Project FAST- Five hundred meter Aperture Spherical radio Telescope

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Opening angle - sky coverage (cont.)300mZA205m30º 60ºIf FPA technology could form an irregular beam tofully match the desired portionWe can have a large single dish ~ 200m at zenith 60°We are interested to have the Roger’s talk on FPA14
Frequency range0.13 0.327 1.42 3458(GHz)In layout 2000First phaseSecond phaseHI surveying70MHzz~20EoRPulsar300MHzHCOOHCH3OH OH(4) HC5N(4) CH(4) CH4Water hole5.2GHzH2CO(6)VLBI17 LinesSETIS BandC BandX BandSpace science15
Page 5 and 6: Neutral hydrogen (HI) surveyCosmic
Page 7 and 8: Duffy et alNumber of galaxiesto be
Page 9 and 10: A ‘master’ of VLBI networkBonn1
Page 11 and 12: 2. General Technical SpecificationS
Page 13: Opening angle - sky coverageSky cov
Page 17 and 18: 3.Technical plan- critical technolo
Page 19 and 20: Quick Bird Fly Oct. 6, 200519
Page 21 and 22: Central part of sphere is close to
Page 25 and 26: Three main parts of cabin suspensio
Page 27 and 28: Measurement - precise, quick and in
Page 31 and 32: Receiver -- Schematic DiagramFeed+
Page 33 and 34: Exploration in depression site and
Page 35 and 36: Prototyping the back-structureof re
Page 37 and 38: Spatial truss backup (costly)Deform
Page 39 and 40: Prime focus position controlExperim
Page 41 and 42: NCollaboration with MT and TUDOptim
Page 43 and 44: • under the wind 8m/s, 1st adjust
Page 45 and 46: CCD:20Hz;0.5cmDGPS:10Hz;1cmLaser Tr
Page 47 and 48: FAST model construction process1. t
Page 49 and 50: 5. Current state of FAST projectTot

Project FAST- Five hundred meter Aperture Spherical radio Telescope

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