No subject
Andrea Preite Martinez
andrea.preitemartinez at rm.iasf.cnr.it
Mon Nov 7 07:47:55 PST 2005
Dear all,
I received from the IVOA Exec a request to modify all UCD1+ words that
do not conform to what is said in the standard UCD document, i.e.:
UCD1+ words at the same level in the hierarchy cannot be a starting
substring of another
that is, we cannot have phot.flux and phot.fluxDens
As you know, the document at
http://www.ivoa.net/Documents/latest/UCDlist.html
is in the PR status, and will be moved to IVOA Recommendation after an
appropriate action on the words concerned.
The rule mentioned above is violated for the following ucd1+ words:
E | phot.fluxDens | Flux density (per wl/freq/energy interval)
E | phot.fluxDens.sb | Flux density surface brightness
Q | phys.atmol | Atomic and molecular physics (shared
properties)
Q | phys.atmol.branchingRatio | Branching ratio
Q | phys.atmol.coll | Related to collisions
Q | phys.atmol.configuration | Configuration
Q | phys.atmol.crossSection | Atomic / molecular cross-section
Q | phys.atmol.element | Element
Q | phys.atmol.excitation | Atomic molecular excitation parameter
Q | phys.atmol.final | Quantity refers to atomic/molecular
final/ground state, level, ecc.
Q | phys.atmol.initial | Quantity refers to atomic/molecular
initial state, level, ecc.
Q | phys.atmol.ion | Ion
S | phys.atmol.ionization | Related to ionization
S | phys.atmol.level | Atomic level
Q | phys.atmol.lifetime | Lifetime of a level
Q | phys.atmol.lineShift | Line shifting coefficient
Q | phys.atmol.parity | Parity
Q | phys.atmol.sweight | Statistical weight
S | phys.atmol.trans | Transition between states
Q | phys.energyDensity | Energy-density
Q | phys.massToLight | Mass to light ratio
Q | phys.massYield | Mass yield
because of the already existing words
phot.flux
phys.at
phys.energy
phys.mass
In order to reach a rapid convergence on the reformulation of these
words, I?m suggesting a possible solution for each of them in the list
that follows:
Present Suggested new
E | phot.fluxDens | phot.flux.fluxDens or: phot.flux.density
E | phot.fluxDens.sb | phot.flux.fluxDens.sb or:
phot.flux.density.sb
Q | phys.atmol | suppress
Q | phys.atmol.branchingRatio | phys.branchingRatio
Q | phys.atmol.coll | phys.collision
Q | phys.atmol.configuration | phys.state.configuration
Q | phys.atmol.crossSection | phys.crossSection
Q | phys.atmol.element | phys.element
Q | phys.atmol.excitation | phys.excitation
Q | phys.atmol.final | phys.state.final
Q | phys.atmol.initial | phys.state.initial
Q | phys.atmol.ion | phys.element.ion S |
phys.atmol.ionization | phys.ionization
S | phys.atmol.level | phys.level
Q | phys.atmol.lifetime | phys.level.lifetime
Q | phys.atmol.lineShift | phys.lineShift
Q | phys.atmol.parity | phys.state.parity
Q | phys.atmol.sweight | phys.state.sweight
S | phys.atmol.trans | phys.state.trans Q |
phys.energyDensity | phys.energy.density
Q | phys.massToLight | phys.mass.light
Q | phys.massYield | phys.mass.yield
The other possibility for the phys.atmol.xxx group is to suppress the
word phys.at
Please let me know your opinion and/or your suggestions.
Andrea
==============================================================================
Andrea Preite Martinez andrea.preitemartinez at rm.iasf.cnr.it
Istituto di Astrofisica Spaziale Tel.:+39.06.4993.4641
Area di Ricerca di Tor Vergata Fax.:+39.06.2066.0188
Via del Fosso del Cavaliere 100 Cell:+39.320.43.15.383
00133 Roma CDS :+33.3.90242473
==============================================================================
More information about the ucd
mailing list