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AIDA WP7, Task 2

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AIDA WP7, Task 2 – PowerPoint PPT presentation

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Title: AIDA WP7, Task 2


1
WP7, Task 2
  • Server conversion libraries from spectra native
    format to IVOA SED format

2
Intent
  • The problem
  • SSA allows for spectra in native FITS format
  • a multitude of different conventions
  • tools need to cope with all these conventions
  • The solution
  • convert native spectra to Spectrum DM, on the
    server-side
  • First step
  • use ESO non-raw spectra as samples

3
Investigation (1)
  • ESO Spectra Data
  • Flux
  • 1-d image on primary HDU
  • naxis 1, naxis1 n
  • 1-row 2-d image on primary HDU
  • naxis 2, naxis1 n, naxis2 1
  • Wavelength
  • ( i - crpix1 ) cdelt1 crval1
  • i 1..n
  • No error information

4
Investigation (2)
  • ESO Spectra Metadata
  • Required for data transformation
  • naxis
  • crpix1, cdelt1, crval1
  • Essential
  • cunit1 (Wave unit), bunit (Flux unit)
  • multiple syntaxes (A, Angstrom, erg/cm2/s/A,
    erg/cm2/A/sec, erg/cm2/s/angstrom)
  • Spectrum DM compliance
  • metadata lives in a DB

5
Status
  • Proof of concept
  • Python transformation CGI
  • Input
  • URL pointing to a 1d image
  • Output
  • SED recommended FITS (i.e., BINTABLE with 1 row
    for 1 spectrum)
  • Header currently copied over as is

6
To do
  • Check whether erroneous metadata can be
    recognised and fixed automatically
  • Add SPECTRUM DM suggested keywords (Coverage,
    sampling, curation, etc.)
  • Massive test against all ESO reduced spectra
  • What other FITS conventions are out there?
  • AIDA_WP7T2_at_eurovo.org
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