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dc.contributor.authorCasarosa G.en_US
dc.contributor.authorAihara H.en_US
dc.contributor.authorAziz T.en_US
dc.contributor.authorBacher S.en_US
dc.contributor.authorBahinipati S.en_US
dc.contributor.authorBarberio E.en_US
dc.contributor.authorBaroncelli T.en_US
dc.contributor.authorBaroncelli T.en_US
dc.contributor.authorBasith A.K.en_US
dc.contributor.authorBatignani G.en_US
dc.contributor.authorBauer A.en_US
dc.contributor.authorBehera P.K.en_US
dc.contributor.authorBertacchi V.en_US
dc.contributor.authorBettarini S.en_US
dc.contributor.authorBhuyan B.en_US
dc.contributor.authorBilka T.en_US
dc.contributor.authorBosi F.en_US
dc.contributor.authorBosisio L.en_US
dc.contributor.authorBozek A.en_US
dc.contributor.authorBuchsteiner F.en_US
dc.contributor.authorCaria G.en_US
dc.contributor.authorCeccanti M.en_US
dc.contributor.author?ervenkov D.en_US
dc.contributor.authorCorona L.en_US
dc.contributor.authorCzank T.en_US
dc.contributor.authorDash N.en_US
dc.contributor.authorDe Nuccio M.en_US
dc.contributor.authorDole�al Z.en_US
dc.contributor.authorForti F.en_US
dc.contributor.authorFriedl M.en_US
dc.contributor.authorGobbo B.en_US
dc.contributor.authorGrimaldo J.A.M.en_US
dc.contributor.authorHalder S.en_US
dc.contributor.authorHara K.en_US
dc.contributor.authorHiguchi T.en_US
dc.contributor.authorIrmler C.en_US
dc.contributor.authorIshikawa A.en_US
dc.contributor.authorJeon H.B.en_US
dc.contributor.authorJoo C.en_US
dc.contributor.authorKaleta M.en_US
dc.contributor.authorKandra J.en_US
dc.contributor.authorKang K.H.en_US
dc.contributor.authorKody� P.en_US
dc.contributor.authorKohriki T.en_US
dc.contributor.authorKomarov I.en_US
dc.contributor.authorKumar M.en_US
dc.contributor.authorKumar R.en_US
dc.contributor.authorKvasni?ka P.en_US
dc.contributor.authorLa Licata C.en_US
dc.contributor.authorLalwani K.en_US
dc.contributor.authorLanceri L.en_US
dc.contributor.authorLee J.Y.en_US
dc.contributor.authorLee S.C.en_US
dc.contributor.authorLi Y.en_US
dc.contributor.authorLibby J.en_US
dc.contributor.authorLueck T.en_US
dc.contributor.authorMammini P.en_US
dc.contributor.authorMartini A.en_US
dc.contributor.authorMayekar S.N.en_US
dc.contributor.authorMohanty G.B.en_US
dc.contributor.authorMorii T.en_US
dc.contributor.authorNakamura K.R.en_US
dc.contributor.authorNatkaniec Z.en_US
dc.contributor.authorOnuki Y.en_US
dc.contributor.authorOstrowicz W.en_US
dc.contributor.authorPaladino A.en_US
dc.contributor.authorPaoloni E.en_US
dc.contributor.authorPark H.en_US
dc.contributor.authorPrasanth K.en_US
dc.contributor.authorProfeti A.en_US
dc.contributor.authorRao K.K.en_US
dc.contributor.authorRashevskaya I.en_US
dc.contributor.authorResmi P.K.en_US
dc.contributor.authorRizzo G.en_US
dc.contributor.authorRozanska M.en_US
dc.contributor.authorSahoo D.en_US
dc.contributor.authorSasaki J.en_US
dc.contributor.authorSato N.en_US
dc.contributor.authorSchultschik S.en_US
dc.contributor.authorSchwanda C.en_US
dc.contributor.authorStypula J.en_US
dc.contributor.authorSuzuki J.en_US
dc.contributor.authorTanaka S.en_US
dc.contributor.authorTanigawa H.en_US
dc.contributor.authorTaylor G.N.en_US
dc.contributor.authorThalmeier R.en_US
dc.contributor.authorTsuboyama T.en_US
dc.contributor.authorUrquijo P.en_US
dc.contributor.authorVitale L.en_US
dc.contributor.authorWan K.en_US
dc.contributor.authorWatanabe M.en_US
dc.contributor.authorWatanuki S.en_US
dc.contributor.authorWatson I.J.en_US
dc.contributor.authorWebb J.en_US
dc.contributor.authorWiechczynski J.en_US
dc.contributor.authorWilliams S.en_US
dc.contributor.authorYin H.en_US
dc.contributor.authorZani L.en_US
dc.contributor.authorBelle II SVD Collaborationen_US
dc.date.accessioned2020-01-16T06:11:27Z-
dc.date.available2020-01-16T06:11:27Z-
dc.date.issued2019-
dc.identifier.urihttp://dx.doi.org/10.1016/j.nima.2019.05.025-
dc.identifier.urihttp://10.10.32.48:8080/jspui/handle/2008/2498-
dc.description.abstractThe Belle II experiment at the SuperKEKB collider of KEK (Japan) will accumulate 50 ab?1 of e+e- collision data at an unprecedented instantaneous luminosity of 8? 1035 cm?2s?1, about 40 times larger than its predecessor. The Belle II vertex detector plays a crucial role in the rich Belle II physics program, especially for time-dependent measurements. It consists of two layers of DEPFET-based pixels and four layers of double sided silicon strip sensors (SVD detector). We report here results of the standalone commissioning of the SVD and highlights from the first cosmic runs acquired in Belle II. We also report on reconstruction performances of a reduced-scale version of the SVD operated during the accelerator commissioning in 2018. � 2019en_US
dc.language.isoenen_US
dc.subjectCommissioningen_US
dc.subjectStrip detectoren_US
dc.subjectVertex detectoren_US
dc.titleCommissioning of the Belle II Silicon Vertex Detectoren_US
dc.typeArticleen_US
Appears in Collections:Research Publications

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