Obstap Polarization data discovery
François Bonnarel
francois.bonnarel at astro.unistra.fr
Wed Mar 16 15:46:44 PDT 2011
To be more precise:
- if we want to use the mandatory fields only o_ucd can be used to
specify that phot.flux.density is completed by phys.polarization or
phys.polarization.*. This gives a polarization "falvor" to the flux and
can be searched by
ADQL queries.
- this is sufficient for data discovery, but only the pol_states
optional field can give us the full list of available polarization
states in the data set.
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