UCDs and arrays
Frederic V. Hessman
hessman at astro.physik.uni-goettingen.de
Mon May 7 10:17:32 CEST 2018
In a pinch one could use stat.likelihood (stat.distribution would be sort of the same), especially since one already has stat.probability (which I would use over stat.likelihood for simple single probabilities), but a stat.distribution would be a much cleaner solution.
Rick
> On 4 May 2018, at 19:40, Markus Demleitner <msdemlei at ari.uni-heidelberg.de> wrote:
>
> Dear Semantics,
>
> I'm having more and more array-valued columns in my TAP service.
> Examples include:
>
> * photometry points from Gaia DR2 (see the gaia.dr2epochflux table on
> http://dc.g-vo.org/tap)
> * the gavo_histogram aggregate function, again on http://dc.g-vo.org/tap
> (cf. capabilities there), which computes, well, a histogram over a
> column.
>
> The question is: What should happen to the UCDs of such columns? For
> instance, in gaia.dr2epochflux, there are the columns rp_flux
> (current UCD: phot.flux;em.opt.R -- yeah, we could quarrel whether
> the R is a good choice here, but that's not my point now) and
> rp_obs_time (current UCD: time.epoch).
>
> I feel that's not quite right -- there's not *a* flux in rp_flux,
> there's a *collection* of fluxes. You could, of course, say that
> clients can work out that it's a collection by inspecting the type,
> and I'd not be disinclined to agree. Does anyone disagree? If you
> disagree: What else should I put into the UCD attribute there?
>
> The second case is, I think, even trickier. Consider:
>
> with sample as (
> select top 200000 *
> from gaia.dr2light where parallax is not null)
> select gavo_histogram(round(parallax), 0, 200, 20) as hist
> from sample
>
> I guess I *should* have some UCD on the hist column ("this is a
> distribution or parallaxes"). I don't right now (there's no UCD at
> all). pos.parallax certainly would be wrong.
>
> However, there's already stat.min and stat.max (which are required
> secondary, which makes perfect sense, since a minimal parallax
> still is a parallax), and there's stat.error (which is required
> primary, which again makes sense since the error on a parallax isn't
> a parallax).
>
> Now, I wonder: Could we have a stat.distribution (or something like
> this) atom that would be mandatory primary (since a distribution of
> parallaxes really can't be interpreted as a parallax)? Would anyone
> support such a proposal? Would anyone object to it?
>
> -- Markus
>
>
>
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