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Titolo:
An X-ray photon-counting imaging spectrometer based on a Ta absorber with four superconducting tunnel junctions
Autore:
den Hartog, R; Verhoeve, P; Martin, D; Rando, N; Peacock, A; Krumrey, M; Goldie, DJ;
Indirizzi:
European Space Agcy, Estec, Dept Space Sci, Div Astrophys, NL-2200 AG Noordwijk, Netherlands European Space Agcy Noordwijk Netherlands NL-2200 AG rdwijk, Netherlands Phys Tech Bundesanstalt, D-10587 Berlin, Germany Phys Tech Bundesanstalt Berlin Germany D-10587 , D-10587 Berlin, Germany Oxford Instruments Sci Res Div, Cambridge CB4 4WY, England Oxford Instruments Sci Res Div Cambridge England CB4 4WY B4 4WY, England
Titolo Testata:
NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT
fascicolo: 1-2, volume: 444, anno: 2000,
pagine: 278 - 282
SICI:
0168-9002(20000411)444:1-2<278:AXPISB>2.0.ZU;2-7
Fonte:
ISI
Lingua:
ENG
Tipo documento:
Article
Natura:
Periodico
Settore Disciplinare:
Physical, Chemical & Earth Sciences
Engineering, Computing & Technology
Citazioni:
9
Recensione:
Indirizzi per estratti:
Indirizzo: den Hartog, R European Space Agcy, Estec, Dept Space Sci, Div Astrophys, POB 299, NL-2200 AG Noordwijk, Netherlands European Space Agcy POB 299 Noordwijk Netherlands NL-2200 AG
Citazione:
R. den Hartog et al., "An X-ray photon-counting imaging spectrometer based on a Ta absorber with four superconducting tunnel junctions", NUCL INST A, 444(1-2), 2000, pp. 278-282

Abstract

We present the first results obtained with a two-dimensional X-ray imagingspectrometer consisting of a 200 x 200 mu m(2) Ta absorber and read out byfour Ta/Al superconducting tunnel junctions (STJs). A preliminary image reconstruction algorithm allows the visualisation of the diffraction pattern from a 5 mu m pinhole illuminated with 10 keV X-rays. The image suggests a spatial resolution better than 10 mu m The algorithm does not take into account quasi-particle losses in the absorber. Hence, the pulse-height reconstruction is not optimal and the energy resolution varies significantly across the absorber. The best energy resolution is obtained for a 20 x 20 mu m(2) area in the centre of the absorber. and amounts to similar to 77 eV at a photon energy of 5895 eV, with a 70 eV electronic noise contribution, (C) 2000 Elsevier Science B.V. All rights reserved.

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Documento generato il 23/05/13 alle ore 15:57:48