Dear Andrea et al.,
you will find below some comments, mainly on the current UCD list,
prepared by Ana and myself. If I interpret correctly your last message
to the UCD SciBoard, we have passed the deadline, when the contributions
from the UCD SciBoard were expected to come. If so, we have obviously
missed some important information about the time-line. We apologize for
that. Should our comment be arrived beyond the time horizon, feel free
to ignore them for the time being, and to postpone them for the next
round of comments, if anyhow interesting:
- we propose to remove all the words containing an explicit
specification of the wavelength or frequency range. They should be
replaced by words of the type: "em.wl.start; em.wl.end" (these words do
not exist, and should be added). Rationale: the current method lacks
flexibility, and is very likely not to cover all the interesting
wavelengths ranges in existing catalogues, where "standard" wavelength
ranges do not exist (e.g., high-energy)
- we propose to substitute "instr.${band}" for all words of the type
"em.${band}". Rationale: the sensitive bandpass is a property of the
detector
- we propose to add the words "em.wl.start" and "em.wl.stop".
Rationale: they may be useful and flexible characterizations of the
bandpass
- we propose to move "instr.obsty.site.seeing" to "obs.seeing".
Rationale: this is a property of an observation rather than of an instrument
- we propose to unify "instr.beam" and "instr.det.psf" into
"instr.psf". Rationale: in most cases, users are interested in the
overall PSF (optics+detector). "Beam" is the radio jargon for PSF.
Should the detector PSF be necessary, one could use: "instr.psf; instr.det"
- we propose to remove "instr.precision". Rationale: too generic,
probably useless
- we propose to add the following radio-related words:
"instr.interferometry", and "instr.resolution". Rationale: the former is
self-explaining; the latter indicates the spatial resolution
- we propose to change the word code of "instr.filter.transm" and
"instr.spect.resolution" to "V". Rationale: the filter transmission is
an intrinsically vectorial quantity; the spectral resolution as well
(dependence on energy and/or order)
- we propose to add a further atom to the "Multiplicity of binarity
flag": "meta.code.multip.star", "meta.code.multip.planet". Rationale:
self-explaining
- we propose to add a further "meta" atom: "meta.subexp". Rationale:
this will allow to characterize the rank of sub-exposures in a
multi-exposure observations, whenever useful for, e.g., variability studies
- we propose to add a further "meta" atom: "meta.rank". Rationale:
useful to indicate an element in an intrinsically vectorial quantity
- we propose to move "meta.id" and "meta.id.assoc" to "src.id" and
"src.id.assoc". Rationale: they belong to "sources" rather then to
"metadata"
- we believe that the following "phys" word should be moved to "src":
"phys.angArea", "phys.AngSize" (and associated words), "phys.area",
"phys.size" (and associated words). Rationale: the same as #12 above
- we believe that words belonging to the following categories: "phot",
"pos", "spec", should be placed under the category "src" (e.g.:
"phot.antennaTemp" -> "src.phot.antennaTemp", "pos.angDistance" ->
"src.pos.angDistance"; "spect.Doppler" -> "src.spect.Doppler".
Rationale: all these words ultimately describe source properties
- the words for coupling of quantum numbers do not cover all the
possible coupling cases. A more general method is needed, and the Data
Line Model sub-group is indeed working on this. We propose to wait for
the conclusion of their work, before this issue is ultimately addressed
- a new word "pos.offaxis" should be added. Rationale: the off-axis
angle may be a useful quantity is some catalogs
- "pos.earth", "pos.earth.lat", "pos.earth.lon" should be placed under
the "obs" category. Rationale: these quantity belongs logically to an
observation, not to (the position of) a source
- "pos.earth.nutation" should be removed. Rationale: it is no longer
consistent with the IAU specification
- a new word "src.ephem" should be added. Rationale: it is necessary
to separate "observatory" from "source" ephemeris
- "spect.veloc" should be replaced by "src.radial.vel". Rationale: it
is a property of the source, rather than of a spectrum
- we propose to add "src.stellarityIndex". Rationale: it may be useful
to easily discriminate point-like from extended sources
- we propose to add the following words in the "stat" category:
"stat.distribution", "stat.fit.model". Rationale: without them, the
information on the statistical quantities and/or the fit are incomplete
- we propose to replace "stat.moment" (as a vectorial quantity) for
"stat.mean" and "stat.stdev". Any of the statistical moments could be
therefore indicated by the UCD: "stat.moment; meta.rank". Rationale: the
proposed method is more flexible, and could avoid the proliferation of
new words to indicate skewness, kurtosis ...
- the following words should be moved from the category "time" to
"src": "time.age", "time.crossing", "time.period", "time.phase",
"time.relax". E.g.: "time.age" -> "src.time.age". Rationale: they
logically belong to a source rather them to the 4th dimension
- we propose to add the following word: "time.deadtime". Rationale:
useful for photon-counting devices based catalogues
An additional point that we have discussed concerns the units in which
interferometric data shall be provided. Is it accepted that data
providers have to convert them in physical units at the server level? If
not, we need probably to include specific UCD words to deal with
"images" in the Fourier space.
I again apologize for the long and late message. Thanks for your attention.
Regards, Matteo & Ana
--
Matteo Guainazzi
XMM-Newton SOC Matteo.Guainazzi-at-sciops.esa.int
European Space Astronomy Center of ESA Phone: +34 91 8131 176
VILSPA, Apartado 50727, E-28080 Madrid Fax: +34 91 8131 172
Received on 2005-07-13Z09:45:56