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Statements

Subject Item
n2:RIV%2F68407700%3A21340%2F14%3A00223572%21RIV15-MSM-21340___
rdf:type
n18:Vysledek skos:Concept
rdfs:seeAlso
http://arxiv.org/ftp/arxiv/papers/1408/1408.6539.pdf
dcterms:description
LOFT (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 m2-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 reproposed 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. (2014) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only. LOFT (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 m2-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 reproposed 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. (2014) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
dcterms:title
The large area detector of LOFT: the Large Observatory for X-ray Timing The large area detector of LOFT: the Large Observatory for X-ray Timing
skos:prefLabel
The large area detector of LOFT: the Large Observatory for X-ray Timing The large area detector of LOFT: the Large Observatory for X-ray Timing
skos:notation
RIV/68407700:21340/14:00223572!RIV15-MSM-21340___
n3:aktivita
n8:P
n3:aktivity
P(GA13-33324S), P(LH13065)
n3:dodaniDat
n13:2015
n3:domaciTvurceVysledku
n21:8215154
n3:druhVysledku
n22:D
n3:duvernostUdaju
n20:S
n3:entitaPredkladatele
n14:predkladatel
n3:idSjednocenehoVysledku
25652
n3:idVysledku
RIV/68407700:21340/14:00223572
n3:jazykVysledku
n10:eng
n3:klicovaSlova
Observatories; Sensors; X-rays; Equipment and services; X-ray sources
n3:klicoveSlovo
n15:Sensors n15:Equipment%20and%20services n15:Observatories n15:X-rays n15:X-ray%20sources
n3:kontrolniKodProRIV
[91E927283F7D]
n3:mistoKonaniAkce
Montréal
n3:mistoVydani
Bellingham
n3:nazevZdroje
Proceedings of SPIE vol. 9144: Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray
n3:obor
n23:JB
n3:pocetDomacichTvurcuVysledku
1
n3:pocetTvurcuVysledku
59
n3:projekt
n17:LH13065 n17:GA13-33324S
n3:rokUplatneniVysledku
n13:2014
n3:tvurceVysledku
Argan, A. Bradley, L. Zampa, G. Smith, P. Wilms, J. Fraser, G. Campana, R. Cais, P. Bertuccio, G. Marisaldi, M. Suchy, S. Winter, B. Rachevski, A. de Rosa, A. Schmid, C. Orlandini, M. den Herder, J. W. Evangelista, Y. Walton, D. Bozzo, E. Cadoux, F. di Cosimo, S. Cros, A. Feldman, C. Bodin, P. Hailey, M. R. Ahangarianabhari, M. Zampa, N. Hudec, René Santangelo, A. Martindale, A. Kennedy, T. Tenzer, C. Azzarello, P. Uttley, P. Nowak, M. Vacchi, A. Muleri, F. Baldazzi, G. Malcovati, P. Seyler, J. Y. Barret, D. Barbera, M. Favre, Y. Zane, S. Donnarumma, I. Pacciani, L. Pohl, M. Fuschino, F. del Monte, E. Feroci, M. Labanti, C. Coker, J. Grassi, M. Petráček, Vojtěch Macera, D. Perinati, E. Soffitta, P. Mineo, T.
n3:typAkce
n11:WRD
n3:zahajeniAkce
2014-06-22+02:00
s:issn
0277-786X
s:numberOfPages
19
n9:doi
10.1117/12.2054654
n12:hasPublisher
SPIE
n16:isbn
978-0-8194-9612-6
n6:organizacniJednotka
21340