TIPS-JIM Meeting 19 April 2007, 10am, Auditorium 1. INS Division News Jerry Kriss 2. Results of the Cycle 16 HST Peer Review Brett Blacker 3. ACS/WFC Geometric Distortion and CTE Vera Kozhurina-Platais 4. JWST FGS-Guider Critical Design Review Pierre Chayer Next TIPS Meeting will be held on 17 May 2007. TIPS-JIM Meeting 19 April 2007, 10am, Auditorium 1. INS Division News Jerry Kriss 2. Results of the Cycle 16 HST Peer Review Brett Blacker 3. ACS/WFC Geometric Distortion and CTE Vera Kozhurina-Platais 4. JWST FGS-Guider Critical Design Review Pierre Chayer Next TIPS Meeting will be held on 17 May 2007. Cycle 16 Results Summary from the Science Policies Division of the Panel/TAC Deliberations 04/19/2007 Cycle 16 Director's Review Executive Summary • • • • • • GO Acceptance Rate: ~1/4.5 for proposals and ~1/5.6 for orbits SNAP Acceptance rate: 1/5 for proposals and ~1/4 for targets Regular AR Acceptance rate: 1/3.4 for proposals and 1/3.7 for $ Theory Acceptance rate: 1/3.6 for proposals and ~1/3 for $ AR Legacy Acceptance rate: 1/2.7 for proposals and ~1/4 for $ Acceptance rate approximately the same independent of size. • Slight dip in the 30-40 & 50-99 orbit bins • • 27% of program awarded to Large/Treasury Programs. • ESA acceptance fraction 13% for proposals and 12.6% for orbits Instrument breakdown for GO Programs: ACS/SBC (11.6%), NICMOS (41%), WFPC2 (41%), FGS (6.4%) 04/19/2007 Cycle 16 Director's Review 4 Executive Summary Continued • Chandra: 3 out of 12 proposals, or 89 ksecs out of 703 • • • • • • • submitted NOAO: No time awarded (Once again) Spitzer: 4 out of 20 proposals, or 203 hours out of 635 submitted Calibration: 5 proposals approved for 2 orbits/$477K ToO’s: 1 fast (< 2 week) + 14 other activations 1 Pure Parallel program awarded time (only 1 submitted) Once again very few future cycle orbits allocated No Survey Programs approved 04/19/2007 Cycle 16 Director's Review 5 Summary Results 04/19/2007 Cycle 16 Director's Review 6 • Cycle 16 Program Assessment Science assessment • Comments from TAC Chair •“In part because of the extreme proposal pressure...the decisions and cuts were decidedly painful. “ •“…. I came away from the review with the strong conviction that HST continues to do cutting edge and potentially transformative science, in spite of its longevity - or perhaps because of it - because over those same 16 cycles, astrophysics has itself changed dramatically (in part due to HST)….” • • Panel Chairs would strongly support extending panel allocations by 30-40% without further review Do we need a supplemental call? • • Cycle 16 (as is) is almost fully subscribed 1-2 month slip in SM4 (300-600 orbits) can be easily accommodated by promoting Cycle 16 proposals •We propose issuing a supplemental call only if SM4 slips to 2009 04/19/2007 Cycle 16 Director's Review 7 GO Instrument Summary 04/19/2007 Cycle 16 Director's Review 8 Over-subscription by Cycle Approved Orbits and Proposals by Cycle Acceptance Fraction by Size ESA Acceptance Fraction 04/19/2007 Cycle 16 Director's Review 12 Approved PI Institutions orbs & props 04/19/2007 Cycle 16 Director's Review 13 Institutional Acceptance Fraction 04/19/2007 Cycle 16 Director's Review 14 Orbit Size by Cycle Calibration Proposals • 6 Proposals Submitted: • 1 GOs for 2 prime orbits • Approved as requested: Bob O’Dell, Vanderbilt University, Calibration of the WFPC2 HeII and [SII] Filters • 5 ARs for $477K • 4 Approved for $379K • Bernard McNamara, New Mexico State University, Establishing a Zero Motion Reference • • Frame for the FGS Rolf Jansen, Arizona State University, Removing the herring-bone pattern-noise from *all* STIS Side-2 CCD data: a factor ~3 enhancement in sensitivity Bob O’Dell, Vanderbilt University, A Final Calibration of the Primary WFPC2 EmissionLine Filters Using the Orion Nebula • Andrew Dolphin, Raytheon, WFPC2 CTE and Photometric Zero Points 04/19/2007 Cycle 16 Director's Review 16 Chandra Coordinated Proposals • 12 GO Proposals were submitted for 404 HST Orbits and 703 ksecs of Chandra time. • 3 were approved for 33 HST Orbits and 89 ksecs of Chandra time • Hartmann • Biretta • Herczeg 04/19/2007 A Hard Look at Stellar Disks at the Epoch of Planet Formation (6 HST Orbits and 40 Chandra Ksecs) Monitoring the Giant Flare of HST-1 in the M87 Jet (9 HST Orbits and 35 Chandra Ksecs) Evaluating the Role of Photoevaporation of Protoplanetary Disk Dispersal (18 HST Orbits and 14 Chandra Ksecs) Cycle 16 Director's Review 17 NOAO Coordinated Proposals • 8 GO Proposals were submitted for 358 HST Orbits and 32 NOAO nights • None approved 04/19/2007 Cycle 16 Director's Review 18 Spitzer Coordinated Proposals • 20 GO Proposals were submitted for 1031 HST Orbits and 635.2 Spitzer hours • The 5 Large HST-Spitzer Coordinated programs were discussed by the HST • TAC. 2 were approved as noted in bold text below and the other 3 all ended up in the 3rd quartile. 4 Joint Proposals were approved for 300 HST Orbits and 203.1 Spitzer hours • Egami Characterizing the Stellar Populations in Lyman-Alpha Emitters and Lyman Break • • • Galaxies at 5.7<z<7 in the Subaru Deep Field (72 HST Orbits/102 Spitzer Hours) Malhotra The Physical Nature and Age of Lyman Alpha Galaxies (44 HST Orbits/20 Spitzer Hours) Meixner SEEDS: The Search for Evolution of Emission from Dust in Supernovae with HST and Spitzer (34 HST Orbits & 16 Spitzer Hours) Yan Revealing the Physical Nature of Infrared Luminous Galaxies at 0.3<z<2.7 Using HST and Spitzer (150 HST Orbits and 65 Spitzer Hours) 04/19/2007 Cycle 16 Director's Review 19 Future Cycle Allocations • 53 Orbits allocated to Cycle 17 from 4 proposals • 12 Orbits allocated to Cycle 18 from 1 proposals 04/19/2007 Cycle 16 Director's Review 20 Targets of Opportunity 04/19/2007 Cycle 16 Director's Review 21 Countries of PIs 04/19/2007 Cycle 16 Director's Review 22 States of PIs 04/19/2007 Cycle 16 Director's Review 23 04/19/2007 Cycle 16 Director's Review Cycle 16/17 boundaries •SM4 is scheduled for September 2008 • • • SM4 complete by late September 2008 SMOV during October 2008 HST available for observations ~November 2008 (WFC3 ~Dec 2008?) •Cycle 16/17 boundary will be set at SM4 • Avoid multiple instrument suites during a cycle • • • • • CP17 release – 1 December 2007 Proposal deadline – ~1 March 2008 (2 weeks before Chandra) HST TAC meets – May 12-16 2008 Phase II reviews – July/August 2008 (pre-SM4) Cycle 17 ends December 31 2009 • Calendar balances (internal STScI) workload for proposal implementation & SM4/SMOV •Proposed Cycle 17 schedule (still not formally finalised) •Revised schedule 04/19/2007 Cycle 16 Director's Review 27 TIPS-JIM Meeting 19 April 2007, 10am, Auditorium 1. INS Division News Jerry Kriss 2. Results of the Cycle 16 HST Peer Review Brett Blacker 3. ACS/WFC Geometric Distortion and CTE Vera Kozhurina-Platais 4. JWST FGS-Guider Critical Design Review Pierre Chayer Next TIPS Meeting will be held on 17 May 2007. ACS/WFC Geometric Distortion and CTE V. Kozhurina-Platais & ACS team ACS/WFC geometric distortion is changing linearly with time Anderson J., ISR-ACS/WFC , August 2006 a) Standard astrometric reference field (47Tuc) ~ 53,000 stars b) User friendly software - XYM2MAT Our plan was to: a) Check the time-dependency on FLT images; b) Implement the time dependency in MultiDrizzle c) Verify the implementation The observations of 47Tuc • F606W filter • 2002-2006 (PIP-9018-10771) • different orientations • different postargs • different exposures: 22 - 1200s The reductions: • effective PSF fitting on FLT - X,Y mag; • standard frame: 2002 March, 690s, F606W,θ=-163° Kiselev A.A, 1989, pub.,”Nauka”, St.Petersburg, Russia Ouv - standard orthogonal system MXY - measured system Y v θ u AB X − X o uo = + v CDY − Y o vo Y vo u B tgθ = D Yo O uo € M θ Xo X X 90 € A tg(θ + γ ) = − C A⋅ B+ C ⋅D tgγ = − A⋅D−C ⋅ B 720 s , θ =-163°.2 2002.4 22 s , θ = -122°.9 2004.5 22 s , θ =- -23°.9 2004.7 22 s , θ = -67°.8 2005.0 22 s , θ = -117°.9 2002.4 22 s, θ = 51°.9 2005.9 The skew term as A ⋅ B + C ⋅ D γ = arctan− A ⋅ D − C ⋅ B α = 0.095 + 0.090 ⋅ (date − 2004.5)/2.5 β = −0.029 − 0.030 ⋅ (date − 2004.5)/2.5 € f x = (Xc − 2048) 2048 f y = (Yc − 2048) 2048 € Xo = fx + β ⋅ fx + α ⋅ fy Yo = f y + β ⋅ f y + α ⋅ f x € Many variables: • exposure • pointing • orientation • epoch PID - 10368: • • • The same pointing Exposures - 400s, 30s Two orientations : +154.8, -29.4 400sec--> 400sec, 154.7-> 154.7 LAMP=OFF/OFF 400sec--> 400sec, 154.7-> -29.4 LAMP=OFF/OFF 30sec--> 400sec, 154.7-> 154.7 LAMP=OFF/OFF 30sec--> 400sec, 154.7-> 154.7 LAMP=MED/OFF 30sec--> 400sec, 154.7-> 154.7 LAMP=HIGH/OFF 30sec--> 400sec, -29.4->-29.4 LAMP=LOW/OFF Schematic illustration of the WFC1 and WFC2 plane: - Red arrows show the readout direction - Green color shows the PSF profile affected by CTE Conclusions ♦ The CTE-induced centroid shift depends on: magnitude of a star position on a CCD chip sky background ♦ The amplitude of CTE-induced centroid shift is ~ 0.1 pix ♦ CTE effect leads to a discontinuity in the reference frame ♦ Accounting for CTE effect is critical to reach a 1 mas accuracy requirement for JWST standard astrometric field TIPS-JIM Meeting 19 April 2007, 10am, Auditorium 1. INS Division News Jerry Kriss 2. Results of the Cycle 16 HST Peer Review Brett Blacker 3. ACS/WFC Geometric Distortion and CTE Vera Kozhurina-Platais 4. JWST FGS-Guider Critical Design Review Pierre Chayer Next TIPS Meeting will be held on 17 May 2007. JWST FGS FGS Guider Critical Design Review FGS Guider CDR – April 19, 2007 © Copyright 2007 Her Majesty the Queen in Right of Canada Subject to Controlled Goods Regulations of Canada Pierre Chayer (HIA/STScI) March 14th & 15th 2007 COM DEV Ottawa 303 Terry Fox Drive Kanata, ON, K2K 3J1 44 FGS-Guider CDR • • • • • The Critical Design Review (CDR) is a presentation of the detailed instrument system design. CDR allows for the final FGS requirements, resource allocations, verification plans, and detailed designs to be presented, discussed, modified (if necessary) and approved. CDR discloses the complete system design in full detail. CDR ascertains that technical problems and design anomalies have been resolved. CDR ensures that the design maturity justifies the decision to initiate Flight Unit fabrication, integration and verification of mission hardware and software. FGS Guider CDR – April 19th, 2007 © Copyright 2006 Her Majesty the Queen in Right of Canada Subject to Controlled Goods Regulations of Canada 45 FGS-Guider CDR Agenda (Day 1) E1 E2 E3 01 02 03 04 05 06 06 GUIDER CDR AGENDA TOPIC Arrival Introduction FGS Science background Guider Operations & Constraints CDR Agenda & Programmatic Baseline & Assumptions for CDR Non-compliance statement PA PA Presentation 04A Requirements, Reliability, Parts, M&P, Contamination 04B Guider Radiation Analysis BREAK Guider Architecture Region 2 Electronics 06A Region 2 Electronics - Electrical Design Overview 06D 06E 06F 06G 07 N/A DAY2 TIME DAY 3 D. Provencal J. Hutchings P. Chayer M. Lihou I. Barnard G. Richardson P. Woods 7:45 8:00 8:10 8:20 8:40 9:00 9:20 9:35 10 10 20 20 20 15 45 P. Woods 9:35 30 H. Rufenacht / K. Man N. Rowlands A. Csizmar/D. Henry D. Henry 10:05 10:20 10:30 11:30 11:30 15 10 60 8236 45 8237 12:15 13:00 13:00 13:15 13:55 45 A. Csizmar/D. Henry D. Henry P. Kenyon D. Henry BREAK Region 2 Electronics (Cont'd) Focus Housekeeping Board SIDECAR Control Electronics Board Power Control Unit System Level EMC Analysis 14:40 14:50 14:50 15:35 16:20 16:50 10 A. Csizmar/D. Henry D. Henry E. Hartwig J. Metcalf K. Man 45 45 30 30 8240 8241 8242 8243 BREAK Assembly, Integration & Test Status CDR Board Meeting G. Reis D. Provencal 17:20 17:30 18:15 10 45 15 8244 LUNCH Region 2 Electronics Cont'd 06A Region 2 Electronics - Electrical Design Overview (Cont.) 06B Structural & Thermal Analysis 06C SpaceWire Board 06 DAY 1 PRESENTER FGS Guider CDR – April 19th, 2007 © Copyright 2006 Her Majesty the Queen in Right of Canada Subject to Controlled Goods Regulations of Canada 15 40 45 8228 8229 8230 8231 8232 8233 8234 8239 46 FGS-Guider CDR Agenda (Day 2) 08 08A 08B 08C 08D 08E 08 08F 08G 08H 08 08K 08J 08L 08M 08N E4 09 9A 9B 10 11 12 13 14 N/A Guider Optical Assembly Overview / OA Layout Optical Design and Analysis Stray Light Control Design & Analysis Structural Analysis Thermal Analysis BREAK Guider Optical Assembly (Cont'd) STOP Analysis Optical Bench Assembly Relay TMA (Design & Analysis) LUNCH Guider Optical Assembly (Cont'd) Fine Focus Mechanism Guider Detector Assembly FPA and SIDECAR Status Guider Calibration Source FGS Alignment (AIT) Unit Level Cryogenic Facilities at DFL BREAK Guider Performance (NEA) Guider Performance (NEA) Guider Performance (ID/ACQ) Margin Summary Verification Software Status Harness Design Status TFI Design Status CDR Board Meeting FGS Guider CDR – April 19th, 2007 © Copyright 2006 Her Majesty the Queen in Right of Canada Subject to Controlled Goods Regulations of Canada A. McColgan A. McColgan C. Evans E. Greenberg A. McColgan D. Aldridge A. McColgan A. McColgan P. Cameron D. Aldridge A. McColgan L. Richards D. Aldridge D. Gulbransen N. Rowlands C. Evans R. Leblanc N. Rowlands N. Rowlands H. Rufenacht G. Richardson H. Rufenacht J. Zhou W. Lunscher N. Rowlands D. Provencal 8:00 8:00 8:25 8:50 9:05 10:05 10:25 10:35 10:35 11:05 11:25 11:45 13:00 13:00 13:45 14:00 14:20 14:35 14:50 15:05 15:15 15:15 16:05 16:45 17:05 17:20 17:30 17:40 17:50 n/a 25 25 15 60 20 10 8246 8247 8248 8249 8250 30 20 20 8251 8252 8253 n/a 45 15 20 15 15 15 10 8255 8254 8256 8257 8258 8245 50 40 20 15 10 10 10 TBD 8259 8260 8261 8262 8263 8264 8265 47 FGS-Guider Operations FGS Guider CDR – April 19th, 2007 © Copyright 2006 Her Majesty the Queen in Right of Canada Subject to Controlled Goods Regulations of Canada 48 Identification: Guide Star Recognition 2048 pixels (2.3 ') FGS FOV 2048 pixels (2.3 ') guide star full frame readout, pattern match of observed stars to uplinked reference stars to identify guide star. FGS Guider CDR – April 19th, 2007 © Copyright 2006 Her Majesty the Queen in Right of Canada Subject to Controlled Goods Regulations of Canada 49 FGS-Guider Optical Layout Pick-off mirror Focus mirror TMA Detector 2m 100 mm FGS Guider CDR – April 19th, 2007 © Copyright 2006 Her Majesty the Queen in Right of Canada Subject to Controlled Goods Regulations of Canada 50 FGS Optical Assembly - Guider Side FGS Guider CDR – April 19th, 2007 © Copyright 2006 Her Majesty the Queen in Right of Canada Subject to Controlled Goods Regulations of Canada 51 FGS Optical Assembly - With Baffles Guider Plan View FGS Guider CDR – April 19th, 2007 © Copyright 2006 Her Majesty the Queen in Right of Canada Subject to Controlled Goods Regulations of Canada 52 FGS in the ISIM Structural Context MIRI NIRCam FGS-TFI FGS-Guider NIRSpec FGS Guider CDR – April 19th, 2007 © Copyright 2006 Her Majesty the Queen in Right of Canada Subject to Controlled Goods Regulations of Canada 53 Main Bench Design Features 2 mm thick ribs, 90mm deep 4 mm thick sidewalls, 110mm deep Higher density rib pattern Hardpoints added for MGSE Thermal strap wall 6mm thick KM mounting pad thickness increased to 21mm Guider POM deck raised FGS Guider CDR – April 19th, 2007 Structure added to bolster KM2 – KM3 span © Copyright 2006 Her Majesty the Queen in Right of Canada Subject to Controlled Goods Regulations of Canada 54 Thermal Analysis: Cold Steady State Cold Case: Requirement Tested: •Detector absolute temperature below 41 K Boundary Conditions: •ISIM Conductive temperature = 30.0 K •Radiative Environment = 32K, ε =0.01 •Heat strap interface temperature = 30.0 K •Steady State Heat Loads Results •Maximum detector temperatures (30.440 K) are well below the requirement. •Gradient in the optical bench is 0. 225 K FGS Guider CDR – April 19th, 2007 © Copyright 2006 Her Majesty the Queen in Right of Canada Subject to Controlled Goods Regulations of Canada 55 FGS Identification Timing Budget • • • • Identification duration is dominated by the readout time for the double read • Double read = reset-read-reset-read, allows Cosmic Ray hits to be filtered out. As per agreement post-ISIM PDR, FGS allocation of 45 sec applies to readout time only FGS & ISIM collaborate on overall timing estimate for ISIM allocation of 60 seconds ID duration estimate is compliant at the ISIM level (< 60 secs per ID attempt, ISIM-266) Contributor FGS FSW Command Item Duration (seconds) Total Duration (seconds) SP / ICDH ID & SCE Setup Commands 3.648 3.648 Includes first start exposure command FGS Strip Readout Duration 1.357 46.33 Double Read: 34 strips (4 pixel overlap assumed) FGS Requirement (SRD154) FGS/ ICDH Strip Data Transfer Time 0.95 FGS FSW Last Strip Image Processing 0.775 0.775 Only the last strip image processing time adds to the total FGS FSW Identification Algorithm 7.198 7.198 Algorithm assumes 50 bright objects & 30 triads SP / ICDH FGS & ICDH Clean up commands 0.512 0.512 Total FGS Guider CDR – April 19th, 2007 © Copyright 2006 Her Majesty the Queen in Right of Canada Subject to Controlled Goods Regulations of Canada Note Does not contribute – shorter than readout 58.46 Requirement at ISIM level is < 60 seconds 56 Non-Compliance Statement • SRD154 • Requirement text - The total time for an identification image to be collected, plus execution of the identification algorithm shall be 45 seconds or less (per attempt) • Traced from – IPFR requirement FGS237 • Status – The estimated duration is 46.33 s • Discussion – Excess duration is due to need for double detector read to mitigate SEU. See Section 09B of this package for further details. It has been agreed that the requirement should be against the readout time only • Proposed resolution – Raise Class 1 ECN to remove algorithm execution time from requirement. Discuss with CSA and NASA and come to a consensus on path forward on residual non-compliance. Likely acceptable as is FGS Guider CDR – April 19th, 2007 © Copyright 2006 Her Majesty the Queen in Right of Canada Subject to Controlled Goods Regulations of Canada 57 Pack and Ship June 2009 FGS Guider CDR – April 19th, 2007 © Copyright 2006 Her Majesty the Queen in Right of Canada Subject to Controlled Goods Regulations of Canada 58 TIPS-JIM Meeting 19 April 2007, 10am, Auditorium 1. INS Division News Jerry Kriss 2. Results of the Cycle 16 HST Peer Review Brett Blacker 3. ACS/WFC Geometric Distortion and CTE Vera Kozhurina-Platais 4. JWST FGS-Guider Critical Design Review Pierre Chayer Next TIPS Meeting will be held on 17 May 2007.