Nausicaa Delmotte
ndelmott at eso.org
Mon Nov 7 09:27:06 PST 2005
Hi,
But what is preventing us from adding the semicolon as ending separator?
I do apologize for asking a question that seems to have already been
answered in the past, but I could not find the answer in the archive
mailing-list and since I did not follow all the UCD developments from
the very beginning, probably I missed something.
Could anybody give me a pointer to a discussion or a very brief
comment on it?
Or is it maybe to avoid having a possible NULL word at the end when
parsing a UCD, assuming the ending semicolon?
Thank you
Nausicaa
Alberto Micol wrote:
>
> Hi Andrea,
>
> Sorry to come back with this, but there is another possibility...
> If we state that each UCD word MUST end with the ';' character,
> -that is, even if there are no other subsequent words- then
> no UCD can ever be a substring of another one.
>
> Example:
>
> phot.flux; is not a substring of phot.fluxDens;
>
> The beauty of it is that no other changes are required.
>
> It is my laziness... I always prefer to change the least...
>
> Alberto
> PS: I send this email because I'm sure you are expecting it from me ;-)
> PPS: And I promise that this is the last time I mention this.
>
> On Nov 7, 2005, at 16:47, Andrea Preite Martinez wrote:
>
>> 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
>> =======================================================================
>> =======
>>
>>
> Alberto Micol
> ST-ECF HST Archive Scientist
--
Dr Nausicaa Delmotte @..@ ndelmott at eso.org
European Southern Observatory (----) Tel: +49 (0)89 3200 6418
Karl-Schwarzschild-Str. 2 ( >__< ) Fax: +49 (0)89 3200 6480
D-85748 Garching bei Muenchen ^^ ~~ ^^ http://www.eso.org/~ndelmott/
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