Institut d'Astrophysique Spatiale (IAS) 0.1-15KeV synchrotron radiation facility beam lines.

被引:10
|
作者
Dhez, P
Jourdain, E
Hainaut, O
Hochedez, JF
Labeque, A
Salvetat, P
Song, XY
机构
关键词
X-UV; CCD; proportional counter; SiLi; calibration; synchrotron source;
D O I
10.1117/12.278911
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
Two beam lines have been built at the Institut d'Astrophysique Spatiale (IAS) d'Orsay to perform absolute calibration of the EPIC (European Photon Imaging Camera). EPIC consists of three X-ray Charge Coupled Device (CCD) cameras having imaging and spectroscopic performances set al the Welter telescope focal planes on board the X-ray Multi Mirror Mission (XMM) planned to be launched by ESA in August 1999. To cover the desired 0.1-15 keV range a dedicated beam line has been built on each synchrotron sources of the Laboratoire pour l'Utilisation du Rayonnement Synchrotron (LURE) : SACO (0.8 GeV) and DCI (1.5 GeV). Both beam lines are merging in a clean 23 m(3) vacuum tank containing the camera to calibrate. The SACO windowless beam line is equipped with a grating monochromator. Four plane VLS gratings are used to cover the low energy range (0.1-1.2 keV). A triple grazing incidence mirror system set in front of the entrance slit removes the overlapping orders. The high energy beam line on DCI has a 50 mu m beryllium window and a double flat crystals monochromator equipped with four different crystal pairs. A double grazing incidence mirror system set close to the source absorbs the high energy photon spectra. CCD calibrations will be performed during 1997 second semester and years 1998.
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页码:134 / 142
页数:9
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