1 NGAO Instrumentation Studies Overview By Sean Adkins November 14, 2006.

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

S Y S T E M S E N G I N E E R I N G.
Project Management 6e..
Área de Instrumentación NAHUAL Mechanical Concept Current Status F. Javier Fuentes Instituto de Astrofísica de Canarias September
Systems Analysis and Design in a Changing World
Maximizing GSMT Science Return with Scientific Figures of Merit.
1 LBNL Enterprise Computing (EC) January 2003 LBNL Enterprise Computing.
NGAO System Design Review Response Peter Wizinowich, Rich Dekany, Don Gavel, Claire Max for NGAO Team SSC Meeting June 18, 2008.
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.
NGAO Instrumentation Overview September 2008 Updated Sean Adkins.
Build to Cost Meeting: Goals, Agenda & New Directions Peter Wizinowich NGAO Team Meeting September 11-12, 2008.
Trying to connect WBSs with people and phases Relevant questions to my work: How the realistic NGAO strategies will/should affect the work in progress?
NGAO Science Instrument Reuse Part 2: Update and required feedback NGAO IWG Anna Moore, Sean Adkins NGAO Team Meeting January 22, 2007.
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.
WFS Preliminary design phase report I V. Velur, J. Bell, A. Moore, C. Neyman Design Meeting (Team meeting #10) Sept 17 th, 2007.
Planning “Science Operations” tasks for the PD phase NGAO PD Phase D. Le Mignant W. M. Keck Observatory 08/19/2008.
NGAO Instrumentation Cost Drivers and Cost Savings September 2008 Sean Adkins.
NGAO Science Instruments Build to Cost Status February 5, 2009 Sean Adkins.
WBS & AO Controls Jason Chin, Don Gavel, Erik Johansson, Mark Reinig Design Meeting (Team meeting #10) Sept 17 th, 2007.
NGAO Management Update Peter Wizinowich NGAO Meeting #11 November 5, 2007.
NGAO System Design Phase Management Report - Replan NGAO Meeting #6 Peter Wizinowich April 25, 2007.
NGAO interface control documents: Christopher Neyman W. M. Keck Observatory Keck NGAO PD phase Meeting #6 March 19, 2007 Videoconference.
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.
NGAO System Design Phase System & Functional Requirements Documents NGAO Meeting #6 Peter Wizinowich April 25, 2007.
Design Team Report: AO Operational Tools (aka Acquisition and Diagnostics) Christopher Neyman W. M. Keck Observatory (for the Operational tools team) Keck.
System Architecture WBS 3.1 Mid-Year Replan Richard Dekany NGAO Team Meeting #6 April 25-26, 2007 UCSC.
4. 2Object-Oriented Analysis and Design with the Unified Process Objectives  Explain the elements of project management and the responsibilities of a.
NGAO High-Contrast Performance Budget (WBS aka Companion Sensitivity) Initial WFE budget and status report NGAO Team meeting #4, WMKO Kamuela.
NGAO Instrumentation WBS Replan By Sean Adkins April 25, 2007.
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.
NGAO Instrumentation Preliminary Design Phase Planning September 2008 Sean Adkins.
1 NGAO Science Instrument Reuse Part 1: NIRC2 NGAO IWG December 12, 2006.
Functional Requirements for NGAO Christopher Neyman W. M. Keck Observatory NGAO Team Meeting #9 August 24, 2007.
Trade Study Report: NGAO versus Keck AO Upgrade NGAO Meeting #5 Peter Wizinowich March 7, 2007.
Trying to connect WBSs with people and phases Relevant questions to my work: How the re 8 -planning will affect the work in progress? Priorities to capture.
Design Team Report: AO Operational Tools (aka Acquisition and Diagnostics) Christopher Neyman W. M. Keck Observatory (for the Operational tools team) Keck.
Build to Cost Meeting: Major NGAO system cost savings ideas Don Gavel NGAO Team Meeting September 11-12, 2008.
Defining the Activities. Documents  Goal Statement defines why helps manage expectations  Statement of Work what gets delivered defines scope  Software.
LSU 10/09/2007System Design1 Project Management Unit #2.
GMT Instrument Development Gary Da Costa ANU Representative GMT Science Advisory Committee.
W. M. Keck Observatory Subaru Users’ Meeting
Conceptual Design Review Design Requirements The Systems Perspective Rob Hubbard Systems Engineering.
1 FRIDA Engineering Status 17/05/07 Engineering Status May 17, 2007 F.J. Fuentes InFraRed Imager and Dissector for Adaptive Optics.
Integral Field Spectrograph Eric PRIETO CNRS,INSU,France,Project Manager 11 November 2003.
CHECKPOINTS OF THE PROCESS Three sequences of project checkpoints are used to synchronize stakeholder expectations throughout the lifecycle: 1)Major milestones,
NGSTNGST ASWG 22 Oct. ASWG Charter & Role  NGST Scientific Goals & Metrics  Refine actual goals and put in DRM √  Refine DRM model assumptions √  Assist.
NIRSpec Status and PDR Results Jeff Valenti & Mike Regan 2006 March 16 TIPS/JIM.
Software Project Management (SEWPZG622) BITS-WIPRO Collaborative Programme: MS in Software Engineering SECOND SEMESTER /1/ "The content of this.
System Performance Metrics and Current Performance Status George Angeli.
SRR and PDR Charter & Review Team Linda Pacini (GSFC) Review Chair.
Keck Next Generation AO Next Generation Adaptive Optics Meeting #2 Caltech November 14, 2006 P. Wizinowich for NGAO Executive Committee.
The Field Camera Unit Results from technical meeting S. Scuderi INAF – Catania.
Week 2 – Risk Planning & Identification. Risk & Risk Management.
Role of The Software Development Plan (SDP)
Science Priorities and Implications of Potential Cost Savings Ideas
Systems Analysis – ITEC 3155 Evaluating Alternatives for Requirements, Environment, and Implementation.
An IFU slicer spectrometer for SNAP
Defining the Activities
NGAO System Design Project Plans and Schedule
Project Management Unit #2
NGAO Trade Study GLAO for non-NGAO instruments
Presentation transcript:

1 NGAO Instrumentation Studies Overview By Sean Adkins November 14, 2006

2 Presentation Outline Study Strategy Study Plan Major Objectives Science Instrument Reuse Trade Study

3 Study Strategy The NGAO Instruments Working Group (IWG) is formed –Exists for the duration of the NGAO SD phase –Focused on instrumentation related matters Instrument specialist perspective for NGAO Resource for AO system design team on instrumentation issues –Organization 6 to 8 members 3 to 4 are funded from current NGAO plan –Responsible for most of the technical work related to the NGAO instrumentation WBS 3 to 4 are volunteers from the NGAO science team –Primary contacts with NGAO science team for instrument related science requirements Regular meetings will be held involving the entire group

4 NGAO IWG Membership Funded positions Sean Adkins – chair of IWG, overall systems, detectors, electronics and interfaces Anna Moore – instrument generalist, optical and mechanical TBD – instrument generalist, optical and mechanical, experience with cryogenics TBD – software engineer NGAO Science Team TBD Additional assistance and advice will be sought from the diverse base of the collective instrumentation and technical resources at UC and CIT

5 Study Plan IWG direct WBS element responsibilities from SEMP – Instrument Balance – Instrument Reuse – Notional Allocation of Function to Science Instruments Version 1 – Notional Allocation of Function to Science Instruments Version 2 –3.5 Science Instruments Reuse and Compatibility New Instruments Other areas where IWG should be involved or consulted –Instrument requirements in element 2.1 –2.2.2 Observatory Interface Requirements –2.2.3 Science Operations Requirements –Various items in elements 3.1, 3.2, 3.3, 3.4 – Science Instruments Test Plan –4.4.2 System Integration & Test Plans

6 Study Plan, cont’d. Priorities 1.Science instruments re-use 2.Instrument balance 3.Near-IR deployable IFU 4.Imagers 5.Visible IFU 6.Preferred solution to near-IR IFU & thermal near-IR imager

7 Study Timeline

8 Major Objectives “…take the science instruments to a proposal level…” –What constitutes an instrument proposal? This is addressed by the WMKO instrumentation development process –Science requirements analysis and flow down –Derived technical requirements –Use case definition and analysis –Technical analysis –Interface requirements –Management »Risk analysis and mitigation plan »WBS »Schedule and budget »Project plan –What is the best way to accomplish the objective? IWG workups? Solicitation of proposals from prospective builders?

9 Scope Focus on science requirements –Wavelength Coverage Range and bands –FOV –Plate Scales IFU Imaging –Spectral Resolution –Sensitivity & background –Residual wavefront error –Auxiliary functions Coronagraphs, polarimeters, etc. –Calibration –Data reduction –Packaging Orientation of input optical axis Field derotation Overall size, weight, power, cooling requirements, etc.

10 Current NGAO Instrument List

11 Science Instruments Reuse Trade Study Objective –evaluate the potential for reuse of OSIRIS and NIRC-2 with NGAO Estimate the performance of OSIRIS with NGAO in the role of the near-IR IFU Determine the nature, feasibility and ROM cost of possible improvements to OSIRIS to take advantage of NGAO such as an increased FOV Review and summarize the constraints on NGAO design that are imposed by the current OSIRIS ICD –Ditto NIRC-2 as the thermal near-IR imager Main parameters to be considered –Wavelength coverage –FOV –Plate scales (IFU and imaging) –Slit size(s) - real and virtual –Spectral resolution(s) –Sensitivity and instrument background –Residual wavefront error –Constraints on NGAO design imposed by instrument ICD Packaging - orientation of optical axis, field derotation Interfaces - input focal ratio, software, etc. –NGAO vs. other telescope AO instrumentation and overall instrument balance –Feasibility and cost/benefit of upgrades for NGAO