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Study of High Energy Astrophysics

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Studio Astrofisica delle Alte Energie-Missioni-Roma January ... PHAROS. 24.690,69. 24.690,69. INAF-IASF-MI. CLAIR. 43.436,00. 31.322,77. 41.982,41. 116.741,18 ... – PowerPoint PPT presentation

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Title: Study of High Energy Astrophysics


1
Study of High Energy Astrophysics
  • Pourpose of the meeting
  • To review the activity of the first year
  • To discuss the activity for the second year.
  • AGENDA

2
(No Transcript)
3
Guidelines
  • Around 1 M/year for the study of future missions
    that
  • must be based on space instrumentation
  • are not yet supported by a dedicated contract
  • can solve the largest number of hot topics in
    High Energy Astrophysics
  • have a significant role played by italians (at
    the level of mission or instrument PI)
  • have a reasonable hypothesis on how to arrive to
    fly
  • What about recent ASI AOOs?
  • missions proposed to the AOO for Small Missions
    or for Mission of Opportunity should not be
    supported by this contract, unless a reasonable
    hypothesis is there not covered by the AOO
    (please declare)
  • missions proposed to the AOO for technologies
    should not overlap (please send a copy of the
    proposal)

4
Difference with respect to the first year
  • In the first year the selection of major projects
    was based on the outcome of the Study Costa,
    Perola, Puglierin.
  • In the second year the selection of the projects
    will follow the same headlines, with updating
    based on
  • New discoveries. (SWIFT, AUGER, TeV.) Updating
    of the hot topics list.
  • Updated Strategies of Institutions Long Term
    Plan of INAF, Road Map of INFN
  • New landscape of missions SIMBOL-X to B-phase,
    CV selection, SMEX AOO, PAMELA launched, AGILE
    launched, GLAST close,
  • ASI has a new organization but we are still on
    the saddle
  • The Mission Board is supported by international
    Reviewers. One of them (Josh Grindlay) is
    attending the meeting. Two more will provide
    remote review.
  • The composition of the Mission Board is changed.
    Giuseppe Cesare Perola cannot contribute any more
    with his competence and engagement and will be
    substituted by myself.
  • A message from Cesare
  • .. vorrei che giungesse a tutti il mio
    piu'sincero augurio di un seguito ricco di
    successi. Il che per se sarebbe la piu' grande
    delle soddisfazioni.











5
The first year
  • Disciplinary Lines Direct Output of the 2004
    Study
  • UHECR from space ? EUSO/CROSS
  • X-Ray Polarimetry ? POLARIX/HXMT/XEUS
  • Hard X-Ray Astronomy with ML Optics ?
    HEXIT-SAT/SIMBOL-X
  • Cosmology with X-.RaysWFXRI ESTREMO ? EDGE
  • Low Energy Gamma Ray Astronomy with Laue Lenses
  • Almost an additonal disciplinary line
  • Nucleon Composition of CR at the knee
  • Various Mission of Opportunity

6
The first year
7
Second year
8
What are you expected to present?
  • Science Case which hot topic you expect to
    solve
  • The technical solution. Demonstrate that it is
    adequate to science goals. Declared sensitivity
    must be justified.
  • The italian role in conceiving, performing and
    exploiting the experiment (Mission PI, Instrument
    PI, CoI with visible responsibility)
  • Manpower please single out the Manpower hired
    on this contract.
  • Motivated financial requests
  • Whether the study has generated proposals at
    AOOs (ASI Small Missions, ASI Mission of
    Opportunity, ESA Cosmic Vision, other Agencies)
  • The strategy proposed to arrive to a mission or
    to participate to a mission.

9
What Next
  • Debate in this meeting (the total money is an
    invariant so put questions)
  • Reviewers present to the meeting
  • Proposals and Presentations submitted to
    referees
  • Assessment done by Mission Board on the basis
    of the debate and of referee reports. Executive
    Plan for the 2d year
  • Updating of the document of HEA for the part
    of future Missions
  • Delivery of the result to ASI at a progress
    meeting
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