Project FAST- Five hundred meter Aperture Spherical radio Telescope

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Neutral hydrogen (HI) surveyCosmic history is written in the characters of weakHI line emission. To read this encyclopaedia, a supersensitive telescope is requiredBlind detection of HI clouds with an interference-freeobserving period of 1h, z~0.7Warm HI shell around AGN, the detection range limitin a moderate integration time, z~35
Page 6 and 7: Kravtsov - Simulation ondark matter
Page 8 and 9: FAST Pulsar SurveyThere are ~ 6 X 1
Page 10 and 11: Early sciences with FAST- bilateral
Page 12 and 13: ★ S 2★ S 1Optical geometryO12
Page 14 and 15: Opening angle - sky coverage (cont.
Page 16 and 17: ObservatoryObservatory buildingComp
Page 18 and 19: Site Surveying in GuizhouGuiyangLoc
Page 20 and 21: 3.Technical plan- critical technolo
Page 22 and 23: ~2400 winches~4600 panelsAdaptive c
Page 24 and 25: Feed supportmechanical-electronic-o
Page 26 and 27: 3.Technical plan- critical technolo
Page 28 and 29: PhotogrammetrySurveying reflector p
Page 30 and 31: 9 sets of FAST receivers NAOC - JBO
Page 32 and 33: 4. Feasibility study of critical te
Page 34 and 35: eaking load experimentcablesnodes34
Page 36 and 37: Prototyping rear ribLess than 1mm c
Page 38 and 39: Prototyping the winches• worm-whe
Page 40 and 41: Dynamic experiment on Stewart stabi
Page 42 and 43: 1st harmonic (0.182455Hz)2nd harmon
Page 44 and 45: Most precise laser rangerAPIMaximum
Page 46 and 47: Receiver layout• Main focus, -13d
Page 48 and 49: HI was observed using 50mmodel in S
Page 50: Approval appears on SKA webpagehttp

Project FAST- Five hundred meter Aperture Spherical radio Telescope

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