A mid infrared imager for the next generation space telescope: MIRIM, the MIRI imager

被引：0
|
作者：
Dubreuil, D [1 ]
Bensammar, S [1 ]
机构：
[1] CEA Saclay, SAP, F-91191 Gif Sur Yvette, France
来源：
ASTRONOMY WITH HIGH CONTRAST IMAGING: FROM PLANETARY SYSTEMS TO ACTIVE GALACTIC NUCLEI | 2003年 / 8卷
关键词：
D O I：
10.1051/eas:2003058
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
MTRI is the mid infrared instrument planned for the NGST. Working in the 5 mum - 28 mum band, it includes 3 units: a spectrograph, an imager and a calibration facility. We describe here briefly MIRIM, the MIRI imager channel as it is at the end of the phase A study. MIRIM provides 3 observing modes: in imaging mode, with a, Field Of View of 1.3 arcmin x 1.7 arcmin and a Pixel Field Of View of 0.1 arcsec/pixel, a coronagraphic mode and a low resolution mode for point sources, between 5 mum and 1.0 mum, with a spectral resolution R = lambda/Deltalambda around 100.
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页码：147 / 157
页数：11
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