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TKP Amsterdam 2012 Discussion

transientskp
December 04, 2012

TKP Amsterdam 2012 Discussion

Rob Fender

transientskp

December 04, 2012
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  1. Discussion
    1. Readiness for Cycle 0:
    Resources Manpower & Task Allocation
    2. What do we want from MSSS?
    3. Preparing for Cycle 1

    View Slide

  2. Proposal
    number
    PI TItle Request
    003 Fender
    (general)
    Wide field searches for image-plane radio
    transients
    196
    005 Courtin
    (Planets WG)
    A determination of the abundance of
    water in Saturn's deep
    atmosphere with LOFAR
    20
    006 De Pater
    (Planets WG)
    LOFAR Observations of Jupiter's
    Synchrotron Radiation
    23
    007 Zarka
    (Planets WG)
    Exoplanet radio search and
    characterization
    43
    008 Stappers
    (Pulsars WG)
    LOFAR studies of pulsars, fast transients
    and the ISM
    85
    010 Karastergiou ARTEMIS on LOFAR: 260
    011 Verbiest
    (Pulsars WG)
    Pulsar timing with LOFAR 45
    013 Osten
    (Flare stars WG)
    Stellar Radio Astronomy with LOFAR 24
    014 Serylak
    (Pulsars WG)
    Studying pulsars and the interstellar
    medium using International
    LOFAR stations
    364

    View Slide

  3. Proposal
    number
    PI TItle Request
    23 Griessmeier
    (Planets WG)
    Measuring the energy of Saturn's
    lightning
    30
    34 Hessels
    (Pulsars WG)
    LOTAAS: The LOFAR Tied-Array All-Sky
    Survey for Pulsars and Fast
    Transients
    200
    35 Van Leeuwen
    (Pulsars WG)
    Targeted searches for pulsars and fast
    transients
    90
    39 Miller-Jones
    (Jets WG)
    Variable jet sources in the LOFAR band 78
    (not including Karastergiou and Serylak) TOTAL 834 hr

    View Slide

  4. Proposal
    number
    PI TItle Request
    17 Lazio A Search for radio emissions from HD
    80606b
    30
    22 Ransom LOFAR timing of pulsars and rotating radio
    transients in GBT 350-MHz surveys
    114
    31 McNamara AGN outburst in MS0735.6+7421 15
    36 Beskin Low-frequency polarization observations of
    radio pulsars to
    determine the properties of the plasma
    12
    40 Cordes Using Diffractive Interstellar Scintillations
    (DISS) to Resolve Pulsar
    magnetospheres
    18
    42 Lewandowska Multi-frequency observations of giant radio
    pulse emission from pulsars
    22
    Open-time proposals in 'our' area
    (some of these include TKSP members) TOTAL 211 hr

    View Slide

  5. Results (teaser) from ASTRON:
    “So today I have to suffice by saying that both large
    proposals LC0_003 and LC0_008 did very well in the
    process, and will get very significant allocations, while most
    of the smaller proposals from your group, but not all, can
    probably be scheduled in part. I think your team will be
    loaded with more than enough data soon enough!
    We hope to have more news in the next few days, and to
    settle all allocations well before Christmas.”
    (Interlude: several more emails)
    “Okay, I think the only additional suggestion I feel I can give
    right now is that your group really should prepare to deal
    with a major fraction of the data requested.”

    View Slide

  6. STSci
    ICRAR
    Manc.
    So'ton
    ASTRON
    Ams.
    ASTRON
    Nancay
    P / O ~ 1 means we can only do limited stuff on CEP – just NDPPP?
    and then do all the rest of our processing on local facilities?Are there
    enough? How is transients database synchronised between sites?
    Essential that there is a stable version of TraP available from now on
    In preparation...

    View Slide

  7. 2. What do we want from MSSS? and what issues would you
    like me to take to the KSP PI meeting next week?
    Commissioning of fast modes in 2013?
    NCP (Stewart)
    Comparison of variability with VLSS ?
    Survey of high-energy sources (e.g. XRBs, Fermi sources)?
    (G. Heald)
    31.2%
    18.2%
    32.5%
    13.0%
    4.5%
    0.6%

    View Slide

  8. 3. Preparing for cycle 1
    Provisional deadline March 15
    Strategy will depend on:
    – what projects got time in cycle 0
    – what the cycle 0 projects got
    → we need to have some quantifiable results from the
    Cycle 0 projects
    → for the larger projects that may mean making
    sure that key measurements are made on some
    subset of the data rather than half-finishing

    View Slide

  9. Bid for funding has gone in for joint
    MeerKAT/ASKAP/LOFAR transients
    meeting
    Proposed dates: 8-12 July 2013
    With.... SuperJEDI

    View Slide