NGAO System Design Review Response Peter Wizinowich, Rich Dekany, Don Gavel, Claire Max for NGAO Team SSC Meeting June 18, 2008.

Slides:



Advertisements
Similar presentations
Flow-down of Strategic Priorities to Annual and 5-year WMKO Plan Taft Armandroff Hilton Lewis September 18, 2009 Taft Armandroff Hilton Lewis September.
Advertisements

Roadmap for Sourcing Decision Review Board (DRB)
Project Management Process. Project Complexity means that: a team of people are needed to supply expertise the work needs to be broken into manageable.
Science Group: Status, Plans, and Issues Claire Max Liz McGrath August 19, 2008.
Laser guide star adaptive optics at the Keck Observatory Adam R. Contos, Peter L. Wizinowich, Scott K. Hartman, David Le Mignant, Christopher R. Neyman,
W. M. Keck Observatory Keck Next Generation AO Next Generation Adaptive Optics Irvine Meeting September 14, 2006 P. Wizinowich for NGAO Executive Committee.
W. M. Keck Observatory’s Next Generation Adaptive Optics Preliminary Design & Path Forward Peter Wizinowich, Sean Adkins, Rich Dekany, Don Gavel, Claire.
Impact of Cost Savings Ideas on NGAO Instrumentation December 19, 2008 Sean Adkins.
NGAO System Design Phase Update Peter Wizinowich, Rich Dekany, Don Gavel, Claire Max, Sean Adkins for NGAO Team SSC Meeting February 20, 2008.
Build to Cost Meeting: Goals, Agenda & New Directions Peter Wizinowich NGAO Team Meeting September 11-12, 2008.
1 NGAO Instrumentation Studies Overview By Sean Adkins November 14, 2006.
WMKO Next Generation Adaptive Optics: Build to Cost Concept Review Peter Wizinowich et al. ~ March 20, 2009 February 5, 2009 DRAFT.
1 Laser Guide Star Wavefront Sensor Mini-Review 6/15/2015Richard Dekany 12/07/2009.
Functional Requirements Status and Plans Christopher Neyman W. M. Keck Observatory Viswa Velur California Institute of Technology Keck NGAO Team Meeting.
NGAO Report February 18, 2009 Waimea NGAO Report February 18, 2009 Waimea P. Wizinowich for the NGAO Team.
What should we propose to ATI? Peter Wizinowich NGAO Team Meeting September 11-12, 2008.
1 Keck NGAO Proposal: Management Overview Presenter: P. Wizinowich SSC Meeting June 21, 2006.
NGAO System Design: AO System (WBS 3.2) & Laser Facility (WBS 3.3) Design Inputs & Outputs Peter Wizinowich NGAO Team Meeting #9 August 24, 2007.
Science Operations Update NGAO - Meeting 11 D. Le Mignant, E. McGrath & C. Max W. M. Keck Observatory 11/05/2007.
California Association for Research in Astronomy W. M. Keck Observatory KPAO Keck Precision Adaptive Optics Keck Precision AO (KPAO) SSC Presentation January.
Build to Cost Directions & Guidelines Peter Wizinowich SSC Meeting November 3, 2008.
The Path to NGAO Core Science Requirements Claire Max and Liz McGrath NGAO Team Meeting September 11-12, 2008.
NGAO Meeting #3 Introduction NGAO Meeting #3 Peter Wizinowich December 13, 2006.
Planning “Science Operations” tasks for the PD phase NGAO PD Phase D. Le Mignant W. M. Keck Observatory 08/19/2008.
NGAO Management Update Peter Wizinowich NGAO Meeting #11 November 5, 2007.
Science Operations Replan NGAO - Meeting 6 D. Le Mignant W. M. Keck Observatory 04/25/2007.
NGAO System Design Phase Management Report - Replan NGAO Meeting #6 Peter Wizinowich April 25, 2007.
Science Operations Plan NGAO - Meeting 10 D. Le Mignant W. M. Keck Observatory 09/17/2007.
NGAO Status R. Dekany January 31, Next Generation AO at Keck Nearing completion of 18 months System Design phase –Science requirements and initial.
NGAO Team Meeting Management Peter Wizinowich May 26, 2009.
The Future of AO at Keck Sept 2004 Mike Brown, for the AOWG and Keck AO team.
NGAO System Design Phase System & Functional Requirements Documents NGAO Meeting #6 Peter Wizinowich April 25, 2007.
NGAO: Cost Comparison with First Light TMT AO Peter Wizinowich, Richard Dekany, Don Gavel with input & review by Brent Ellerbroek SSC Meeting November.
NGAO Team Meeting Management Peter Wizinowich March 19, 2009.
System Architecture WBS 3.1 Mid-Year Replan Richard Dekany NGAO Team Meeting #6 April 25-26, 2007 UCSC.
Senior Review Evaluations (1 of 5) Proposals due: 6 March 2015 Panel evaluations: Week of 22 April 2015 Performance factors to be evaluated will include.
NGAO High-Contrast Performance Budget (WBS aka Companion Sensitivity) Initial WFE budget and status report NGAO Team meeting #4, WMKO Kamuela.
Major Management & Systems Engineering Ideas for Reducing Costs Peter Wizinowich NGAO Team Meeting September 11-12, 2008.
NGAO Meeting #5 Introduction NGAO Meeting #5 Peter Wizinowich March 7, 2007.
WMKO Next Generation Adaptive Optics: Build to Cost Concept Review Peter Wizinowich et al. December 2, 2008 DRAFT.
W. M. Keck Observatory’s Next Generation Adaptive Optics (NGAO) Facility Peter Wizinowich, Sean Adkins, Rich Dekany, Don Gavel, Claire Max for NGAO Team:
NGAO Instrumentation Preliminary Design Phase Planning September 2008 Sean Adkins.
Functional Requirements for NGAO Christopher Neyman W. M. Keck Observatory NGAO Team Meeting #9 August 24, 2007.
Plan to develop system requirements through science cases Claire Max Sept 14, 2006 NGAO Team Meeting.
Trade Study Report: NGAO versus Keck AO Upgrade NGAO Meeting #5 Peter Wizinowich March 7, 2007.
NGAO System Design Phase Update Peter Wizinowich, Rich Dekany, Don Gavel, Claire Max, Sean Adkins for NGAO Team SSC Meeting November 6, 2007.
What Requirements Drive NGAO Cost? Richard Dekany NGAO Team Meeting September 11-12, 2008.
IS&T Project Management: Project Management 101 June, 2006.
IS&T Project Management: How to Engage the Customer September 27, 2005.
Project Execution.
Pan-STARRS PS1 Published Science Products Subsystem Preliminary Design Review May 9-10, 2006 IPAC.
Advancing GSMT SWG Recommendations: AURA’s Proposal to the NSF Stephen E. Strom AURA New Initiatives Office Presented to the GSMT SWG 12 February, 2004.
Lecture 11 Managing Project Execution. Project Execution The phase of a project in which work towards direct achievement of the project’s objectives and.
Executive Session Director’s CD-3b Review of the MicroBooNE Project January 18, 2012 Dean Hoffer.
Report from Subaru Advisory Committee The main issues of the current SAC: ・ Extensive (strategic) program of Subaru telescope ・ International collaborations.
John Peoples for the DES Collaboration BIRP Review August 12, 2004 Tucson1 DES Management  Survey Organization  Survey Deliverables  Proposed funding.
24-Aug-11 ILCSC -Mumbai Global Design Effort 1 ILC: Future after 2012 preserving GDE assets post-TDR pre-construction program.
SSC SI Data Processing Pipeline Plans Tom Stephens USRA Information Systems Development Manager SSSC Meeting – Sept 29, 2009.
Project Organization Chart Roles & Responsibilities Matrix Add Project Name.
Keck Next Generation AO Next Generation Adaptive Optics Meeting #2 Caltech November 14, 2006 P. Wizinowich for NGAO Executive Committee.
SEDAR Update Policies and Procedures, Assessment Classifications, & SEDAR 26 Activities Prepared for the June 2011 Caribbean Council Meeting Julie A Neer.
Keck Precision Adaptive Optics Authors: Christopher Neyman 1, Richard Dekany 2, Mitchell Troy 3 and Peter Wizinowich 1. 1 W.M. Keck Observatory, 2 California.
Trigo White Ltd Practical project risk assessment VIII Conferencia Internacional Hotel Tivoli Oriente, Lisbon 28 th November 2014 Simon White Consultant,
Science Priorities and Implications of Potential Cost Savings Ideas
(Additional materials)
Project Organization Chart Roles & Responsibilities Matrix
NGAO System Design Project Plans and Schedule
Preliminary Project Execution Plan
DEVELOPMENT IMPACT FEES AB 1600 UPDATE
Presentation transcript:

NGAO System Design Review Response Peter Wizinowich, Rich Dekany, Don Gavel, Claire Max for NGAO Team SSC Meeting June 18, 2008

2 Presentation Sequence Response to SDR Panel Recommendations –Plan to address Phased Implementation & Descope Options Response to SSC Recommendations This is valuable input and we are actively using it in refining our preliminary design phase plans.

3 SDR Panel Recommendations: Response Panel report documented in KAON 588 NGAO response documented in KAON 593 –Results incorporated in preliminary design replan (KAON 595) Recommendations divided into 12 categories –Complete the science cases –Requirements development –Consider L’ imaging –More performance modeling & validation –Component performance assumptions –More systems engineering –Re-evaluate benefit/cost of d-IFS –Perform science instrument conceptual designs –Complete the risk register & develop mitigation plans –Produce a staged implementation & descope plan –Re-examine the cost & develop a full schedule –Implement management structure changes

4 Phased Implementation & Descope Options Proposed Approach (documented in KAON 594) –Investigate & report on the costs & schedules for the following: The SDR proposed NGAO system. A staged implementation of the SDR proposed NGAO system. –Science capabilities, performance, cost & risk will be considered in determining the optimal sequencing. Keck AO upgrades that might benefit the program or provide fallback science. A few tbd descope options. A few tbd cost savings options. –Cost estimates will be deltas relative to the existing cost estimate, modulo changes from a cost comparison to NFIRAOS. Report will be distributed prior to the Nov. SSC meeting –Would like to present the results at this meeting

5 SSC Recommendations: Response Recommendations & response documented in KAON 596: accept our kudos and congratulations on the successful NGAO effort to date. –We appreciate the SSC’s support & that many SSC members attended the SDR –We look forward to working more with SSC members to ensure that NGAO meets the community’s scientific needs start planning detailed responses to points made in the review panel report. By June the SSC would like to see the schedule for delivering these responses. –Changes to the preliminary design plan are documented in KAON 595 –The plan to address the joint panel & SSC recommendation to develop an implementation plan is documented in KAON 594 (see previous slide) –Each panel recommendation will be addressed in a report as part of the preliminary design phase deliverables

6 SSC Recommendations: Response better engage scientists, probably in the integrated scientific and technical case for NGAO and its instrumentation suite, where they both care more and can contribute more relative to the NGAO system itself. –We hope to engage significantly more scientists during the PD 24 astronomers contributed to the proposal & 22 to the system design science case requirements document Difficult to get time from busy scientists Would be good to get more CIT/UC faculty members engaged –We would like to strengthen & better understand the requirements for some science cases & utilize community expertise in defining science instruments –Directors plan to establish a working NGAO Science Advisory Team (SAT) –Welcome SSC input on how to move the instrument designs forward ATI has not funded the deployable integral field spectrograph system design WMKO management working on how to address/fund instrument designs WMKO instrument program manager to provide leadership

7 SSC Recommendations: Response produce a plan for developing a reliable cost, including a cost floor below which the system achieved for the money spent is deemed not worth having on the Keck telescopes. –Review panel approved of our cost estimation process but were uncomfortable with the cost estimate itself especially in comparison to NFIRAOS. SDR package included a cost comparison with comparable systems TMT recently provided their detailed NFIRAOS cost estimate. We will endeavor to understand the differences, & where appropriate update our estimates, by the time of the Nov. SSC meeting. –A preliminary design level cost estimate, based on a more mature design concept and better understanding of the risks, component costs, vendor options and labor requirements, will be a product of the preliminary design. –Some cost floor information will come out of the phased implementation work. –We will consider cost as a driver & issue throughout the preliminary design.

8 SSC Recommendations: Response facilitate connection of the technical trades to the science –We have been very careful to make our technical trades based on the science requirements. –We would like more active astronomer involvement in evaluating the science performance based on predicted PSFs, backgrounds, etc., & on such topics as observing sequences & interfaces. –We expect the SAT to actively contribute in this area. identify the break points in major technology areas (e.g. tomography, laser power, wavefront error, realtime control, etc.) that make NGAO a major leap over existing capabilities (either at Keck or elsewhere), and where significant break points in cost might lie in the path toward the achieving [of] the goals of NGAO –We will endeavor to identify break points during our work on a phased implementation plan.

9 NGAO Papers at SPIE 08 Conference WMKO’s NGAO Facility. Wizinowich et al. KAON 597 The Science Case for the NGAO at WMKO. Max et al. Sharpening low-order NGS using patrolling LGS. Dekany et al. Concept for the Keck NGAO system. Gavel et al. Science operations for NGAO at the system design phase. Le Mignant et al. KAON 599 AO PSF reconstruction at the WMKO. Flicker et al. Low-order wavefront sensing in tomographic multibeacon AO systems. Velur et al.

10 Cost Comparisons