Telecon 20060315

Date/Time 14.00 GMT on 15 Mar 2006

Present: AMSR, NAW, MA, EGLEZ

Science Issues for Stage 3: based on analysis of science cases, and Technical Plans

  • what is required for the TAP (stage 3) meeting
    • list of applications/ capabilities needed to meet the two cases in VotcSciStageTwo
  • Need to find out when the TAP is and bring the following issues below to them.
    • there are a number of capabilities which have recurred - e.g. fit minimisation tool, flux conversio, coverage that need to be addressed.
    • otherwise, focus should be on stablising current implementations.

IMF

  • Positional search
  • Catalogue data selection: through a registry query - in aladin and/or workbench
  • Main catalogues required:
    • Spitzer is the main catalogue - and we are matching against that with objects from 2MASS, IRAS, IUE
    • search catalogues and federate to create a master catalogue
  • Conversion of 2MASS from mags to Spitzer fluxes
    • could be done with in VOSpec?
    • ISSUE: magnitude to flux conversion tool: ESO DS4? TOPCAT?
    • ISSUE: Construct SEDs - DS4 ESO? (SpecFIND is only radio)
  • Run of MOCASSIN
    • ISSUE: integrate MOCASSIN into CEA (DS3?)
  • Comparison of observed SED with model
    • ISSUE: tool to do chi2 minimisation - DS4 work? (or a specific app for this case from Jeremy Yates)

Clusters

  • Positional search: need to be covered by SLOAN + Spitzer
  • Catalogues - sloan and spitzer
    • ISSUE: availability of Spitzer catalogues (~600MB/catalogue - SWIRE/per field) - need to get these from IPAC
  • Xmatch - AG, STILTS, CDS
  • Photometric redshifts
    • HyperZ, Bpz, AstroNeural
    • ISSUE: AstroNeural in stage 3.
  • Random catalogue - need to generate this from a monte carlo simulation
    • ISSUE: the 'mask' step may need to be done manually (requires use of MANGLE)
    • ISSUE: configure MANGE to run in a workflow
  • Object selection - catalogue cut based on selection criteria (Aladin, STILTS)
  • Calculate correlation function - use VisIVO
    • ISSUE: use of VisIVO - reading VOTables in Stage 3.
  • 2-d fit - data vs model
    • ISSUE: tool to do chi2 minimisation (note relationship of errors) - DS4 TOPCAT work?

Comments on Stage 3 work

DS4

  • AstroGrid - minimisation tool important
  • INAF - model data interface > generate the mocassin models?
  • CDS - x-match tool, integration plastic, DAL std --> coverage : could some extension on the SED work be considered?
  • ESO - SED construction - important - and a flux conversion tool?

DS5

  • AstroGrid - no plan on the wiki - so hard to comment
  • CDS/INAF - could some extension on the SED work be considered?
  • ESO - std unit conversion could be interesting - not sure what it is?

DS6

  • AstroGrid - Plastic - fucntionality probably ok as is now - make sure it is fully debugged and robust plus documented. k-d trees could be used to index the large cluster catalogues.
  • INAF - AstroNeural and VisIVO through plastic? probably through a workflow/CEA
  • CDS - footprint work?


Check sfit for model/observation fitting


-- NicholasWalton - 15 Mar 2006
Topic revision: r3 - 2006-03-21 - 15:33:52 - NicholasWalton
 
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