The Hard X-ray Modulation Telescope Mission

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CCD236 55 Fe spectrum@-30.7°CE(keV)=0.00641*Ch-2.761FWHM=128eV@5.9keV; rms=6.9e -HXMT @China-US bilateral workshop on astronomy 16
Advantages of LE for X-<strong>ray</strong> timing/spectroscopyDetectorArea(cm 2 @ 6keV)Time resolution Energy resolution(@ 6 keV)EXOSAT/ME 1600 ~ms 1200 eVNoteGinga/LAC 4000 ~msASCA/GIS 250 0.06 msRXTE/PCA 5000 1μs1200 eV460 eV1125 eVChandra/ACIS200 3 ms 130 eV High pileup effect(CC mode)Chandra/HRC 40 16μsbadfor strong sourceXMM/MOS 768 1.5 ms 130 eV High pileup effect forstrong sourceHXMT/LE 240 1 ms 130 eV No pileup for 10Crab sourceHXMT @China-US bilateral workshop on astronomy 17
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: Charge flowReal & dummyoutputs in g
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 and 32: Simulated HXMT AGN luminosity funct
Page 33 and 34: Scientific objectives of the pointe
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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