Microsoft PowerPoint - InstWS a.pptx
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- みひな すすむ
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1 トモエのつくりかた 東京 学 学院理学系研究科附属天 学教育研究センター 科学技術振興機構さきがけ 酒向重 第 6 回可視 外線観測装置技術ワークショップ :50-11:10, 国 天 台三鷹
2 1. 曽超広視野 速 CMOS カメラ Tomo-e Gozen 2. トモエのつくりかた
3 Sako et al. 2016, SPIE Ohsawa et al. 2016, SPIE Extremely wide field high speed camera the Tomo e Gozen Telescope Kiso 105 cm wide field Schmidt Field of view 20 deg 2 in φ9 deg, AΩ = 28 Image sensors 84 chips of CMOS Data acquisition rate 2 fps (max) Data production rate 30 TB/night (max) Commissioning Aug chips of high sensitive CMOS sensors 常温 常圧運, フィルタ ( 透過, g, r, grism) 中のみ交換
4 Completion of survey powers for transient events 100 CMOS CCD Field of View (deg 2 ) unexplored universe 17 Tomo e 18 TAOS II ZTF Temporal resolution (sec) LSST Pan STARRS iptf Decam 20 KWFC HSC 22 SDSS The numbers in the circles show limiting magnitudes.
5 New fields developed by Tomo e Survey for extremely rare transient events 極めて稀な時間変動イベントの探査 Survey for rapid transient events with τ < 1 sec 1 秒以下で変化するイベントの探査 Shock Breakout of core collapse SN Explosion of Nova Optical follow up of Gravitational wave Afterglow of Gamma ray burst Optical candidate of fast radio burst NASA Optical counterpart of GW NASA Neutron star merger X ray time variable objects Transit of Exoplanet Occultation by Trans Neptune object Potentially Hazardous Asteroid Faint meteor YouTube Potentially hazardous asteroid NASA Transit of exoplanet
6 Timeline for Development Commissioning in 2018 present day Sensor development Sensor evaluation Data acquisition system Camera body Data analyzing system Assemble Test observations commissioning commissioning
7 Tomo e Gozen Prototype model 8 chips of CMOS sensor Spider structure of telescope 380 mm Tomo e Gozen prototype model 590 mm Sako et al. 2016, SPIE Ohsawa et al. 2016, SPIE Kiso 105cm Schmidt telescope
8 Test observations Observation date First light on 24 th Nov Dec. 1 st 21 st, 2015 (21 nights, usable ~11nights) Main observation mode 2 fps, full frame, no filter, Gain=High Data production rate 3 TB/night (average), 35 TB/run Targets Flash survey, Meteors, Comet
9 Data sample obtained by Tomo e PM First light image, h x Per open star cluster (1 chip, 5 sec exposure, FoV of 39.7 x 22.4 ) High dynamic image of M42 Orion nebula (1 chip, 0.5 sec/exposure x 5,018 frames) Sporadic meteors of > 5,000 events/night detected Movie data (10 fps, partial readout, 1 chip)
10 Faint meteors Trail of faint meteor Faint meteors up to 14 mag detected. (> 9 mag in previous study) About 1,000 events of sporadic meteors detected in a night.
11 Ground based observation of X ray space telescope HITOMI N E S HITOMI / JAXA 8.2 deg W Sensor 7 Sensor 6 Sensor 5 Sensor 4 Light curve 2 fps, 50 sec starting from 20:24:08 31 st Mar Relative brightness Time (sec) Press release from Kiso observatory. U. of Tokyo Used in press releases at JAXA Reported in NHK news and major news papers
12 Flash Unidentified Flash Objects detected in frames taken in 2 fps
13 Contamination of Artificial stellar objects Low orbit satellite Example of flashing and moving object Geostationary orbit satellite JCSAT2 30 th Nov. 2015, 10 fps JCSAT2/Boeing YouTube Geostationary orbit satellite, 36,000 km Space debris with φ 1 cm on the geostationary orbit can be detected. Rotating debris are observed as flash phenome. Serious problem!!
14 1. 超広視野 速 CMOS カメラ Tomo-e Gozen 2. トモエのつくりかた まだ完成していないので成功例とはかぎらない
15 2010 年ある 某所 はじまり C 社 : 実は こんな CMOS センサがあるのですが なにかに使えませんか? 私 : ああ この仕様だと 天 観測では使えませんねえ C 社 : そうですか しかし ご迷惑でなければ試させていただけませんか? 私 : そうですねえ 搭載は簡単そうなので やってみましょうか あまり期待しないでください 2011 年 1 曽観測所 C 社 : 私 : C 社 : 私 : わあ さすがに星がたくさん写りますね はい これくらいは写ると思います あ 雲がきた あ! 衛星 あ! 流れ星 また これも?? なんだろうこの違和感は 観測に使 した 200mm x 200mm CMOS センサを搭載した試験カメラ 教訓 仕様値からは想像できないことがある データに触れて初めて感じることがある 分野外の専 家のコメントは 切に 2011 年 9 15 キヤノン記者発表の様
16 2012 年ある 某所 やってみる C 社 : 実は こんな CMOS センサもあるのですが 使えませんか? 私 : C 社 : 私 : ああ この仕様だと天 観測では使えませんが 画素サイズはマッチしてますね 試験観測をやってみましょうか 評価 の読み出し装置はありますよ ああ この仕様だと天 観測では使えませんが すぐに試験ができて便利なのでお貸しください 2012 年 12 曽観測所 私 : まあまあ写りますね でも バックグラウンドが いですね C 社 : 私 : C 社 : 冷却ですからね 触ると熱いくらいですから 天 観測に いるには 冷却が必須なのですよ そうですものね 冷却がなければ楽なんですけどね カメラを準備する様 (B4 藤堂さんら ) 教訓 すぐに試験できる環境を持つことが 切 すぐに試験する意思が 切 これらこそ 学の研究室の役割 2012 年 12 35mm センサの 1 回 の試験観測の様
17 速観測では CCD より CMOS の が 感度 しかも 冷却で実現が可能 等級 検出限界等級 2012 年度東 B4 卒業研究藤堂 より 0.2 mag due to dqe 積分時間 [sec/frame] V-band, S/N = 5, Seeing = 3 読み出し時間による観測効率の損失をふくまず 検出限界等級 (CMOS) 積分時間 (sec) 等級 1/ 天 CCD と同程度の感度を達成 - 10sec/frame 以下では CCD を上回る感度を達成
18 業界の伝統を疑ってみる センサの冷却は必要なのか? センサの真空設置は必要なのか? センサの温度制御は必要なのか? センサは粗末に扱うと壊れるのか? センサは 感度でないと使えないのか? 練習中に を呑んではだめなのか? 教訓 技術はいつのまにか進んでいる 伝統が かせになっていないか 伝統を 度はうたがってみるべき
19 トモエゴゼンの設計ポリシー シンプルなシステムの追求 - 軽量 - 冷却 真空 - 駆動部なし - 組み て簡単 シンプルな 的 ( サイエンス ) の追求 - 突発天体の 発 に注 する - フィルタ交換は 中のみ 動 - データを全て保存しない 他に類の無い観測装置の実現につながる
20 皆直 我独横 榊莫 んさかきばくざ
21 横 は慎重に 横 すると決めたら慎重に歩くべき 地雷が埋まっているかも 慎重でも迅速にやらないと 直 する世間に取り残される 要素試験を迅速に繰り返す
22 トモエゴゼンの開発 針 計算はほどほどに 実物を ながら考える 試験機を迅速に製作 迅速に測定 設計にフィードバック これまでに製作した試験機 2012 年 2014 年 2015 年 2016 年 2016 年 2017 年予定 センサ単体試験機センサ実験室評価試験機センサ8 台試験機 (Tomo e PM) 熱試験機コネクタ試験機光通信試験機 フラットケーブルを通す のサイズを検討するためだけの試験機
23 トモエゴゼンの開発体制 トモエサイエンスチーム 筐体 橋 ATC/NAOJ センテンシア社 光学系 酒向 オプトクラフト社 酒向 例会議 電気 酒向 東 院 キヤノン社 インターフェース社 望遠鏡 猿楽 曽スタッフ 東 院 ソフト 澤 他研究機関のアドバイザ 特徴 試験装置をメーカに依頼 試験を 学が担当 試験結果をメーカに迅速にフィードバック 学院 にシステム概念設計を担当させる 実機へつなげる
24 既存技術をとりいれる 既存技術をそのまま使うのではなく いかに味付け ( 応 ) して 使うかがポイント アイデアだけでなく試験も 切 コンシュマー向け35mm CMOSセンサ ( キヤノン社 ) 半導体 熱伝導両 テープ (3M 社 ) 汎 アナログー光変換システム ( インターフェース社 ) 精密加 技術 ( 先端技術センター / 国 天 台 ) 外線 CMOSセンサ 動画読み出しシステム ( 東京 学 ) 外線 CMOS センサ データ伝送システム ( 東京 学 ) 超広視野望遠鏡 (1974 年建設 東京 学 曽観測所 ) 情報数理処理技術 ( 統計数理研 情報研 各 学 ) 熱伝導両 テープの 期耐久 較試験の様 結果 3M 社 が選ばれる
25 トモエゴゼンの開発ツール トモエチーム ( 学 ) が利 するソフト ドキュメント作成 Power Point, Excel CAD Sketch up(3d, 指 書 ), Auto CAD(2D, 製造 ) 回路設計 EAGLE, Xilinxデザインツール 観測視野確認 ステラナビゲータ ( 広い視野をカバー ) トモエチーム ( 学 ) が利 するサービス 情報管理 Pukiwiki スケジューリング みんなでガント.com 電 回路部品 Chip1Stop, RSコンポーネンツ 電気 般 アルミ製品 MISUMI, タカチ電機 ( ラック ) 電気基板製作 実装 P 板.com Web 即時購 Amazon.com, モノタロウ, アズワン
26 Data flow for 1 night data Conceptual design Telescope building KISO OBSERVATORY Support building Telescopes around the world 30 TB/night Camera Controller 50 TB/d τ ~ 3 days 150 TB Servers for scientific projects supernova GW alert Analysis Server +WCS file split meteor debris 50 TB 50 TB/d τ ~ 1 day day time flash pulsar Servers on external site 30 TB Light curves of all sources Text files 1 2 TB/d Short timescale events Masked movie Detected fast moving objects Image files τ ~ 1 month Co added Image files copy 300 TB Onsite DB 1 2 TB/d τ ~ 1 year copy every month External DB
27 Machine learning Informatical approach Collaborator: Wide field survey team/crest, IPMU (PI Prof. Yoshida) Source detection Classification These studies are now ongoing under collaborative research. Supernova on parent galaxy = Sparse modeling Ref image Obs image Subtracted image Collaborator: Prof. Ikeda, Dr. CREST, ISM Flash detection Raw data GoDec method Low Rank Sparse Movie compression Data mining / compression Collaborator: Dr. SAKIGAKE, Yamanashi U. Source detection Fast computation
28 Looking for Spark joy = ときめき in Movie Big data. When keeping only the items you feel spark joy, you will definitely become happy. ときめくモノだけを残すとかならず幸せになれます KONDO Marie The Life Changing Magic of Tidying Up ISBN (2014) 近藤 理恵 がときめく づけの魔法 ISBN (2010)
29 トモエ PM での失敗例 加 は精確だった 図 をまちがえた 正しい 数値が間違っていた (21.265) (24.766) (27.099) (27.854) (27.854) (27.099) (24.766) (21.265) 基準線 IOA- 035D IOA- 035C IOA- 035B IOA- 035A SIDE VIEW IOA- 035A IOA- 035B IOA- 035C IOA- 035D 間違い 筐体内の空冷のために圧縮乾燥空気を通す をあけた でも がでない 計算をまちがえた 筐体内の空冷を中 アナログ 速通信の線が すぎて通信エラーが多発 光ファイバに変換
30 まとめ 曽超広視野 速カメラ Tomo e Gozen 世界初の天 広視野 CMOSカメラ CMOS x 84 枚 20 平 度 最 2fps 最 30 TB/ 夜 2018 年完成予定 トモエのつくりかた データに触れて初めて感じることがある すぐに試験する環境と意思が 切 学の研究室の役割 装置の設計とサイエンスを 的をできる限りシンプルにする 技術はいつの間にか進んでいる 伝統を疑う 既存技術をできるだけ上 に使う 使うときは少し 夫と試験をする 試験装置の開発もメーカの援助を受けて迅速化する ビッグデータ的考え を導 する
Microsoft PowerPoint - SchmidtSympo a.pptx
曽超広視野 CMOS カメラ Tomo-e Gozen 計画の現状 東京 学 学院理学系研究科附属天 学教育研究センター酒向重 2017/7/5-6, シュミットシンポ 2017, 曽町 化交流センター 巴御前出陣図 東京国 博物館蔵, 蔀関 ( しとみかんげつ, 1747-1797) Image: TNM Image Archives Advanced large survey program of
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東京大学大学院理学系研究科附属天文学教育研究センター木曽観測所次期広視野観測装置計画 木曽超広視野高速 CMOS カメラ Tomoe Gozen の開発の進捗報告 酒向重行, 小林尚人, 土居守, 本原顕太郎, 宮田隆志, 諸隈智貴, 高橋英則, 大澤亮, 菊池勇輝, 猿楽祐樹, 青 木勉, 征矢野隆夫, 樽沢賢一, 三戸洋之, 中田好一 ( 東京大学天文学教育研究センター ), 臼井文彦, 松永
258 5) GPS 1 GPS 6) GPS DP 7) 8) 10) GPS GPS 2 3 4 5 2. 2.1 3 1) GPS Global Positioning System
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