CERN Accelerating science

000567322 001__ 567322
000567322 003__ SzGeCERN
000567322 005__ 20210715034623.0
000567322 0247_ $$2DOI$$a10.1016/S0168-9002(01)01229-3
000567322 0248_ $$aoai:cds.cern.ch:567322$$pcerncds:FULLTEXT$$pcerncds:CERN:FULLTEXT$$pcerncds:CERN
000567322 035__ $$9CERCER$$a2325198
000567322 035__ $$9INSPEC$$a7278073
000567322 035__ $$9CERN annual report$$a2002-3.0801
000567322 035__ $$9Inspire$$a554879
000567322 037__ $$9arXiv$$ahep-ex/0104002$$chep-ex
000567322 041__ $$aeng
000567322 100__ $$aAkhmadalev, S.
000567322 245__ $$aHadron energy reconstruction for the ATLAS calorimetry in the framework of the nonparametrical method
000567322 246__ $$aA TOROIDAL LHC APPARATUS
000567322 246__ $$aLARGE HADRON COLLIDER
000567322 260__ $$c2002
000567322 269__ $$c2001-04
000567322 300__ $$a33 p
000567322 500__ $$9arXiv$$a33 pages, 13 figures, Will be published in NIMA
000567322 520__ $$aThis paper discusses hadron energy reconstruction for the ATLAS barrel prototype combined calorimeter (consisting of a lead-liquid argon electromagnetic part and an iron-scintillator hadronic part) in the framework of the nonparametrical method. The nonparametrical method utilizes only the known e/h ratios and the electron calibration constants and does not require the determination of any parameters by a minimization technique. Thus, this technique lends itself to an easy use in a first level trigger. The reconstructed mean values of the hadron energies are within +or-1% of the true values and the fractional energy resolution is [(58+or-3)%/ square root E+(2.5+or-0.3)%](+)(1.7+or-0.2)/E. The value of the e/h ratio obtained for the electromagnetic compartment of the combined calorimeter is 1.74+or-0.04 and agrees with the prediction that e/h >1.66 for this electromagnetic calorimeter. Results of a study of the longitudinal hadronic shower development are also presented. The data have been taken in the H8 beam line of the CERN SPS using pions of energies from 10 to 300 GeV. (32 refs).
000567322 520__ $$9arXiv$$aThis paper discusses hadron energy reconstruction for the ATLAS barrel prototype combined calorimeter (consisting of a lead-liquid argon electromagnetic part and an iron-scintillator hadronic part) in the framework of the non-parametrical method. The non-parametrical method utilizes only the known $e/h$ ratios and the electron calibration constants and does not require the determination of any parameters by a minimization technique. Thus, this technique lends itself to an easy use in a first level trigger. The reconstructed mean values of the hadron energies are within $\pm 1%$ of the true values and the fractional energy resolution is $[(58\pm3)% /\sqrt{E}+(2.5\pm0.3)%]\oplus (1.7\pm0.2)/E$. The value of the $e/h$ ratio obtained for the electromagnetic compartment of the combined calorimeter is $1.74\pm0.04$ and agrees with the prediction that $e/h > 1.7$ for this electromagnetic calorimeter. Results of a study of the longitudinal hadronic shower development are also presented. The data have been taken in the H8 beam line of the CERN SPS using pions of energies from 10 to 300 GeV.
000567322 595__ $$aSIS INSP2002
000567322 595__ $$i7278073
000567322 65017 $$2SzGeCERN$$aDetectors and Experimental Techniques
000567322 690C_ $$aARTICLE
000567322 690C_ $$aCERN
000567322 694__ $$9INSPEC$$aA2940M (Scintillation detectors; scintillators and photomultipliers)
000567322 694__ $$9INSPEC$$aA2970G (Energy loss and energy range relations in radiation measurement)
000567322 694__ $$9INSPEC$$aA2940B (Ionisation chambers)
000567322 694__ $$9INSPEC$$aA0620H (Measurement standards and calibration)
000567322 693__ $$aCERN LHC$$eATLAS
000567322 694__ $$9INSPEC$$aB7420 (Particle and radiation detection and measurement)
000567322 693__ $$aCERN SPS$$bH8
000567322 694__ $$9INSPEC$$aCI Ar el; Pb el; Fe el
000567322 694__ $$9INSPEC$$aNI electron volt energy: 1
000567322 695__ $$9INSPEC$$acalibration
000567322 695__ $$9INSPEC$$acalorimeters
000567322 695__ $$9INSPEC$$aliquid-ionisation-chambers
000567322 695__ $$9INSPEC$$aparticle-calorimetry
000567322 695__ $$9INSPEC$$asolid-scintillation-detectors
000567322 700__ $$aAmaral, P.$$iINSPIRE-00229165
000567322 700__ $$aAmbrosini, G.
000567322 700__ $$aAmorim, A.$$iINSPIRE-00210710
000567322 700__ $$aAnderson, K.$$iINSPIRE-00210757
000567322 700__ $$aAndrieux, M.L.$$iINSPIRE-00229181
000567322 700__ $$aAubert, Bernard$$iINSPIRE-00063251
000567322 700__ $$aAuge, E.$$iINSPIRE-00063283
000567322 700__ $$aBadaud, F.$$iINSPIRE-00063691
000567322 700__ $$aBaisin, L.
000567322 700__ $$aBarreiro, F.$$iINSPIRE-00064758
000567322 700__ $$aBattistoni, G.$$iINSPIRE-00065157
000567322 700__ $$aBazan, A.$$iINSPIRE-00387751
000567322 700__ $$aBazizi, K.
000567322 700__ $$aBelymam, A.
000567322 700__ $$aBenchekroun, D.$$iINSPIRE-00211372
000567322 700__ $$aBerglund, S.
000567322 700__ $$aBerset, J.C.
000567322 700__ $$aBlanchot, G.$$iINSPIRE-00179599
000567322 700__ $$aBogush, A.
000567322 700__ $$aBohm, C.$$iINSPIRE-00324763
000567322 700__ $$aBoldea, V.$$iINSPIRE-00305639
000567322 700__ $$aBonivento, W.
000567322 700__ $$aBosman, M.$$iINSPIRE-00227227
000567322 700__ $$aBouhemaid, N.
000567322 700__ $$aBreton, D.$$iINSPIRE-00229422
000567322 700__ $$aBrette, P.
000567322 700__ $$aBromberg, C.$$iINSPIRE-00069431
000567322 700__ $$aBudagov, J.$$iINSPIRE-00211819
000567322 700__ $$aBurdin, S.$$iINSPIRE-00022855
000567322 700__ $$aCaloba, L.$$iINSPIRE-00211947
000567322 700__ $$aCamarena, F.
000567322 700__ $$aCamin, D.V.
000567322 700__ $$aCanton, B.
000567322 700__ $$aCaprini, M.$$iINSPIRE-00211990
000567322 700__ $$aCarvalho, J.
000567322 700__ $$aCasado, P.$$iINSPIRE-00071410
000567322 700__ $$aCastillo, M.V.$$iINSPIRE-00212120
000567322 700__ $$aCavalli, D.$$iINSPIRE-00212386
000567322 700__ $$aCavalli-Sforza, M.$$iINSPIRE-00071735
000567322 700__ $$aCavasinni, V.$$iINSPIRE-00212398
000567322 700__ $$aChadelas, R.
000567322 700__ $$aChalifour, M.
000567322 700__ $$aShekhtman, Lev I.
000567322 700__ $$aChevalley, J.L.
000567322 700__ $$aChirikov-Zorin, I.
000567322 700__ $$aChlachidze, G.
000567322 700__ $$aCitterio, M.$$iINSPIRE-00339611
000567322 700__ $$aCleland, W.E.$$iINSPIRE-00171510
000567322 700__ $$aClement, C.$$iINSPIRE-00147062
000567322 700__ $$aCobal-Grassmann, Marina$$iINSPIRE-00073873
000567322 700__ $$aCogswell, F.
000567322 700__ $$aColas, J.$$iINSPIRE-00229740
000567322 700__ $$aCollot, Johann$$iINSPIRE-00074106
000567322 700__ $$aCologna, S.
000567322 700__ $$aConstantinescu, S.$$iINSPIRE-00212724
000567322 700__ $$aCosta, G.
000567322 700__ $$aCostanzo, D.$$iINSPIRE-00212803
000567322 700__ $$aCrouau, M.
000567322 700__ $$aDaudon, F.
000567322 700__ $$aDavid, J.
000567322 700__ $$aDavid, M.
000567322 700__ $$aDavidek, T.$$iINSPIRE-00075913
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000567322 700__ $$aDe, K.$$iINSPIRE-00300320
000567322 700__ $$aDe la Taille, C.$$iINSPIRE-00130254
000567322 700__ $$aDel Peso, J.$$iINSPIRE-00173501
000567322 700__ $$aDel Prete, T.$$iINSPIRE-00186417
000567322 700__ $$aDe Saintignon, P.$$iINSPIRE-00233349
000567322 700__ $$aDi Girolamo, B.$$iINSPIRE-00085048
000567322 700__ $$aDinkespiller, B.
000567322 700__ $$aDita, S.$$iINSPIRE-00306991
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000567322 700__ $$aDowning, R.
000567322 700__ $$aDugne, J.J.
000567322 700__ $$aDzahini, D.$$iINSPIRE-00230020
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000567322 700__ $$aEvans, H.$$iINSPIRE-00080060
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000567322 700__ $$aFassi, F.$$iINSPIRE-00308854
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000567322 700__ $$aFerrari, A.
000567322 700__ $$aFerrer, A.
000567322 700__ $$aFlaminio, V.
000567322 700__ $$aFournier, D.$$iINSPIRE-00144690
000567322 700__ $$aFumagalli, G.
000567322 700__ $$aGallas, E.$$iINSPIRE-00083337
000567322 700__ $$aGaspar, M.
000567322 700__ $$aGiakoumopoulou, V.$$iINSPIRE-00007684
000567322 700__ $$aGianotti, F.$$iINSPIRE-00084688
000567322 700__ $$aGildemeister, O.$$iINSPIRE-00230282
000567322 700__ $$aGiokaris, N.$$iINSPIRE-00084938
000567322 700__ $$aGlagolev, V.
000567322 700__ $$aGlebov, V.
000567322 700__ $$aGomes, A.$$iINSPIRE-00226662
000567322 700__ $$aGonzalez, V.
000567322 700__ $$aGonzalez De La Hoz, S.$$iINSPIRE-00214978
000567322 700__ $$aGrabsky, V.
000567322 700__ $$aGrauges, E.
000567322 700__ $$aGrenier, P.$$iINSPIRE-00050339
000567322 700__ $$aHakopian, H.
000567322 700__ $$aHaney, M.
000567322 700__ $$aHebrard, C.
000567322 700__ $$aHenriques, A.$$iINSPIRE-00305891
000567322 700__ $$aHervas, L.$$iINSPIRE-00215643
000567322 700__ $$aHigon, E.$$iINSPIRE-00215655
000567322 700__ $$aHolmgren, S.$$iINSPIRE-00233421
000567322 700__ $$aHostachy, J.Y.$$iINSPIRE-00215837
000567322 700__ $$aHoummada, A.$$iINSPIRE-00215849
000567322 700__ $$aHuston, J.$$iINSPIRE-00091715
000567322 700__ $$aImbault, D.$$iINSPIRE-00230663
000567322 700__ $$aIvanyushenkov, Yu.
000567322 700__ $$aJenny, P.
000567322 700__ $$aJezequel, S.$$iINSPIRE-00216174
000567322 700__ $$aJohansson, Erik Karl$$iINSPIRE-00216255
000567322 700__ $$aJon-And, Kerstin B.$$iINSPIRE-00180510
000567322 700__ $$aJones, R.
000567322 700__ $$aJuste, A.$$iINSPIRE-00094149
000567322 700__ $$aKakurin, S.
000567322 700__ $$aKaryukhin, A.$$iINSPIRE-00216469
000567322 700__ $$aKhokhlov, Yu.A.
000567322 700__ $$aKhubua, J.$$iINSPIRE-00305959
000567322 700__ $$aKlyukhin, V.
000567322 700__ $$aKolachev, G.$$iINSPIRE-00230968
000567322 700__ $$aKopikov, S.$$iINSPIRE-00231000
000567322 700__ $$aKostrikov, M.
000567322 700__ $$aKozlov, V.
000567322 700__ $$aKrivkova, P.$$iINSPIRE-00478638
000567322 700__ $$aKukhtin, V.$$iINSPIRE-00218599
000567322 700__ $$aKulagin, M.
000567322 700__ $$aKulchitsky, Y.$$iINSPIRE-00098974
000567322 700__ $$aKuzmin, M.
000567322 700__ $$aLabarga, L.$$iINSPIRE-00099500
000567322 700__ $$aLaborie, G.
000567322 700__ $$aLacour, D.$$iINSPIRE-00099578
000567322 700__ $$aLaforge, B.$$iINSPIRE-00057788
000567322 700__ $$aLami, S.$$iINSPIRE-00099761
000567322 700__ $$aLapin, V.$$iINSPIRE-00231090
000567322 700__ $$aLe Dortz, O.$$iINSPIRE-00218897
000567322 700__ $$aLefebvre, M.$$iINSPIRE-00198481
000567322 700__ $$aLe Flour, T.
000567322 700__ $$aLeitner, R.$$iINSPIRE-00301106
000567322 700__ $$aLeltchouk, M.$$iINSPIRE-00231176
000567322 700__ $$aLi, J.
000567322 700__ $$aLiablin, M.
000567322 700__ $$aLinossier, O.
000567322 700__ $$aLissauer, D.$$iINSPIRE-00304230
000567322 700__ $$aLobkowicz, F.
000567322 700__ $$aLokajicek, M.$$iINSPIRE-00278790
000567322 700__ $$aLomakin, Yu.
000567322 700__ $$aLopez Amengual, J.M.
000567322 700__ $$aLund-Jensen, B.$$iINSPIRE-00103080
000567322 700__ $$aMaio, A.$$iINSPIRE-00219689
000567322 700__ $$aMakowiecki, D.
000567322 700__ $$aMalyukov, S.$$iINSPIRE-00219768
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000567322 700__ $$aMansoulie, B.$$iINSPIRE-00104458
000567322 700__ $$aMapelli, L.$$iINSPIRE-00219888
000567322 700__ $$aMarin, C.P.
000567322 700__ $$aMarrocchesi, P.
000567322 700__ $$aMarroquin, F.
000567322 700__ $$aMartin, P.
000567322 700__ $$aMaslennikov, A.$$iINSPIRE-00220055
000567322 700__ $$aMassol, N.$$iINSPIRE-00220073
000567322 700__ $$aMataix, L.
000567322 700__ $$aMazzanti, M.$$iINSPIRE-00231552
000567322 700__ $$aMazzoni, E.$$iINSPIRE-00231563
000567322 700__ $$aMerritt, F.$$iINSPIRE-00107035
000567322 700__ $$aMichel, B.
000567322 700__ $$aMiller, R.$$iINSPIRE-00107723
000567322 700__ $$aMinashvili, I.$$iINSPIRE-00306048
000567322 700__ $$aMiralles, L.$$iINSPIRE-00231694
000567322 700__ $$aMnatsakanian, E.
000567322 700__ $$aMonnier, E.$$iINSPIRE-00326813
000567322 700__ $$aMontarou, G.
000567322 700__ $$aMornacchi, G.$$iINSPIRE-00220784
000567322 700__ $$aMoynot, M.
000567322 700__ $$aMuanza, G.S.$$iINSPIRE-00109389
000567322 700__ $$aNayman, P.
000567322 700__ $$aNemecek, S.$$iINSPIRE-00110909
000567322 700__ $$aNessi, M.$$iINSPIRE-00221084
000567322 700__ $$aNicoleau, S.
000567322 700__ $$aNiculescu, M.
000567322 700__ $$aNoppe, J.M.
000567322 700__ $$aOnofre, A.$$iINSPIRE-00221372
000567322 700__ $$aPallin, D.$$iINSPIRE-00221552
000567322 700__ $$aPantea, D.$$iINSPIRE-00114319
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000567322 700__ $$aPark, I.C.
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000567322 700__ $$aParsons, J.$$iINSPIRE-00114789
000567322 700__ $$aPereira, A.
000567322 700__ $$aPerini, L.$$iINSPIRE-00221789
000567322 700__ $$aPerlas, J.A.
000567322 700__ $$aPerrodo, P.$$iINSPIRE-00232085
000567322 700__ $$aPilcher, J.$$iINSPIRE-00116477
000567322 700__ $$aPinhao, J.
000567322 700__ $$aPlothow-Besch, H.
000567322 700__ $$aPoggioli, L.$$iINSPIRE-00221996
000567322 700__ $$aPoirot, S.
000567322 700__ $$aPrice, L.$$iINSPIRE-00117710
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000567322 700__ $$aProudfoot, J.$$iINSPIRE-00117915
000567322 700__ $$aPuzo, P.$$iINSPIRE-00222199
000567322 700__ $$aRadeka, V.$$iINSPIRE-00304240
000567322 700__ $$aRahm, D.$$iINSPIRE-00118541
000567322 700__ $$aReinmuth, G.
000567322 700__ $$aRenzoni, G.
000567322 700__ $$aRescia, S.$$iINSPIRE-00304255
000567322 700__ $$aResconi, S.$$iINSPIRE-00222441
000567322 700__ $$aRichards, R.$$iINSPIRE-00119971
000567322 700__ $$aRicher, J.P.
000567322 700__ $$aRiu, I.$$iINSPIRE-00120419
000567322 700__ $$aRoda, C.$$iINSPIRE-00222584
000567322 700__ $$aRodier, S.$$iINSPIRE-00232287
000567322 700__ $$aRoldan, J.
000567322 700__ $$aRomance, J.B.
000567322 700__ $$aRomanov, V.$$iINSPIRE-00222655
000567322 700__ $$aRomero, P.
000567322 700__ $$aRossel, F.
000567322 700__ $$aRussakovich, N.$$iINSPIRE-00301212
000567322 700__ $$aSala, P.$$iINSPIRE-00122664
000567322 700__ $$aSanchis, E.$$iINSPIRE-00345218
000567322 700__ $$aSanders, H.
000567322 700__ $$aSantoni, C.$$iINSPIRE-00161887
000567322 700__ $$aSantos, J.
000567322 700__ $$aSauvage, D.
000567322 700__ $$aSauvage, G.$$iINSPIRE-00222998
000567322 700__ $$aSawyer, L.$$iINSPIRE-00123608
000567322 700__ $$aSays, L.P.$$iINSPIRE-00306241
000567322 700__ $$aSchaffer, A.C.$$iINSPIRE-00223168
000567322 700__ $$aSchwemling, P.$$iINSPIRE-00124725
000567322 700__ $$aSchwindling, J.$$iINSPIRE-00223337
000567322 700__ $$aSeguin-Moreau, N.
000567322 700__ $$aSeidl, W.
000567322 700__ $$aSeixas, J.M.$$iINSPIRE-00306265
000567322 700__ $$aSellden, B.$$iINSPIRE-00223427
000567322 700__ $$aSeman, M.$$iINSPIRE-00232481
000567322 700__ $$aSemenov, A.
000567322 700__ $$aSerin, L.$$iINSPIRE-00223468
000567322 700__ $$aShaldaev, E.
000567322 700__ $$aShochet, M.$$iINSPIRE-00126064
000567322 700__ $$aSidorov, V.$$iINSPIRE-00007941
000567322 700__ $$aSilva, J.
000567322 700__ $$aSimaitis, V.
000567322 700__ $$aSimion, S.$$iINSPIRE-00223610
000567322 700__ $$aSissakian, A.$$iINSPIRE-00003863
000567322 700__ $$aSnopkov, R.
000567322 700__ $$aSoderqvist, J.
000567322 700__ $$aSolodkov, Alexander A.$$iINSPIRE-00127668
000567322 700__ $$aSoloviev, A.
000567322 700__ $$aSoloviev, I.$$iINSPIRE-00390496
000567322 700__ $$aSonderegger, P.
000567322 700__ $$aSoustruznik, K.
000567322 700__ $$aSpano, F.$$iINSPIRE-00051714
000567322 700__ $$aSpiwoks, R.$$iINSPIRE-00223859
000567322 700__ $$aStanek, R.$$iINSPIRE-00128391
000567322 700__ $$aStarchenko, E.$$iINSPIRE-00223911
000567322 700__ $$aStavina, P.$$iINSPIRE-00223944
000567322 700__ $$aStephens, R.
000567322 700__ $$aSuk, M.$$iINSPIRE-00224089
000567322 700__ $$aSurkov, A.
000567322 700__ $$aSykora, I.$$iINSPIRE-00224134
000567322 700__ $$aTakai, H.$$iINSPIRE-99155656
000567322 700__ $$aTang, F.$$iINSPIRE-00380536
000567322 700__ $$aTardell, S.
000567322 700__ $$aTartarelli, F.$$iINSPIRE-00130743
000567322 700__ $$aTas, P.$$iINSPIRE-00306326
000567322 700__ $$aTeiger, J.
000567322 700__ $$aTeubert, F.
000567322 700__ $$aThaler, J.
000567322 700__ $$aThion, J.
000567322 700__ $$aTikhonov, Y.$$iINSPIRE-00198040
000567322 700__ $$aTisserant, S.$$iINSPIRE-00131587
000567322 700__ $$aTokar, S.$$iINSPIRE-00131686
000567322 700__ $$aTopilin, N.$$iINSPIRE-00224555
000567322 700__ $$aTrka, Z.
000567322 700__ $$aTurcotte, M.
000567322 700__ $$aValkar, S.$$iINSPIRE-00224924
000567322 700__ $$aVaranda, M.J.
000567322 700__ $$aVartapetian, A.$$iINSPIRE-00225055
000567322 700__ $$aVazeille, F.$$iINSPIRE-00225072
000567322 700__ $$aVichou, I.$$iINSPIRE-00161358
000567322 700__ $$aVinogradov, V.$$iINSPIRE-00227012
000567322 700__ $$aVorozhtsov, S.
000567322 700__ $$aVuillemin, V.
000567322 700__ $$aWhite, A.$$iINSPIRE-00013505
000567322 700__ $$aWielers, M.$$iINSPIRE-00225743
000567322 700__ $$aWingerter-Seez, I.$$iINSPIRE-00136245
000567322 700__ $$aWolters, H.$$iINSPIRE-00225832
000567322 700__ $$aYamdagni, N.
000567322 700__ $$aYosef, C.
000567322 700__ $$aZaitsev, A.$$iINSPIRE-00170475
000567322 700__ $$aZitoun, R.$$iINSPIRE-00233264
000567322 700__ $$aZolnierowski, Y.P.$$iINSPIRE-00233288
000567322 710__ $$gATLAS Collaboration
000567322 710__ $$5EP
000567322 773__ $$c508-23$$n2-3$$pNucl. Instrum. Methods Phys. Res., A$$v480$$y2002
000567322 8564_ $$81444890$$s28577$$uhttps://cds.cern.ch/record/567322/files/comb96_1.png$$y00002 Schematic layout of the experimental setup for the combined LAr and Tile calorimeters run (side view). The S3 and S4 are scintillation counters, the BC3 is a beam proportional chamber, and the midsampler and the ``muon wall'' are scintillation hodoscopes.
000567322 8564_ $$81444891$$s11655$$uhttps://cds.cern.ch/record/567322/files/epi_50.png$$y00005 The distributions of the $(e/\pi)_{LAr}$ ratio for beam energies of 20 and 50 GeV (top row, left to right), and beam energies of 100 and 300 GeV (bottom row, left to right).
000567322 8564_ $$81444892$$s511517$$uhttps://cds.cern.ch/record/567322/files/arXiv:hep-ex_0104002.pdf
000567322 8564_ $$81444893$$s16433$$uhttps://cds.cern.ch/record/567322/files/vpro-fig-our-long-conb-bock-26.png$$y00018 The experimental differential mean longitudinal energy depositions at 10 GeV (crosses), 20 GeV (black top triangles), 40 GeV (open squares), 50 GeV (black squares), 80 GeV (open circles), 100 GeV (black circles), 150 GeV (stars), 300 GeV (black bottom triangles) energies as a function of the longitudinal coordinate $z$ in units $\lambda_{\pi}$ for the combined calorimeter and the results of the description by the modified parameterization for the equation (\ref{elong03}).
000567322 8564_ $$81444894$$s18477$$uhttps://cds.cern.ch/record/567322/files/vpro-fig-our-long-conb-bock-27.png$$y00017 The comparison between the experimental differential mean energy depositions at 10 GeV (crosses), 20 GeV (black top triangles), 40 GeV (open squares), 50 GeV (black squares), 80 GeV (open circles), 100 GeV (black circles), 150 GeV (stars), 300 GeV (black bottom triangles) and the calculated curves (\ref{elong03}) as a function of the longitudinal coordinate $z$ in units $\lambda_{\pi}$. The errors on the data points are the errors of the mean values and there are within symbols size.
000567322 8564_ $$81444895$$s12551$$uhttps://cds.cern.ch/record/567322/files/epi_20.png$$y00004 The distributions of the $(e/\pi)_{LAr}$ ratio for beam energies of 20 and 50 GeV (top row, left to right), and beam energies of 100 and 300 GeV (bottom row, left to right).
000567322 8564_ $$81444896$$s12729$$uhttps://cds.cern.ch/record/567322/files/energy_50.png$$y00012 The energy distributions for beam energies of 20 and 50 GeV (top row, left to right), and beam energies of 100 and 300 GeV (bottom row, left to right).
000567322 8564_ $$81444897$$s12411$$uhttps://cds.cern.ch/record/567322/files/energy_100.png$$y00013 The energy distributions for beam energies of 20 and 50 GeV (top row, left to right), and beam energies of 100 and 300 GeV (bottom row, left to right).
000567322 8564_ $$81444898$$s9707$$uhttps://cds.cern.ch/record/567322/files/epi_300.png$$y00007 The distributions of the $(e/\pi)_{LAr}$ ratio for beam energies of 20 and 50 GeV (top row, left to right), and beam energies of 100 and 300 GeV (bottom row, left to right).
000567322 8564_ $$81444899$$s105359$$uhttps://cds.cern.ch/record/567322/files/chapter1_fig3.png$$y00001 Three-dimensional cutaway view of the ATLAS calorimeters.
000567322 8564_ $$81444900$$s11676$$uhttps://cds.cern.ch/record/567322/files/energy_20.png$$y00011 The energy distributions for beam energies of 20 and 50 GeV (top row, left to right), and beam energies of 100 and 300 GeV (bottom row, left to right).
000567322 8564_ $$81444901$$s11588$$uhttps://cds.cern.ch/record/567322/files/ehl_rd3_0.png$$y00009 The $(e/\pi)_{LAr}$ ratios as a function of the beam energy. for $e/h$ method (black circles) and for weighting method (open circles for \cite{stipcevic93} and open squares for \cite{Gingrich95}). The lines are the result of a fit of equations (\ref{ev10}) and (\ref{ev10-0}) with free $e/h$ parameter and $k=0.11$: solid line is for our data, dashed line is for the \cite{stipcevic93} data and dash-doted line is for the \cite{Gingrich95} data.
000567322 8564_ $$81444902$$s19155$$uhttps://cds.cern.ch/record/567322/files/lin-comb-s-01.png$$y00016 The energy resolutions obtained with the $e/h$ method (black circles), the benchmark method (crosses) and the cells weighting method (circles).
000567322 8564_ $$81444903$$s11680$$uhttps://cds.cern.ch/record/567322/files/lar-tile-en.png$$y00019 Energy deposition (percentage) in the LAr and Tile calorimeters at different beam energies. The circles (squares) are the measured energy depositions in the LAr (Tile) calorimeter, the diamonds (crosses) are the calculated energy depositions.
000567322 8564_ $$81444904$$s12250$$uhttps://cds.cern.ch/record/567322/files/energy_300.png$$y00014 The energy distributions for beam energies of 20 and 50 GeV (top row, left to right), and beam energies of 100 and 300 GeV (bottom row, left to right).
000567322 8564_ $$81444905$$s8505$$uhttps://cds.cern.ch/record/567322/files/lin-comb-010.png$$y00010 Energy linearity as a function of the beam energy for the $e/h$ method obtained using the iteration procedure with $\epsilon = 0.1\%$ (black circles) and with the first approximation (open circles).
000567322 8564_ $$81444906$$s33182$$uhttps://cds.cern.ch/record/567322/files/pro-fig28tp0.png$$y00003 Conceptual design of a Tile calorimeter module.
000567322 8564_ $$81444907$$s10806$$uhttps://cds.cern.ch/record/567322/files/epi_100.png$$y00006 The distributions of the $(e/\pi)_{LAr}$ ratio for beam energies of 20 and 50 GeV (top row, left to right), and beam energies of 100 and 300 GeV (bottom row, left to right).
000567322 8564_ $$81444908$$s9094$$uhttps://cds.cern.ch/record/567322/files/ehl.png$$y00008 The mean value of the $(e/\pi)_{LAr}$ ratio as a function of the beam energy. The curve is the result of a fit of equations (\ref{ev10}) and (\ref{ev10-0}).
000567322 8564_ $$81444909$$s10544$$uhttps://cds.cern.ch/record/567322/files/lin-comb-001.png$$y00015 Energy linearity as a function of the beam energy for the $e/h$ method (black circles) and the cells weighting method (open circles).
000567322 8564_ $$82306891$$s9563$$uhttps://cds.cern.ch/record/567322/files/fig00000.png$$y00000 noimg: Mean reconstructed energy, energy resolution and fractional energy resolution for the various beam energies.: The differential mean energy depositions $\Delta E/ \Delta z$ ($GeV/\lambda_\pi$) as a function of the longitudinal coordinate $z$ for the various beam energies.
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