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The Large Area Detector of LOFT: the Large Observatory for X-ray Timing

dc.contributor.authorZANE, S.
hal.structure.identifierMullard Space Science Laboratory [MSSL]
dc.contributor.authorWALTON, D.
dc.contributor.authorKENNEDY, T.
dc.contributor.authorFEROCI, M.
dc.contributor.authorHERDER, J. -W. Den
dc.contributor.authorAHANGARIANABHARI, M.
dc.contributor.authorARGAN, A.
dc.contributor.authorAZZARELLO, P.
dc.contributor.authorBALDAZZI, G.
dc.contributor.authorBARBERA, M.
dc.contributor.authorBARRET, D.
dc.contributor.authorBERTUCCIO, G.
dc.contributor.authorBODIN, P.
dc.contributor.authorBOZZO, E.
hal.structure.identifierMullard Space Science Laboratory [MSSL]
dc.contributor.authorBRADLEY, L.
dc.contributor.authorCADOUX, F.
hal.structure.identifierFORMATION STELLAIRE 2014
dc.contributor.authorCAIS, Ph.
dc.contributor.authorCAMPANA, R.
hal.structure.identifierMullard Space Science Laboratory [MSSL]
dc.contributor.authorCOKER, J.
hal.structure.identifierInteractions et dynamique des environnements de surface [IDES]
dc.contributor.authorCROS, A.
dc.contributor.authorDEL MONTE, E.
dc.contributor.authorDE ROSA, A.
dc.contributor.authorDI COSIMO, S.
dc.contributor.authorDONNARUMMA, I.
dc.contributor.authorEVANGELISTA, Y.
dc.contributor.authorFAVRE, Y.
dc.contributor.authorFELDMAN, C.
dc.contributor.authorFRASER, G.
dc.contributor.authorFUSCHINO, F.
dc.contributor.authorGRASSI, M.
dc.contributor.authorHAILEY, M. R.
dc.contributor.authorHUDEC, R.
dc.contributor.authorLABANTI, C.
dc.contributor.authorMACERA, D.
dc.contributor.authorMALCOVATI, P.
dc.contributor.authorMARISALDI, M.
dc.contributor.authorMARTINDALE, A.
dc.contributor.authorMINEO, T.
dc.contributor.authorMULERI, F.
dc.contributor.authorNOWAK, M.
dc.contributor.authorORLANDINI, M.
dc.contributor.authorPACCIANI, L.
dc.contributor.authorPERINATI, E.
dc.contributor.authorPETRACEK, V.
dc.contributor.authorPOHL, M.
dc.contributor.authorRACHEVSKI, A.
dc.contributor.authorSMITH, P.
dc.contributor.authorSANTANGELO, A.
hal.structure.identifierCentre National d'Études Spatiales [Toulouse] [CNES]
dc.contributor.authorSEYLER, J. -Y.
dc.contributor.authorSCHMID, C.
dc.contributor.authorSOFFITTA, P.
dc.contributor.authorSUCHY, S.
dc.contributor.authorTENZER, C.
dc.contributor.authorUTTLEY, P.
dc.contributor.authorVACCHI, A.
dc.contributor.authorZAMPA, G.
dc.contributor.authorZAMPA, N.
dc.contributor.authorWILMS, J.
dc.contributor.authorWINTER, B.
dc.date.created2014-08-27
dc.date.issued2014
dc.date.conference2014
dc.description.abstractEnLOFT (Large Observatory for X-ray Timing) is one of the five candidates that were considered by ESA as an M3 mission (with launch in 2022-2024) and has been studied during an extensive assessment phase. It is specifically designed to perform fast X-ray timing and probe the status of the matter near black holes and neutron stars. Its pointed instrument is the Large Area Detector (LAD), a 10 m 2 -class instrument operating in the 2-30keV range, which holds the capability to revolutionise studies of variability from X-ray sources on the millisecond time scales. The LAD instrument has now completed the assessment phase but was not down-selected for launch. However, during the assessment, most of the trade-offs have been closed leading to a robust and well documented design that will be re- proposed in future ESA calls. In this talk, we will summarize the characteristics of the LAD design and give an overview of the expectations for the instrument capabilities.
dc.language.isoen
dc.source.titleProc. SPIE 9144, Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray, 91442W; doi:10.1117/12.2054654- Montreal 22 au 27-06-2014
dc.title.enThe Large Area Detector of LOFT: the Large Observatory for X-ray Timing
dc.typeCommunication dans un congrès
dc.identifier.doi10.1117/12.2054654
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Instrumentation et méthodes pour l'astrophysique [astro-ph.IM]
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Instrumentation et méthodes pour l'astrophysique [astro-ph.IM]
dc.identifier.arxiv1408.6539
bordeaux.page-
bordeaux.volume9144
bordeaux.countryCA
bordeaux.title.proceedingProc. SPIE 9144, Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray, 91442W; doi:10.1117/12.2054654- Montreal 22 au 27-06-2014
bordeaux.conference.cityMontreal
bordeaux.peerReviewedoui
hal.identifierhal-01061592
hal.version1
hal.invitednon
hal.proceedingsoui
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01061592v1
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