彭勃，中国科学院国家天文台研究员，1993年获天体物理博士学位。 1993年参与10国大射电望远镜LT（SKA）筹备，共同发起、提出和发展SKA中国概念及其先导FAST。1994年组建并任LT课题组长，1998年FAST项目委员会主任，1999年SKA组织董事，2005年大射电望远镜实验室主任，2008年FAST工程副经理，2012年SKA 973首席科学家。长期从事射电源巡天、瞬变天体、星系形成与演化、天文技术与方法研究。主持完成国家自然科学基金（重大）、中科院（重点）及科技部973项目等。发表国际第一篇SKA（Square Kilometre Array）无线电环境选址论文等约130篇，做邀请报告上百次。 现任贵州射电天文台台长、FAST工程经理部副经理、国家天文台射电天文技术实验室主任。自1994年，代表中国长期参与平方公里阵望远镜（SKA）国际合作，与荷兰、德国、英国、南非、澳大利亚等射电天文学家建立了长期友好合作。
目錄：
Review of FAST HⅠ Survey Plan001
Ming Zhu， Mei Ai， Yuanqi Guo and the FAST teamFAST and the Pathway to Cosmic Magnetism in the SKA Era010
A. Russell TaylorApertifFAST Synergy for Studies of Low Surface Brightness Emission018
Elizabeth A. K. Adams， Ming Zhu， Bjrn Adebahr， W.J.G. de Blok，Kelley M. Hess，
Danielle M. Lucero， Raffaella Morganti， Tom A. Oosterloo，J.M. van der Hulst，
Marc A. W. Verheijen， Rurong Chen， Mei Ai， Bo ZhangTelescope Synergies for HⅠ and Intensity Mapping Observations030
Natasha Maddox， Yidong Xu， W.J.G. de Blok，Ming Zhu， Xuelei Chen，
Lister StaveleySmithHow Shall We Determine Detection Sensitivity in Radio Pulsar Search?037
Meng YuSingle Pulse Study with FAST042
Jiguang Lu and Bo PengInvestigation of New Double Pulsar Candidate PSR J1906 0746050
C.M. Zhang， Y.Y. Yang， D. Li， Z.C. PanPulsar Study in the Globular Cluster M28 with the Large European Array
for Pulsars057
L. Wang， B. W. Stappers， J. W. McKee， C. G. Bassa， I. Cognard，S. Chen，
M. Gaikwad， G. H. Janssen， R. Karuppusamy， M. Kramer，K. J. Lee， K. Liu，
D. Perrodin， S. A. Sanidas，R. Smits， and W. W. ZhuA Method for Fast Radio Burst Detection with FAST Based on FocalField
Feature Matching066
Decheng Wu， Jin Fan， Hailin Cao， Zhoujian Chen， and Shizhong YangFASTMWA Synergies in Pulsar and Fast Radio Burst Science075
N. D. Ramesh Bhat， Nicholas A. Swainston， and Bradley W. MeyersLooking for Low Column Density Gas with MeerKAT & FAST087
Claude CarignanFrom Spectra to Spatially Resolved HⅠ Observations096
Gyula I. G. JzsaConstraining Inflationary Features with 21 cm Intensity Mapping107
Yidong Xu， Jan Hamann， and Xuelei ChenCombining 21cm and LargeScale Structure Surveys for Cosmology and
Galaxy Evolution Constraints118
Moumita Aich， Warren Naidoo， Kavilan MoodleyEffect of NonCircular Motions on the Rotation Curves of Barred Galaxies128
Toky H. Randriamampandry， Claude Carignan，and Nathan DegDifferential Observation Techniques for the SZE21 cm and Low
Frequency Radio Emission138
Charles Mpho Takalana， Sergio Colafrancesco， and Paolo MarchegianiCold Gas in Galaxies： SingleDish HⅠ Surveys in the SKA Era154
Barbara Catinella & Luca CorteseThe Synergy between HⅠ SingleDish and Optical IntegralField
Spectroscopic Surveys163
Luca Cortese & Barbara CatinellaProgress on FAST Extragalactic Survey Data Reduction Pipeline174
Bo Zhang， Jian Xiao， Ce Yu， Qi Luo， Zhicheng Yang， and Ming ZhuAutomated 3D Source Finding for LargeScale HⅠ Surveys181
Tobias Westmeier， Nadine Giese， Thijs van der Hulst， Russell Jurek，Attila Popping，
and Paolo SerraSpectralLine Data Reduction Pipeline for HⅠ Extragalactic Survey
with FAST193
V.Kitaeff， M. Zhu， L. StaveleySmith， R. Tobar， K. Vinsen， A. Wicenec， C. WuMultiBand Studies of Radio Stars203
Hongpeng Lu， Liyun ZhangMeasuring Distances of Supernova Remnants Using HⅠ Absorption208
Shuai Wang and Liyun ZhangFASTMeerKAT and SKA Pathfinders SynergiesContents
內容試閱：
Spherical radio Telescope FAST is funded by the National Development and Reform Commission NDRC and managed by the National Astronomical Observatories of the Chinese Academy of Sciences NAOC, together with Guizhou provincial government as a cooperation partner. Multibeam and multiband receivers have been installed on the FAST, covering a frequency range of 70MHz3 GHz with capacity for upgrade to X band. The FAST is being commissioned at the moment with the key science drivers focusing on Pulsar and HⅠstudies.
Construction of MeerKAT, a 64element array of 13.5m offset parabolic antennas, is just completed in July close to the SKA central site on the South African Karoo plateau and should start its Large Survey ProjectsLSPs in the 2nd half year 2018. It will be merged with 133 15m SKA antennas in about 2025 to become SKA1mid. Large surveys will also get soon underway on the SKA pathfinders ASKAP in Australia and Apertif in the Netherlands. The CHILES survey highz galaxies at HⅠ is well underway and CHIME will start soon his intensity mappingexperiments.
With FAST and the SKA pathfinders MeerKAT, ASKAP, Apertif, LOFAR, MWA, resulting from the SKA global cooperation, we will be able to detect hundreds and even some thousands of new pulsars, as well as study in details the HⅠgas in nearby galaxies. With improvements in both sensitivity and resolution, the combination of FAST single dish and the array pathfinders instruments can probe the low column density gas cosmic web and low mass galaxies in a large area of their common sky, while HⅠintensity mapping can map large volume for cosmological BAO measurement.
In order to strengthen the science cooperation between the FAST the worlds largest single dish telescope in China and the different precursors of the SKA, we had a 2.5 days workshop, held in the Astronomy Town of Pingtang County close to the FAST site, in Guizhou Province on June 1315, 2018.
FASTMeerKAT and SKA Pathfinders SynergiesThe main goal is to explore the synergies between the FAST and the different SKA pathfinders as a leadin to the SKAera. The main science themes are： Pulsar research, HⅠresearch, HⅠintensity mapping, Cosmic Magnetism and Radio Instrumentation. This meeting is part of the activity of the 2018 Radio Astronomical Forum RAF 2018, which is an astronomical event held in Guizhou Province every year.
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