SCIENCE WITH THE HARD X-RAY MODULATION TELESCOPE

被引：4

作者：

Li, Tipei ^{[1
]}

机构：

[1] Chinese Acad Sci, Inst High Energy Phys, Dept Phys, Beijing, Peoples R China

来源：

INTERNATIONAL JOURNAL OF MODERN PHYSICS D | 2013年 / 22卷 / 11期

关键词：

Hard X-ray modulation telescope; direct demodulation; AGN; black hole; neutron star; SUPERMASSIVE BLACK-HOLES; TIDAL DISRUPTION; GALACTIC NUCLEI; ACTIVE GALAXIES; IGR J11215-5952; SURVEY CATALOG; NEUTRON-STARS; BINARIES; TRANSIENTS; OUTBURST;

D O I：

10.1142/S0218271813600055

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The hard X-ray modulation telescope (HXMT) is a slat-collimated instrument sensitive in the 1-250 keV energy band. It will use the direct demodulation technique to conduct an all sky imaging survey with both high sensitivity and high spatial resolution. The moderate field of view also allows for sensitive spectroscopic and timing observations of bright sources in the pointed mode. The wide energy coverage and large collecting area in the hard X-ray band (nearly 5000 cm(2) effective area at 30-100 keV) make HXMT a unique instrument for some scientific goals. Here we give brief discussion about scientific objectives that can be addressed with HXMT, involving black holes at a variety of scales and equations of states of matter at extreme conditions.

引用

页数：8

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