THE MPI AIT X-RAY IMAGER (MAXI) - HIGH-SPEED PN CCDS FOR X-RAY-DETECTION

被引:67
作者
STRUDER, L
BRAUNINGER, H
MEIER, M
PREDEHL, P
REPPIN, C
STERZIK, M
TRUMPER, J
CATTANEO, P
HAUFF, D
LUTZ, G
SCHUSTER, KF
SCHWARZ, A
KENZIORRA, E
STAUBERT, A
GATTI, E
LONGONI, A
SAMPIETRO, M
RADEKA, V
REHAK, P
RESCIA, S
MANFREDI, PF
BUTTLER, W
HOLL, P
KEMMER, J
PRECHTEL, U
ZIEMANN, T
机构
[1] MAX PLANCK INST PHYS & ASTROPHYS,WERNER HEISENBERG INST PHYS,W-8000 MUNICH 40,GERMANY
[2] UNIV TUBINGEN,INST ASTRON,W-7400 TUBINGEN 1,GERMANY
[3] POLITECN MILAN,I-20133 MILAN,ITALY
[4] BROOKHAVEN NATL LAB,UPTON,NY 11973
[5] UNIV PAVIA,I-27100 PAVIA,ITALY
[6] FRAUNHOFER INST MICROELECTR,DUISBURG,GERMANY
[7] MESSERSCHMITT BOLKOW BLOHM GMBH,W-8000 MUNICH,GERMANY
关键词
D O I
10.1016/0168-9002(90)90490-W
中图分类号
TH7 [仪器、仪表];
学科分类号
0804 ; 080401 ; 081102 ;
摘要
MAXI (MPI/AIT X-ray Imager) is part of a proposal submitted to the European Space Agency (ESA) as focal plane instrumentation of the X-ray Multi Mirror Mission (XMM). Within a collaboration of 13 European institutes we have proposed a fully depleted (sensitive) pn CCD of 280 μm thickness with a homogeneous sensitive area of 36 cm2 and a pixel size of 150×150 μm2 which is well matched with the telescope's angular resolution of 30 arcsec translating to a position resolution of approximately 1 mm in the focal plane. The X-ray sensitivity will be higher than 90% from 250 eV up to 10 keV, the readout time in the full frame mode of the complete focal plane will be 2 ms with a readout noise of better than 5 e- (rms). Prototypes of all individual components of the camera system have been fabricated and tested. The camera concept will be presented. The measured transfer properties of the CCD and the on-chip electronics will be treated. Taking into account the coupling of the on-chip amplifier to the following front-end electronics the expected performance will be derived. © 1990.
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页码:227 / 235
页数:9
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