\tpldesc{Solar system data via EPN-TAP 2.0} \now \commonmeta //epntap2#table-2_0 //epntap2#localfile-2_0 '\\schema.epn_core' %upper limit of spatial resolution in coordinate 1% %lower limit of spatial resolution in coordinate 1% %coverage, lower limit in the first coordinate% %coverage, upper limit in the first coordinate% %upper limit of spatial resolution in coordinate 2% %lower limit of spatial resolution in coordinate 2% %coverage, lower limit in the second coordinate% %coverage, upper limit in the second coordinate% %upper limit of spatial resolution in coordinate 3% %lower limit of spatial resolution in coordinate 3% %coverage, lower limit in the third coordinate% %coverage, upper limit in the third coordinate% %Date of first entry of this granule% %'im' for image, 'sp' for spectrum; see http://dc.g-vo.org/tableinfo/titan.epn_core#note-et_prod for what values are defined here.% %Emergence angle during data acquisition, upper limit% %Emergence angle during data acquisition, lower limit.% %set to equal values to group related granules; make it a constant string if you don't have groups% %Unique id for this thing (within this table; use \\srcstem if publishing files)% %Incidence angle (solar zenithal angle) during data acquisition, upper limit% %Incidence angle (solar zenithal angle) during data acquisition, lower limit.% %see http://www.minorplanetcenter.net/iau/lists/ObsCodesF.html or http://nssdc.gsfc.nasa.gov/nmc/ for terms to use here% %use complete name + usual acronym, as in 'VISIBLE AND INFRARED THERMAL IMAGING SPECTROMETER VIRTIS'% %UCD(s) defining the data, with multiple entries separated by hash (#) characters.% %Date of last modification (used to handle mirroring; have a datetime instance or an ISO string here)% %Should be identical for granules resulting from the same observation; put in the file name if you have nothing else.% %Phase angle during data acquisition, upper limit% %Phase angle during data acquisition, lower limit.% %CODMAC calibration level; see http://dc.g-vo.org/tableinfo/titan.epn_core#note-et_cal for what values are defined here.% %Start of public access period% %A spatial footprint of a dataset located on a spherical coordinate system% %An acronym helpful when combining rows from multiple services% %Spectral range, upper limit, in Hz% %Spectral range, lower limit, in Hz% %Spectral resolution, upper limit, in Hz% %Spectral resolution, lower limit, in Hz% %Spectral sampling step, upper limit, in Hz% %Spectral sampling step, lower limit, in Hz% %Choose from asteroid, dwarf_planet, planet, satellite, comet, exoplanet, interplanetary_medium, ring, sample, sky, spacecraft, spacejunk, star, UNKNOWN% %Name of the target object, preferably according to the official IAU nomenclature. As appropriate, take these from the exoplanet encyclopedia http://exoplanet.eu, the meteor catalog at http://www.lpi.usra.edu/meteor/, the catalog of stardust samples at http://curator.jsc.nasa.gov/stardust/catalog/% %Substructure observed (e.g., Atmosphere, Surface). Take terms from them Spase dictionary at http://www.spase-group.org/docs/dictionary% %Integration time of the measurement, upper limit, in s% %Integration time of the measurement, lower limit, in s% %Acquisition stop time (in JD)% %Acquisition start time (in JD)% %Sampling time for measurements of dynamical phenomena, upper limit, in s% %Sampling time for measurements of dynamical phenomena, lower limit, in s% %Time scale used for the various times. Choose from TT, TDB, TOG, TOB, TAI, UTC, GPS, UNKNOWN% %Reference position used for the various times. The standard is a bit vague at this time. Remove this if unsure.% /tap/sync rec = self.getFirstVOTableRow() print(rec) self.fail("write some assertions about the record just shown")