1. The Fundamental Performance of FAST with 19-beam Receiver at L Band
- Author
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Jiang, Peng, Tang, Ning-Yu, Hou, Li-Gang, Liu, Meng-Ting, Krco, Marko, Qian, Lei, Sun, Jing-Hai, Ching, Tao-Chung, Liu, Bin, Duan, Yan, Yue, You-Ling, Gan, Heng-Qian, Yao, Rui, Li, Hui, Pan, Gao-Feng, Yu, Dong-Jun, Liu, Hong-Fei, Li, Di, Peng, Bo, Yan, Jun, and Collaboration, FAST
- Subjects
Physics ,L band ,010308 nuclear & particles physics ,Aperture ,business.industry ,FOS: Physical sciences ,Astronomy and Astrophysics ,Astrophysics ,01 natural sciences ,Astrophysics - Astrophysics of Galaxies ,Standard deviation ,Radio telescope ,Optics ,Pulsar ,Space and Planetary Science ,Astrophysics of Galaxies (astro-ph.GA) ,0103 physical sciences ,Sensitivity (control systems) ,business ,Astrophysics - Instrumentation and Methods for Astrophysics ,010303 astronomy & astrophysics ,Instrumentation and Methods for Astrophysics (astro-ph.IM) ,Zenith ,Beam (structure) - Abstract
The Five-hundred-meter Aperture Spherical radio Telescope (FAST) passed national acceptance and is taking pilot cycle of 'Shared-Risk' observations. The 19-beam receiver covering 1.05-1.45 GHz was used for most of these observations. The electronics gain fluctuation of the system is better than 1\% over 3.5 hours, enabling enough stability for observations. Pointing accuracy, aperture efficiency and system temperature are three key parameters of FAST. The measured standard deviation of pointing accuracy is 7.9$''$, which satisfies the initial design of FAST. When zenith angle is less than 26.4$^\circ$, the aperture efficiency and system temperature around 1.4 GHz are $\sim$ 0.63 and less than 24 K for central beam, respectively. The measured value of these two parameters are better than designed value of 0.6 and 25 K, respectively. The sensitivity and stability of the 19-beam backend are confirmed to satisfy expectation by spectral HI observations toward N672 and polarization observations toward 3C286. The performance allows FAST to take sensitive observations in various scientific goals, from studies of pulsar to galaxy evolution., 29 pages, 28 figures, accepted by Research in Astronomy and Astrophysics
- Published
- 2020