Commissioning progress of the FAST

The Five-hundred-meter Aperture Spherical radio Telescope (FAST) was completed with its main structure installed on September 25, 2016, after which it entered the commissioning phase. This paper aims to introduce the commissioning progress of the FAST over the past two years. To improve its operatio...

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Vydané v:	Science China. Physics, mechanics & astronomy Ročník 62; číslo 5; s. 959502
Hlavní autori:	Jiang, Peng, Yue, YouLing, Gan, HengQian, Yao, Rui, Li, Hui, Pan, GaoFeng, Sun, JingHai, Yu, DongJun, Liu, HongFei, Tang, NingYu, Qian, Lei, Lu, JiGuang, Yan, Jun, Peng, Bo, Zhang, ShuXin, Wang, QiMing, Li, Qi, Li, Di
Médium:	Journal Article
Jazyk:	English
Vydavateľské údaje:	Beijing Science China Press 01.05.2019 Springer Springer Nature B.V
Predmet:	Astronomy Classical and Continuum Physics Commissioning Control methods Control systems Costs (Law) Invited Review Noise temperature Observations and Techniques Performance indices Physics Physics and Astronomy Pulsars Radio telescopes Support systems Telescope Telescopes Ultrawideband radio telescopes and instrumentation algorithms and implementation radio wave receivers astronomical observations control systems
ISSN:	1674-7348, 1869-1927
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Abstract	The Five-hundred-meter Aperture Spherical radio Telescope (FAST) was completed with its main structure installed on September 25, 2016, after which it entered the commissioning phase. This paper aims to introduce the commissioning progress of the FAST over the past two years. To improve its operational reliability and ensure effective observation time, FAST has been equipped with a real-time information system for the active reflector system and hierarchical commissioning scheme for the feed support system, which ultimately achieves safe operation of the two systems. For meeting the high-performance indices, a high-precision measurement system was set up based on the effective control methods that were implemented for the active reflector system and feed support system. Since the commissioning of the FAST, a low-frequency ultra-wideband receiver and 19-beam 1.05-1.45 GHz receiver have been mainly used. Telescope efficiency, pointing accuracy, and system noise temperature were completely tested and ultimately achieved the acceptance indices of the telescope. The FAST has been in the process of national acceptance preparations and has begun to search for pulsars. In the future, it will still strive to improve its capabilities and expand its application prospects.
AbstractList	The Five-hundred-meter Aperture Spherical radio Telescope (FAST) was completed with its main structure installed on September 25, 2016, after which it entered the commissioning phase. This paper aims to introduce the commissioning progress of the FAST over the past two years. To improve its operational reliability and ensure effective observation time, FAST has been equipped with a real-time information system for the active reflector system and hierarchical commissioning scheme for the feed support system, which ultimately achieves safe operation of the two systems. For meeting the high-performance indices, a high-precision measurement system was set up based on the effective control methods that were implemented for the active reflector system and feed support system. Since the commissioning of the FAST, a low-frequency ultra-wideband receiver and 19-beam 1.05-1.45 GHz receiver have been mainly used. Telescope efficiency, pointing accuracy, and system noise temperature were completely tested and ultimately achieved the acceptance indices of the telescope. The FAST has been in the process of national acceptance preparations and has begun to search for pulsars. In the future, it will still strive to improve its capabilities and expand its application prospects. The Five-hundred-meter Aperture Spherical radio Telescope (FAST) was completed with its main structure installed on September 25, 2016, after which it entered the commissioning phase. This paper aims to introduce the commissioning progress of the FAST over the past two years. To improve its operational reliability and ensure effective observation time, FAST has been equipped with a real-time information system for the active reflector system and hierarchical commissioning scheme for the feed support system, which ultimately achieves safe operation of the two systems. For meeting the high-performance indices, a high-precision measurement system was set up based on the effective control methods that were implemented for the active reflector system and feed support system. Since the commissioning of the FAST, a low-frequency ultra-wideband receiver and 19-beam 1.05-1.45 GHz receiver have been mainly used. Telescope efficiency, pointing accuracy, and system noise temperature were completely tested and ultimately achieved the acceptance indices of the telescope. The FAST has been in the process of national acceptance preparations and has begun to search for pulsars. In the future, it will still strive to improve its capabilities and expand its application prospects. radio telescopes and instrumentation, astronomical observations, radio wave receivers, algorithms and implementation, control systems PACS number(s): 95.55.Jz, 95.85.-e, 07.57.Kp, 07.05.Kf, 07.05.Dz
ArticleNumber	959502
Audience	Academic
Author	Yao, Rui Yu, DongJun Li, Qi Lu, JiGuang Peng, Bo Li, Hui Gan, HengQian Yue, YouLing Liu, HongFei Tang, NingYu Sun, JingHai Jiang, Peng Qian, Lei Zhang, ShuXin Wang, QiMing Li, Di Pan, GaoFeng Yan, Jun
Author_xml	– sequence: 1 givenname: Peng surname: Jiang fullname: Jiang, Peng email: pjiang@nao.cas.cn organization: CAS Key Laboratory of FAST, National Astronomical Observatories, Chinese Academy of Sciences – sequence: 2 givenname: YouLing surname: Yue fullname: Yue, YouLing organization: CAS Key Laboratory of FAST, National Astronomical Observatories, Chinese Academy of Sciences – sequence: 3 givenname: HengQian surname: Gan fullname: Gan, HengQian organization: CAS Key Laboratory of FAST, National Astronomical Observatories, Chinese Academy of Sciences – sequence: 4 givenname: Rui surname: Yao fullname: Yao, Rui email: ryao@nao.cas.cn organization: CAS Key Laboratory of FAST, National Astronomical Observatories, Chinese Academy of Sciences – sequence: 5 givenname: Hui surname: Li fullname: Li, Hui organization: CAS Key Laboratory of FAST, National Astronomical Observatories, Chinese Academy of Sciences – sequence: 6 givenname: GaoFeng surname: Pan fullname: Pan, GaoFeng organization: CAS Key Laboratory of FAST, National Astronomical Observatories, Chinese Academy of Sciences – sequence: 7 givenname: JingHai surname: Sun fullname: Sun, JingHai organization: CAS Key Laboratory of FAST, National Astronomical Observatories, Chinese Academy of Sciences – sequence: 8 givenname: DongJun surname: Yu fullname: Yu, DongJun organization: CAS Key Laboratory of FAST, National Astronomical Observatories, Chinese Academy of Sciences – sequence: 9 givenname: HongFei surname: Liu fullname: Liu, HongFei organization: CAS Key Laboratory of FAST, National Astronomical Observatories, Chinese Academy of Sciences – sequence: 10 givenname: NingYu surname: Tang fullname: Tang, NingYu organization: CAS Key Laboratory of FAST, National Astronomical Observatories, Chinese Academy of Sciences – sequence: 11 givenname: Lei surname: Qian fullname: Qian, Lei organization: CAS Key Laboratory of FAST, National Astronomical Observatories, Chinese Academy of Sciences – sequence: 12 givenname: JiGuang surname: Lu fullname: Lu, JiGuang organization: CAS Key Laboratory of FAST, National Astronomical Observatories, Chinese Academy of Sciences – sequence: 13 givenname: Jun surname: Yan fullname: Yan, Jun organization: CAS Key Laboratory of FAST, National Astronomical Observatories, Chinese Academy of Sciences – sequence: 14 givenname: Bo surname: Peng fullname: Peng, Bo email: pb@nao.cas.cn organization: CAS Key Laboratory of FAST, National Astronomical Observatories, Chinese Academy of Sciences – sequence: 15 givenname: ShuXin surname: Zhang fullname: Zhang, ShuXin organization: CAS Key Laboratory of FAST, National Astronomical Observatories, Chinese Academy of Sciences – sequence: 16 givenname: QiMing surname: Wang fullname: Wang, QiMing organization: CAS Key Laboratory of FAST, National Astronomical Observatories, Chinese Academy of Sciences – sequence: 17 givenname: Qi surname: Li fullname: Li, Qi organization: CAS Key Laboratory of FAST, National Astronomical Observatories, Chinese Academy of Sciences – sequence: 18 givenname: Di surname: Li fullname: Li, Di organization: CAS Key Laboratory of FAST, National Astronomical Observatories, Chinese Academy of Sciences, School of Astronomy and Space Science, University of Chinese Academy of Sciences
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Keywords	radio telescopes and instrumentation algorithms and implementation radio wave receivers astronomical observations control systems
Language	English
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PublicationTitle	Science China. Physics, mechanics & astronomy
PublicationTitleAbbrev	Sci. China Phys. Mech. Astron
PublicationYear	2019
Publisher	Science China Press Springer Springer Nature B.V
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Astron.20196295950610.1007/s11433-019-9383-y – reference: LuJ GPengBLiuKJiangPYueY LYuMYuY-ZKouF FWangLFAST CollaborationSci. China-Phys. Mech.2019Astron.6295950310.1007/s11433-018-9372-7 – reference: YuY-ZPengBLiuKM. ZhangCWangLKouF FLuJ GYuMFAST CollaborationSci. China-Phys. Mech. Astron.20196295950410.1007/s11433-018-9358-8 – reference: BianZ FSurveying2002BeijingChina Agriculture Press – reference: NanRSci China Ser G-Phys. Mech. Astron.2006491292006ScChG..49..129N10.1007/s11433-006-0129-9 – reference: JiangPLiQ WNanR DRes. Astron. Astrophys.20171792017RAA....17....9L10.1088/1674-4527/17/1/9 – reference: JiangPNanR DQianLYueY LRes. Astron. Astrophys.20151510 – reference: LiHYaoRAdv. Mech. Eng.2014671609710.1155/2014/716097 – reference: YaoRLiQ WSunJ HZhuW BJ. Mech. Eng.2017533610.3901/JME.2017.17.036 – volume: 62 start-page: 959506 year: 2019 ident: 9376_CR4 publication-title: Sci. China-Phys. Mech. 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Snippet	The Five-hundred-meter Aperture Spherical radio Telescope (FAST) was completed with its main structure installed on September 25, 2016, after which it entered...
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SubjectTerms	Astronomy Classical and Continuum Physics Commissioning Control methods Control systems Costs (Law) Invited Review Noise temperature Observations and Techniques Performance indices Physics Physics and Astronomy Pulsars Radio telescopes Support systems Telescope Telescopes Ultrawideband
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Title	Commissioning progress of the FAST
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