Status and perspectives of the CRAFTS extra-galactic HI survey
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  • 英文篇名:Status and perspectives of the CRAFTS extra-galactic HI survey
  • 作者:Kai ; Zhang ; JingWen ; Wu ; Di ; Li ; Marko ; Kro ; Lister ; Staveley-Smith ; NingYu ; Tang ; Lei ; Qian ; MengTing ; Liu ; ChengJin ; Jin ; YouLing ; Yue ; Yan ; Zhu ; HongFei ; Liu ; DongJun ; Yu ; JingHai ; Sun ; GaoFeng ; Pan ; Hui ; Li ; HengQian ; Gan ; Rui ; Yao
  • 英文作者:Kai Zhang;JingWen Wu;Di Li;Marko Kro;Lister Staveley-Smith;NingYu Tang;Lei Qian;MengTing Liu;ChengJin Jin;YouLing Yue;Yan Zhu;HongFei Liu;DongJun Yu;JingHai Sun;GaoFeng Pan;Hui Li;HengQian Gan;Rui Yao;National Astronomical Observatories,Chinese Academy of Sicences;University of Chinese Academy of Sciences;CAS Key Laboratory of FAST,National Astronomical Observatories,Chinese Academy of Sciences;International Centre for Radio Astronomy Research (ICRAR),The University of Western Australia;ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D),The University of Western Australia;FAST Collaboration;
  • 英文关键词:HI regions and 21-cm lines;;radio telescopes and instrumentation;;statistical and correlative studies of properties
  • 中文刊名:JGXG
  • 英文刊名:中国科学:物理学 力学 天文学(英文版)
  • 机构:National Astronomical Observatories, Chinese Academy of Sicences;University of Chinese Academy of Sciences;CAS Key Laboratory of FAST, National Astronomical Observatories, Chinese Academy of Sciences;International Centre for Radio Astronomy Research (ICRAR), The University of Western Australia;ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), The University of Western Australia;FAST Collaboration;
  • 出版日期:2019-03-22 11:13
  • 出版单位:Science China(Physics,Mechanics & Astronomy)
  • 年:2019
  • 期:v.62
  • 基金:supported by the National Key R&D Program of China(Grant Nos.2017YFA0402600,and 2016YFA0400702);; the National Natural Science Foundation of China(Grant Nos.11690024,11725313,11590783,and 11803051);; the International Partnership Program of Chinese Academy of Sciences(Grant No.114A11KYSB20160008);the Young Researcher Grant of National Astronomical Observatories,Chinese Academy of Sciences;; the CAS “Light of West China” Program
  • 语种:英文;
  • 页:JGXG201905006
  • 页数:9
  • CN:05
  • ISSN:11-5849/N
  • 分类号:56-64
摘要
The Five-hundred-meter Aperture Spherical radio Telescope(FAST) is expected to complete its commissioning in 2019. FAST will soon begin the Commensal Radio Astronomy FasT Survey(CRAFTS), a novel and unprecedented commensal drift scan survey of the entire sky visible from FAST. The goal of CRAFTS is to cover more than 20000 deg2 and reach redshift up to about 0.35. We provide empirical measurements of the beam size and sensitivity of FAST across the 1.05 to 1.45 GHz frequency range of the FAST L-band array of 19-beams(FLAN). Using a simulated HI-galaxy catalogue based on the HI Mass Function(HIMF), we estimate the number of galaxies that CRAFTS may detect. At redshifts below 0.35, over 6 × 105 HI galaxies may be detected. Below the redshift of 0.07, the CRAFTS HIMF will be complete above a mass threshold of 109.5 M⊙. FAST will be able to investigate the environmental and redshift dependence of the HIMF to an unprecedented depth, shedding light onto the missing baryon and missing satellite problems.
        The Five-hundred-meter Aperture Spherical radio Telescope(FAST) is expected to complete its commissioning in 2019. FAST will soon begin the Commensal Radio Astronomy FasT Survey(CRAFTS), a novel and unprecedented commensal drift scan survey of the entire sky visible from FAST. The goal of CRAFTS is to cover more than 20000 deg2 and reach redshift up to about 0.35. We provide empirical measurements of the beam size and sensitivity of FAST across the 1.05 to 1.45 GHz frequency range of the FAST L-band array of 19-beams(FLAN). Using a simulated HI-galaxy catalogue based on the HI Mass Function(HIMF), we estimate the number of galaxies that CRAFTS may detect. At redshifts below 0.35, over 6 × 105 HI galaxies may be detected. Below the redshift of 0.07, the CRAFTS HIMF will be complete above a mass threshold of 109.5 M⊙. FAST will be able to investigate the environmental and redshift dependence of the HIMF to an unprecedented depth, shedding light onto the missing baryon and missing satellite problems.
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