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dc.date.accessioned2021-03-04T10:03:48Z
dc.date.available2021-03-04T10:03:48Z
dc.identifier.citationFeroci M., den Herder J. W. , Bozzo E., Barret D., Brandt S., Hernanz M., van der Klis M., Pohl M., Santangelo A., Stella L., et al., "The Large Observatory For x-ray Timing", Conference on Space Telescopes and Instrumentation - Ultraviolet to Gamma Ray, Montreal, Kanada, 22 - 26 Haziran 2014, cilt.9144
dc.identifier.othervv_1032021
dc.identifier.otherav_6b57a548-90e2-4032-80a6-35c800abf251
dc.identifier.urihttp://hdl.handle.net/20.500.12627/74232
dc.identifier.urihttps://doi.org/10.1117/12.2055913
dc.description.abstractThe Large Observatory For x-ray Timing (LOFT) was studied within ESA M3 Cosmic Vision framework and participated in the final downselection for a launch slot in 2022-2024. Thanks to the unprecedented combination of effective area and spectral resolution of its main instrument, LOFT will study the behaviour of matter under extreme conditions, such as the strong gravitational field in the innermost regions of accretion flows close to black holes and neutron stars, and the supranuclear densities in the interior of neutron stars. The science payload is based on a Large Area Detector (LAD, 10 m(2) effective area, 2-30 keV, 240 eV spectral resolution, 1 degrees collimated field of view) and a Wide Field Monitor (WFM, 2-50 keV, 4 steradian field of view, 1 arcmin source location accuracy, 300 eV spectral resolution). The WFM is equipped with an on-board system for bright events (e.g. GRB) localization. The trigger time and position of these events are broadcast to the ground within 30 s from discovery. In this paper we present the status of the mission at the end of its Phase A study.
dc.language.isoeng
dc.subjectTemel Bilimler (SCI)
dc.subjectALETLER & GÖSTERİM
dc.subjectMühendislik
dc.subjectMühendislik, Bilişim ve Teknoloji (ENG)
dc.subjectOPTİK
dc.subjectFizik
dc.subjectAstronomi ve Astrofizik
dc.subjectElektromanyetizma, Akustik, Isı Transferi, Klasik Mekanik ve Akışkanlar Dinamiği
dc.subjectOptik
dc.subjectTemel Bilimler
dc.subjectMühendislik ve Teknoloji
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.subjectUzay bilimi
dc.titleThe Large Observatory For x-ray Timing
dc.typeBildiri
dc.contributor.departmentIstituto Nazionale Astrofisica (INAF) , ,
dc.identifier.volume9144
dc.contributor.firstauthorID2212223


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