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SKA Science Report (Mostly )

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1 SKA Science Report (Mostly 2018-2019)
Contents News from SKAO SKAJ Science Activity 赤堀卓也 グループサイエンティスト/マネージャー 2019/9/2 SKA-Japanシンポジウム2019

2 1. News from SKAO Welcome MeerKAT!
MeerKAT inauguration (開所式) was held in July 13, 2018 Some large projects and conditional open-use in progress in 2019 2019/9/2 SKA-Japanシンポジウム2019

3 1. News from SKAO Science Highlights
★Source6 ★Source8 ★Source2 ★Source3 ★Source1 ★Source4 ★Source7 ★Source5 Bowman+18, Nature EDGES experience at MRO A signal of HI absorption in CMB radiation at z=15-20? Shannon+18, Nature ASKAP 1.4GHz PAF FRBs can be classified into “repeater” and “one-off”? 2019/9/2 SKA-Japanシンポジウム2019

4 1. News from SKAO Science Community
Including 22JPs (2.5%) SKA General Science Workshop UK SKA Science Working Group membership has grown by a factor of four in the past 5 years. There ware about 300 registrants in the last SKA Science Workshop 2019. Cosmology Redbook (2019) has been published The 14th Group “Gravitational Wave” was established 2019/9/2 SKA-Japanシンポジウム2019

5 1. News from SKA Office SKA Data Challenge (SDC) #1
Some 107 sources based on T-RECS sky model (Bonaldi+18). 1 Oxford-ICRAR /UK-AU 2 ICRAR/AU 3 EngageSKA /Portugal 4 ARCIt-CACAO /IT 5 hs/DE, IITK/IN, IPM/Iran, JLRAT/CN, Shanghai/CN ←8, ↑1000, 100→ Integration Time (hr) 17 teams registered 9 teams submitted To get the community familiar with SKA data product To develop efficient methods for source finding & source characterization 2019/9/2 SKA-Japanシンポジウム2019

6 1. News from SKAO SDP HPC Breakdown
SKA-TEL-SKO DFT in ICAL 2019/9/2 SKA-Japanシンポジウム2019

7 1. News from SKAO SKA Regional Center (SRC)
SKA-TEL-SKO “京”=10PFLOPs If 8TB=2万円, 1EB=25億円 PFLOPs 30 20 10 ExaByte 3 2 1 100Gbit/s, 5.2M€/yr (in operation cost) Forecast SRC requirements 2019/9/2 SKA-Japanシンポジウム2019

8 1. News from SKAO Beyond Band 5
Freq. (GHz) LOW Band 1 Band 2 Band 3 Band 4 Band 5a Band 5b Band 5c/6 Band B 0.05 0.3 1.0 1.7 3 5 8 15 25~50 Solar System Planet Formation Astrochemistry & Life Tomoya Hirota Star Formation & Stellar Evolution Tomoya Hirota/Toshihiro Handa/Takeru Murase/Yuushi Hirata/Hiroshi Imai/Koichiro Sugiyama Galactic Structure Hiroshi Imai/Toshihiro Handa/Tomoya Hirota Nearby Galaxies Kazuhiro Hada/Yuki Kudoh History of the Universe Takuya Akahori Cosmology Kohji Yoshikawa Fundamental Physics Transient Phenomena Takuya Akahori/Sujin Eie/Haruka Sakemi/Mami Machida 13 Japanese people will contribute to use cases Deadline End of September 2019 2019/9/2 SKA-Japanシンポジウム2019

9 2. SKAJ Science Section Risks of Calibration/Imaging
F: far sidelobe error, S: near sidelobe error, P: Statistical pointing error, P’: instantaneous pointing error Q: primary beam error, B: primary beam freq. error, M: source model error Clear Need a factor of several improvement Need one order of magnitude improvement All 10hr x 100 epochs Shimwell+17, A&A, 598, A104 Q. Can a 1000 hr integration reach the thermal- noise limit? Error budget analysis (SKA-TEL-SKO ) Large gain error. Must do self-calibration Need good primary beam shape & pointing stability Q. Can a dynamic range reach 50dB of the requirement? Self-cal. using bright compact sources LOFAR achieved 60dB (but depends highly on the sky) Need intelligent high-speed pipeline 2019/9/2 SKA-Japanシンポジウム2019

10 2. SKAJ Science Section Comparison with ALMA/ngVLA
Snow line of protoplanetary disk 5 AU = pc 150km 25GHz ≒ 18mas of ALMA B6 But the brightness-temperature sensitivity is limited. SKA’s targets are: Inner/equatorial disk where ALMA bands are optically-thick Jets, ionized wind, flare Some molecular lines that are difficult to study at ALMA bands In 2030s, SKA2 will exceed ngVLA. Can SKA extend up to 50 GHz? Calc. by H. Kobayashi Good Sensitivty SKA2 Good Ang. Resolution 2019/9/2 SKA-Japanシンポジウム2019

11 2. SKAJ Science Section SKAJ SKA Regional Center Task Force
Mission To list the services needed for us To develop our participation plan for the SRC alliance Particularly, China SRC Evaluate the cost Roadmap Members Name Affiliate Role Tomoya Hirota SKAJ Chair, Cont., Line, Pol. Takuya Akahori SKAO, Magnetism Yuuki Adachi MVO VERA Misato Fukagawa ALMA ARC ALMA Kohji Yoshikawa Tsukuba U. HPC, Cosmology Kenji Hasegawa Nagoya U. HPC, EoR 2019.7 #1 MTG Mission Definition 9 #2 MTG Learn SRC Define AIs 11 @Shanghai SKA-WPC 12 #3 MTG WPC report Resolve AIs 2020.3 #4 MTG 5 6 #5 MTG 2020.9 #6 MTG Draft start 11 @Shanghai Consultation 12 #7 MTG First draft 2021.3 #8 MTG Second draft 2021.6 #9 MTG Final report 2019/9/2 SKA-Japanシンポジウム2019

12 Summary Report from SKAO SKAJ Science Activity
SKA Precursors/Pathfinders go well! SKA Community is increasing significantly Science Data Challenge: #1 closed, #2 on going HPC and SRC forecasts Beyond Band 5 use case SKAJ Science Activity Risks of calibration/imaging Comparison with ALMA/ngVLA SKAJ SRC Task Force 2019/9/2 SKA-Japanシンポジウム2019


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