The Five-Hundred-Meter Aperture Spherical Radio Telescope (FAST) Project
arXiv:1105.3794 · doi:10.1142/S0218271811019335
Abstract
Five-hundred-meter Aperture Spherical radio Telescope (FAST) is a Chinese mega-science project to build the largest single dish radio telescope in the world. Its innovative engineering concept and design pave a new road to realize a huge single dish in the most effective way. FAST also represents Chinese contribution in the international efforts to build the square kilometer array (SKA). Being the most sensitive single dish radio telescope, FAST will enable astronomers to jump-start many science goals, for example, surveying the neutral hydrogen in the Milky Way and other galaxies, detecting faint pulsars, looking for the first shining stars, hearing the possible signals from other civilizations, etc. The idea of sitting a large spherical dish in a karst depression is rooted in Arecibo telescope. FAST is an Arecibo-type antenna with three outstanding aspects: the karst depression used as the site, which is large to host the 500-meter telescope and deep to allow a zenith angle of 40 degrees; the active main reflector correcting for spherical aberration on the ground to achieve a full polarization and a wide band without involving complex feed systems; and the light-weight feed cabin driven by cables and servomechanism plus a parallel robot as a secondary adjustable system to move with high precision. The feasibility studies for FAST have been carried out for 14 years, supported by Chinese and world astronomical communities. The project time is 5.5 years from the commencement of work in March of 2011 and the first light is expected to be in 2016. This review intends to introduce FAST project with emphasis on the recent progress since 2006. In this paper, the subsystems of FAST are described in modest details followed by discussions of the fundamental science goals and examples of early science projects.
36 pages, 28 figures, accepted for publication in International Journal of Modern Physics D
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- Prospects for gravitational wave astronomy with next generation large-scale pulsar timing arrays
- History of Astronomy in Australia: Big-Impact Astronomy from World War II until the Lunar Landing (1945-1969)
- Integrated HI emission in galaxy groups and clusters
- Identification and characterization of optical companions to the population of millisecond pulsars in the globular cluster M3
- FAST search for circumstellar atomic hydrogen. II. Is BD+303639 an interacting planetary nebula?
- New Constraints on Preferred Frame Effects from Binary Pulsars
- Pulsar Population Synthesis with Magnetorotational Evolution: Constraining the Decay of Magnetic field
- Map Reconstruction of radio observations with Conditional Invertible Neural Networks
- FASHI: A search for extragalactic OH megamasers with FAST
- The Northern High Time Resolution Universe pulsar survey: II. Single-pulse search set-up and simulations
- FAST drift scan survey for HI intensity mapping: simulation on hunting HI filament with pairwise stacking
- Adiabatic Duality: Duality of cosmological models with varying slow-roll parameter and sound speed
- Challenges in Forming Millisecond Pulsar-Black Holes from Isolated Binaries
- Dual-Backend Multibeam Position Switching Targeted SETI Observations toward Nearby Active Planet-Hosting Systems with FAST
- Distinct polarization properties for two emission states of four pulsars
- An independent test on the local position invariance of gravity with the triple pulsar PSR J0337+1715
- Enhanced Remote Astronomical Archive System Based on the File-Level Unlimited Sliding-Window Technique
- Imprints of relic gravitational waves on pulsar timing
- Extracting 21cm signal by frequency and angular filtering
- Dealing with the data imbalance problem on pulsar candidates sifting based on feature selection
- Rapidly Spinning Massive Pulsars as an Indicator of Quark Deconfinement
- The link between galaxy structure properties and star formation in local galaxies
- Forecasts on Interacting Dark Energy from 21-cm Angular Power Spectrum with BINGO and SKA observations
- Estimation of neutron star mass and radius of FRB 20240114A by identification of crustal oscillations
- Reflections on "Can AI Understand Our Universe?"
- Narrowband Radio Technosignature Search toward 3I/ATLAS with FAST
- An Improved Machine Learning Approach for Radio Frequency Interference Mitigation in FAST-SETI Survey Archival Data
- A Method for Pulsar Searching: Combining a Two-dimensional Autocorrelation Profile Map and a Deep Convolutional Neural Network
- Comprehensive analysis of dissipative effects in the induced gravitational waves
- Simultaneous view of the FRB~180301 with FAST and NICER during a bursting phase
- Radio pulse search from Aql X-1
- Similar Scale-invariant Behaviors between Soft Gamma-ray Repeaters and An Extreme Epoch from FRB 121102
- HI Intensity Mapping cross-correlation with thermal SZ fluctuations: forecasted cosmological parameters estimation for FAST and Planck
- Big Data Challenges of FAST
- Illuminating Hidden Pulsars: Scintillation-Enhanced Discovery of Two Binary Millisecond Pulsars in M13 with FAST
- A Target Search for Fast Radio Bursts Associated with Two Fast Blue Optical Transients: AT2018cow and CSS161010
- Synchrotron spectrum of fast cooling electrons in GRBs
- Measurements of the diffuse Galactic synchrotron spectral index and curvature from MeerKLASS pilot data
- AGILE observations of a sample of repeating Fast Radio Burst sources
- Estimating constraints on cosmological parameters via the canonical and the differential redshift drift with SKA HI 21-cm observations
- Revealing the Unseen: The Discovery of Long-Awaited Radiation from the Intermittent Pulsar PSR B1931+24
- Main and interpulse interaction in PSRs J1842+0358 and J1926+0737: evidence for interpole communication
- Streaming Velocity Effects on the Post-reionization 21 cm Baryon Acoustic Oscillation Signal
- Neutral Stellar Winds Toward the High-Mass Star-Forming Region G176.51+00.20
- Squared-field cross-correlation between kinetic Sunyaev-Zel'dovich effect and 21-cm intensity mapping
- The BINGO project X. Cosmological parameter constraints from HI Intensity Mapping lognormal simulations
- Long-term timing of the relativistic binary PSR J1906+0746
- Simulating a full-sky high resolution Galactic synchrotron spectral index map using neural networks
- AVID: A Near-Major Post-Merger of Late-Type Dwarfs beneath a Regularly Rotating HI Disk (VCC 693)
- Estimation of Solar Observations with the Five-hundred-meter Aperture Spherical Radio Telescope (FAST)
- Probing the large-scale structure with 21cm-galaxy cross-bispectrum: Estimates from simulations and forecasts for upcoming cosmological surveys
- Electromagnetic Precursors to Binary Neutron Star Mergers: Kinetic Simulations of Magnetospheric Flaring
- The FAST Hundred-Deg HI Deep (HD) Survey: Early Results from the Pilot Survey
- Indication for Decreasing Dispersion Measure in the Population of Repeating Fast Radio Bursts and Connection to Young Supernova Remnant Expansion
- Search for Periodic Radio Signals from Double Neutron Star System Companions Using the Fast Folding Algorithm
- Searching for A Generic Gravitational Wave Background via Bayesian Nonparametric Analysis with Pulsar Timing Arrays
- Mass measurements of the double neutron star system PSR J0641+0448
- Searching radio signals from two magnetars and a high-magnetic field pulsar and the serendipitous discovery of a new radio pulsar PSR J1935+2200
- FAST Observation and Results for Core Collapse Globular Cluster M15 and NGC 6517
- Pulsar timing residuals due to individual non-evolving gravitational wave sources
- Measuring the speed of scalar induced gravitational waves from observations
- The Northern High Time Resolution Universe pulsar survey: III. Single-pulse search continuation, follow-up observations, and initial results
- Spatial Modulation Search Applied to the Search and Confirmation of Highly Scintillated Pulsars at FAST with A Pulsar Discovered in M3
- TransientVerse: A Comprehensive Real-Time Alert and Multi-Wavelength Analysis System for Transient Astronomical Events
- Energy and waiting time distributions of FRB 121102 observed by FAST
- Search for Low-Energy Signals from Fast Radio Bursts with the Borexino Detector