A set of X-ray Polarimeters for the New Hard X-Ray Imaging and Polarimetric Mission

被引:7
|
作者
Soffitta, Paolo [1 ]
Costa, Enrico [1 ]
Muleri, Fabio [1 ]
Campana, Riccardo [1 ]
Del Monte, Ettore [1 ]
Di Cosimo, Sergio [1 ]
Evangelista, Yuri [1 ]
Fabiani, Sergio [1 ]
Feroci, Marco [1 ]
Lazzarotto, Francesco [1 ]
Rubini, Alda [1 ]
Bellazzini, Ronaldo
Brez, Alessandro
Minuti, Massimo
Omodei, Nicola
Pinchera, Michele
Razzano, Massimiliano
Sgro, Carmelo
Spandre, Gloria
Argan, Andrea
Matt, Giorgio
机构
[1] IASF Roma INAF, I-00133 Rome, Italy
来源
SPACE TELESCOPES AND INSTRUMENTATION 2010: ULTRAVIOLET TO GAMMA RAY | 2010年 / 7732卷
关键词
X-ray; Polarimetry; Mission; Detectors; GAS PIXEL DETECTOR; POLARIZATION; ASTRONOMY;
D O I
10.1117/12.856434
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The New Hard X-Ray Imaging and Polarimetric Mission(1) makes a synergic use of Hard X-Ray Imaging, Spectroscopy and Polarimetry, as independent diagnostic of the same physical systems. It exploits the technology of multi-layer optics that, with a focal length of 10 m, allow for spectroscopic and imaging, with a resolution from 15 to 20 arcseconds, on the band 0.2 - 80 keV. One of the four telescopes is devoted to polarimetry. Since the band of a photoelectric polarimeter is not that wide, we foresee two of them, one tuned on the lower energy band (2-10 keV) and another one tuned on higher energies (6 - 35 keV). The blurring due to the inclined penetration of photons in the gas, thanks to the long focal length is practically negligible. In practice the polarimeters fully exploit the resolution the telescope and NHXM can perform angular resolved simultaneous spectroscopy and polarimetry on the band 2 - 35 keV. We are also studying the possibility to extend the band up to 80 keV by means of a focal plane scattering polarimeter.
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页数:13
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