ask for merge of last corrections for loumir/pen1_6 into ivoa-std/WD-1.6 #99
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| Original file line number | Diff line number | Diff line change |
|---|---|---|
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@@ -35,7 +35,8 @@ | |
| \author{Markus Demleitner} | ||
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| \editor[mailto:[email protected]]{Baptiste Cecconi, Mireille Louys} | ||
| \previousversion[https://www.ivoa.net/documents/UCD1+/20210616]{UCD1+ EN | ||
| 1.5, 2023-01-25} | ||
| \previousversion[https://www.ivoa.net/documents/UCD1+/20210616]{UCD1+ EN | ||
| 1.4, 2021-06-16} | ||
| \previousversion[https://ivoa.net/documents/UCD1+/20180527/index.html]{UCD1+ | ||
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@@ -243,6 +244,7 @@ \section{List of valid words} | |
| P & \ucd{meta.code.multip}& Multiplicity or binarity flag\\ | ||
| P & \ucd{meta.code.qual}& Quality, precision, reliability flag or code\\ | ||
| P & \ucd{meta.code.status}& Status code (e.g.: status of a proposal/observation)\\ | ||
| Q & \ucd{meta.coverage}& A coverage (spatial, temporal, spectral, etc) with any combination of physical axes (such as moc, tmoc, stmoc)\\ | ||
| P & \ucd{meta.cryptic}& Unknown or impossible to understand quantity\\ | ||
| Q & \ucd{meta.curation}& Parameter informing about the curation of the data\\ | ||
| Q & \ucd{meta.dataset}& Dataset\\ | ||
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@@ -282,7 +284,13 @@ \section{List of valid words} | |
| Q & \ucd{obs.airMass}& Airmass\\ | ||
| S & \ucd{obs.atmos}& Atmosphere, atmospheric phenomena affecting an observation\\ | ||
| Q & \ucd{obs.atmos.extinction}& Atmospheric extinction\\ | ||
| Q & \ucd{obs.atmos.humidity}& Amount of air humidity at observing site during an observation\\ | ||
| Q & \ucd{obs.atmos.rain}& Amount of rain at the telescope site during an observation\\ | ||
| Q & \ucd{obs.atmos.refractAngle}& Atmospheric refraction angle\\ | ||
| S & \ucd{obs.atmos.turbulence}& Related to atmospheric turbulence at the telescope site\\ | ||
| P & \ucd{obs.atmos.turbulence.isoplanatic}& Isoplanatic angle characterising the atmospheric turbulence at telescope site\\ | ||
| Q & \ucd{obs.atmos.water}& Amount of atmospheric water at observing site\\ | ||
| S & \ucd{obs.atmos.wind}& Related to atmospheric wind at observing site\\ | ||
| S & \ucd{obs.calib}& Calibration observation\\ | ||
| S & \ucd{obs.calib.flat}& Related to flat-field calibration observation (dome, sky, ..)\\ | ||
| S & \ucd{obs.calib.dark}& Related to dark current calibration\\ | ||
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@@ -398,6 +406,7 @@ \section{List of valid words} | |
| Q & \ucd{phys.flux.energy}& Energy flux, heat flux\\ | ||
| Q & \ucd{phys.gauntFactor}& Gaunt factor/correction\\ | ||
| Q & \ucd{phys.gravity}& Gravity\\ | ||
| Q & \ucd{phys.inspiralSpin}& Effective inspiral spin in binary mergers (used in GW detections)\\ | ||
| Q & \ucd{phys.ionizParam}& Ionization parameter\\ | ||
| Q & \ucd{phys.ionizParam.coll}& Collisional ionization\\ | ||
| Q & \ucd{phys.ionizParam.rad}& Radiative ionization\\ | ||
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@@ -451,6 +460,7 @@ \section{List of valid words} | |
| Q & \ucd{phys.size.sminAxis}& Linear semi minor axis\\ | ||
| Q & \ucd{phys.size.smedAxis}& Linear semi median axis for 3D ellipsoids\\ | ||
| Q & \ucd{phys.temperature}& Temperature\\ | ||
| Q & \ucd{phys.temperature.dew}& Dew temperature measured at the telescope site during an observation\\ | ||
| Q & \ucd{phys.temperature.effective}& Effective temperature\\ | ||
| Q & \ucd{phys.temperature.electron}& Electron temperature\\ | ||
| Q & \ucd{phys.transmission}& Transmission (of filter, instrument, ...)\\ | ||
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@@ -466,6 +476,7 @@ \section{List of valid words} | |
| Q & \ucd{phys.veloc.transverse}& Transverse / tangential velocity\\ | ||
| S & \ucd{phys.virial}& Related to virial quantities (mass, radius, ...)\\ | ||
| Q & \ucd{phys.volume}& Volume (in cubic units)\\ | ||
| Q & \ucd{phys.voltage}& Electric potential difference over a distance or measured by an instrument\\ | ||
| Q & \ucd{pos}& Position and coordinates\\ | ||
| Q & \ucd{pos.angDistance}& Angular distance, elongation\\ | ||
| Q & \ucd{pos.angResolution}& Angular resolution\\ | ||
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@@ -519,7 +530,6 @@ \section{List of valid words} | |
| S & \ucd{pos.heliocentric}& Heliocentric position coordinate (solar system bodies)\\ | ||
| Q & \ucd{pos.HTM}& Hierarchical Triangular Mesh\\ | ||
| Q & \ucd{pos.incidenceAng}& Incidence angle of optical ray on an interface\\ | ||
| S & \ucd{pos.lg}& Local Group reference frame\\ | ||
| S & \ucd{pos.lsr}& Local Standard of Rest reference frame\\ | ||
| Q & \ucd{pos.lunar}& Lunar coordinates\\ | ||
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@@ -535,6 +545,7 @@ \section{List of valid words} | |
| V & \ucd{pos.pm}& Proper motion\\ | ||
| Q & \ucd{pos.posAng}& Position angle of a given vector\\ | ||
| V & \ucd{pos.precess}& Precession (in equatorial coordinates)\\ | ||
| Q & \ucd{pos.projection}& 2D spatial projection\\ | ||
| Q & \ucd{pos.resolution}& Spatial linear resolution (not angular)\\ | ||
| S & \ucd{pos.spherical}& Related to spherical coordinates\\ | ||
| Q & \ucd{pos.spherical.azi}& Azimuthal angle (spherical coordinates)\\ | ||
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@@ -607,10 +618,13 @@ \section{List of valid words} | |
| Q & \ucd{src.var.pulse}& Pulse\\ | ||
| Q & \ucd{stat}& Statistical parameters\\ | ||
| Q & \ucd{stat.asymmetry}& Measure of asymmetry\\ | ||
| P & \ucd{stat.confidenceLevel}& Level of confidence for a detection or classification process\\ | ||
| P & \ucd{stat.correlation}& Correlation between two parameters\\ | ||
| P & \ucd{stat.covariance}& Covariance between two parameters\\ | ||
| P & \ucd{stat.error}& Statistical error\\ | ||
| P & \ucd{stat.error.sys}& Systematic error\\ | ||
| Q & \ucd{stat.falsePositive}& Rate of false alarm in detection problems\\ | ||
| Q & \ucd{stat.falseNegative}& Rate of missed or false negative detection\\ | ||
|
There was a problem hiding this comment. Is there a rationale for making them Q? Where would these be in a secondary position? |
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| Q & \ucd{stat.filling}& Filling factor (volume, time, ...)\\ | ||
| Q & \ucd{stat.fit}& Fit\\ | ||
| P & \ucd{stat.fit.chi2}& Chi2\\ | ||
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@@ -637,7 +651,7 @@ \section{List of valid words} | |
| P & \ucd{stat.rms}& Root mean square as square root of sum of squared values or quadratic mean\\ | ||
| P & \ucd{stat.skewness}& Skewness of a probability distribution (third moment)\\ | ||
| P & \ucd{stat.snr}& Signal to noise ratio\\ | ||
| Q & \ucd{stat.stdev}& Standard deviation as the square root of the variance\\ | ||
| S & \ucd{stat.uncalib}& Qualifier of a generic uncalibrated quantity\\ | ||
| Q & \ucd{stat.value}& Miscellaneous value\\ | ||
| P & \ucd{stat.variance}& Variance\\ | ||
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@@ -653,6 +667,7 @@ \section{List of valid words} | |
| Q & \ucd{time.interval}& Time interval, time-bin, time elapsed between two events, not the duration of an event\\ | ||
| Q & \ucd{time.lifetime}& Lifetime\\ | ||
| Q & \ucd{time.period}& Period, interval of time between the recurrence of phases in a periodic phenomenon\\ | ||
| Q & \ucd{time.period.pulsation}& Period of pulsation or oscillation of a body or a phenomenon\\ | ||
| Q & \ucd{time.period.revolution}& Period of revolution of a body around a primary one (similar to year)\\ | ||
| Q & \ucd{time.period.rotation}& Period of rotation of a body around its axis (similar to day)\\ | ||
| Q & \ucd{time.phase}& Phase, position within a period\\ | ||
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@@ -852,6 +867,36 @@ \subsection{Version tags in companion lists of terms: ucd-list.txt and ucd-list- | |
| external software products. | ||
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| \section{Changes from previous versions} | ||
| \subsection{Changes from UCDList EN v1.5 following RFM} | ||
| \subsubsection*{Additions} | ||
| \begin{itemize} | ||
| \item meta.coverage | ||
| \item time.period.pulsation | ||
| \item stat.confidenceLevel | ||
| \item stat.falseNegative | ||
| \item stat.falsePositive | ||
| \item phys.inspiralSpin | ||
| \item phys.voltage | ||
| \end{itemize} | ||
| Atmospheric measures at the telescope site : | ||
| \begin{itemize} | ||
| \item obs.atmos.humidity | ||
| \item obs.atmos.rain | ||
| \item obs.atmos.turbulence | ||
| \item obs.atmos.turbulence.isoplanatic | ||
| \item obs.atmos.water | ||
| \item obs.atmos.wind | ||
| \item phys.temperature.dew | ||
| \end{itemize} | ||
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| \subsubsection*{Amendment} | ||
| Change position tag of stat.stdev to Q in order to combine it to stat.confidenceLevel, for instance | ||
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| \subsubsection*{Deletion} | ||
| Deprecate term \emph{pos.lambert} (appearing in one table only) and propose \emph{pos.projection} instead. | ||
| In the future setting up a VO vocabulary to record projection names and identifiers together with the associated | ||
| parameters if needed, as defined in the Calabreta and Greisen FITS Paper \citep{2002A&A...395.1077C} on table 13. | ||
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| \subsection{Changes from UCDList EN v1.4 following RFM} | ||
| \subsubsection*{Additions} | ||
| \ucd{stat.skewness}, \ucd{stat.kurtosis},\ucd{stat.mad} \\ | ||
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Submodule ivoatex
updated
38 files
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| +26 −8 | Makefile | |
| +5 −5 | Makefile.template | |
| +14 −3 | README.rst | |
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| +7 −7 | vo-dml2ivoatex.xslt |
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I'm a CI skeptic and am not sure what this does, but if this is "WD" rather "PEN", there's something wrong with the underlying CI code, and that would need to be fixed.