Difference: InterOpMay2011Splinter (13 vs. 14)

Revision 142011-05-18 - IgorChilingarian

 
META TOPICPARENT name="InterOpMay2011"

Splinter meetings and hack-a-thon

Sessions slots

  • Wednesday May 18 16:30-18:00 in various rooms in the conference centre
  • Thursday May 19 16:30-18:00 outside venues (e.g. cafés) as the conference centre will be closed

Ideas and requests listed here

  • So many DAL servcies for SED Science Case!
    • Goal: Discuss and determine the necessity and practicality of having 3 different DAL services - 1 revised and 2 new ones - for this set of use cases. Wednesday at 16:30? -- PatrickDowler

  • STC-S Support
    • Goal: Develop a BNF (or equivalent) that can be used to develop software that can parse and write STC-S descriptions of regions
    • Comment: The STC Java library is on the schedule for Year 1 of the VAO at CfA. This will include STC-S parsing. Delivery date may be negotiable. I can show prototype GUI. -- ArnoldRots - 17 May 2011

  • Photometry data modeling: 16:30 Room ?? merge with DAL SED??
    • how can we identify the various use-cases covered by the different proposed DMs : PhotDM, SpectrumDM-v1.2, SED DM
    • how can we go from simple spectrum to avanced data product like uniform SED?( SED DM)
    • how can we identify the various types of serialisations these DM are producing
    • tools to consume these various types of products
Participants: D.Tody, M.Allen, J.Salgado, M.Louys, Jonathan via video conf facility ????,

_Please add your name if you wish _ -- MireilleLouys

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  • A usecase for (synthetic) stellar spectra within the VO (Wednesday afternoon, time and place TBD)
    • Goal: Fit an observed spectrum with a synthetic spectrum to extract information on rotation

Participants: A. Palacios, M. Sanguillon, P. Maeght, P. Skoda _Please add your name if you wish _

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  • A joint synthetic spectra / spectral fitting meeting will take place on Wednesday (18/May/2011) in Room B at 16:15
    • A usecase for (synthetic) stellar spectra within the VO (Wednesday afternoon, time and place TBD)
      • Goal: Fit an observed spectrum with a synthetic spectrum to extract information on rotation
    • Full spectrum fitting UWS demo (Wednesday afternoon, 16:30 place TBD - with projector)
      • Extended version of the demo from the DM3 session by IgorChilingarian and the follow-up discussion on the scientific usage of UWS (workflows, automatic interface generation from WADL etc.) Participants: I.Chilingarian, F.Bonnarel,A. Palacios ,M. Sanguillon, P. Maeght, P.Skoda, P.Harrison Please add your name if you wish to attend
Deleted:
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  • Full spectrum fitting UWS demo (Wednesday afternoon, 16:30 place TBD - with projector)
    • Extended version of the demo from the DM3 session by IgorChilingarian and the follow-up discussion on the scientific usage of UWS (workflows, automatic interface generation from WADL etc.) Participants: I.Chilingarian, F.Bonnarel,A. Palacios ,M. Sanguillon, P. Maeght, P.Skoda, P.Harrison Please add your name if you wish to attend
 
  • New Accessdata modes and data links within Aladin DAL interfaces (Thursday afternoon, time and place TBD) This demo is related to the Data Link presentation in DAL 3 session * Participants: F.Bonnarel Please add your name if you wish to attend


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