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1 WFIRST and Subaru in Middle 2020 s
2 Euclid μm WISH 1 5μm Wide field Space Missions in 2020 s WFIRST 0.6 2μm (option 2.4μm)
3 Wide-field Imaging Surveyor for High-redshift 超広視野初期宇宙探査衛星計画 ISAS Call for Proposals was issued (deadline Feb.16) Toru Yamada on behalf of JAXA/ISAS WISH Working Group with the contribution to WISH Science Workshop
4 DISCUSSION TODAY Sharing Scientific Complementarity and Synergy between Subaru optical Wide-field Capabilities and WFIRST (and WISH, Euclid ) HSC and PFS SSPs and WFIRST Collaborative Survey Strategies toward/in 2020 s What is the strongest synergy? Uniqueness of Subaru (e.g., LSST.) What is OUR desire? Development of Coronagraph Instrument Subaru/JAXA heritage and future plan
5 WFIRST-AFTA - NASA s future Flagship Mission in Astronomy in middle 2020 s after JWST - Wide-area surveys focused, 25%Guest Observations 1.5yrs - Dark Energy (Precision Cosmology) 2.5yrs Micro-lensing Exoplanet Survey 1yr Deep and Wide-field NIR Survey 1yr High-Contrast Instrument (Coronagraph) 1yr for Exoplanets - Current Baseline Model: 2.4m TMA telescope 0.4-2μm - Instruments Wide Field Instrument (Imager,grism,IFU) / Coronagraph - Potential International Interests Japan (JAXA) / Canada (CSA) / Europe (ESA) / Korea (KASI)
6 WFIRST-AFTA WFIRST is the top-ranked large space mission in the New Worlds, New Horizon (NWNH) Decadal Survey of Astronomy and Astrophysics in US (2010). It was started with the Design Reference Model (DRM) with 1.3m diameter telescope (JDEM-like), but in 2012, the two 2.4m NRO wide-field telescopes (nearly completed) are given to NASA WFIRST Astrophysics Focused Telescope Assets High-Contrast Coronagraph Instrument has been added to the payload for direct imaging of exoplanets and debris disks (2013) step toward future exoplanet-optimized mission
7 WFIRST-AFTA Time Line 2013 WFIRST-AFTA SDT started / NASA WFIRST-AFTA Office 2014 Coronagraph Instrument Architectures down selected (Hybrid Liyot primary / PIAA as backup) WFIRST-AFTA SDT Interim Report Jan WFIRST-AFTA-SDT Final Report - Feb CATE (cost appraisal and technical evaluation) - ~ US WFIRST-AFTA Science Team Formulation (International potential partners will participate) Maturing key technologies to TRL 5 by FY17 and TRL 6 by FY Start of Formulation : Launch
8 WFIRST DRM1 1.3m DRM2 1.1m Cost down NRO 2.4m 2012 NASA に供与 US Astro2010 Decadal survey JDEM の衛星案に基づく DRM=Design Reference Model 米国 Decadal Survey で宇宙論 系外惑星 ( マイクロレンズ ) サーベイの複合計画 WFIRST SDT による検討 (DRM1 / DRM2) 2012 NASA がNROから2.4m 望遠鏡を供与される WFIRST AFTA として2.4m 版を検討 系外惑星直接観測コロナグラフ装置を加えた案を検討 JWST につづく戦略ミッション 2015/1/15 8
9 WFIRST-AFTA Instruments
10 Current Plan for Surveys A fraction of the survey area may be located in Northern sky! D.Spergel in WFIR meeting 2014 Nov
11 WFIRST: activities in Japan T. Sumi was a member of WFIRST-SDT In 2013, WFIRST-AFTA SDT was formed and JAXA was invited to send a representative as an observer (T. Yamada) WFIRST Preparative Consortium ( 連絡会 ) ~25 members Great interests of Japanese astronomers, in the field of cosmology / galaxy formation / Galactic bulge / microlensing / astrometry / exoplanets Contribution in developing Coronagraph Instrument (Tamura, Enya, Murakami, Nishikawa, Kotani,.) JAXA/ISAS Space Science Steering Committee WACO Working Group for Small/International Program
12 JAXA ISAS WACO Working Group started in 2014 (WG for small/international collaboration projects) Possible hardware contributions for WFIRST/AFTA have been discussed mainly on coronagraph instruments so far in Japan. We call the Japanese contribution part in WFIRST/AFTA Coronagraph as WACO=和光 To soften light in Japanese Or Japanese pirates 倭寇 or a Japanese restaurant in Pasadena (WAKO=和光)??
13 Possible Japanese Contributions to WFIRST Coronagraph Instrument Hardware/development contribution - polarization module - innovative masks and analysis techniques - vacuum testbeds at JAXA/ISAS - a PIAA module using reflective elements Wide-field Survey - Collaborative/Coordinated Ground-based Survey with PFS (calibration of photo-z) HSC (optical band) in northern hemisphere - HSC/PFS SSPs (to be public by middle 2020 s) + Coordinated Survey in 2020 s w/ community support Micro-lensing survey / Galactic bulge science - preparative survey / field selection (HSC)
14 DISCUSSION TODAY Sharing Scientific Complementarity and Synergy between Subaru optical Wide-field Capabilities and WFIRST (and WISH, Euclid ) HSC and PFS SSPs and WFIRST Collaborative Survey Strategies toward/in 2020 s What is the strongest synergy? Uniqueness of Subaru (e.g., LSST.) What is OUR desire? Development of Coronagraph Instrument Subaru heritage and future plan
15 Wide-field Surveys WFIRST High Latitude Survey Y<26.7 J<26.9 H<26.7 F180<26.2AB 2400deg 2 (total) Northern Hemisphere - Early observations at HSC/PFS field - Coordinated New Survey at Pole? ~ deg 2 ~ 2-4 x HSC SSP Deep (a few100 nights) ~ coordinated with WISH-UDS Survey 27-28AB 1-5μm 100deg 2
16 HSC SSP Survey Depth WFIRST High Latitude Survey (HLS) Y<26.7 J<26.9 H<26.7 F180< deg 2 (total) HSC Wide / WISH UWS HSC Deep/ WISH UDS
17 Hubble μm Spitzer IRAC 3 10μm 特に3.6 & 4.5μm バンド Akari IRC NIR 2 5μm
18 Euclid μm 可視広視野撮像分光 近赤外測光 精密宇宙論 暗黒エネルギー WFIRST 0.6 2μm (option 2.4μm) WISH 1 5μm
19 WFIRST Wide-Field Imager: Filters (Plan)
20 WFIRST Capabilities and Surveys +6.3 x6 点源 5σ 7σ
21 Guest Observer Capability and Coronagraph Capabilities
22 コロナグラフ装置について 太陽系外惑星の直接観測によるキャラクタリゼーションを行うためこれに特化した装置の搭載を検討する ミッションの寿命を 5 年 6 年とし 1 年間の観測時間を割り当てる NASA Astrophysics 部門では 並行して Probe Class の系外惑星ミッションを 2 方式で検討する STDT を立ち上げていたが WFIRST AFTA コロナグラフが可能な場合 これに収束する見込み WFIRST は高コントラスト観測に最適化されたミッションではないが 将来の地球型惑星の直接観測が可能なミッションへの技術的ステップとも位置づける 科学目標 : 近傍の 200 個程度の系のサーベイ ~10 20 個の 4 地球半径以上の惑星の多色撮像 ~6 10 個の巨大惑星の分光 最大 4 個程度の 4 地球半径以下の惑星の直接検出 13 年 12 月にコロナグラフ装置のアーキテクチャを選定 ~2016 までに TRL5~TRL6 のレベルでの技術実証を目指す (IWG~0.2, 10 9 コントラスト 広帯域 ) National Research Council のレビュー (2014/03) では コスト スケジュールを含むリスクに対する強い関心 / 早期の技術的実証の必要性が指摘されている 2015/1/15 22
23
24 Scale Structure 2000Large sq deg High latitude Survey Theory HLS Euclid MW halo Bullet clusters CLASH: Cluster lenses Z > 8 galaxies Quad lenses: DM sustructure QSO LF faint end and LF high z Proto clusters Rare galaxy galaxy lenses
25 WFIRST Exoplanet Study 2015/1/15 25
26 WFIRST マイクロレンズ系外惑星研究 Kepler WFIRST 2015/1/15 26
27 WFIRST Coronagraph Instrument 2015/1/15 27
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次世代赤外線天文衛星 SPICA の概要 2011 年 1 月 6 日中川貴雄 (JAXA) SPICA team 企画セッション :SPICA の挑戦 概要 次世代赤外線天文衛星 SPICA の概要 ( 中川 JAXA ) SPICA 観測装置 ( 片坐 JAXA ) 科学目的 SPICA の目指すもの ( 松原 JAXA ) SPICA で探る太陽系科学 ( 渡部 天文台 ) SPICA による系外惑星研究
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