Recap of Recent Events and Schedule for Next 3 Months

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Recap of Recent Events and Schedule for Next 3 Months

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T. Decker, LLNL. Lead Elect. Engr. J. Oliver, Harvard. Focal Plane Assy. S. Aronson, BNL ... Neutrinoless Double Beta Decay. X. K0PI0. X. CLEO-c. X. Reactor n ... –

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Title: Recap of Recent Events and Schedule for Next 3 Months


1
Recap of Recent Events and Schedule for Next 3
Months
  • S. Kahn

2
Summary
  • It has now been 5 1/2 mos. since the camera
    kick-off meeting.
  • There has been a lot of progress on the
    organizational and political side (see following
    slides).
  • DOE involvement is now fairly secure. DOE-OS
    still needs to find the money (especially in
    FY05) but this is being worked.
  • It is now time to do some real work. To keep
    this project on-track, we want to push for CD-0
    early in the Fall of 04 (see Althouse
    presentation following). This will require a
    much higher level of technical specification than
    currently exists for all camera subsystems.

3
Events Since Kick-Off
  • NSF DD Proposal formally submitted January 04.
    It is currently still out for review.
  • Presentation to SAGENAP made in April 04. Letter
    of Intent for DOE participation included in the
    presentation. First presentation of a camera
    budget through construction.
  • Physics of the Universe report released by OSTP
    in April 04. Highlights LSST as a joint NSF/DOE
    project with beginning of operations in 2012.
  • Quantum Universe report released by HEPAP in May
    04. Includes LSST as HEP project addressing dark
    matter and dark energy.
  • First presentation on DOE involvement made at
    LSSTC Board Meeting in May 04.
  • Science Requirements Meeting held in Tucson in
    May 04.
  • Data Management kick-off meeting held in Tucson
    in May 04.

4
Institutional Roles in DOE-LOI
  • SLAC overall camera project management camera
    mechanical and optical elements focal plane
    assembly camera integration and test front-end
    DAQ supporting science activities, modeling and
    analysis.
  • BNL sensor and FEE development integration of
    sensors with FEE support for focal plane
    assembly and test, and camera integration and
    test collaboration in the front-end DAQ
    supporting science activities, modeling and
    analysis.
  • LLNL mechanical and optical engineering
    participation in the assembly and test of the
    focal plane support for camera integration and
    test supporting science activities, modeling and
    analysis.
  • Harvard electronics engineering support for
    FEE/sensor integration and test support focal
    plane assembly and test, and camera integration
    and test supporting science activities, modeling
    and analysis.
  • UIUC camera control software support for
    camera integration and test supporting science
    activities, modeling and analysis.

5
LSST Camera Project Organization
Camera S. Kahn, Sci Lead W. Althouse, Proj Mgr
  • Camera Project Support
  • Project Controls Risk Mgmt
  • Performance Safety Assur.
  • Administration

6
Manpower
7
Funding
8
DOE Manpower Funding
9
Summary Schedule
10
(No Transcript)
11
Smaller Facilities in US Program
12
What are the next steps?
  • SAGENAP will issue a recommendation, hopefully
    endorsing DOE involvement in LSST. Comments from
    individual committee members suggest that the
    report will be very favorable.
  • We will probably then be asked to make a
    presentation to HEPAP, apprising them about the
    project.
  • Formal approval will have to come from P5. My
    guess is that this will occur next year, probably
    in response to a formal proposal from us to DOE.
  • We are hoping to get a CD-0 review in October
    04. This will give the project a formal status
    with the agency. Our insides sources tell us
    that LSST is viewed very favorably at DOE, but
    that finding the money for it will be a challenge
    in the current budget climate.

13
Key Challenges Over the Next 3 Months
  • Optical design must be frozen by August. There
    are two aspects to this
  • Long vs Short design decision. This has a
    big effect on the camera location and its
    mounting to the telescope.
  • Definition of FOV. Affects the size of the array
    (linear) as well as the lenses (faster than
    linear). We need to understand the cost/schedule
    and complexity implications.
  • Other outstanding zeroth order issues requiring
    near-term resolution
  • Camera rotation requirements. We need to
    understand the implications and limitations.
  • Filter exchange mechanism. Internal or external
    to the camera can? Number of filters mounted on
    the camera at any given time? Filter
    refurbishability?
  • Wave-front sensing implementation. Dedicated
    sensors? How many? Where? Read-out
    requirements?
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