Town Hall Meeting - PowerPoint PPT Presentation

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Town Hall Meeting

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What is SHARE? SHARE = Study of Hubble Archive & Reprocessing Enhancements Chartered by Rodger Doxsey Study participants include Jerry Kriss (chair) HST/STIS & NGST – PowerPoint PPT presentation

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Title: Town Hall Meeting


1
What is SHARE?
  • SHARE Study of Hubble Archive Reprocessing
    Enhancements
  • Chartered by Rodger Doxsey
  • Study participants include
  • Jerry Kriss (chair) HST/STIS NGST Howard
    Bushouse ESS/SSG Mark Dickinson HST/NICMOS Me
    gan Donahue ACDSD ( FASST Chair) Dorothy
    Fraquelli ACDSD Mauro Giavalisco HST/WFC3 Tony
    Keyes HST/COS Anton Koekemoer HST/WFPC2 Gerh
    ard Meurer JHU/ACS
  • Paolo Padovani ACDSD Bill Sparks HST/ACS D
    aryl Swade ESS

2
The SHARE Charter
  • The Deployment of On-The-Fly Reprocessing (OTFR)
    enables potential new services utilizing the HST
    archive. The SHARE study is chartered to
  • Evaluate and recommend general capabilities,
    services and enhancements to these systems.
  • Evaluate and recommend specific new scientific
    services and enhancements to these systems.
    These should be augmentations with clear and
    substantial added benefit for the research
    community.
  • Provide a rough road map or order for the
    implementation of the recommendations made in
    item 1 and 2.
  • Recommend a process for encouraging astronomical
    community participation in the development of
    such enhancements.
  • Recommend a process for regularly assessing and
    prioritizing enhancements of this type in the
    future.

3
Ideas for Reprocessing Enhancements
  • Improvements to the accuracy of the World
    Coordinate System in the headers of calibrated
    data products.
  • Combining images to produce a wide-field mosaic
    or deep stacked image.
  • Identifying and classifying objects in a single
    image or a combined set of images.
  • Producing a catalog of objects in a single image
    or a combined set of images.
  • Determining photometric redshifts for objects in
    a region of sky which is imaged in a number of
    different bands.
  • Combining spectra from several different
    observations or from dithered STIS observations.
  • Using the time history of data and calibrations
    to enhance the reprocessing.
  • Providing better quality information for data
    sets in the archive.
  • Allow users to specify customized parameters to
    be used when running OTFR to tailor the pipeline
    calibration to their scientific needs.
  • Creating "data cubes" from dithered long-slit
    spectroscopic observations.

4
Recommendations for Implementation
  • Assess the resources required for each idea
  • Evaluate the likely timescales for implementation
  • Given the required resources and timescales,
    reassess our priorities and recommend a
    development road map

5
Encouraging Community Participation
  • Advertise and discuss ideas for reprocessing
    enhancements at ADASS meetings
  • Encourage contributed software/data products
    through a special category of archival proposals

6
Assessing and Prioritizing Future Enhancements
  • Report updates on progress in Archive Newsletters
  • Make regular presentations to the STUC as
    enhancements proceed
  • Advertise current work at ADASS conferences and
    AAS meetings
  • Hold discussions at yearly ADASS meetings
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