[Radioig] Obscore extension for radio: review, implementation
Markus Demleitner
msdemlei at ari.uni-heidelberg.de
Mon Dec 11 13:46:53 CET 2023
Dear DM, dear Radio IG,
I've put support for (most of) the 2023-09-29 edition of the obscore
radio extension into DaCHS (see below) and I've done a test
publication of such a thing in Heidelberg. However, I'm still lacking
good metadata of this sort (even for what radio data I have), so that
table is empty (though discoverable) at this point. If you have
radio data you would like to publish in this way, by all means get in
touch with me.
As part of this effort, I have written two sections on operations and
discovery for the extension. Please review at
https://github.com/ivoa-std/ObsCoreExtensionForRadioData/pull/43
And then, here is some general feedback:
(1) The longer I think about them, the less I like f_min and f_max. If
you look at use case 1.3: "range inside the 1 to 1.5 Ghz band" -- and
then people have to write f_min > 1000 AND f_max < 1500 and thus do
some conversion anyway, and to the relatively random unit MHz on top.
Please let's reconsider this; I have sympathies for not wanting to
write the λ-ν conversions manually, but if
1 = ivo_interval_overlaps(
em_min, em_max,
ivo_specconv(1.5, "GHz", "m"),
ivo_specconv(1, "GHz", "m"))
doesn't work for you, let's think again and figure out something that's
less verbose. But let's not define something parallel to em_min and
em_max with an even more random unit than m.
(2) I have to say I find the use cases relatively unconvincing
because at this point they take some constraints out of thin air and
then repeat them three times with slightly differenty syntaxes. That's
not very helpful for working out why anything in the extension is the
way it is.
I'd find it a lot convincing if the use cases stated a scientifically
meaningful discovery problem -- for instance, *why* would one look for
a "dataset with a field of view larger than 0.5 degree"?
Also, at this point I don't believe in *any* use case involving
target_name -- we don't have reliable rules for how to write them
(and likely will never have them for "ordinary" objects). Don't fool
people into believing they could do all-VO searches using
target_name. Convert all of them into positional queries, because
that's the only interoperable technique for this kind of thing at
this point (but of course it's fine and even welcome to mention
object names in the use case formulation).
For solar system objects with their fast-changing positions, the
whole problem might pose itself differently, but then that's more
epn-tap's problem and arguably doesn't belong here.
Of course, all the queries will have to be re-done if PR #43 is
merged, but that's minor, and I'd volunteer. But before such an
update, let's have (perhaps fewer but) more meaningful use cases,
preferably giving, in sum, justification to each and every column in
the extension.
(3) As usual, I have utype quibbles; in particular, it looks funny if
there suddenly are underscore-separated words in there
("Provenance.Observation.tracking_mode") where I think all other utypes
(including some here) are CamelCase.
Also as usual, I don't think the column utypes here have any
discernable function -- can't we just drop them altogether?
I'd be willing to bet that *nothing* negative happens if we do.
(yeah, we're doing something with the *table* utype, so that's
different)
(4) The column descriptions need more work. Ideally, a non-domain
expert should be able to figure out what something might roughly be by
reading the description. Something like "targeted, alt-azimuth, wobble,
...)" (currently on tracking_mode) won't do that for them.
(5) In general, if you have word lists, think about some way to maintain
them. I'm happy to advise from a vocabulary point of view. If you
put an ellipsis (...) into the spec, you'll almost certainly creating
something that's not validatable and that will likely quickly turn
into a mess.
(6) Also in general: Please don't retain commented-out stuff in the
source. It makes it hard to read, makes the document history a lot
harder to follow, and in general it's much preferred to keep obsolete
items in the VCS history; it's a major reason to do version control
in the first place. If what you want is a placeholder for future
discussions, use \todo (cf. ivoatexDoc).
(7) The short standard name (ObsCoreExtensionForRadioData) is a lot
too long. The Registry has a limit for a resource's shortName of 16
characters. I'm now proposing ObsRadio in the utype used for
discovery, ivo://ivoa.net/std/obsradio#table-1.0. If nobody is too
abhorred by that: Can we rename the document source like that, too?
(8) The columns the DaCHS extension now offers are f_resolution,
instrument_ant_diameter, instrument_ant_max_dist,
instrument_ant_min_dist, instrument_ant_number, instrument_feed,
obs_publisher_did, s_fov_max, s_fov_min, s_maximum_angular_scale,
s_resolution_max, s_resolution_min, scan_mode, t_exp_max, t_exp_mean,
t_exp_min, tracking_mode, uv_distance_max, uv_distance_min,
uv_distribution_ecc, uv_distribution_fill
(select column_name from tap_schema.columns
where table_name='ivoa.obs_radio'
order by column_name)
This doesn't mean I'm convinced all of them should be in. But it
does mean that I'm pretty sure all others should go from table 1; in
particular, the "via DataLink" things I think are just confusing in
there.
Don't get me wrong, to a radio layman, the extra "via DataLink" items
do them look reasonable, but the way to specify them is to have a
section saying "here's a few extra artefacts that you should provide,
too, and we suggest that you serve DataLink documents with your data,
and in there you identify this artefact in that way" (where I suspect
you'll want to involve <http://www.ivoa.net/datalink/core>).
Thanks,
Markus
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