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Hard X-ray Modulation Telescope (HXMT) also known as Insight () is a Chinese
X-ray X-rays (or rarely, ''X-radiation'') are a form of high-energy electromagnetic radiation. In many languages, it is referred to as Röntgen radiation, after the German scientist Wilhelm Conrad Röntgen, who discovered it in 1895 and named it ' ...
space observatory, launched on June 15, 2017 to observe
black hole A black hole is a region of spacetime where gravity is so strong that nothing, including light or other electromagnetic waves, has enough energy to escape it. The theory of general relativity predicts that a sufficiently compact mass can defo ...
s,
neutron star A neutron star is the collapsed core of a massive supergiant star, which had a total mass of between 10 and 25 solar masses, possibly more if the star was especially metal-rich. Except for black holes and some hypothetical objects (e.g. w ...
s,
active galactic nuclei An active galactic nucleus (AGN) is a compact region at the center of a galaxy that has a much-higher-than-normal luminosity over at least some portion of the electromagnetic spectrum with characteristics indicating that the luminosity is not prod ...
and other phenomena based on their X-ray and gamma-ray emissions. Andrew Jones. It is based on the JianBing 3 imagery reconnaissance satellite series platform. The project, a joint collaboration of the Ministry of Science and Technology of China, the
Chinese Academy of Sciences The Chinese Academy of Sciences (CAS); ), known by Academia Sinica in English until the 1980s, is the national academy of the People's Republic of China for natural sciences. It has historical origins in the Academia Sinica during the Repub ...
, and
Tsinghua University Tsinghua University (; abbr. THU) is a national public research university in Beijing, China. The university is funded by the Ministry of Education. The university is a member of the C9 League, Double First Class University Plan, Projec ...
, has been under development since 2000.


Payload

The main scientific instrument is an array of 18 NaI(Tl)/CsI(na) slat-collimated "phoswich" scintillation detectors, collimated to 5.7°×1° overlapping fields of view.HXMT.cn
Configuration
(Hard X-ray telescope design) c.2004
The main NaI detectors have an area of 286 cm2 each, and cover the 20–200 keV energy range. Data analysis is planned to be by a direct algebraic method, "direct demodulation",HXMT.cn
The direct demodulation method
(Imaging by direct deconvolution) c.2004
which has shown promise in de-convolving the raw data into images while preserving excellent angular and energy resolution. The satellite has three payloads, the high energy X-ray Telescope (20–250 keV), the medium energy X-ray telescope (5–30 keV), and the low energy X-ray telescope (1–15 keV)


See also

* X-ray astronomy *
X-ray astronomy satellite An X-ray astronomy satellite studies X-ray emissions from celestial objects, as part of a branch of space science known as X-ray astronomy. Satellites are needed because X-radiation is absorbed by the Earth's atmosphere, so instruments to detect ...


References

{{DEFAULTSORT:Hard X-Ray Modulation Telescope Space telescopes X-ray telescopes Chinese telescopes 2017 in China Spacecraft launched in 2017 Satellites of China Spacecraft launched by Long March rockets