFN, Bologna
002153377 700__ $$aCleymans, Jean Willy Andre$$iINSPIRE-00073783$$uCape Town U.
002153377 700__ $$aColamaria, Fabio Filippo$$iINSPIRE-00246108$$uBari U.$$uINFN, Bari
002153377 700__ $$aColella, Domenico$$iINSPIRE-00361034$$uKosice, IEF$$uCERN
002153377 700__ $$aCollu, Alberto$$iINSPIRE-00361046$$uLBL, Berkeley
002153377 700__ $$aColocci, Manuel$$iINSPIRE-00382468$$uBologna U.$$uINFN, Bologna
002153377 700__ $$aConesa Balbastre, Gustavo$$iINSPIRE-00247256$$uLPSC, Grenoble
002153377 700__ $$aConesa Del Valle, Zaida$$iINSPIRE-00026575$$uOrsay, IPN
002153377 700__ $$aConnors, Megan Elizabeth$$iINSPIRE-00255007$$uYale U.
002153377 700__ $$aContreras Nuno, Jesus Guillermo$$iINSPIRE-00240060$$uPrague, Tech. U.
002153377 700__ $$aCormier, Thomas Michael$$iINSPIRE-00261783$$uOak Ridge
002153377 700__ $$aCorrales Morales, Yasser$$iINSPIRE-00261791$$uTurin U.$$uINFN, Turin
002153377 700__ $$aCortes Maldonado, Ismael$$iINSPIRE-00210299$$uPuebla U., Mexico
002153377 700__ $$aCortese, Pietro$$iINSPIRE-00037929$$uPiemonte Orientale U., Alessandria
002153377 700__ $$aCosentino, Mauro Rogerio$$iINSPIRE-00289338$$uSao Paulo U.
002153377 700__ $$aCosta, Filippo$$iINSPIRE-00289393$$uCERN
002153377 700__ $$aCrkovska, Jana$$iINSPIRE-00538124$$uOrsay, IPN
002153377 700__ $$aCrochet, Philippe$$iINSPIRE-00250128$$uClermont-Ferrand U.
002153377 700__ $$aCruz Albino, Rigoberto$$iINSPIRE-00382506$$uCINVESTAV, IPN
002153377 700__ $$aCuautle Flores, Eleazar$$iINSPIRE-00075170$$uMexico U., ICN
002153377 700__ $$aCunqueiro Mendez, Leticia$$iINSPIRE-00289410$$uMunster U.$$uCERN
002153377 700__ $$aDahms, Torsten$$iINSPIRE-00039260$$uTech. U., Munich (main)$$uMunich, Tech. U., Universe
002153377 700__ $$aDainese, Andrea$$iINSPIRE-00250006$$uINFN, Padua
002153377 700__ $$aDanisch, Meike Charlotte$$iINSPIRE-00560270$$uHeidelberg U.
002153377 700__ $$aDanu, Andrea$$iINSPIRE-00249445$$uBucharest, Inst. Space Science
002153377 700__ $$aDas, Debasish$$iINSPIRE-00289436$$uSaha Inst.
002153377 700__ $$aDas, Indranil$$iINSPIRE-00249433$$uSaha Inst.
002153377 700__ $$aDas, Supriya$$iINSPIRE-00058401$$uBose Inst., Kolkata$$uCAPSS, Kolkata
002153377 700__ $$aDash, Ajay Kumar$$iINSPIRE-00249421$$uBhubaneswar, NISER
002153377 700__ $$aDash, Sadhana$$iINSPIRE-00181086$$uIndian Inst. Tech., Mumbai
002153377 700__ $$aDe, Sudipan$$iINSPIRE-00289444$$uSao Paulo U.
002153377 700__ $$aDe Caro, Annalisa$$iINSPIRE-00249410$$uEnrico Fermi Ctr., Rome$$uSalerno U.$$uINFN, Salerno
002153377 700__ $$aDe Cataldo, Giacinto$$iINSPIRE-00289454$$uINFN, Bari
002153377 700__ $$aDe Conti, Camila$$iINSPIRE-00537075$$uSao Paulo U.
002153377 700__ $$aDe Cuveland, Jan$$iINSPIRE-00249403$$uFrankfurt U., FIAS
002153377 700__ $$aDe Falco, Alessandro$$iINSPIRE-00080339$$uCagliari U.$$uINFN, Cagliari
002153377 700__ $$aDe Gruttola, Daniele$$iINSPIRE-00249391$$uEnrico Fermi Ctr., Rome$$uSalerno U.$$uINFN, Salerno
002153377 700__ $$aDe Marco, Nora$$iINSPIRE-00254814$$uINFN, Turin
002153377 700__ $$aDe Pasquale, Salvatore$$iINSPIRE-00114896$$uSalerno U.$$uINFN, Salerno
002153377 700__ $$aDerradi De Souza, Rafael$$iINSPIRE-00181156$$uCampinas State U.
002153377 700__ $$aDeisting, Alexander$$iINSPIRE-00507268$$uHeidelberg U.$$uDarmstadt, EMMI
002153377 700__ $$aDeloff, Andrzej$$iINSPIRE-00189124$$uWarsaw, Inst. Nucl. Studies
002153377 700__ $$aDenes, Ervin Sandor$$iINSPIRE-00076673$$uWigner RCP, Budapest
002153377 700__ $$aDeplano, Caterina$$iINSPIRE-00258120$$uNIKHEF, Amsterdam
002153377 700__ $$aDhankher, Preeti$$iINSPIRE-00531295$$uIndian Inst. Tech., Mumbai
002153377 700__ $$aDi Bari, Domenico$$iINSPIRE-00064510$$uBari U.$$uINFN, Bari
002153377 700__ $$aDi Mauro, Antonio$$iINSPIRE-00105894$$uCERN
002153377 700__ $$aDi Nezza, Pasquale$$iINSPIRE-00139137$$uFrascati
002153377 700__ $$aDi Ruzza, Benedetto$$iINSPIRE-00030649$$uINFN, Padua
002153377 700__ $$aDiaz Corchero, Miguel Angel$$iINSPIRE-00361060$$uMadrid, CIEMAT
002153377 700__ $$aDietel, Thomas$$iINSPIRE-00262178$$uCape Town U.
002153377 700__ $$aDillenseger, Pascal$$iINSPIRE-00416124$$uFrankfurt U., Inst. Kernphys.
002153377 700__ $$aDivia, Roberto$$iINSPIRE-00262189$$uCERN
002153377 700__ $$aDjuvsland, Oeystein$$iINSPIRE-00249457$$uBergen U.
002153377 700__ $$aDobrin, Alexandru Florin$$iINSPIRE-00247195$$uNIKHEF, Amsterdam$$uBucharest, Inst. Space Science
002153377 700__ $$aDomenicis Gimenez, Diogenes$$iINSPIRE-00382641$$uSao Paulo U.
002153377 700__ $$aDonigus, Benjamin$$iINSPIRE-00249342$$uFrankfurt U., Inst. Kernphys.
002153377 700__ $$aDordic, Olja$$iINSPIRE-00249337$$uOslo U.
002153377 700__ $$aDrozhzhova, Tatiana$$iINSPIRE-00364225$$uFrankfurt U., Inst. Kernphys.
002153377 700__ $$aDubey, Anand Kumar$$iINSPIRE-00241469$$uCalcutta, VECC
002153377 700__ $$aDubla, Andrea$$iINSPIRE-00361083$$uUtrecht U.
002153377 700__ $$aDucroux, Laurent$$iINSPIRE-00262200$$uLyon, IPN
002153377 700__ $$aDupieux, Pascal$$iINSPIRE-00078560$$uClermont-Ferrand U.
002153377 700__ $$aEhlers Iii, Raymond James$$iINSPIRE-00382746$$uYale U.
002153377 700__ $$aElia, Domenico$$iINSPIRE-00079305$$uINFN, Bari
002153377 700__ $$aEndress, Eric$$iINSPIRE-00527308$$uLima, Pont. U. Catolica
002153377 700__ $$aEngel, Heiko$$iINSPIRE-00246250$$uGoethe U., Frankfurt, Inst. Inform.
002153377 700__ $$aEpple, Eliane$$iINSPIRE-00476843$$uYale U.
002153377 700__ $$aErazmus, Barbara Ewa$$iINSPIRE-00183847$$uSUBATECH, Nantes
002153377 700__ $$aErdemir, Irem$$iINSPIRE-00522444$$uFrankfurt U., Inst. Kernphys.
002153377 700__ $$aErhardt, Filip$$iINSPIRE-00507377$$uZagreb U.
002153377 700__ $$aEspagnon, Bruno$$iINSPIRE-00262220$$uOrsay, IPN
002153377 700__ $$aEstienne, Magali Danielle$$iINSPIRE-00181336$$uSUBATECH, Nantes
002153377 700__ $$aEsumi, Shinichi$$iINSPIRE-00241535$$uTsukuba U.
002153377 700__ $$aEum, Jongsik$$iINSPIRE-00507489$$uPusan Natl. U.
002153377 700__ $$aEvans, David$$iINSPIRE-00162820$$uBirmingham U.
002153377 700__ $$aEvdokimov, Sergey$$iINSPIRE-00382834$$uSerpukhov, IHEP
002153377 700__ $$aEyyubova, Gyulnara$$iINSPIRE-00262232$$uPrague, Tech. U.
002153377 700__ $$aFabbietti, Laura$$iINSPIRE-00164656$$uTech. U., Munich (main)$$uMunich, Tech. U., Universe
002153377 700__ $$aFabris, Daniela$$iINSPIRE-00262240$$uINFN, Padua
002153377 700__ $$aFaivre, Julien$$iINSPIRE-00243836$$uLPSC, Grenoble
002153377 700__ $$aFantoni, Alessandra$$iINSPIRE-00139125$$uFrascati
002153377 700__ $$aFasel, Markus$$iINSPIRE-00249303$$uLBL, Berkeley
002153377 700__ $$aFeldkamp, Linus$$iINSPIRE-00361095$$uMunster U.
002153377 700__ $$aFeliciello, Alessandro$$iINSPIRE-00080709$$uINFN, Turin
002153377 700__ $$aFeofilov, Grigorii$$iINSPIRE-00243848$$uSt. Petersburg State U.
002153377 700__ $$aFerencei, Jozef$$iINSPIRE-00185039$$uRez, Nucl. Phys. Inst.
002153377 700__ $$aFernandez Tellez, Arturo$$iINSPIRE-00247175$$uPuebla U., Mexico
002153377 700__ $$aGonzalez Ferreiro, Elena$$iINSPIRE-00080969$$uSantiago de Compostela U.
002153377 700__ $$aFerretti, Alessandro$$iINSPIRE-00033003$$uTurin U.$$uINFN, Turin
002153377 700__ $$aFestanti, Andrea$$iINSPIRE-00361107$$uPadua U.$$uINFN, Padua
002153377 700__ $$aFeuillard, Victor Jose Gaston$$iINSPIRE-00522324$$uIRFU, Saclay$$uClermont-Ferrand U.
002153377 700__ $$aFigiel, Jan$$iINSPIRE-00172410$$uCracow, INP
002153377 700__ $$aAraujo Silva Figueredo, Marcel$$iINSPIRE-00249268$$uLiverpool U.$$uSao Paulo U.
002153377 700__ $$aFilchagin, Sergey$$iINSPIRE-00249256$$uRFNC-VNIIEF, Sarov
002153377 700__ $$aFinogeev, Dmitry$$iINSPIRE-00262286$$uMoscow, INR
002153377 700__ $$aFionda, Fiorella$$iINSPIRE-00249244$$uCagliari U.$$uINFN, Cagliari
002153377 700__ $$aFiore, Enrichetta Maria$$iINSPIRE-00262299$$uBari U.$$uINFN, Bari
002153377 700__ $$aFleck, Martin Gabriel$$iINSPIRE-00522825$$uHeidelberg U.
002153377 700__ $$aFloris, Michele$$iINSPIRE-00262309$$uCERN
002153377 700__ $$aFoertsch, Siegfried Valentin$$iINSPIRE-00249232$$uiThemba LABS
002153377 700__ $$aFoka, Panagiota$$iINSPIRE-00250159$$uDarmstadt, EMMI
002153377 700__ $$aFokin, Sergey$$iINSPIRE-00241560$$uKurchatov Inst., Moscow
002153377 700__ $$aFragiacomo, Enrico$$iINSPIRE-00250163$$uINFN, Trieste
002153377 700__ $$aFrancescon, Andrea$$iINSPIRE-00361119$$uCERN
002153377 700__ $$aFrancisco, Audrey$$iINSPIRE-00564016$$uSUBATECH, Nantes
002153377 700__ $$aFrankenfeld, Ulrich Michael$$iINSPIRE-00249193$$uDarmstadt, EMMI
002153377 700__ $$aFronze, Gabriele Gaetano$$iINSPIRE-00548353$$uTurin U.$$uINFN, Turin
002153377 700__ $$aFuchs, Ulrich$$iINSPIRE-00289521$$uCERN
002153377 700__ $$aFurget, Christophe$$iINSPIRE-00179002$$uLPSC, Grenoble
002153377 700__ $$aFurs, Artur$$iINSPIRE-00419390$$uMoscow, INR
002153377 700__ $$aFusco Girard, Mario$$iINSPIRE-00249181$$uSalerno U.$$uINFN, Salerno
002153377 700__ $$aGaardhoeje, Jens Joergen$$iINSPIRE-00243865$$uBohr Inst.
002153377 700__ $$aGagliardi, Martino$$iINSPIRE-00247151$$uTurin U.$$uINFN, Turin
002153377 700__ $$aGago Medina, Alberto Martin$$iINSPIRE-00083116$$uLima, Pont. U. Catolica
002153377 700__ $$aGajdosova, Katarina$$iINSPIRE-00538159$$uBohr Inst.
002153377 700__ $$aGallio, Mauro$$iINSPIRE-00250190$$uTurin U.$$uINFN, Turin
002153377 700__ $$aDuarte Galvan, Carlos$$iINSPIRE-00563971$$uSinaloa U.
002153377 700__ $$aGangadharan, Dhevan Raja$$iINSPIRE-00181636$$uLBL, Berkeley
002153377 700__ $$aGanoti, Paraskevi$$iINSPIRE-00249171$$uAthens U.
002153377 700__ $$aGao, Chaosong$$iINSPIRE-00419488$$uHua-Zhong Normal U.
002153377 700__ $$aGarabatos Cuadrado, Jose$$iINSPIRE-00247140$$uDarmstadt, EMMI
002153377 700__ $$aGarcia-Solis, Edmundo Javier$$iINSPIRE-00319408$$uChicago State U.
002153377 700__ $$aGargiulo, Corrado$$iINSPIRE-00304950$$uCERN
002153377 700__ $$aGasik, Piotr Jan$$iINSPIRE-00386209$$uTech. U., Munich (main)$$uMunich, Tech. U., Universe
002153377 700__ $$aGauger, Erin Frances$$iINSPIRE-00531301$$uTexas U.
002153377 700__ $$aGermain, Marie$$iINSPIRE-00046404$$uSUBATECH, Nantes
002153377 700__ $$aGheata, Mihaela$$iINSPIRE-00249146$$uCERN$$uBucharest, Inst. Space Science
002153377 700__ $$aGhosh, Premomoy$$iINSPIRE-00181669$$uCalcutta, VECC
002153377 700__ $$aGhosh, Sanjay Kumar$$iINSPIRE-00385559$$uBose Inst., Kolkata$$uCAPSS, Kolkata
002153377 700__ $$aGianotti, Paola$$iINSPIRE-00084690$$uFrascati
002153377 700__ $$aGiubellino, Paolo$$iINSPIRE-00085080$$uINFN, Turin$$uCERN
002153377 700__ $$aGiubilato, Piero$$iINSPIRE-00017284$$uPadua U.$$uINFN, Padua
002153377 700__ $$aGladysz-Dziadus, Ewa$$iINSPIRE-00250209$$uCracow, INP
002153377 700__ $$aGlassel, Peter$$iINSPIRE-00262357$$uHeidelberg U.
002153377 700__ $$aGomez Coral, Diego Mauricio$$iINSPIRE-00531313$$uMexico U.
002153377 700__ $$aGomez Ramirez, Andres$$iINSPIRE-00416173$$uGoethe U., Frankfurt, Inst. Inform.
002153377 700__ $$aSanchez Gonzalez, Andres$$iINSPIRE-00560286$$uCERN
002153377 700__ $$aGonzalez, Victor$$iINSPIRE-00537090$$uMadrid, CIEMAT
002153377 700__ $$aGonzalez Zamora, Pedro$$iINSPIRE-00249119$$uMadrid, CIEMAT
002153377 700__ $$aGorbunov, Sergey$$iINSPIRE-00262379$$uFrankfurt U., FIAS
002153377 700__ $$aGorlich, Lidia Maria$$iINSPIRE-00185075$$uCracow, INP
002153377 700__ $$aGotovac, Sven$$iINSPIRE-00249102$$uSplit Tech. U.
002153377 700__ $$aGrabski, Varlen$$iINSPIRE-00086274$$uMexico U.
002153377 700__ $$aGrachov, Oleg Anatolievich$$iINSPIRE-00059999$$uYale U.
002153377 700__ $$aGraczykowski, Lukasz Kamil$$iINSPIRE-00245450$$uWarsaw U. of Tech.
002153377 700__ $$aGraham, Katie Leanne$$iINSPIRE-00522271$$uBirmingham U.
002153377 700__ $$aGrelli, Alessandro$$iINSPIRE-00247138$$uUtrecht U.
002153377 700__ $$aGrigoras, Alina Gabriela$$iINSPIRE-00249077$$uCERN
002153377 700__ $$aGrigoras, Costin$$iINSPIRE-00249065$$uCERN
002153377 700__ $$aGrigoryev, Vladislav$$iINSPIRE-00262389$$uMoscow Phys. Eng. Inst.
002153377 700__ $$aGrigoryan, Ara$$iINSPIRE-00249053$$uYerevan Phys. Inst.
002153377 700__ $$aGrigoryan, Smbat$$iINSPIRE-00262398$$uDubna, JINR
002153377 700__ $$aGrynyov, Borys$$iINSPIRE-00245887$$uBITP, Kiev
002153377 700__ $$aGrion, Nevio$$iINSPIRE-00262401$$uINFN, Trieste
002153377 700__ $$aGronefeld, Julius Maximilian$$iINSPIRE-00537113$$uDarmstadt, EMMI
002153377 700__ $$aGrosa, Fabrizio$$uTurin U.$$uINFN, Turin
002153377 700__ $$aGrosse-Oetringhaus, Jan Fiete$$iINSPIRE-00247126$$uCERN
002153377 700__ $$aGrosso, Raffaele$$iINSPIRE-00262426$$uDarmstadt, EMMI
002153377 700__ $$aGruber, Lukas$$iINSPIRE-00296124$$uStefan Meyer Inst. Subatomare Phys.
002153377 700__ $$aGuber, Fedor$$iINSPIRE-00262430$$uMoscow, INR
002153377 700__ $$aGuernane, Rachid$$iINSPIRE-00262443$$uLPSC, Grenoble
002153377 700__ $$aGuerzoni, Barbara$$iINSPIRE-00249016$$uBologna U.$$uINFN, Bologna
002153377 700__ $$aGulbrandsen, Kristjan Herlache$$iINSPIRE-00039494$$uBohr Inst.
002153377 700__ $$aGunji, Taku$$iINSPIRE-00033137$$uTokyo U.
002153377 700__ $$aGupta, Anik$$iINSPIRE-00181730$$uJammu U.
002153377 700__ $$aGupta, Ramni$$iINSPIRE-00254573$$uJammu U.
002153377 700__ $$aHaake, Rudiger$$iINSPIRE-00382877$$uMunster U.$$uCERN
002153377 700__ $$aHadjidakis, Cynthia Marie$$iINSPIRE-00244486$$uOrsay, IPN
002153377 700__ $$aHaiduc, Maria$$iINSPIRE-00250275$$uBucharest, Inst. Space Science
002153377 700__ $$aHamagaki, Hideki$$iINSPIRE-00088248$$uTokyo U.
002153377 700__ $$aHamar, Gergoe$$iINSPIRE-00262460$$uWigner RCP, Budapest
002153377 700__ $$aHamon, Julien Charles$$iINSPIRE-00548368$$uStrasbourg, IPHC
002153377 700__ $$aHarris, John William$$iINSPIRE-00301628$$uYale U.
002153377 700__ $$aHarton, Austin Vincent$$iINSPIRE-00245718$$uChicago State U.
002153377 700__ $$aHatzifotiadou, Despina$$iINSPIRE-00244493$$uINFN, Bologna
002153377 700__ $$aHayashi, Shinichi$$iINSPIRE-00361149$$uTokyo U.
002153377 700__ $$aHeckel, Stefan Thomas$$iINSPIRE-00245584$$uFrankfurt U., Inst. Kernphys.
002153377 700__ $$aHellbar, Ernst$$iINSPIRE-00560290$$uFrankfurt U., Inst. Kernphys.
002153377 700__ $$aHelstrup, Haavard$$iINSPIRE-00089682$$uBergen Coll. Higher Educ.
002153377 700__ $$aHerghelegiu, Andrei Ionut$$iINSPIRE-00248972$$uBucharest, IFIN-HH
002153377 700__ $$aHerrera Corral, Gerardo Antonio$$iINSPIRE-00089895$$uCINVESTAV, IPN
002153377 700__ $$aHess, Benjamin Andreas$$iINSPIRE-00361150$$uTubingen U.
002153377 700__ $$aHetland, Kristin Fanebust$$iINSPIRE-00080364$$uBergen Coll. Higher Educ.
002153377 700__ $$aHillemanns, Hartmut$$iINSPIRE-00507591$$uCERN
002153377 700__ $$aHippolyte, Boris$$iINSPIRE-00262496$$uStrasbourg, IPHC
002153377 700__ $$aHorak, David$$iINSPIRE-00548374$$uPrague, Tech. U.
002153377 700__ $$aHosokawa, Ritsuya$$iINSPIRE-00522280$$uTsukuba U.
002153377 700__ $$aHristov, Peter Zahariev$$iINSPIRE-00091290$$uCERN
002153377 700__ $$aHughes, Charles$$iINSPIRE-00564077$$uTennessee U.
002153377 700__ $$aHumanic, Thomas$$iINSPIRE-00091603$$uOhio State U.
002153377 700__ $$aHussain, Nur$$iINSPIRE-00416277$$uGauhati U.
002153377 700__ $$aHussain, Tahir$$iINSPIRE-00507708$$uAligarh Muslim U.
002153377 700__ $$aHutter, Dirk$$iINSPIRE-00382970$$uFrankfurt U., FIAS
002153377 700__ $$aHwang, Dae Sung$$iINSPIRE-00091772$$uSejong U.
002153377 700__ $$aIlkaev, Radiy$$iINSPIRE-00248935$$uRFNC-VNIIEF, Sarov
002153377 700__ $$aInaba, Motoi$$iINSPIRE-00241821$$uTsukuba U.
002153377 700__ $$aIncani, Elisa$$iINSPIRE-00246059$$uCagliari U.$$uINFN, Cagliari
002153377 700__ $$aIppolitov, Mikhail$$iINSPIRE-00250300$$uMoscow Phys. Eng. Inst.$$uKurchatov Inst., Moscow
002153377 700__ $$aIrfan, Muhammad$$iINSPIRE-00248911$$uAligarh Muslim U.
002153377 700__ $$aIsakov, Vladimir$$iINSPIRE-00564085$$uMoscow, INR
002153377 700__ $$aIvanov, Marian$$iINSPIRE-00262538$$uDarmstadt, EMMI$$uCERN
002153377 700__ $$aIvanov, Vladimir$$iINSPIRE-00262542$$uSt. Petersburg, INP
002153377 700__ $$aIzucheev, Vladimir$$iINSPIRE-00506818$$uSerpukhov, IHEP
002153377 700__ $$aJacak, Barbara$$iINSPIRE-00155696$$uLBL, Berkeley
002153377 700__ $$aJacazio, Nicolo$$iINSPIRE-00548380$$uBologna U.$$uINFN, Bologna
002153377 700__ $$aJacobs, Peter Martin$$iINSPIRE-00181871$$uLBL, Berkeley
002153377 700__ $$aJadhav, Manoj Bhanudas$$iINSPIRE-00531323$$uIndian Inst. Tech., Mumbai
002153377 700__ $$aJadlovska, Slavka$$iINSPIRE-00522452$$uKosice Tech. U.
002153377 700__ $$aJadlovsky, Jan$$iINSPIRE-00537120$$uKosice Tech. U.$$uKosice, IEF
002153377 700__ $$aJahnke, Cristiane$$iINSPIRE-00383021$$uSao Paulo U.
002153377 700__ $$aJakubowska, Monika Joanna$$iINSPIRE-00537133$$uWarsaw U. of Tech.
002153377 700__ $$aJanik, Malgorzata Anna$$iINSPIRE-00244548$$uWarsaw U. of Tech.
002153377 700__ $$aPahula Hewage, Sandun$$iINSPIRE-00246609$$uHouston U.
002153377 700__ $$aJena, Chitrasen$$iINSPIRE-00181905$$uPadua U.$$uINFN, Padua
002153377 700__ $$aJena, Satyajit$$iINSPIRE-00248878$$uHouston U.
002153377 700__ $$aJimenez Bustamante, Raul Tonatiuh$$iINSPIRE-00355862$$uDarmstadt, EMMI
002153377 700__ $$aJones, Peter Graham$$iINSPIRE-00181937$$uBirmingham U.
002153377 700__ $$aJusko, Anton$$iINSPIRE-00250331$$uBirmingham U.
002153377 700__ $$aKalinak, Peter$$iINSPIRE-00247100$$uKosice, IEF
002153377 700__ $$aKalweit, Alexander Philipp$$iINSPIRE-00248849$$uCERN
002153377 700__ $$aKang, Ju Hwan$$iINSPIRE-00241999$$uYonsei U.
002153377 700__ $$aKaplin, Vladimir$$iINSPIRE-00248837$$uMoscow Phys. Eng. Inst.
002153377 700__ $$aKar, Somnath$$iINSPIRE-00383167$$uCalcutta, VECC
002153377 700__ $$aKarasu Uysal, Ayben$$iINSPIRE-00245978$$uKaratay U.
002153377 700__ $$aKaravichev, Oleg$$iINSPIRE-00262581$$uMoscow, INR
002153377 700__ $$aKaravicheva, Tatiana$$iINSPIRE-00262593$$uMoscow, INR
002153377 700__ $$aKarayan, Lilit$$iINSPIRE-00522297$$uHeidelberg U.$$uDarmstadt, EMMI
002153377 700__ $$aKarpechev, Evgeny$$iINSPIRE-00248813$$uMoscow, INR
002153377 700__ $$aKebschull, Udo Wolfgang$$iINSPIRE-00248807$$uGoethe U., Frankfurt, Inst. Inform.
002153377 700__ $$aKeidel, Ralf$$iINSPIRE-00248795$$uFachhochsch., Worms
002153377 700__ $$aKeijdener, Darius Laurens$$iINSPIRE-00416339$$uUtrecht U.
002153377 700__ $$aKeil, Markus$$iINSPIRE-00216636$$uCERN
002153377 700__ $$aKhan, Mohammed Mohisin$$iINSPIRE-00244581$$uAligarh Muslim U.
002153377 700__ $$aKhan, Palash$$iINSPIRE-00289764$$uSaha Inst.
002153377 700__ $$aKhan, Shuaib Ahmad$$iINSPIRE-00243963$$uCalcutta, VECC
002153377 700__ $$aKhanzadeev, Alexei$$iINSPIRE-00242036$$uSt. Petersburg, INP
002153377 700__ $$aKharlov, Yury$$iINSPIRE-00095925$$uSerpukhov, IHEP
002153377 700__ $$aKhatun, Anisa$$iINSPIRE-00564120$$uAligarh Muslim U.
002153377 700__ $$aKileng, Bjarte$$iINSPIRE-00262606$$uBergen Coll. Higher Educ.
002153377 700__ $$aKim, Do Won$$iINSPIRE-00188519$$uGangneung-Wonju Natl. U.
002153377 700__ $$aKim, Dong Jo$$iINSPIRE-00242076$$uJyvaskyla U.
002153377 700__ $$aKim, Daehyeok$$iINSPIRE-00548392$$uYonsei U.
002153377 700__ $$aKim, Hyeonjoong$$iINSPIRE-00410042$$uYonsei U.
002153377 700__ $$aKim, Jinsook$$iINSPIRE-00243973$$uGangneung-Wonju Natl. U.
002153377 700__ $$aKim, Jiyoung$$iINSPIRE-00564110$$uHeidelberg U.
002153377 700__ $$aKim, Minwoo$$iINSPIRE-00262636$$uYonsei U.
002153377 700__ $$aKim, Se Yong$$iINSPIRE-00254770$$uSejong U.
002153377 700__ $$aKim, Taesoo$$iINSPIRE-00361198$$uYonsei U.
002153377 700__ $$aKirsch, Stefan$$iINSPIRE-00250347$$uFrankfurt U., FIAS
002153377 700__ $$aKisel, Ivan$$iINSPIRE-00262045$$uFrankfurt U., FIAS
002153377 700__ $$aKiselev, Sergey$$iINSPIRE-00262051$$uMoscow, ITEP
002153377 700__ $$aKisiel, Adam Ryszard$$iINSPIRE-00182054$$uWarsaw U. of Tech.
002153377 700__ $$aKiss, Gabor$$iINSPIRE-00386128$$uWigner RCP, Budapest
002153377 700__ $$aKlay, Jennifer Lynn$$iINSPIRE-00050656$$uCal. Poly.
002153377 700__ $$aKlein, Carsten$$iINSPIRE-00506923$$uFrankfurt U., Inst. Kernphys.
002153377 700__ $$aKlein, Jochen$$iINSPIRE-00262064$$uCERN
002153377 700__ $$aKlein-Boesing, Christian$$iINSPIRE-00003561$$uMunster U.
002153377 700__ $$aKlewin, Sebastian$$iINSPIRE-00537149$$uHeidelberg U.
002153377 700__ $$aKluge, Alexander$$iINSPIRE-00250353$$uCERN
002153377 700__ $$aKnichel, Michael Linus$$iINSPIRE-00245547$$uHeidelberg U.
002153377 700__ $$aKnospe, Anders Garritt$$iINSPIRE-00182064$$uTexas U.$$uHouston U.
002153377 700__ $$aKobdaj, Chinorat$$iINSPIRE-00227795$$uSuranaree U. of Tech.
002153377 700__ $$aKofarago, Monika$$iINSPIRE-00410392$$uCERN
002153377 700__ $$aKollegger, Thorsten$$iINSPIRE-00182076$$uDarmstadt, EMMI
002153377 700__ $$aKolozhvari, Anatoly$$iINSPIRE-00244610$$uSt. Petersburg State U.
002153377 700__ $$aKondratev, Valerii$$iINSPIRE-00248784$$uSt. Petersburg State U.
002153377 700__ $$aKondratyeva, Natalia$$iINSPIRE-00262112$$uMoscow Phys. Eng. Inst.
002153377 700__ $$aKondratyuk, Evgeny$$iINSPIRE-00507275$$uSerpukhov, IHEP
002153377 700__ $$aKonevskikh, Artem$$iINSPIRE-00248772$$uMoscow, INR
002153377 700__ $$aKopcik, Michal$$iINSPIRE-00522467$$uKosice Tech. U.
002153377 700__ $$aKour, Mandeep$$iINSPIRE-00522474$$uJammu U.
002153377 700__ $$aKouzinopoulos, Charalampos$$iINSPIRE-00507396$$uCERN
002153377 700__ $$aKovalenko, Oleksandr$$iINSPIRE-00507510$$uWarsaw, Inst. Nucl. Studies
002153377 700__ $$aKovalenko, Vladimir$$iINSPIRE-00361228$$uSt. Petersburg State U.
002153377 700__ $$aKowalski, Marek$$iINSPIRE-00262137$$uCracow, INP
002153377 700__ $$aKoyithatta Meethaleveedu, Greeshma$$iINSPIRE-00245600$$uIndian Inst. Tech., Mumbai
002153377 700__ $$aKralik, Ivan$$iINSPIRE-00098249$$uKosice, IEF
002153377 700__ $$aKravcakova, Adela$$iINSPIRE-00248740$$uKosice U.
002153377 700__ $$aKrivda, Marian$$iINSPIRE-00248727$$uKosice, IEF$$uBirmingham U.
002153377 700__ $$aKrizek, Filip$$iINSPIRE-00262142$$uRez, Nucl. Phys. Inst.
002153377 700__ $$aKryshen, Evgeny$$iINSPIRE-00262643$$uSt. Petersburg, INP$$uCERN
002153377 700__ $$aKrzewicki, Mikolaj$$iINSPIRE-00248715$$uFrankfurt U., FIAS
002153377 700__ $$aKubera, Andrew Michael$$iINSPIRE-00507630$$uOhio State U.
002153377 700__ $$aKucera, Vit$$iINSPIRE-00383170$$uRez, Nucl. Phys. Inst.
002153377 700__ $$aKuhn, Christian Claude$$iINSPIRE-00244002$$uStrasbourg, IPHC
002153377 700__ $$aKuijer, Paulus Gerardus$$iINSPIRE-00098956$$uNIKHEF, Amsterdam
002153377 700__ $$aKumar, Ajay$$iINSPIRE-00522302$$uJammu U.
002153377 700__ $$aKumar, Jitendra$$iINSPIRE-00361265$$uIndian Inst. Tech., Mumbai
002153377 700__ $$aKumar, Lokesh$$iINSPIRE-00182175$$uPanjab U.
002153377 700__ $$aKumar, Shyam$$iINSPIRE-00531331$$uIndian Inst. Tech., Mumbai
002153377 700__ $$aKurashvili, Podist$$iINSPIRE-00247073$$uWarsaw, Inst. Nucl. Studies
002153377 700__ $$aKurepin, Alexander$$iINSPIRE-00244630$$uMoscow, INR
002153377 700__ $$aKurepin, Alexey$$iINSPIRE-00244643$$uMoscow, INR
002153377 700__ $$aKuryakin, Alexey$$iINSPIRE-00248681$$uRFNC-VNIIEF, Sarov
002153377 700__ $$aKweon, Min Jung$$iINSPIRE-00242248$$uInha U.
002153377 700__ $$aKwon, Youngil$$iINSPIRE-00242258$$uYonsei U.
002153377 700__ $$aLa Pointe, Sarah Louise$$iINSPIRE-00182214$$uFrankfurt U., FIAS$$uINFN, Turin
002153377 700__ $$aLa Rocca, Paola$$iINSPIRE-00247061$$uCatania U.$$uINFN, Catania
002153377 700__ $$aLadron De Guevara, Pedro$$iINSPIRE-00250250$$uCINVESTAV, IPN
002153377 700__ $$aLagana Fernandes, Caio$$iINSPIRE-00205674$$uSao Paulo U.
002153377 700__ $$aLakomov, Igor$$iINSPIRE-00289795$$uCERN
002153377 700__ $$aLangoy, Rune$$iINSPIRE-00361289$$uVestfold U. Coll., Tonsberg
002153377 700__ $$aLapidus, Kirill$$iINSPIRE-00560319$$uMunich, Tech. U., Universe$$uYale U.
002153377 700__ $$aLara Martinez, Camilo Ernesto$$iINSPIRE-00244024$$uGoethe U., Frankfurt, Inst. Inform.
002153377 700__ $$aLardeux, Antoine Xavier$$iINSPIRE-00262675$$uIRFU, Saclay
002153377 700__ $$aLattuca, Alessandra$$iINSPIRE-00383220$$uTurin U.$$uINFN, Turin
002153377 700__ $$aLaudi, Elisa$$iINSPIRE-00506820$$uCERN
002153377 700__ $$aLea, Ramona$$iINSPIRE-00244658$$uTrieste U.$$uINFN, Trieste
002153377 700__ $$aLeardini, Lucia$$iINSPIRE-00416390$$uHeidelberg U.
002153377 700__ $$aLee, Seongjoo$$iINSPIRE-00506940$$uYonsei U.
002153377 700__ $$aLehas, Fatiha$$iINSPIRE-00522311$$uNIKHEF, Amsterdam
002153377 700__ $$aLehner, Sebastian$$iINSPIRE-00560343$$uStefan Meyer Inst. Subatomare Phys.
002153377 700__ $$aLemmon, Roy Crawford$$iINSPIRE-00385690$$uDaresbury
002153377 700__ $$aLenti, Vito$$iINSPIRE-00101126$$uINFN, Bari
002153377 700__ $$aLeogrande, Emilia$$iINSPIRE-00416444$$uUtrecht U.
002153377 700__ $$aLeon Monzon, Ildefonso$$iINSPIRE-00248605$$uSinaloa U.
002153377 700__ $$aLeon Vargas, Hermes$$iINSPIRE-00248593$$uMexico U.
002153377 700__ $$aLeoncino, Marco$$iINSPIRE-00246248$$uTurin U.$$uINFN, Turin
002153377 700__ $$aLevai, Peter$$iINSPIRE-00162508$$uWigner RCP, Budapest
002153377 700__ $$aLi, Shuang$$iINSPIRE-00383233$$uHua-Zhong Normal U.$$uClermont-Ferrand U.
002153377 700__ $$aLi, Xiaomei$$iINSPIRE-00242399$$uBeijing, Inst. Atomic Energy
002153377 700__ $$aLien, Jorgen Andre$$iINSPIRE-00101774$$uVestfold U. Coll., Tonsberg
002153377 700__ $$aLietava, Roman$$iINSPIRE-00206588$$uBirmingham U.
002153377 700__ $$aLindal, Svein$$iINSPIRE-00262704$$uOslo U.
002153377 700__ $$aLindenstruth, Volker$$iINSPIRE-00171460$$uFrankfurt U., FIAS
002153377 700__ $$aLippmann, Christian$$iINSPIRE-00247046$$uDarmstadt, EMMI
002153377 700__ $$aLisa, Michael Annan$$iINSPIRE-00182345$$uOhio State U.
002153377 700__ $$aLjunggren, Hans Martin$$iINSPIRE-00361314$$uLund U.
002153377 700__ $$aLodato, Davide Francesco$$iINSPIRE-00383301$$uUtrecht U.
002153377 700__ $$aLonne, Per-Ivar$$iINSPIRE-00262720$$uBergen U.
002153377 700__ $$aLoginov, Vitaly$$iINSPIRE-00262733$$uMoscow Phys. Eng. Inst.
002153377 700__ $$aLoizides, Constantinos$$iINSPIRE-00052306$$uLBL, Berkeley
002153377 700__ $$aLopez, Xavier Bernard$$iINSPIRE-00244058$$uClermont-Ferrand U.
002153377 700__ $$aLopez Torres, Ernesto$$iINSPIRE-00248566$$uHavana, CEADEN
002153377 700__ $$aLowe, Andrew John$$iINSPIRE-00219444$$uWigner RCP, Budapest
002153377 700__ $$aLuettig, Philipp Johannes$$iINSPIRE-00246111$$uFrankfurt U., Inst. Kernphys.
002153377 700__ $$aLunardon, Marcello$$iINSPIRE-00289820$$uPadua U.$$uINFN, Padua
002153377 700__ $$aLuparello, Grazia$$iINSPIRE-00248554$$uTrieste U.$$uINFN, Trieste
002153377 700__ $$aLupi, Matteo$$iINSPIRE-00564238$$uCERN
002153377 700__ $$aLutz, Tyler Harrison$$iINSPIRE-00548403$$uYale U.
002153377 700__ $$aMaevskaya, Alla$$iINSPIRE-00248542$$uMoscow, INR
002153377 700__ $$aMager, Magnus$$iINSPIRE-00248536$$uCERN
002153377 700__ $$aMahajan, Sanjay$$iINSPIRE-00244673$$uJammu U.
002153377 700__ $$aMahmood, Sohail Musa$$iINSPIRE-00416518$$uOslo U.
002153377 700__ $$aMaire, Antonin$$iINSPIRE-00248522$$uStrasbourg, IPHC
002153377 700__ $$aMajka, Richard Daniel$$iINSPIRE-00182435$$uYale U.
002153377 700__ $$aMalaev, Mikhail$$iINSPIRE-00247010$$uSt. Petersburg, INP
002153377 700__ $$aMaldonado Cervantes, Ivonne Alicia$$iINSPIRE-00248497$$uMexico U., ICN
002153377 700__ $$aMalinina, Liudmila$$iINSPIRE-00361332$$uSINP, Moscow$$uDubna, JINR
002153377 700__ $$aMal'Kevich, Dmitry$$iINSPIRE-00289856$$uMoscow, ITEP
002153377 700__ $$aMalzacher, Peter$$iINSPIRE-00248471$$uDarmstadt, EMMI
002153377 700__ $$aMamonov, Alexander$$iINSPIRE-00247009$$uRFNC-VNIIEF, Sarov
002153377 700__ $$aManko, Vladislav$$iINSPIRE-00242429$$uKurchatov Inst., Moscow
002153377 700__ $$aManso, Franck$$iINSPIRE-00250406$$uClermont-Ferrand U.
002153377 700__ $$aManzari, Vito$$iINSPIRE-00104539$$uCERN$$uINFN, Bari
002153377 700__ $$aMao, Yaxian$$iINSPIRE-00261802$$uHua-Zhong Normal U.
002153377 700__ $$aMarchisone, Massimiliano$$iINSPIRE-00245991$$uiThemba LABS$$uWitwatersrand U.$$uTurin U.$$uINFN, Turin
002153377 700__ $$aMares, Jiri$$iINSPIRE-00289864$$uPrague, Inst. Phys.
002153377 700__ $$aMargagliotti, Giacomo Vito$$iINSPIRE-00104694$$uTrieste U.$$uINFN, Trieste
002153377 700__ $$aMargotti, Anselmo$$iINSPIRE-00172043$$uINFN, Bologna
002153377 700__ $$aMargutti, Jacopo$$iINSPIRE-00507060$$uUtrecht U.
002153377 700__ $$aMarin, Ana Maria$$iINSPIRE-00244688$$uDarmstadt, EMMI
002153377 700__ $$aMarkert, Christina$$iINSPIRE-00104805$$uTexas U.
002153377 700__ $$aMarquard, Marco$$iINSPIRE-00361344$$uFrankfurt U., Inst. Kernphys.
002153377 700__ $$aMartin, Nicole Alice$$iINSPIRE-00361356$$uDarmstadt, EMMI
002153377 700__ $$aMartinengo, Paolo$$iINSPIRE-00254826$$uCERN
002153377 700__ $$aMartinez Hernandez, Mario Ivan$$iINSPIRE-00300172$$uPuebla U., Mexico
002153377 700__ $$aMartinez-Garcia, Gines$$iINSPIRE-00105190$$uSUBATECH, Nantes
002153377 700__ $$aMartinez Pedreira, Miguel$$iINSPIRE-00507190$$uCERN
002153377 700__ $$aMas, Alexis Jean-Michel$$iINSPIRE-00245930$$uSao Paulo U.
002153377 700__ $$aMasciocchi, Silvia$$iINSPIRE-00272436$$uDarmstadt, EMMI
002153377 700__ $$aMasera, Massimo$$iINSPIRE-00105418$$uTurin U.$$uINFN, Turin
002153377 700__ $$aMasoni, Alberto$$iINSPIRE-00289880$$uINFN, Cagliari
002153377 700__ $$aMastroserio, Annalisa$$iINSPIRE-00248428$$uBari U.$$uINFN, Bari
002153377 700__ $$aMatyja, Adam Tomasz$$iINSPIRE-00244090$$uCracow, INP
002153377 700__ $$aMayer, Christoph$$iINSPIRE-00361368$$uCracow, INP
002153377 700__ $$aMazer, Joel Anthony$$iINSPIRE-00361370$$uTennessee U.
002153377 700__ $$aMazzoni, Alessandra Maria$$iINSPIRE-00106051$$uINFN, Rome
002153377 700__ $$aMcdonald, Daniel$$iINSPIRE-00385767$$uHouston U.
002153377 700__ $$aMeddi, Franco$$iINSPIRE-00250415$$uRome U.$$uINFN, Rome
002153377 700__ $$aMelikyan, Yuri$$iINSPIRE-00531341$$uMoscow Phys. Eng. Inst.
002153377 700__ $$aMenchaca-Rocha, Arturo Alejandro$$iINSPIRE-00244703$$uMexico U.
002153377 700__ $$aMeninno, Elisa$$iINSPIRE-00507326$$uSalerno U.$$uINFN, Salerno
002153377 700__ $$aMercado-Perez, Jorge$$iINSPIRE-00289899$$uHeidelberg U.
002153377 700__ $$aMeres, Michal$$iINSPIRE-00245096$$uComenius U.
002153377 700__ $$aMhlanga, Sibaliso$$iINSPIRE-00564240$$uCape Town U.
002153377 700__ $$aMiake, Yasuo$$iINSPIRE-00242486$$uTsukuba U.
002153377 700__ $$aMieskolainen, Matti Mikael$$iINSPIRE-00507452$$uHelsinki Inst. of Phys.
002153377 700__ $$aMikhaylov, Konstantin$$iINSPIRE-00245462$$uMoscow, ITEP$$uDubna, JINR
002153377 700__ $$aMilano, Leonardo$$iINSPIRE-00254899$$uLBL, Berkeley$$uCERN
002153377 700__ $$aMilosevic, Jovan$$iINSPIRE-00191774$$uOslo U.
002153377 700__ $$aMischke, Andre$$iINSPIRE-00182548$$uUtrecht U.
002153377 700__ $$aMishra, Aditya Nath$$iINSPIRE-00361381$$uIndian Inst. Tech., Indore
002153377 700__ $$aMiskowiec, Dariusz Czeslaw$$iINSPIRE-00108019$$uDarmstadt, EMMI
002153377 700__ $$aMitra, Jubin$$iINSPIRE-00416586$$uCalcutta, VECC
002153377 700__ $$aMitu, Ciprian Mihai$$iINSPIRE-00248369$$uBucharest, Inst. Space Science
002153377 700__ $$aMohammadi, Naghmeh$$iINSPIRE-00416653$$uUtrecht U.
002153377 700__ $$aMohanty, Bedangadas$$iINSPIRE-00146508$$uBhubaneswar, NISER
002153377 700__ $$aMohler, Christian$$uHeidelberg U.
002153377 700__ $$aMolnar, Levente$$iINSPIRE-00254710$$uStrasbourg, IPHC
002153377 700__ $$aMontano Zetina, Luis Manuel$$iINSPIRE-00289907$$uCINVESTAV, IPN
002153377 700__ $$aMontes Prado, Esther$$iINSPIRE-00248345$$uMadrid, CIEMAT
002153377 700__ $$aMoreira De Godoy, Denise Aparecida$$iINSPIRE-00245954$$uMunster U.
002153377 700__ $$aPerez Moreno, Luis Alberto$$iINSPIRE-00531356$$uPuebla U., Mexico
002153377 700__ $$aMoretto, Sandra$$iINSPIRE-00289922$$uPadua U.$$uINFN, Padua
002153377 700__ $$aMorreale, Astrid$$iINSPIRE-00142798$$uSUBATECH, Nantes
002153377 700__ $$aMorsch, Andreas$$iINSPIRE-00289930$$uCERN
002153377 700__ $$aMuccifora, Valeria$$iINSPIRE-00139164$$uFrascati
002153377 700__ $$aMudnic, Eugen$$iINSPIRE-00248333$$uSplit Tech. U.
002153377 700__ $$aMuhlheim, Daniel Michael$$iINSPIRE-00416728$$uMunster U.
002153377 700__ $$aMuhuri, Sanjib$$iINSPIRE-00248321$$uCalcutta, VECC
002153377 700__ $$aMukherjee, Maitreyee$$iINSPIRE-00361435$$uCalcutta, VECC
002153377 700__ $$aMulligan, James Declan$$iINSPIRE-00507724$$uYale U.
002153377 700__ $$aGameiro Munhoz, Marcelo$$iINSPIRE-00182574$$uSao Paulo U.
002153377 700__ $$aMunning, Konstantin$$iINSPIRE-00564280$$uBonn U., HISKP
002153377 700__ $$aMunzer, Robert Helmut$$iINSPIRE-00531366$$uTech. U., Munich (main)$$uMunich, Tech. U., Universe$$uFrankfurt U., Inst. Kernphys.
002153377 700__ $$aMurakami, Hikari$$iINSPIRE-00548414$$uTokyo U.
002153377 700__ $$aMurray, Sean$$iINSPIRE-00383510$$uiThemba LABS
002153377 700__ $$aMusa, Luciano$$iINSPIRE-00250444$$uCERN
002153377 700__ $$aMusinsky, Jan$$iINSPIRE-00385520$$uKosice, IEF
002153377 700__ $$aNaik, Bharati$$iINSPIRE-00531375$$uIndian Inst. Tech., Mumbai
002153377 700__ $$aNair, Rahul$$iINSPIRE-00531380$$uWarsaw, Inst. Nucl. Studies
002153377 700__ $$aNandi, Basanta Kumar$$iINSPIRE-00182588$$uIndian Inst. Tech., Mumbai
002153377 700__ $$aNania, Rosario$$iINSPIRE-00172055$$uINFN, Bologna
002153377 700__ $$aNappi, Eugenio$$iINSPIRE-00110416$$uINFN, Bari
002153377 700__ $$aNaru, Muhammad Umair$$iINSPIRE-00507883$$uCOMSATS, Islamabad
002153377 700__ $$aFerreira Natal Da Luz, Pedro Hugo$$iINSPIRE-00511516$$uSao Paulo U.
002153377 700__ $$aNattrass, Christine$$iINSPIRE-00301613$$uTennessee U.
002153377 700__ $$aRosado Navarro, Sebastian$$iINSPIRE-00548422$$uPuebla U., Mexico
002153377 700__ $$aNayak, Kishora$$iINSPIRE-00416777$$uBhubaneswar, NISER
002153377 700__ $$aNayak, Ranjit$$iINSPIRE-00548439$$uIndian Inst. Tech., Mumbai
002153377 700__ $$aNayak, Tapan Kumar$$iINSPIRE-00182590$$uCalcutta, VECC
002153377 700__ $$aNazarenko, Sergey$$iINSPIRE-00289965$$uRFNC-VNIIEF, Sarov
002153377 700__ $$aNedosekin, Alexander$$iINSPIRE-00060091$$uMoscow, ITEP
002153377 700__ $$aNegrao De Oliveira, Renato Aparecido$$iINSPIRE-00564311$$uCERN
002153377 700__ $$aNellen, Lukas$$iINSPIRE-00110793$$uMexico U., ICN
002153377 700__ $$aNg, Fabian$$iINSPIRE-00507999$$uHouston U.
002153377 700__ $$aNicassio, Maria$$iINSPIRE-00246928$$uDarmstadt, EMMI
002153377 700__ $$aNiculescu, Mihai$$iINSPIRE-00361459$$uBucharest, Inst. Space Science
002153377 700__ $$aNiedziela, Jeremi$$iINSPIRE-00508100$$uCERN
002153377 700__ $$aNielsen, Borge Svane$$iINSPIRE-00111394$$uBohr Inst.
002153377 700__ $$aNikolaev, Sergey$$iINSPIRE-00111550$$uKurchatov Inst., Moscow
002153377 700__ $$aNikulin, Sergey$$iINSPIRE-00248281$$uKurchatov Inst., Moscow
002153377 700__ $$aNikulin, Vladimir$$iINSPIRE-00248270$$uSt. Petersburg, INP
002153377 700__ $$aNoferini, Francesco$$iINSPIRE-00248268$$uINFN, Bologna$$uEnrico Fermi Ctr., Rome
002153377 700__ $$aNomokonov, Petr$$iINSPIRE-00246900$$uDubna, JINR
002153377 700__ $$aNooren, Gerardus$$iINSPIRE-00248256$$uUtrecht U.
002153377 700__ $$aCabanillas Noris, Juan Carlos$$iINSPIRE-00522336$$uPuebla U., Mexico
002153377 700__ $$aNorman, Jaime$$iINSPIRE-00416828$$uLiverpool U.
002153377 700__ $$aNyanin, Alexander$$iINSPIRE-00242683$$uKurchatov Inst., Moscow
002153377 700__ $$aNystrand, Joakim Ingemar$$iINSPIRE-00244103$$uBergen U.
002153377 700__ $$aOeschler, Helmut Oskar$$iINSPIRE-00244115$$uHeidelberg U.
002153377 700__ $$aOh, Saehanseul$$iINSPIRE-00361447$$uYale U.
002153377 700__ $$aOh, Sun Kun$$iINSPIRE-00290016$$uKonkuk U.
002153377 700__ $$aOhlson, Alice Elisabeth$$iINSPIRE-00254942$$uCERN
002153377 700__ $$aOkatan, Ali$$iINSPIRE-00385578$$uKaratay U.
002153377 700__ $$aOkubo, Tsubasa$$iINSPIRE-00508134$$uHiroshima U.
002153377 700__ $$aOleniacz, Janusz$$iINSPIRE-00248235$$uWarsaw U. of Tech.
002153377 700__ $$aOliveira Da Silva, Antonio Carlos$$iINSPIRE-00361460$$uSao Paulo U.
002153377 700__ $$aOliver, Michael Henry$$iINSPIRE-00508240$$uYale U.
002153377 700__ $$aOnderwaater, Jacobus$$iINSPIRE-00383785$$uDarmstadt, EMMI
002153377 700__ $$aOppedisano, Chiara$$iINSPIRE-00290024$$uINFN, Turin
002153377 700__ $$aOrava, Risto$$iINSPIRE-00113286$$uHelsinki Inst. of Phys.
002153377 700__ $$aOravec, Matej$$iINSPIRE-00564321$$uKosice Tech. U.
002153377 700__ $$aOrtiz Velasquez, Antonio$$iINSPIRE-00248229$$uMexico U., ICN
002153377 700__ $$aOskarsson, Anders Nils Erik$$iINSPIRE-00242747$$uLund U.
002153377 700__ $$aOtwinowski, Jacek Tomasz$$iINSPIRE-00244142$$uCracow, INP
002153377 700__ $$aOyama, Ken$$iINSPIRE-00113667$$uHeidelberg U.$$uNagasaki Inst. Appl. Sci.
002153377 700__ $$aOzdemir, Mahmut$$iINSPIRE-00419619$$uFrankfurt U., Inst. Kernphys.
002153377 700__ $$aPachmayer, Yvonne Chiara$$iINSPIRE-00290030$$uHeidelberg U.
002153377 700__ $$aPagano, Davide$$iINSPIRE-00313673$$uU. Brescia
002153377 700__ $$aPagano, Paola$$iINSPIRE-00290049$$uSalerno U.$$uINFN, Salerno
002153377 700__ $$aPaic, Guy$$iINSPIRE-00113938$$uMexico U., ICN
002153377 700__ $$aPal, Susanta Kumar$$iINSPIRE-00182683$$uCalcutta, VECC
002153377 700__ $$aPalni, Prabhakar$$iINSPIRE-00265540$$uHua-Zhong Normal U.
002153377 700__ $$aPan, Jinjin$$iINSPIRE-00508257$$uWayne State U.
002153377 700__ $$aPandey, Ashutosh Kumar$$iINSPIRE-00522482$$uIndian Inst. Tech., Mumbai
002153377 700__ $$aPapikyan, Vardanush$$iINSPIRE-00246268$$uYerevan Phys. Inst.
002153377 700__ $$aPappalardo, Giuseppe$$iINSPIRE-00178786$$uINFN, Catania
002153377 700__ $$aPareek, Pooja$$iINSPIRE-00383898$$uIndian Inst. Tech., Indore
002153377 700__ $$aPark, Woojin$$iINSPIRE-00242771$$uDarmstadt, EMMI
002153377 700__ $$aParmar, Sonia$$iINSPIRE-00416870$$uPanjab U.
002153377 700__ $$aPassfeld, Annika$$iINSPIRE-00361472$$uMunster U.
002153377 700__ $$aPaticchio, Vincenzo$$iINSPIRE-00290079$$uINFN, Bari
002153377 700__ $$aPatra, Rajendra Nath$$iINSPIRE-00522505$$uCalcutta, VECC
002153377 700__ $$aPaul, Biswarup$$iINSPIRE-00361484$$uINFN, Turin
002153377 700__ $$aPei, Hua$$iINSPIRE-00242789$$uHua-Zhong Normal U.
002153377 700__ $$aPeitzmann, Thomas$$iINSPIRE-00182726$$uUtrecht U.
002153377 700__ $$aPeng, Xinye$$iINSPIRE-00564353$$uHua-Zhong Normal U.
002153377 700__ $$aPereira Da Costa, Hugo Denis Antonio$$iINSPIRE-00242790$$uIRFU, Saclay
002153377 700__ $$aPeresunko, Dmitry Yurevich$$iINSPIRE-00246415$$uKurchatov Inst., Moscow$$uMoscow Phys. Eng. Inst.
002153377 700__ $$aPerez Lezama, Edgar$$iINSPIRE-00433111$$uFrankfurt U., Inst. Kernphys.
002153377 700__ $$aPeskov, Vladimir$$iINSPIRE-00115907$$uFrankfurt U., Inst. Kernphys.
002153377 700__ $$aPestov, Yury$$iINSPIRE-00248095$$uNovosibirsk, IYF
002153377 700__ $$aPetracek, Vojtech$$iINSPIRE-00250478$$uPrague, Tech. U.
002153377 700__ $$aPetrov, Viacheslav$$iINSPIRE-00508460$$uSerpukhov, IHEP
002153377 700__ $$aPetrovici, Mihai$$iINSPIRE-00290111$$uBucharest, IFIN-HH
002153377 700__ $$aPetta, Catia$$iINSPIRE-00250481$$uCatania U.$$uINFN, Catania
002153377 700__ $$aPiano, Stefano$$iINSPIRE-00249971$$uINFN, Trieste
002153377 700__ $$aPikna, Miroslav$$iINSPIRE-00116456$$uComenius U.
002153377 700__ $$aPillot, Philippe$$iINSPIRE-00290120$$uSUBATECH, Nantes
002153377 700__ $$aOzelin De Lima Pimentel, Lais$$iINSPIRE-00548449$$uBohr Inst.
002153377 700__ $$aPinazza, Ombretta$$iINSPIRE-00290138$$uINFN, Bologna$$uCERN
002153377 700__ $$aPinsky, Lawrence$$iINSPIRE-00116547$$uHouston U.
002153377 700__ $$aPiyarathna, Danthasinghe$$iINSPIRE-00246340$$uHouston U.
002153377 700__ $$aPloskon, Mateusz Andrzej$$iINSPIRE-00248071$$uLBL, Berkeley
002153377 700__ $$aPlaninic, Mirko$$iINSPIRE-00182770$$uZagreb U.
002153377 700__ $$aPluta, Jan Marian$$iINSPIRE-00182781$$uWarsaw U. of Tech.
002153377 700__ $$aPochybova, Sona$$iINSPIRE-00248060$$uWigner RCP, Budapest
002153377 700__ $$aPodesta Lerma, Pedro Luis Manuel$$iINSPIRE-00049100$$uSinaloa U.
002153377 700__ $$aPoghosyan, Martin$$iINSPIRE-00249924$$uOak Ridge
002153377 700__ $$aPolishchuk, Boris$$iINSPIRE-00248058$$uSerpukhov, IHEP
002153377 700__ $$aPoljak, Nikola$$iINSPIRE-00182793$$uZagreb U.
002153377 700__ $$aPoonsawat, Wanchaloem$$iINSPIRE-00508526$$uSuranaree U. of Tech.
002153377 700__ $$aPop, Amalia$$iINSPIRE-00290166$$uBucharest, IFIN-HH
002153377 700__ $$aPoppenborg, Hendrik$$iINSPIRE-00564335$$uMunster U.
002153377 700__ $$aPorteboeuf, Sarah Julie$$iINSPIRE-00207321$$uClermont-Ferrand U.
002153377 700__ $$aPorter, R Jefferson$$iINSPIRE-00254707$$uLBL, Berkeley
002153377 700__ $$aPospisil, Jan$$iINSPIRE-00508637$$uRez, Nucl. Phys. Inst.
002153377 700__ $$aPrasad, Sidharth Kumar$$iINSPIRE-00244190$$uBose Inst., Kolkata$$uCAPSS, Kolkata
002153377 700__ $$aPreghenella, Roberto$$iINSPIRE-00246857$$uINFN, Bologna$$uCERN
002153377 700__ $$aPrino, Francesco$$iINSPIRE-00270661$$uINFN, Turin
002153377 700__ $$aPruneau, Claude Andre$$iINSPIRE-00182834$$uWayne State U.
002153377 700__ $$aPshenichnov, Igor$$iINSPIRE-00117975$$uMoscow, INR
002153377 700__ $$aPuccio, Maximiliano$$iINSPIRE-00508690$$uTurin U.$$uINFN, Turin
002153377 700__ $$aPuddu, Giovanna$$iINSPIRE-00250538$$uCagliari U.$$uINFN, Cagliari
002153377 700__ $$aPujahari, Prabhat Ranjan$$iINSPIRE-00182850$$uWayne State U.
002153377 700__ $$aPunin, Valery$$iINSPIRE-00248029$$uRFNC-VNIIEF, Sarov
002153377 700__ $$aPutschke, Jorn Henning$$iINSPIRE-00001210$$uWayne State U.
002153377 700__ $$aQvigstad, Henrik$$iINSPIRE-00245912$$uOslo U.
002153377 700__ $$aRachevski, Alexandre$$iINSPIRE-00250549$$uINFN, Trieste
002153377 700__ $$aRaha, Sibaji$$iINSPIRE-00360571$$uBose Inst., Kolkata$$uCAPSS, Kolkata
002153377 700__ $$aRajput, Sonia$$iINSPIRE-00508791$$uJammu U.
002153377 700__ $$aRak, Jan$$iINSPIRE-00242842$$uJyvaskyla U.
002153377 700__ $$aRakotozafindrabe, Andry Malala$$iINSPIRE-00030930$$uIRFU, Saclay
002153377 700__ $$aRamello, Luciano$$iINSPIRE-00118788$$uPiemonte Orientale U., Alessandria
002153377 700__ $$aRami, Fouad$$iINSPIRE-00531399$$uStrasbourg, IPHC
002153377 700__ $$aRaniwala, Rashmi$$iINSPIRE-00182881$$uRajasthan U.
002153377 700__ $$aRaniwala, Sudhir$$iINSPIRE-00182870$$uRajasthan U.
002153377 700__ $$aRasanen, Sami Sakari$$iINSPIRE-00290180$$uHelsinki Inst. of Phys.
002153377 700__ $$aRascanu, Bogdan Theodor$$iINSPIRE-00361496$$uFrankfurt U., Inst. Kernphys.
002153377 700__ $$aRathee, Deepika$$iINSPIRE-00290197$$uPanjab U.
002153377 700__ $$aRavasenga, Ivan$$iINSPIRE-00564657$$uTurin U.$$uINFN, Turin
002153377 700__ $$aRead, Kenneth Francis$$iINSPIRE-00119330$$uTennessee U.$$uOak Ridge
002153377 700__ $$aRedlich, Krzysztof$$iINSPIRE-00119427$$uWarsaw, Inst. Nucl. Studies
002153377 700__ $$aReed, Rosi Jan$$iINSPIRE-00182908$$uWayne State U.
002153377 700__ $$aRehman, Attiq Ur$$iINSPIRE-00244772$$uBergen U.
002153377 700__ $$aReichelt, Patrick Simon$$iINSPIRE-00245747$$uFrankfurt U., Inst. Kernphys.
002153377 700__ $$aReidt, Felix$$iINSPIRE-00246160$$uCERN$$uHeidelberg U.
002153377 700__ $$aRen, Xiaowen$$iINSPIRE-00508864$$uHua-Zhong Normal U.
002153377 700__ $$aRenfordt, Rainer Arno Ernst$$iINSPIRE-00119620$$uFrankfurt U., Inst. Kernphys.
002153377 700__ $$aReolon, Anna Rita$$iINSPIRE-00250550$$uFrascati
002153377 700__ $$aReshetin, Andrey$$iINSPIRE-00119738$$uMoscow, INR
002153377 700__ $$aReygers, Klaus Johannes$$iINSPIRE-00242889$$uHeidelberg U.
002153377 700__ $$aRiabov, Viktor$$iINSPIRE-00242892$$uSt. Petersburg, INP
002153377 700__ $$aRicci, Renato Angelo$$iINSPIRE-00119905$$uINFN, Legnaro
002153377 700__ $$aRichert, Tuva Ora Herenui$$iINSPIRE-00361510$$uLund U.
002153377 700__ $$aRichter, Matthias Rudolph$$iINSPIRE-00244201$$uOslo U.
002153377 700__ $$aRiedler, Petra$$iINSPIRE-00120095$$uCERN
002153377 700__ $$aRiegler, Werner$$iINSPIRE-00250574$$uCERN
002153377 700__ $$aRiggi, Francesco$$iINSPIRE-00290213$$uCatania U.$$uINFN, Catania
002153377 700__ $$aRistea, Catalin-Lucian$$iINSPIRE-00508900$$uBucharest, Inst. Space Science
002153377 700__ $$aRodriguez Cahuantzi, Mario$$iINSPIRE-00247954$$uPuebla U., Mexico
002153377 700__ $$aRodriguez Manso, Alis$$iINSPIRE-00361526$$uNIKHEF, Amsterdam
002153377 700__ $$aRoeed, Ketil$$iINSPIRE-00247948$$uOslo U.
002153377 700__ $$aRogochaya, Elena$$iINSPIRE-00385804$$uDubna, JINR
002153377 700__ $$aRohr, David Michael$$iINSPIRE-00248142$$uFrankfurt U., FIAS
002153377 700__ $$aRoehrich, Dieter$$iINSPIRE-00250583$$uBergen U.
002153377 700__ $$aRonchetti, Federico$$iINSPIRE-00139171$$uCERN$$uFrascati
002153377 700__ $$aRonflette, Lucile$$iINSPIRE-00384171$$uSUBATECH, Nantes
002153377 700__ $$aRosnet, Philippe$$iINSPIRE-00121285$$uClermont-Ferrand U.
002153377 700__ $$aRossi, Andrea$$iINSPIRE-00290284$$uPadua U.$$uINFN, Padua
002153377 700__ $$aRoukoutakis, Filimon$$iINSPIRE-00247900$$uAthens U.
002153377 700__ $$aRoy, Ankhi$$iINSPIRE-00385891$$uIndian Inst. Tech., Indore
002153377 700__ $$aRoy, Christelle Sophie$$iINSPIRE-00182943$$uStrasbourg, IPHC
002153377 700__ $$aRoy, Pradip Kumar$$iINSPIRE-00290300$$uSaha Inst.
002153377 700__ $$aRubio Montero, Antonio Juan$$iINSPIRE-00290319$$uMadrid, CIEMAT
002153377 700__ $$aRui, Rinaldo$$iINSPIRE-00121777$$uTrieste U.$$uINFN, Trieste
002153377 700__ $$aRusso, Riccardo$$iINSPIRE-00361538$$uTurin U.$$uINFN, Turin
002153377 700__ $$aRyabinkin, Evgeny$$iINSPIRE-00246815$$uKurchatov Inst., Moscow
002153377 700__ $$aRyabov, Yury$$iINSPIRE-00306193$$uSt. Petersburg, INP
002153377 700__ $$aRybicki, Andrzej$$iINSPIRE-00250603$$uCracow, INP
002153377 700__ $$aSaarinen, Sampo$$iINSPIRE-00560357$$uHelsinki Inst. of Phys.
002153377 700__ $$aSadhu, Samrangy$$iINSPIRE-00560369$$uCalcutta, VECC
002153377 700__ $$aSadovskiy, Sergey$$iINSPIRE-00247897$$uSerpukhov, IHEP
002153377 700__ $$aSafarik, Karel$$iINSPIRE-00290327$$uCERN
002153377 700__ $$aSahlmuller, Baldo$$iINSPIRE-00242967$$uFrankfurt U., Inst. Kernphys.
002153377 700__ $$aSahoo, Pragati$$iINSPIRE-00384329$$uIndian Inst. Tech., Indore
002153377 700__ $$aSahoo, Raghunath$$iINSPIRE-00182966$$uIndian Inst. Tech., Indore
002153377 700__ $$aSahoo, Sarita$$iINSPIRE-00508953$$uBhubaneswar, Inst. Phys.
002153377 700__ $$aSahu, Pradip Kumar$$iINSPIRE-00122421$$uBhubaneswar, Inst. Phys.
002153377 700__ $$aSaini, Jogender$$iINSPIRE-00246803$$uCalcutta, VECC
002153377 700__ $$aSakai, Shingo$$iINSPIRE-00182972$$uFrascati
002153377 700__ $$aSaleh, Mohammad Ahmad$$iINSPIRE-00509062$$uWayne State U.
002153377 700__ $$aSalzwedel, Jai Samuel Nielsen$$iINSPIRE-00361540$$uOhio State U.
002153377 700__ $$aSambyal, Sanjeev Singh$$iINSPIRE-00247865$$uJammu U.
002153377 700__ $$aSamsonov, Vladimir$$iINSPIRE-00242999$$uSt. Petersburg, INP$$uMoscow Phys. Eng. Inst.
002153377 700__ $$aSandor, Ladislav$$iINSPIRE-00254840$$uKosice, IEF
002153377 700__ $$aSandoval, Andres$$iINSPIRE-00123048$$uMexico U.
002153377 700__ $$aSano, Masato$$iINSPIRE-00290365$$uTsukuba U.
002153377 700__ $$aSarkar, Debojit$$iINSPIRE-00384381$$uCalcutta, VECC
002153377 700__ $$aSarkar, Nachiketa$$iINSPIRE-00560376$$uCalcutta, VECC
002153377 700__ $$aSarma, Pranjal$$iINSPIRE-00548452$$uGauhati U.
002153377 700__ $$aScapparone, Eugenio$$iINSPIRE-00250631$$uINFN, Bologna
002153377 700__ $$aScarlassara, Fernando$$iINSPIRE-00249930$$uPadua U.$$uINFN, Padua
002153377 700__ $$aSchiaua, Claudiu Cornel$$iINSPIRE-00247838$$uBucharest, IFIN-HH
002153377 700__ $$aSchicker, Rainer Martin$$iINSPIRE-00244227$$uHeidelberg U.
002153377 700__ $$aSchmidt, Christian Joachim$$iINSPIRE-00244248$$uDarmstadt, EMMI
002153377 700__ $$aSchmidt, Hans Rudolf$$iINSPIRE-00290373$$uTubingen U.
002153377 700__ $$aSchmidt, Martin$$iINSPIRE-00560380$$uTubingen U.
002153377 700__ $$aSchuchmann, Simone$$iINSPIRE-00290381$$uFrankfurt U., Inst. Kernphys.$$uHeidelberg U.
002153377 700__ $$aSchukraft, Jurgen$$iINSPIRE-00290390$$uCERN
002153377 700__ $$aSchutz, Yves Roland$$iINSPIRE-00174514$$uCERN$$uSUBATECH, Nantes
002153377 700__ $$aSchwarz, Kilian Eberhard$$iINSPIRE-00247800$$uDarmstadt, EMMI
002153377 700__ $$aSchweda, Kai Oliver$$iINSPIRE-00244251$$uDarmstadt, EMMI
002153377 700__ $$aScioli, Gilda$$iINSPIRE-00247797$$uBologna U.$$uINFN, Bologna
002153377 700__ $$aScomparin, Enrico$$iINSPIRE-00291684$$uINFN, Turin
002153377 700__ $$aScott, Rebecca Michelle$$iINSPIRE-00254900$$uTennessee U.
002153377 700__ $$aSefcik, Michal$$iINSPIRE-00537153$$uKosice U.
002153377 700__ $$aSeger, Janet Elizabeth$$iINSPIRE-00124982$$uCreighton U.
002153377 700__ $$aSekiguchi, Yuko$$iINSPIRE-00411670$$uTokyo U.
002153377 700__ $$aSekihata, Daiki$$iINSPIRE-00522342$$uHiroshima U.
002153377 700__ $$aSelyuzhenkov, Ilya$$iINSPIRE-00049715$$uDarmstadt, EMMI
002153377 700__ $$aSenosi, Kgotlaesele$$iINSPIRE-00509280$$uiThemba LABS
002153377 700__ $$aSenyukov, Serhiy$$iINSPIRE-00270653$$uBITP, Kiev$$uCERN
002153377 700__ $$aSerradilla Rodriguez, Eulogio$$iINSPIRE-00247783$$uMadrid, CIEMAT$$uMexico U.
002153377 700__ $$aSevcenco, Adrian$$iINSPIRE-00247771$$uBucharest, Inst. Space Science
002153377 700__ $$aShabanov, Arseniy$$iINSPIRE-00509394$$uMoscow, INR
002153377 700__ $$aShabetai, Alexandre$$iINSPIRE-00361563$$uSUBATECH, Nantes
002153377 700__ $$aShadura, Oksana$$iINSPIRE-00509445$$uBITP, Kiev
002153377 700__ $$aShahoyan, Ruben$$iINSPIRE-00125510$$uCERN
002153377 700__ $$aShangaraev, Artem$$iINSPIRE-00384482$$uSerpukhov, IHEP
002153377 700__ $$aSharma, Ankita$$iINSPIRE-00509560$$uJammu U.
002153377 700__ $$aSharma, Mona$$iINSPIRE-00522357$$uJammu U.
002153377 700__ $$aSharma, Monika$$iINSPIRE-00523366$$uJammu U.
002153377 700__ $$aSharma, Natasha$$iINSPIRE-00291700$$uTennessee U.
002153377 700__ $$aSheikh, Ashik Ikbal$$iINSPIRE-00560398$$uCalcutta, VECC
002153377 700__ $$aShigaki, Kenta$$iINSPIRE-00125910$$uHiroshima U.
002153377 700__ $$aShou, Qiye$$iINSPIRE-00565745$$uHua-Zhong Normal U.
002153377 700__ $$aShtejer Diaz, Katherin$$iINSPIRE-00247746$$uHavana, CEADEN$$uTurin U.$$uINFN, Turin
002153377 700__ $$aSibiryak, Yury$$iINSPIRE-00250642$$uKurchatov Inst., Moscow
002153377 700__ $$aSiddhanta, Sabyasachi$$iINSPIRE-00245363$$uINFN, Cagliari
002153377 700__ $$aSielewicz, Krzysztof Marek$$iINSPIRE-00509501$$uCERN
002153377 700__ $$aSiemiarczuk, Teodor$$iINSPIRE-00291730$$uWarsaw, Inst. Nucl. Studies
002153377 700__ $$aSilvermyr, David Olle Rickard$$iINSPIRE-00003534$$uLund U.
002153377 700__ $$aSilvestre, Catherine Micaela$$iINSPIRE-00243076$$uLPSC, Grenoble
002153377 700__ $$aSimatovic, Goran$$iINSPIRE-00361587$$uZagreb U.
002153377 700__ $$aSimonetti, Giuseppe$$iINSPIRE-00291749$$uCERN
002153377 700__ $$aSingaraju, Rama Narayana$$iINSPIRE-00183080$$uCalcutta, VECC
002153377 700__ $$aSingh, Ranbir$$iINSPIRE-00291757$$uBhubaneswar, NISER
002153377 700__ $$aSinghal, Vikas$$iINSPIRE-00246754$$uCalcutta, VECC
002153377 700__ $$aSarkar - Sinha, Tinku$$iINSPIRE-00244281$$uSaha Inst.
002153377 700__ $$aSitar, Branislav$$iINSPIRE-00244846$$uComenius U.
002153377 700__ $$aSitta, Mario$$iINSPIRE-00291781$$uPiemonte Orientale U., Alessandria
002153377 700__ $$aSkaali, Bernhard$$iINSPIRE-00250655$$uOslo U.
002153377 700__ $$aSlupecki, Maciej$$iINSPIRE-00245476$$uJyvaskyla U.
002153377 700__ $$aSmirnov, Nikolai$$iINSPIRE-00183105$$uYale U.
002153377 700__ $$aSnellings, Raimond$$iINSPIRE-00127370$$uUtrecht U.
002153377 700__ $$aSnellman, Tomas Wilhelm$$iINSPIRE-00509620$$uJyvaskyla U.
002153377 700__ $$aSong, Jihye$$iINSPIRE-00291808$$uPusan Natl. U.
002153377 700__ $$aSong, Myunggeun$$iINSPIRE-00291790$$uYonsei U.
002153377 700__ $$aSong, Zixuan$$iINSPIRE-00509684$$uHua-Zhong Normal U.
002153377 700__ $$aSoramel, Francesca$$iINSPIRE-00247643$$uPadua U.$$uINFN, Padua
002153377 700__ $$aSorensen, Soren Pontoppidan$$iINSPIRE-00243132$$uTennessee U.
002153377 700__ $$aSozzi, Federica$$iINSPIRE-00506480$$uDarmstadt, EMMI
002153377 700__ $$aSpiriti, Eleuterio$$iINSPIRE-00191037$$uFrascati
002153377 700__ $$aSputowska, Iwona Anna$$iINSPIRE-00361599$$uCracow, INP
002153377 700__ $$aSpyropoulou-Stassinaki, Martha$$iINSPIRE-00291811$$uAthens U.
002153377 700__ $$aStachel, Johanna$$iINSPIRE-00128299$$uHeidelberg U.
002153377 700__ $$aStan, Ionel$$iINSPIRE-00434447$$uBucharest, Inst. Space Science
002153377 700__ $$aStankus, Paul$$iINSPIRE-00243169$$uOak Ridge
002153377 700__ $$aStenlund, Evert Anders$$iINSPIRE-00243170$$uLund U.
002153377 700__ $$aSteyn, Gideon Francois$$iINSPIRE-00249942$$uiThemba LABS
002153377 700__ $$aStiller, Johannes Hendrik$$iINSPIRE-00361600$$uHeidelberg U.
002153377 700__ $$aStocco, Diego$$iINSPIRE-00249962$$uSUBATECH, Nantes
002153377 700__ $$aStrmen, Peter$$iINSPIRE-00196247$$uComenius U.
002153377 700__ $$aAlarcon Do Passo Suaide, Alexandre$$iINSPIRE-00183172$$uSao Paulo U.
002153377 700__ $$aSugitate, Toru$$iINSPIRE-00129590$$uHiroshima U.
002153377 700__ $$aSuire, Christophe Pierre$$iINSPIRE-00243206$$uOrsay, IPN
002153377 700__ $$aSuleymanov, Mais Kazim Oglu$$iINSPIRE-00357683$$uCOMSATS, Islamabad
002153377 700__ $$aSuljic, Miljenko$$iINSPIRE-00531401$$uTrieste U.$$uINFN, Trieste
002153377 700__ $$aSultanov, Rishat$$iINSPIRE-00361629$$uMoscow, ITEP
002153377 700__ $$aSumbera, Michal$$iINSPIRE-00183200$$uRez, Nucl. Phys. Inst.
002153377 700__ $$aSumowidagdo, Suharyo$$iINSPIRE-00129750$$uJakarta LIPI, Indonesian Inst. Sci.
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002153377 700__ $$aSzczepankiewicz, Adam$$iINSPIRE-00245899$$uWarsaw U. of Tech.
002153377 700__ $$aSzymanski, Maciej Pawel$$iINSPIRE-00361630$$uWarsaw U. of Tech.
002153377 700__ $$aTabassam, Uzma$$iINSPIRE-00531415$$uCOMSATS, Islamabad
002153377 700__ $$aTakahashi, Jun$$iINSPIRE-00183279$$uCampinas State U.
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002153377 700__ $$aTarhini, Mohamad$$iINSPIRE-00522518$$uOrsay, IPN
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002153377 700__ $$aTarzila, Madalina-Gabriela$$iINSPIRE-00416999$$uBucharest, IFIN-HH
002153377 700__ $$aTauro, Arturo$$iINSPIRE-00247582$$uCERN
002153377 700__ $$aTejeda Munoz, Guillermo$$iINSPIRE-00247570$$uPuebla U., Mexico
002153377 700__ $$aTelesca, Adriana$$iINSPIRE-00247569$$uCERN
002153377 700__ $$aTerasaki, Kohei$$iINSPIRE-00509855$$uTokyo U.
002153377 700__ $$aTerrevoli, Cristina$$iINSPIRE-00246722$$uPadua U.$$uINFN, Padua
002153377 700__ $$aTeyssier, Boris$$iINSPIRE-00509910$$uLyon, IPN
002153377 700__ $$aThaeder, Jochen Mathias$$iINSPIRE-00247557$$uLBL, Berkeley
002153377 700__ $$aThakur, Dhananjaya$$iINSPIRE-00560404$$uIndian Inst. Tech., Indore
002153377 700__ $$aThomas, Deepa$$iINSPIRE-00290473$$uTexas U.
002153377 700__ $$aTieulent, Raphael Noel$$iINSPIRE-00244918$$uLyon, IPN
002153377 700__ $$aTikhonov, Anatoly$$iINSPIRE-00560412$$uMoscow, INR
002153377 700__ $$aTimmins, Anthony Robert$$iINSPIRE-00183330$$uHouston U.
002153377 700__ $$aToia, Alberica$$iINSPIRE-00020233$$uFrankfurt U., Inst. Kernphys.
002153377 700__ $$aTrogolo, Stefano$$iINSPIRE-00509971$$uTurin U.$$uINFN, Turin
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002153377 700__ $$aTrubnikov, Victor$$iINSPIRE-00361654$$uBITP, Kiev
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002153377 700__ $$aTsuji, Tomoya$$iINSPIRE-00290495$$uTokyo U.
002153377 700__ $$aTumkin, Alexandr$$iINSPIRE-00246709$$uRFNC-VNIIEF, Sarov
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002153377 700__ $$aUras, Antonio$$iINSPIRE-00247480$$uLyon, IPN
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002153377 700__ $$aVande Vyvre, Pierre$$iINSPIRE-00250736$$uCERN
002153377 700__ $$aVarga, Dezso$$iINSPIRE-00510156$$uWigner RCP, Budapest
002153377 700__ $$aDiozcora Vargas Trevino, Aurora$$iINSPIRE-00244960$$uPuebla U., Mexico
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002153377 700__ $$aVarma, Raghava$$iINSPIRE-00183420$$uIndian Inst. Tech., Mumbai
002153377 700__ $$aVasileiou, Maria$$iINSPIRE-00246199$$uAthens U.
002153377 700__ $$aVasiliev, Andrey$$iINSPIRE-00261815$$uKurchatov Inst., Moscow
002153377 700__ $$aVauthier, Astrid$$iINSPIRE-00510213$$uLPSC, Grenoble
002153377 700__ $$aVazquez Doce, Oton$$iINSPIRE-00560426$$uTech. U., Munich (main)$$uMunich, Tech. U., Universe
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002153377 700__ $$aVinogradov, Alexander$$iINSPIRE-00140395$$uKurchatov Inst., Moscow
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002153377 700__ $$aZaccolo, Valentina$$iINSPIRE-00361691$$uBohr Inst.
002153377 700__ $$aZaman, Ali$$iINSPIRE-00385199$$uCOMSATS, Islamabad
002153377 700__ $$aZampolli, Chiara$$iINSPIRE-00247387$$uINFN, Bologna$$uCERN
002153377 700__ $$aCorreia Zanoli, Henrique Jose$$iINSPIRE-00510636$$uSao Paulo U.
002153377 700__ $$aZaporozhets, Sergey$$iINSPIRE-00250758$$uDubna, JINR
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002153377 700__ $$aZavyalov, Nikolay$$iINSPIRE-00290800$$uRFNC-VNIIEF, Sarov
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002153377 700__ $$aZgura, Sorin Ion$$iINSPIRE-00245065$$uBucharest, Inst. Space Science
002153377 700__ $$aZhalov, Mikhail$$iINSPIRE-00254612$$uSt. Petersburg, INP
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002153377 700__ $$aZhigareva, Natalia$$iINSPIRE-00385354$$uMoscow, ITEP
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002153377 700__ $$aZhu, Hongsheng$$iINSPIRE-00361728$$uBergen U.$$uHua-Zhong Normal U.
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002153377 700__ $$aZimmermann, Alice$$iINSPIRE-00361741$$uHeidelberg U.
002153377 700__ $$aZimmermann, Markus Bernhard$$iINSPIRE-00385420$$uMunster U.$$uCERN
002153377 700__ $$aZinovjev, Gennady$$iINSPIRE-00290880$$uBITP, Kiev
002153377 700__ $$aZyzak, Maksym$$iINSPIRE-00361753$$uFrankfurt U., FIAS
002153377 710__ $$5PH
002153377 710__ $$gALICE Collaboration
002153377 773__ $$c054908$$oPhys. Rev. C 94, 054908 (2016)$$pPhys. Rev. C$$v94$$y2016
002153377 859__ $$fenrico.scomparin@cern.ch
002153377 8564_ $$81191965$$s658321$$uhttp://cds.cern.ch/record/2153377/files/CERN-EP-DRAFT-ALICE-2016-011 - draft.pdf$$yDraft (restricted)$$zStamped by WebSubmit: 20/05/2016
002153377 8564_ $$uhttp://arxiv.org/pdf/1605.07569$$yPreprint
002153377 8564_ $$81273816$$s1578148$$uhttp://cds.cern.ch/record/2153377/files/PhysRevC.94.054908.pdf$$yAPS Open Access article
002153377 8564_ $$82229707$$s35552$$uhttp://cds.cern.ch/record/2153377/files/figures_Dplus-dsigmadpt-pPb.png$$y00019 $\pt$-differential production cross sections of prompt $\Dzero$ (top-left), $\Dplus$ (top-right), $\Dstar$ (bottom-left) and $\Ds$ (bottom-right) mesons with $-0.96&lt;y_{\rm cms}&lt;0.04$ in p--Pb collisions at $\sqrtsNN=5.02~\tev$, compared with the respective pp reference cross sections scaled by the Pb mass number $A=208$. For the $\Dzero$ meson, the results in $0&lt;\pt&lt;2~\gev/c$ are obtained from the analysis without decay-vertex reconstruction, while those in $2&lt;\pt&lt;24~\gev/c$ are taken from the analysis with decay-vertex reconstruction. The results from the other three D-meson species are the same as in Ref.~\cite{Abelev:2014hha}. The systematic uncertainty of the feed-down correction is displayed separately.
002153377 8564_ $$82229708$$s30677$$uhttp://cds.cern.ch/record/2153377/files/figures_Dstar-dsigmady-pPb.png$$y00025 Production cross sections as a function of rapidity ($y_{\rm cms}$) for prompt $\Dzero$, $\Dplus$ and $\Dstar$ mesons in p--Pb collisions at $\sqrtsNN=5.02~\tev$, for three $\pt$ intervals. The $\Dzero$-meson data are compared with a cross section obtained by multiplying the FONLL~\cite{Cacciari:2012ny} calculation by the mass number $A$ and the nuclear modification factor $R_{\rm pA}$ estimated as a function of $y$ with the MNR NLO pQCD calculation~\cite{Mangano:1991jk}, with CTEQ6M PDFs~\cite{Pumplin:2002vw} and the EPS09NLO nuclear PDF parametrisation~\cite{Eskola:2009uj}.
002153377 8564_ $$82229709$$s11249$$uhttp://cds.cern.ch/record/2153377/files/figures_D0ppCrossSecVsFONLL.png$$y00011 $\pt$-differential production cross section of prompt $\Dzero$ mesons with $|y|&lt;0.5$ in the interval $0&lt;\pt&lt;16~\gev/c$, in pp collisions at $\sqrt s =7~\tev$. The data points in $0&lt;\pt&lt;2~\gev/c$ are obtained from the analysis described in this article, while the data points in $2&lt;\pt&lt;16~\gev/c$ are taken from Ref~\cite{ALICE:2011aa}. The cross section is compared to three pQCD calculations: FONLL~\cite{Cacciari:2012ny} (top-left panel), GM-VFNS~\cite{Kniehl:2012ti} (top-right panel) and a leading order (LO) calculation based on $k_{\rm T}$-factorisation~\cite{Maciula:2013wg} (bottom-left panel). In the bottom-right panel, the ratios of the data to the three calculated cross sections are reported.
002153377 8564_ $$82229710$$s25289$$uhttp://cds.cern.ch/record/2153377/files/InvMassSpectra_pp_bin1.png$$y00005 Invariant-mass distributions of $\DtoKpi$ candidates (and charge conjugates) in pp collisions at $\sqrts=7~\TeV$ for two $\pt$ intervals: $0&lt;\pt&lt;1~\gev/c$ (top panels) and $1&lt;\pt&lt;2~\gev/c$ (bottom panels). For both $\pt$ intervals, the left panels display the invariant-mass distribution of all ULS K$\pi$ pairs together with the background distributions estimated with the LS, event-mixing and track-rotation techniques. The middle and right panels show the invariant-mass distributions after subtraction of the background from the track-rotation and LS techniques. Fit functions are superimposed.
002153377 8564_ $$82229711$$s35306$$uhttp://cds.cern.ch/record/2153377/files/figures_Dstar-dsigmadpt-pPb.png$$y00020 $\pt$-differential production cross sections of prompt $\Dzero$ (top-left), $\Dplus$ (top-right), $\Dstar$ (bottom-left) and $\Ds$ (bottom-right) mesons with $-0.96&lt;y_{\rm cms}&lt;0.04$ in p--Pb collisions at $\sqrtsNN=5.02~\tev$, compared with the respective pp reference cross sections scaled by the Pb mass number $A=208$. For the $\Dzero$ meson, the results in $0&lt;\pt&lt;2~\gev/c$ are obtained from the analysis without decay-vertex reconstruction, while those in $2&lt;\pt&lt;24~\gev/c$ are taken from the analysis with decay-vertex reconstruction. The results from the other three D-meson species are the same as in Ref.~\cite{Abelev:2014hha}. The systematic uncertainty of the feed-down correction is displayed separately.
002153377 8564_ $$82229712$$s30871$$uhttp://cds.cern.ch/record/2153377/files/D0ppCrossSecRatioTopQCD.png$$y00012 Left: $\pt$-differential production cross section of prompt $\Dzero$ mesons with $|y|&lt;0.5$ in the interval $0&lt;\pt&lt;16~\gev/c$, in pp collisions at $\sqrt s =7~\tev$. The data points in $0&lt;\pt&lt;2~\gev/c$ are obtained from the analysis described in this article, while the data points in $2&lt;\pt&lt;16~\gev/c$ are taken from Ref~\cite{ALICE:2011aa}. The cross section is compared to three pQCD calculations: FONLL~\cite{Cacciari:2012ny}, GM-VFNS~\cite{Kniehl:2012ti} and a leading order (LO) calculation based on $k_{\rm T}$-factorisation~\cite{Maciula:2013wg}. Right: ratio of the data to the three calculated cross sections.
002153377 8564_ $$82229713$$s40918$$uhttp://cds.cern.ch/record/2153377/files/figures_Dzero-dsigmadpt-pPb.png$$y00018 $\pt$-differential production cross sections of prompt $\Dzero$ (top-left), $\Dplus$ (top-right), $\Dstar$ (bottom-left) and $\Ds$ (bottom-right) mesons with $-0.96&lt;y_{\rm cms}&lt;0.04$ in p--Pb collisions at $\sqrtsNN=5.02~\tev$, compared with the respective pp reference cross sections scaled by the Pb mass number $A=208$. For the $\Dzero$ meson, the results in $0&lt;\pt&lt;2~\gev/c$ are obtained from the analysis without decay-vertex reconstruction, while those in $2&lt;\pt&lt;24~\gev/c$ are taken from the analysis with decay-vertex reconstruction. The results from the other three D-meson species are the same as in Ref.~\cite{Abelev:2014hha}. The systematic uncertainty of the feed-down correction is displayed separately.
002153377 8564_ $$82229714$$s48588$$uhttp://cds.cern.ch/record/2153377/files/pPbWithModelsCNM.png$$y00027 Nuclear modification factor $R_{\rm pPb}$ of prompt D mesons in p--Pb collisions at $\sqrtsNN=5.02~\tev$: average $R_{\rm pPb}$ of $\Dzero$, $\Dplus$ and $\Dstar$ mesons in the interval $1&lt;\pt&lt;24~\gev/c$~\cite{Abelev:2014hha}, shown together with the $\Dzero$ $R_{\rm pPb}$ in $0&lt;\pt&lt;1~\GeV/c$. In the left-hand panel, the data are compared with results of theoretical calculations including only CNM effects: CGC~\cite{Fujii:2013yja}, NLO pQCD~\cite{Mangano:1991jk} with EPS09 nPDFs~\cite{Eskola:2009uj}, a LO pQCD calculation with CNM effects (Vitev et al.)~\cite{Sharma:2009hn} and a calculation based on incoherent multiple scatterings (Kang et al.)~\cite{Kang:2014hha}. In the right-hand panel, the results of the Duke~\cite{Xu:2015iha} and POWLANG~\cite{Beraudo:2015wsd} transport models are compared to the measured D-meson $R_{\rm pPb}$.
002153377 8564_ $$82229715$$s10613$$uhttp://cds.cern.ch/record/2153377/files/figures_RpPb-DsAverD.png$$y00027 Nuclear modification factor $R_{\rm pPb}$ of prompt D mesons in p--Pb collisions at $\sqrtsNN=5.02~\tev$~\cite{Abelev:2014hha}. Left: $R_{\rm pPb}$ of $\Dzero$, $\Dplus$ and $\Dstar$ mesons. Right: average $R_{\rm pPb}$ of the three non-strange D-meson species and $R_{\rm pPb}$ of $\Ds$ mesons. All results are obtained from the analysis with decay-vertex reconstruction.
002153377 8564_ $$82229716$$s15391$$uhttp://cds.cern.ch/record/2153377/files/enercanvfull.png$$y00013 Total inclusive charm production cross section in nucleon--nucleon collisions as a function of $\sqrt{s}$~\cite{Lourenco:2006vw,Adare:2010de,Adamczyk:2012af,Aaij:2013mga,Abelev:2012vra,Aad:2015zix}. Data are from pA collisions for $\sqrt s&lt;100$~GeV and from pp collisions for $\sqrt s>100$~GeV. Data from pA collisions were scaled by $1/A$. Results from NLO pQCD calculations (MNR~\cite{Mangano:1991jk}) and their uncertainties are shown as solid and dashed lines.
002153377 8564_ $$82229717$$s964684$$uhttp://cds.cern.ch/record/2153377/files/arXiv:1605.07569.pdf
002153377 8564_ $$82229718$$s10613$$uhttp://cds.cern.ch/record/2153377/files/RpPb-DsAverD.png$$y00025 Nuclear modification factor $R_{\rm pPb}$ of prompt D mesons in p--Pb collisions at $\sqrtsNN=5.02~\tev$~\cite{Abelev:2014hha}. Left: $R_{\rm pPb}$ of $\Dzero$, $\Dplus$ and $\Dstar$ mesons. Right: average $R_{\rm pPb}$ of the three non-strange D-meson species and $R_{\rm pPb}$ of $\Ds$ mesons. All results are obtained from the analysis with decay-vertex reconstruction.
002153377 8564_ $$82229719$$s12441$$uhttp://cds.cern.ch/record/2153377/files/D0ppCrossSec.png$$y00009 $\pt$-differential production cross section of $\Dzero$ mesons with $|y|&lt;0.5$ in pp collisions at $\sqrt s =7~\tev$. Left: comparison of prompt and inclusive $\Dzero$ mesons (the latter including also $\Dzero$ mesons from beauty-hadron decays) from the analysis without decay-vertex reconstruction. Right: comparison between the prompt $\Dzero$ cross sections measured with~\cite{ALICE:2011aa} and without decay-vertex reconstruction. Here and in all the following figures the symbols are plotted at the centre of the $\pt$ intervals (shown by the horizontal lines), the vertical lines represent the statistical uncertainties and the vertical size of the boxes corresponds to the systematic uncertainties.
002153377 8564_ $$82229720$$s29516$$uhttp://cds.cern.ch/record/2153377/files/D0ppCrossSecVspQCD.png$$y00011 Left: $\pt$-differential production cross section of prompt $\Dzero$ mesons with $|y|&lt;0.5$ in the interval $0&lt;\pt&lt;16~\gev/c$, in pp collisions at $\sqrt s =7~\tev$. The data points in $0&lt;\pt&lt;2~\gev/c$ are obtained from the analysis described in this article, while the data points in $2&lt;\pt&lt;16~\gev/c$ are taken from Ref~\cite{ALICE:2011aa}. The cross section is compared to three pQCD calculations: FONLL~\cite{Cacciari:2012ny}, GM-VFNS~\cite{Kniehl:2012ti} and a leading order (LO) calculation based on $k_{\rm T}$-factorisation~\cite{Maciula:2013wg}. Right: ratio of the data to the three calculated cross sections.
002153377 8564_ $$82229721$$s35018$$uhttp://cds.cern.ch/record/2153377/files/pPbWithModelsMedium.png$$y00028 Nuclear modification factor $R_{\rm pPb}$ of prompt D mesons in p--Pb collisions at $\sqrtsNN=5.02~\tev$: average $R_{\rm pPb}$ of $\Dzero$, $\Dplus$ and $\Dstar$ mesons in the interval $1&lt;\pt&lt;24~\gev/c$~\cite{Abelev:2014hha}, shown together with the $\Dzero$ $R_{\rm pPb}$ in $0&lt;\pt&lt;1~\GeV/c$. In the left-hand panel, the data are compared with results of theoretical calculations including only CNM effects: CGC~\cite{Fujii:2013yja}, NLO pQCD~\cite{Mangano:1991jk} with EPS09 nPDFs~\cite{Eskola:2009uj}, a LO pQCD calculation with CNM effects (Vitev et al.)~\cite{Sharma:2009hn} and a calculation based on incoherent multiple scatterings (Kang et al.)~\cite{Kang:2014hha}. In the right-hand panel, the results of the Duke~\cite{Xu:2015iha} and POWLANG~\cite{Beraudo:2015wsd} transport models are compared to the measured D-meson $R_{\rm pPb}$.
002153377 8564_ $$82229722$$s47606$$uhttp://cds.cern.ch/record/2153377/files/InvMassSpectra_D0DplusDstar_Ybins.png$$y00001 Distributions of the invariant mass for $\Dzero$ (left column), $\Dplus$ (middle column) candidates and their charge conjugates and of the mass difference for $\Dstar$ (right column) candidates (and charge conjugates) in p--Pb collisions in the rapidity intervals $|y_{\rm lab}| &lt;0.1 $ (top row) and $-0.8 &lt; y_{\mathrm{lab}} &lt; -0.4$ ($-0.7 &lt; y_{\mathrm{lab}} &lt; -0.4$ for $\pt&lt;5~\gev/c$) (bottom row). The dashed lines represent the fit to the background while the solid lines represent the total fit function. One $\pt$ interval is shown for each species: $2&lt;\pt&lt;5~\gevc$ for $\Dzero$, $5&lt;\pt&lt;8~\gevc$ for $\Dplus$ and $8&lt;\pt&lt;16~\gevc$ for $\Dstar$.
002153377 8564_ $$82229723$$s12345$$uhttp://cds.cern.ch/record/2153377/files/figures_D0ppCrossSecVsKtFact.png$$y00013 $\pt$-differential production cross section of prompt $\Dzero$ mesons with $|y|&lt;0.5$ in the interval $0&lt;\pt&lt;16~\gev/c$, in pp collisions at $\sqrt s =7~\tev$. The data points in $0&lt;\pt&lt;2~\gev/c$ are obtained from the analysis described in this article, while the data points in $2&lt;\pt&lt;16~\gev/c$ are taken from Ref~\cite{ALICE:2011aa}. The cross section is compared to three pQCD calculations: FONLL~\cite{Cacciari:2012ny} (top-left panel), GM-VFNS~\cite{Kniehl:2012ti} (top-right panel) and a leading order (LO) calculation based on $k_{\rm T}$-factorisation~\cite{Maciula:2013wg} (bottom-left panel). In the bottom-right panel, the ratios of the data to the three calculated cross sections are reported.
002153377 8564_ $$82229724$$s24942$$uhttp://cds.cern.ch/record/2153377/files/InvMassSpectra_pPb_bin0.png$$y00006 Invariant-mass distributions of $\DtoKpi$ candidates (and charge conjugates) in p--Pb collisions at $\sqrtsNN=5.02~\TeV$ for two $\pt$ intervals: $0&lt;\pt&lt;1~\gev/c$ (top panels) and $1&lt;\pt&lt;2~\gev/c$ (bottom panels). For both $\pt$ intervals, the left panels display the invariant-mass distribution of all ULS K$\pi$ pairs together with the background distributions estimated with the LS, event-mixing and track-rotation techniques. The middle and right panels show the invariant-mass distributions after subtraction of the background from the event-mixing and side-band fit techniques. Fit functions are superimposed.
002153377 8564_ $$82229725$$s39557$$uhttp://cds.cern.ch/record/2153377/files/Dzero-dsigmadpt-pPb.png$$y00016 $\pt$-differential production cross sections of prompt $\Dzero$ (top-left), $\Dplus$ (top-right), $\Dstar$ (bottom-left) and $\Ds$ (bottom-right) mesons with $-0.96&lt;y_{\rm cms}&lt;0.04$ in p--Pb collisions at $\sqrtsNN=5.02~\tev$, compared with the respective pp reference cross sections scaled by the Pb mass number $A=208$. For the $\Dzero$ meson, the results in $0&lt;\pt&lt;2~\gev/c$ are obtained from the analysis without decay-vertex reconstruction, while those in $2&lt;\pt&lt;24~\gev/c$ are taken from the analysis with decay-vertex reconstruction. The results from the other three D-meson species are the same as in Ref.~\cite{Abelev:2014hha}. For the p--Pb results, the systematic uncertainty of the feed-down correction is displayed separately.
002153377 8564_ $$82229726$$s10092$$uhttp://cds.cern.ch/record/2153377/files/figures_AccEff_pPb_WithTopol.png$$y00008 Product of acceptance and efficiency in p--Pb collisions. The ${\rm Acc}\times\epsilon$ values from the analysis with decay-vertex reconstruction were rescaled to account for the different fiducial acceptance, $y_{\rm fid}(\pt)$, selection on the $\Dzero$ rapidity.
002153377 8564_ $$82229727$$s11775$$uhttp://cds.cern.ch/record/2153377/files/RpA_TopolLowPt.png$$y00026 Comparison of the nuclear modification factors of prompt $\Dzero$ mesons as obtained in the analysis with decay-vertex reconstruction~\cite{Abelev:2014hha} and in the analysis without decay-vertex reconstruction.
002153377 8564_ $$82229728$$s11757$$uhttp://cds.cern.ch/record/2153377/files/figures_RpA_TopolLowPt.png$$y00028 Comparison of the nuclear modification factors of prompt $\Dzero$ mesons as obtained in the analysis with decay-vertex reconstruction~\cite{Abelev:2014hha} and in the analysis without decay-vertex reconstruction.
002153377 8564_ $$82229729$$s48638$$uhttp://cds.cern.ch/record/2153377/files/figures_pPbWithModelsCNM.png$$y00029 Nuclear modification factor $R_{\rm pPb}$ of prompt D mesons in p--Pb collisions at $\sqrtsNN=5.02~\tev$: average $R_{\rm pPb}$ of $\Dzero$, $\Dplus$ and $\Dstar$ mesons in the interval $1&lt;\pt&lt;24~\gev/c$~\cite{Abelev:2014hha}, shown together with the $\Dzero$ $R_{\rm pPb}$ in $0&lt;\pt&lt;1~\GeV/c$. In the left-hand panel, the data are compared with results of theoretical calculations including only CNM effects: CGC~\cite{Fujii:2013yja}, NLO pQCD~\cite{Mangano:1991jk} with EPS09 nPDFs~\cite{Eskola:2009uj}, a LO pQCD calculation with CNM effects (Vitev et al.)~\cite{Sharma:2009hn} and a calculation based on incoherent multiple scatterings (Kang et al.)~\cite{Kang:2014hha}. In the right-hand panel, the results of the Duke~\cite{Xu:2015iha} and POWLANG~\cite{Beraudo:2015wsd} transport models are compared to the measured D-meson $R_{\rm pPb}$.
002153377 8564_ $$82229730$$s25767$$uhttp://cds.cern.ch/record/2153377/files/figures_InvMassSpectra_pPb_bin1.png$$y00007 Invariant-mass distributions of $\DtoKpi$ candidates (and charge conjugates) in p--Pb collisions at $\sqrtsNN=5.02~\TeV$ for two $\pt$ intervals: $0&lt;\pt&lt;1~\gev/c$ (top panels) and $1&lt;\pt&lt;2~\gev/c$ (bottom panels). For both $\pt$ intervals, the left panels display the invariant-mass distribution of all ULS K$\pi$ pairs together with the background distributions estimated with the LS, event-mixing and track-rotation techniques. The middle and right panels show the invariant-mass distributions after subtraction of the background from the event-mixing and side-band fit techniques. Fit functions are superimposed.
002153377 8564_ $$82229731$$s25951$$uhttp://cds.cern.ch/record/2153377/files/figures_InvMassSpectra_pPb_bin0.png$$y00006 Invariant-mass distributions of $\DtoKpi$ candidates (and charge conjugates) in p--Pb collisions at $\sqrtsNN=5.02~\TeV$ for two $\pt$ intervals: $0&lt;\pt&lt;1~\gev/c$ (top panels) and $1&lt;\pt&lt;2~\gev/c$ (bottom panels). For both $\pt$ intervals, the left panels display the invariant-mass distribution of all ULS K$\pi$ pairs together with the background distributions estimated with the LS, event-mixing and track-rotation techniques. The middle and right panels show the invariant-mass distributions after subtraction of the background from the event-mixing and side-band fit techniques. Fit functions are superimposed.
002153377 8564_ $$82229732$$s12453$$uhttp://cds.cern.ch/record/2153377/files/figures_D0ppCrossSec.png$$y00009 $\pt$-differential production cross section of $\Dzero$ mesons with $|y|&lt;0.5$ in pp collisions at $\sqrt s =7~\tev$. Left: comparison of prompt and inclusive $\Dzero$ mesons (the latter including also $\Dzero$ mesons from beauty-hadron decays) from the analysis without decay-vertex reconstruction. Right: comparison between the prompt $\Dzero$ cross sections measured with~\cite{ALICE:2011aa} and without decay-vertex reconstruction. Here and in all the following figures the symbols are plotted at the centre of the $\pt$ intervals (shown by the horizontal lines), the vertical lines represent the statistical uncertainties and the vertical size of the boxes corresponds to the systematic uncertainties.
002153377 8564_ $$82229733$$s29203$$uhttp://cds.cern.ch/record/2153377/files/RpPb-D0plusStar.png$$y00024 Nuclear modification factor $R_{\rm pPb}$ of prompt D mesons in p--Pb collisions at $\sqrtsNN=5.02~\tev$~\cite{Abelev:2014hha}. Left: $R_{\rm pPb}$ of $\Dzero$, $\Dplus$ and $\Dstar$ mesons. Right: average $R_{\rm pPb}$ of the three non-strange D-meson species and $R_{\rm pPb}$ of $\Ds$ mesons. All results are obtained from the analysis with decay-vertex reconstruction.
002153377 8564_ $$82229734$$s15399$$uhttp://cds.cern.ch/record/2153377/files/figures_enercanvfull.png$$y00015 Total inclusive charm production cross section in nucleon--nucleon collisions as a function of $\sqrt{s}$~\cite{Lourenco:2006vw,Adare:2010de,Adamczyk:2012af,Aaij:2013mga,Abelev:2012vra,Aad:2015zix}. Data are from pA collisions for $\sqrt s&lt;100$~GeV and from pp collisions for $\sqrt s&gt;100$~GeV. Data from pA collisions were scaled by $1/A$. Results from NLO pQCD calculations (MNR~\cite{Mangano:1991jk}) and their uncertainties are shown as solid and dashed lines.
002153377 8564_ $$82229735$$s10092$$uhttp://cds.cern.ch/record/2153377/files/AccEff_pPb_WithTopol.png$$y00008 Product of acceptance and efficiency in p--Pb collisions. The ${\rm Acc}\times\epsilon$ values from the analysis with decay-vertex reconstruction were rescaled to account for the different fiducial acceptance, $y_{\rm fid}(\pt)$, selection on the $\Dzero$ rapidity.
002153377 8564_ $$82229736$$s24961$$uhttp://cds.cern.ch/record/2153377/files/figures_efficiencies_D0_vsPtvsY.png$$y00002 Product of acceptance and efficiency for $\Dzero$ mesons as a function of $\pt$ (left) and as a function of $y_{\rm lab}$ (right). In the left panel, efficiencies are shown for prompt $\Dzero$ with (solid line) and without (dashed line) PID selection applied, and feed-down $\Dzero$ (dotted line). In the right panel, the ${\rm Acc}\times\epsilon$ values are shown for prompt $\Dzero$ mesons for the three $\pt$ intervals considered in the analysis as a function of rapidity.
002153377 8564_ $$82229737$$s11864$$uhttp://cds.cern.ch/record/2153377/files/figures_D0ppCrossSecVsGMVFNS.png$$y00012 $\pt$-differential production cross section of prompt $\Dzero$ mesons with $|y|&lt;0.5$ in the interval $0&lt;\pt&lt;16~\gev/c$, in pp collisions at $\sqrt s =7~\tev$. The data points in $0&lt;\pt&lt;2~\gev/c$ are obtained from the analysis described in this article, while the data points in $2&lt;\pt&lt;16~\gev/c$ are taken from Ref~\cite{ALICE:2011aa}. The cross section is compared to three pQCD calculations: FONLL~\cite{Cacciari:2012ny} (top-left panel), GM-VFNS~\cite{Kniehl:2012ti} (top-right panel) and a leading order (LO) calculation based on $k_{\rm T}$-factorisation~\cite{Maciula:2013wg} (bottom-left panel). In the bottom-right panel, the ratios of the data to the three calculated cross sections are reported.
002153377 8564_ $$82229738$$s34148$$uhttp://cds.cern.ch/record/2153377/files/Dstar-dsigmadpt-pPb.png$$y00018 $\pt$-differential production cross sections of prompt $\Dzero$ (top-left), $\Dplus$ (top-right), $\Dstar$ (bottom-left) and $\Ds$ (bottom-right) mesons with $-0.96&lt;y_{\rm cms}&lt;0.04$ in p--Pb collisions at $\sqrtsNN=5.02~\tev$, compared with the respective pp reference cross sections scaled by the Pb mass number $A=208$. For the $\Dzero$ meson, the results in $0&lt;\pt&lt;2~\gev/c$ are obtained from the analysis without decay-vertex reconstruction, while those in $2&lt;\pt&lt;24~\gev/c$ are taken from the analysis with decay-vertex reconstruction. The results from the other three D-meson species are the same as in Ref.~\cite{Abelev:2014hha}. For the p--Pb results, the systematic uncertainty of the feed-down correction is displayed separately.
002153377 8564_ $$82229739$$s57926$$uhttp://cds.cern.ch/record/2153377/files/figures_InvMassSpectra_D0DplusDstarDs.png$$y00000 Distributions of the invariant mass for $\Dzero$ (top left), $\Dplus$ (top right), $\Ds$ (bottom left) candidates and their charge conjugates and of the mass difference for $\Dstar$ (bottom right) candidates (and charge conjugates) in the rapidity interval $|y_{\rm lab}|&lt;y_{\mathrm{fid}}(\pt)$ in p--Pb collisions. The dashed lines represent the fit to the background while the solid lines represent the total fit function. One $\pt$ interval is shown for each species: $1&lt;\pt&lt;2~\gevc$ for $\Dzero$, $5&lt;\pt&lt;6~\gevc$ for $\Dplus$, $8&lt;\pt&lt;12~\gevc$ for $\Ds$ and $16&lt;\pt&lt;24~\gevc$ for $\Dstar$.
002153377 8564_ $$82229740$$s13557$$uhttp://cds.cern.ch/record/2153377/files/figures_D0pPbCrossSecVsTopol.png$$y00017 $\pt$-differential production cross section of $\Dzero$ mesons with $-0.96&lt;y_{\rm cms}&lt;0.04$ in p--Pb collisions at $\sqrtsNN =5.02~\tev$. Left: comparison of prompt and inclusive $\Dzero$ mesons (the latter including also $\Dzero$ mesons from beauty-hadron decays) from the analysis without decay-vertex reconstruction. Right: comparison between the prompt $\Dzero$ cross sections measured with~\cite{Abelev:2014hha} and without decay-vertex reconstruction.
002153377 8564_ $$82229741$$s26188$$uhttp://cds.cern.ch/record/2153377/files/figures_InvMassSpectra_pp_bin0.png$$y00004 Invariant-mass distributions of $\DtoKpi$ candidates (and charge conjugates) in pp collisions at $\sqrts=7~\TeV$ for two $\pt$ intervals: $0&lt;\pt&lt;1~\gev/c$ (top panels) and $1&lt;\pt&lt;2~\gev/c$ (bottom panels). For both $\pt$ intervals, the left panels display the invariant-mass distribution of all ULS K$\pi$ pairs together with the background distributions estimated with the LS, event-mixing and track-rotation techniques. The middle and right panels show the invariant-mass distributions after subtraction of the background from the track-rotation and LS techniques. Fit functions are superimposed.
002153377 8564_ $$82229742$$s26249$$uhttp://cds.cern.ch/record/2153377/files/figures_InvMassSpectra_pp_bin1.png$$y00005 Invariant-mass distributions of $\DtoKpi$ candidates (and charge conjugates) in pp collisions at $\sqrts=7~\TeV$ for two $\pt$ intervals: $0&lt;\pt&lt;1~\gev/c$ (top panels) and $1&lt;\pt&lt;2~\gev/c$ (bottom panels). For both $\pt$ intervals, the left panels display the invariant-mass distribution of all ULS K$\pi$ pairs together with the background distributions estimated with the LS, event-mixing and track-rotation techniques. The middle and right panels show the invariant-mass distributions after subtraction of the background from the track-rotation and LS techniques. Fit functions are superimposed.
002153377 8564_ $$82229743$$s54037$$uhttp://cds.cern.ch/record/2153377/files/figures_InvMassSpectra_D0DplusDstar_Ybins.png$$y00001 Distributions of the invariant mass for $\Dzero$ (left column), $\Dplus$ (middle column) candidates and their charge conjugates and of the mass difference for $\Dstar$ (right column) candidates (and charge conjugates) in p--Pb collisions in the rapidity intervals $|y_{\rm lab}| &lt;0.1 $ (top row) and $-0.8 &lt; y_{\mathrm{lab}} &lt; -0.4$ ($-0.7 &lt; y_{\mathrm{lab}} &lt; -0.4$ for $\pt&lt;5~\gev/c$) (bottom row). The dashed lines represent the fit to the background while the solid lines represent the total fit function. One $\pt$ interval is shown for each species: $2&lt;\pt&lt;5~\gevc$ for $\Dzero$, $5&lt;\pt&lt;8~\gevc$ for $\Dplus$ and $8&lt;\pt&lt;16~\gevc$ for $\Dstar$.
002153377 8564_ $$82229744$$s35016$$uhttp://cds.cern.ch/record/2153377/files/Dmeson-Ratios-pp-pPb.png$$y00020 Ratios of prompt D-meson production cross sections as a function of $\pt$ in pp collisions at $\sqrt s=7~\tev$ ($|y_{\rm cms}|&lt;0.5$) and p--Pb collisions at $\sqrtsNN=5.02~\tev$ ($-0.96&lt;y_{\rm cms}&lt;0.04$).
002153377 8564_ $$82229745$$s38575$$uhttp://cds.cern.ch/record/2153377/files/DzeroWithFONLLAndEPS09.png$$y00021 Production cross sections as a function of rapidity ($y_{\rm cms}$) for prompt $\Dzero$, $\Dplus$ and $\Dstar$ mesons in p--Pb collisions at $\sqrtsNN=5.02~\tev$, for three $\pt$ intervals. The $\Dzero$-meson data are compared with a cross section obtained by multiplying the FONLL~\cite{Cacciari:2012ny} calculation by the mass number $A$ and the nuclear modification factor $R_{\rm pA}$ estimated as a function of $y$ with the MNR NLO pQCD calculation~\cite{Mangano:1991jk}, with CTEQ6M PDFs~\cite{Pumplin:2002vw} and the EPS09NLO nuclear PDF parametrisation~\cite{Eskola:2009uj}.
002153377 8564_ $$82229746$$s35062$$uhttp://cds.cern.ch/record/2153377/files/figures_pPbWithModelsMedium.png$$y00030 Nuclear modification factor $R_{\rm pPb}$ of prompt D mesons in p--Pb collisions at $\sqrtsNN=5.02~\tev$: average $R_{\rm pPb}$ of $\Dzero$, $\Dplus$ and $\Dstar$ mesons in the interval $1&lt;\pt&lt;24~\gev/c$~\cite{Abelev:2014hha}, shown together with the $\Dzero$ $R_{\rm pPb}$ in $0&lt;\pt&lt;1~\GeV/c$. In the left-hand panel, the data are compared with results of theoretical calculations including only CNM effects: CGC~\cite{Fujii:2013yja}, NLO pQCD~\cite{Mangano:1991jk} with EPS09 nPDFs~\cite{Eskola:2009uj}, a LO pQCD calculation with CNM effects (Vitev et al.)~\cite{Sharma:2009hn} and a calculation based on incoherent multiple scatterings (Kang et al.)~\cite{Kang:2014hha}. In the right-hand panel, the results of the Duke~\cite{Xu:2015iha} and POWLANG~\cite{Beraudo:2015wsd} transport models are compared to the measured D-meson $R_{\rm pPb}$.
002153377 8564_ $$82229747$$s30803$$uhttp://cds.cern.ch/record/2153377/files/Dplus-dsigmady-pPb.png$$y00022 Production cross sections as a function of rapidity ($y_{\rm cms}$) for prompt $\Dzero$, $\Dplus$ and $\Dstar$ mesons in p--Pb collisions at $\sqrtsNN=5.02~\tev$, for three $\pt$ intervals. The $\Dzero$-meson data are compared with a cross section obtained by multiplying the FONLL~\cite{Cacciari:2012ny} calculation by the mass number $A$ and the nuclear modification factor $R_{\rm pA}$ estimated as a function of $y$ with the MNR NLO pQCD calculation~\cite{Mangano:1991jk}, with CTEQ6M PDFs~\cite{Pumplin:2002vw} and the EPS09NLO nuclear PDF parametrisation~\cite{Eskola:2009uj}.
002153377 8564_ $$82229748$$s24961$$uhttp://cds.cern.ch/record/2153377/files/efficiencies_D0_vsPtvsY.png$$y00002 Product of acceptance and efficiency for $\Dzero$ mesons as a function of $\pt$ (left) and as a function of $y_{\rm lab}$ (right). In the left panel, efficiencies are shown for prompt $\Dzero$ with (solid line) and without (dashed line) PID selection applied, and feed-down $\Dzero$ (dotted line). In the right panel, the ${\rm Acc}\times\epsilon$ values are shown for prompt $\Dzero$ mesons for the three $\pt$ intervals considered in the analysis as a function of rapidity.
002153377 8564_ $$82229749$$s54554$$uhttp://cds.cern.ch/record/2153377/files/InvMassSpectra_D0DplusDstarDs.png$$y00000 Distributions of the invariant mass for $\Dzero$ (top left), $\Dplus$ (top right), $\Ds$ (bottom left) candidates and their charge conjugates and of the mass difference for $\Dstar$ (bottom right) candidates (and charge conjugates) in the rapidity interval $|y_{\rm lab}|&lt;y_{\mathrm{fid}}(\pt)$ in p--Pb collisions. The dashed lines represent the fit to the background while the solid lines represent the total fit function. One $\pt$ interval is shown for each species: $1&lt;\pt&lt;2~\gevc$ for $\Dzero$, $5&lt;\pt&lt;6~\gevc$ for $\Dplus$, $8&lt;\pt&lt;12~\gevc$ for $\Ds$ and $16&lt;\pt&lt;24~\gevc$ for $\Dstar$.
002153377 8564_ $$82229750$$s27907$$uhttp://cds.cern.ch/record/2153377/files/D0pPbCrossSec.png$$y00014 $\pt$-differential production cross section of $\Dzero$ mesons with $-0.96&lt;y_{\rm cms}&lt;0.04$ in p--Pb collisions at $\sqrtsNN =5.02~\tev$. Left: comparison of prompt and inclusive $\Dzero$ mesons (the latter including also $\Dzero$ mesons from beauty-hadron decays) from the analysis without decay-vertex reconstruction. Right: comparison between the prompt $\Dzero$ cross sections measured with~\cite{Abelev:2014hha} and without decay-vertex reconstruction.
002153377 8564_ $$82229751$$s14580$$uhttp://cds.cern.ch/record/2153377/files/Ds-dsigmadpt-pPb.png$$y00019 $\pt$-differential production cross sections of prompt $\Dzero$ (top-left), $\Dplus$ (top-right), $\Dstar$ (bottom-left) and $\Ds$ (bottom-right) mesons with $-0.96&lt;y_{\rm cms}&lt;0.04$ in p--Pb collisions at $\sqrtsNN=5.02~\tev$, compared with the respective pp reference cross sections scaled by the Pb mass number $A=208$. For the $\Dzero$ meson, the results in $0&lt;\pt&lt;2~\gev/c$ are obtained from the analysis without decay-vertex reconstruction, while those in $2&lt;\pt&lt;24~\gev/c$ are taken from the analysis with decay-vertex reconstruction. The results from the other three D-meson species are the same as in Ref.~\cite{Abelev:2014hha}. For the p--Pb results, the systematic uncertainty of the feed-down correction is displayed separately.
002153377 8564_ $$82229752$$s83424$$uhttp://cds.cern.ch/record/2153377/files/ImpParFitAndRes.png$$y00003 Left: Examples of fits to $\Dzero$ (top), $\Dplus$ (middle) and $\Dstar$ (bottom) impact-parameter distributions in the $\pt$ intervals $3&lt;\pt&lt;4~\gevc$, $5&lt;\pt&lt;6~\gevc$ and $6&lt;\pt&lt;8~\gevc$, respectively. The curves show the fit functions describing the prompt, feed-down and background contributions, as well as their sum, as described in the text. Right: fraction of prompt $\Dzero$ (top), $\Dplus$ (middle) and $\Dstar$ (bottom) raw yield as a function of $\pt$ compared to the FONLL-based approach. The results from the data-driven method are shown as square markers with the error bars (boxes) representing the statistical (systematic) uncertainty. The arrow in the interval $1&lt;\pt&lt;2~\gev/c$ represents the minimum value within a 95\% confidence level. The central values of $f_{\rm prompt}$ from the FONLL-based approach are shown by the dashed line and their uncertainty by the red boxes.
002153377 8564_ $$82229753$$s29203$$uhttp://cds.cern.ch/record/2153377/files/figures_RpPb-D0plusStar.png$$y00026 Nuclear modification factor $R_{\rm pPb}$ of prompt D mesons in p--Pb collisions at $\sqrtsNN=5.02~\tev$~\cite{Abelev:2014hha}. Left: $R_{\rm pPb}$ of $\Dzero$, $\Dplus$ and $\Dstar$ mesons. Right: average $R_{\rm pPb}$ of the three non-strange D-meson species and $R_{\rm pPb}$ of $\Ds$ mesons. All results are obtained from the analysis with decay-vertex reconstruction.
002153377 8564_ $$82229754$$s28138$$uhttp://cds.cern.ch/record/2153377/files/figures_D0pPbCrossSec.png$$y00016 $\pt$-differential production cross section of $\Dzero$ mesons with $-0.96&lt;y_{\rm cms}&lt;0.04$ in p--Pb collisions at $\sqrtsNN =5.02~\tev$. Left: comparison of prompt and inclusive $\Dzero$ mesons (the latter including also $\Dzero$ mesons from beauty-hadron decays) from the analysis without decay-vertex reconstruction. Right: comparison between the prompt $\Dzero$ cross sections measured with~\cite{Abelev:2014hha} and without decay-vertex reconstruction.
002153377 8564_ $$82229755$$s24853$$uhttp://cds.cern.ch/record/2153377/files/InvMassSpectra_pPb_bin1.png$$y00007 Invariant-mass distributions of $\DtoKpi$ candidates (and charge conjugates) in p--Pb collisions at $\sqrtsNN=5.02~\TeV$ for two $\pt$ intervals: $0&lt;\pt&lt;1~\gev/c$ (top panels) and $1&lt;\pt&lt;2~\gev/c$ (bottom panels). For both $\pt$ intervals, the left panels display the invariant-mass distribution of all ULS K$\pi$ pairs together with the background distributions estimated with the LS, event-mixing and track-rotation techniques. The middle and right panels show the invariant-mass distributions after subtraction of the background from the event-mixing and side-band fit techniques. Fit functions are superimposed.
002153377 8564_ $$82229756$$s38172$$uhttp://cds.cern.ch/record/2153377/files/figures_Dmeson-Ratios-pp-pPb.png$$y00022 Ratios of prompt D-meson production cross sections as a function of $\pt$ in pp collisions at $\sqrt s=7~\tev$ ($|y_{\rm cms}|&lt;0.5$) and p--Pb collisions at $\sqrtsNN=5.02~\tev$ ($-0.96&lt;y_{\rm cms}&lt;0.04$).
002153377 8564_ $$82229757$$s25221$$uhttp://cds.cern.ch/record/2153377/files/InvMassSpectra_pp_bin0.png$$y00004 Invariant-mass distributions of $\DtoKpi$ candidates (and charge conjugates) in pp collisions at $\sqrts=7~\TeV$ for two $\pt$ intervals: $0&lt;\pt&lt;1~\gev/c$ (top panels) and $1&lt;\pt&lt;2~\gev/c$ (bottom panels). For both $\pt$ intervals, the left panels display the invariant-mass distribution of all ULS K$\pi$ pairs together with the background distributions estimated with the LS, event-mixing and track-rotation techniques. The middle and right panels show the invariant-mass distributions after subtraction of the background from the track-rotation and LS techniques. Fit functions are superimposed.
002153377 8564_ $$82229758$$s12495$$uhttp://cds.cern.ch/record/2153377/files/figures_D0ppCrossSecVsTopol.png$$y00010 $\pt$-differential production cross section of $\Dzero$ mesons with $|y|&lt;0.5$ in pp collisions at $\sqrt s =7~\tev$. Left: comparison of prompt and inclusive $\Dzero$ mesons (the latter including also $\Dzero$ mesons from beauty-hadron decays) from the analysis without decay-vertex reconstruction. Right: comparison between the prompt $\Dzero$ cross sections measured with~\cite{ALICE:2011aa} and without decay-vertex reconstruction. Here and in all the following figures the symbols are plotted at the centre of the $\pt$ intervals (shown by the horizontal lines), the vertical lines represent the statistical uncertainties and the vertical size of the boxes corresponds to the systematic uncertainties.
002153377 8564_ $$82229759$$s38909$$uhttp://cds.cern.ch/record/2153377/files/figures_DzeroWithFONLLAndEPS09.png$$y00023 Production cross sections as a function of rapidity ($y_{\rm cms}$) for prompt $\Dzero$, $\Dplus$ and $\Dstar$ mesons in p--Pb collisions at $\sqrtsNN=5.02~\tev$, for three $\pt$ intervals. The $\Dzero$-meson data are compared with a cross section obtained by multiplying the FONLL~\cite{Cacciari:2012ny} calculation by the mass number $A$ and the nuclear modification factor $R_{\rm pA}$ estimated as a function of $y$ with the MNR NLO pQCD calculation~\cite{Mangano:1991jk}, with CTEQ6M PDFs~\cite{Pumplin:2002vw} and the EPS09NLO nuclear PDF parametrisation~\cite{Eskola:2009uj}.
002153377 8564_ $$82229760$$s13428$$uhttp://cds.cern.ch/record/2153377/files/D0pPbCrossSecVsTopol.png$$y00015 $\pt$-differential production cross section of $\Dzero$ mesons with $-0.96&lt;y_{\rm cms}&lt;0.04$ in p--Pb collisions at $\sqrtsNN =5.02~\tev$. Left: comparison of prompt and inclusive $\Dzero$ mesons (the latter including also $\Dzero$ mesons from beauty-hadron decays) from the analysis without decay-vertex reconstruction. Right: comparison between the prompt $\Dzero$ cross sections measured with~\cite{Abelev:2014hha} and without decay-vertex reconstruction.
002153377 8564_ $$82229761$$s12462$$uhttp://cds.cern.ch/record/2153377/files/D0ppCrossSecVsTopol.png$$y00010 $\pt$-differential production cross section of $\Dzero$ mesons with $|y|&lt;0.5$ in pp collisions at $\sqrt s =7~\tev$. Left: comparison of prompt and inclusive $\Dzero$ mesons (the latter including also $\Dzero$ mesons from beauty-hadron decays) from the analysis without decay-vertex reconstruction. Right: comparison between the prompt $\Dzero$ cross sections measured with~\cite{ALICE:2011aa} and without decay-vertex reconstruction. Here and in all the following figures the symbols are plotted at the centre of the $\pt$ intervals (shown by the horizontal lines), the vertical lines represent the statistical uncertainties and the vertical size of the boxes corresponds to the systematic uncertainties.
002153377 8564_ $$82229762$$s30874$$uhttp://cds.cern.ch/record/2153377/files/figures_D0ppCrossSecRatioTopQCD.png$$y00014 $\pt$-differential production cross section of prompt $\Dzero$ mesons with $|y|&lt;0.5$ in the interval $0&lt;\pt&lt;16~\gev/c$, in pp collisions at $\sqrt s =7~\tev$. The data points in $0&lt;\pt&lt;2~\gev/c$ are obtained from the analysis described in this article, while the data points in $2&lt;\pt&lt;16~\gev/c$ are taken from Ref~\cite{ALICE:2011aa}. The cross section is compared to three pQCD calculations: FONLL~\cite{Cacciari:2012ny} (top-left panel), GM-VFNS~\cite{Kniehl:2012ti} (top-right panel) and a leading order (LO) calculation based on $k_{\rm T}$-factorisation~\cite{Maciula:2013wg} (bottom-left panel). In the bottom-right panel, the ratios of the data to the three calculated cross sections are reported.
002153377 8564_ $$82229763$$s30736$$uhttp://cds.cern.ch/record/2153377/files/Dstar-dsigmady-pPb.png$$y00023 Production cross sections as a function of rapidity ($y_{\rm cms}$) for prompt $\Dzero$, $\Dplus$ and $\Dstar$ mesons in p--Pb collisions at $\sqrtsNN=5.02~\tev$, for three $\pt$ intervals. The $\Dzero$-meson data are compared with a cross section obtained by multiplying the FONLL~\cite{Cacciari:2012ny} calculation by the mass number $A$ and the nuclear modification factor $R_{\rm pA}$ estimated as a function of $y$ with the MNR NLO pQCD calculation~\cite{Mangano:1991jk}, with CTEQ6M PDFs~\cite{Pumplin:2002vw} and the EPS09NLO nuclear PDF parametrisation~\cite{Eskola:2009uj}.
002153377 8564_ $$82229764$$s32037$$uhttp://cds.cern.ch/record/2153377/files/figures_Ds-dsigmadpt-pPb.png$$y00021 $\pt$-differential production cross sections of prompt $\Dzero$ (top-left), $\Dplus$ (top-right), $\Dstar$ (bottom-left) and $\Ds$ (bottom-right) mesons with $-0.96&lt;y_{\rm cms}&lt;0.04$ in p--Pb collisions at $\sqrtsNN=5.02~\tev$, compared with the respective pp reference cross sections scaled by the Pb mass number $A=208$. For the $\Dzero$ meson, the results in $0&lt;\pt&lt;2~\gev/c$ are obtained from the analysis without decay-vertex reconstruction, while those in $2&lt;\pt&lt;24~\gev/c$ are taken from the analysis with decay-vertex reconstruction. The results from the other three D-meson species are the same as in Ref.~\cite{Abelev:2014hha}. The systematic uncertainty of the feed-down correction is displayed separately.
002153377 8564_ $$82229765$$s83567$$uhttp://cds.cern.ch/record/2153377/files/figures_ImpParFitAndRes.png$$y00003 Left: Examples of fits to $\Dzero$ (top), $\Dplus$ (middle) and $\Dstar$ (bottom) impact-parameter distributions in the $\pt$ intervals $3&lt;\pt&lt;4~\gevc$, $5&lt;\pt&lt;6~\gevc$ and $6&lt;\pt&lt;8~\gevc$, respectively. The curves show the fit functions describing the prompt, feed-down and background contributions, as well as their sum, as described in the text. Right: fraction of prompt $\Dzero$ (top), $\Dplus$ (middle) and $\Dstar$ (bottom) raw yield as a function of $\pt$ compared to the FONLL-based approach. The results from the data-driven method are shown as square markers with the error bars (boxes) representing the statistical (systematic) uncertainty. The arrow in the interval $1&lt;\pt&lt;2~\gev/c$ represents the minimum value within a 95\% confidence level. The central values of $f_{\rm prompt}$ from the FONLL-based approach are shown by the dashed line and their uncertainty by the red boxes.
002153377 8564_ $$82229766$$s30694$$uhttp://cds.cern.ch/record/2153377/files/figures_Dplus-dsigmady-pPb.png$$y00024 Production cross sections as a function of rapidity ($y_{\rm cms}$) for prompt $\Dzero$, $\Dplus$ and $\Dstar$ mesons in p--Pb collisions at $\sqrtsNN=5.02~\tev$, for three $\pt$ intervals. The $\Dzero$-meson data are compared with a cross section obtained by multiplying the FONLL~\cite{Cacciari:2012ny} calculation by the mass number $A$ and the nuclear modification factor $R_{\rm pA}$ estimated as a function of $y$ with the MNR NLO pQCD calculation~\cite{Mangano:1991jk}, with CTEQ6M PDFs~\cite{Pumplin:2002vw} and the EPS09NLO nuclear PDF parametrisation~\cite{Eskola:2009uj}.
002153377 8564_ $$82229767$$s34360$$uhttp://cds.cern.ch/record/2153377/files/Dplus-dsigmadpt-pPb.png$$y00017 $\pt$-differential production cross sections of prompt $\Dzero$ (top-left), $\Dplus$ (top-right), $\Dstar$ (bottom-left) and $\Ds$ (bottom-right) mesons with $-0.96&lt;y_{\rm cms}&lt;0.04$ in p--Pb collisions at $\sqrtsNN=5.02~\tev$, compared with the respective pp reference cross sections scaled by the Pb mass number $A=208$. For the $\Dzero$ meson, the results in $0&lt;\pt&lt;2~\gev/c$ are obtained from the analysis without decay-vertex reconstruction, while those in $2&lt;\pt&lt;24~\gev/c$ are taken from the analysis with decay-vertex reconstruction. The results from the other three D-meson species are the same as in Ref.~\cite{Abelev:2014hha}. For the p--Pb results, the systematic uncertainty of the feed-down correction is displayed separately.
002153377 9031_ $$aApproval requested for number CERN-EP-2016-127$$bCERN-EP-2016-127$$cEPPHAPP$$d2016-05-16 20:18:42$$e2016-05-23 20:18:42$$fenrico.scomparin@cern.ch$$swaiting
002153377 9031_ $$aDocument approved$$bCERN-EP-2016-127$$cEPPHAPP$$d2016-05-20 23:07:18$$froger.forty@cern.ch$$sapproved
002153377 916__ $$sn$$w201620
002153377 960__ $$a13
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