The Hard X-ray Modulation Telescope Mission

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Pointed observationsHXMT @China-US bilateral workshop on astronomy 32
Scientific objectives of the pointed observations• X-ray Binary: multi-wavelength X-ray variability;especially the QPO properties of BH binaries atenergy higher than 20 keV;• Cyclotron Resonance Features (CRF) close tothe neutron star surface;• Broad band (1-250 keV) AGN spectrum,reflecting components and high energy cut off;• Hard X-ray emission from clusters of galaxies;• Non-thermal X-ray emission of SNRs andcosmic-ray acceleration。HXMT @China-US bilateral workshop on astronomy 33
Page 1 and 2: The Hard X-ray Modulation Telescope
Page 3 and 4: Payload CabinPlatform CabinHXMT @Ch
Page 5: Characteristics of the HXMT Mission
Page 8 and 9: Shielding RingCollimatorDetectorEac
Page 10 and 11: The medium energy Telescope (ME)Obj
Page 13 and 14: The low energy Telescope (LE)Object
Page 15 and 16: Charge flowReal & dummyoutputs in g
Page 17 and 18: Advantages of LE for X-ray timing/s
Page 19 and 20: Simulated in-space background of HX
Page 21 and 22: SensitivityHXMT/HEHXMT @China-US bi
Page 23 and 24: Observation modes• All-sky Survey
Page 25 and 26: HXMT Sky Survey ObservationsExposur
Page 27 and 28: Simulation of a 0.5mCrab source in
Page 29 and 30: AGN Luminosity function0.42mCrab0.5
Page 31: Simulated HXMT AGN luminosity funct
Page 35 and 36: Cyclotron Resonance Features in neu
Page 37 and 38: Broad band X-ray spectrum of AGN(Po
Page 39 and 40: Hard X-ray from clusters of galaxie
Page 41 and 42: Simulated hard X-ray spectrum of Co
Page 43: Schedule of HXMT• Satellite Ready

The Hard X-ray Modulation Telescope Mission

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