OCA DC TAPivo://OCA/tapObservatoire de la Côte d'AzurObservatoire de la Côte d'Azurhttps://dachs.oca.eu/favicon.png2025-10-15T14:46:35ZGuillaume Verbiese

Observatoire de la Côte d'Azur, Boulevard de l'Observatoire, CS 34229, 06304 Nice Cedex 4, France

guillaume.verbiese@oca.euvirtual-observatoriescatalogsThe OCA Data Center's TAP end point. The Table Access Protocol (TAP) lets you execute queries against our database tables, inspect various metadata, and upload your own data. It is thus the VO's premier way to access public data holdings. Tables exposed through this endpoint include: epn_core from the mp3c_best_epn schema, best, body, mpcorb, name, prop_albedo, prop_diameter, prop_family, prop_g, prop_h, prop_mass, prop_proper_elements, version from the mp3c_main schema, columns, groups, key_columns, keys, schemas, tables from the tap_schema schema, ssobft from the vossp schema.https://dachs.oca.eu/__system__/tap/run/infohttps://dachs.oca.eu/tapADQL2.02.1The Astronomical Data Query Language is the standard IVOA dialect of SQL; it contains a very general SELECT statement as well as some extensions for spherical geometry and higher mathematics.

gavo_getauthority(ivoid TEXT) -> TEXT

returns the authority part of an ivoid (or, more generally a URI). So, ivo://org.gavo.dc/foo/bar#baz becomes org.gavo.dc. The behaviour for anything that's not a full URI is undefined.

gavo_histogram(val REAL, lower REAL, upper REAL, nbins INTEGER) -> INTEGER[]

The aggregate function returns a histogram of val with nbins+2 elements. Assuming 0-based arrays, result[0] contains the number of underflows (i.e., val<lower), result[nbins+1] the number of overflows. Elements 1..nbins are the counts in nbins bins of width (upper-lower)/nbins. Clients will have to convert back to physical units using some external communication, there currently is no (meta-) data as lower and upper in the TAP response.

gavo_ipix(long REAL, lat REAL) -> BIGINT

gavo_ipix returns the q3c ipix for a long/lat pair (it simply wraps the 13c_ang2ipix function). This is probably only relevant when you play tricks with indices or PPMXL ids.

gavo_match(pattern TEXT, string TEXT) -> INTEGER

gavo_match returns 1 if the POSIX regular expression pattern matches anything in string, 0 otherwise.

gavo_mocintersect(moc1 MOC, moc2 MOC) -> MOC

returns the intersection of two MOCs.

gavo_mocunion(moc1 MOC, moc2 MOC) -> MOC

returns the union of two MOCs.

gavo_normal_random(mu REAL, sigma REAL) -> REAL

The function returns a random number drawn from a normal distribution with mean mu and width sigma. Implementation note: Right now, the Gaussian is approximated by summing up and scaling ten calls to random. This, hence, is not very precise or fast. It might work for some use cases, and we will provide a better implemenation if this proves inadequate.

gavo_simbadpoint(identifier TEXT) -> POINT

gavo_simbadpoint queries simbad for an identifier and returns the corresponding point. Note that identifier can only be a literal, i.e., as simple string rather than a column name. This is because our database cannot query simbad, and we probably wouldn't want to fire off millions of simbad queries anyway; use simbad's own TAP service for this kind of application.

gavo_specconv(expr DOUBLE PRECISION, dest_unit TEXT) -> DOUBLE PRECISION

returns the spectral value expr converted to dest_unit. expr has to be in either energy, wavelength, or frequency, and dest_unit must be a VOUnit giving another spectral unit (e.g., MHz, keV, nm, or Angstrom). This is intended to let users express spectral constraints in their preferred unit independently of the choice of unit in the database. Examples:: gavo_specconv(obscore.em_min, "keV") > 300 gavo_specconv(obscore.em_max, "MHz") > 30 gavo_specconv(spectral_start, "Angstrom") > 4000 There is a variant of gavo_specconv accepting expr's unit in a third argument.

gavo_specconv(expr NUMERIC, expr_unit TEXT dest_unit TEXT) -> NUMERIC

returns expr assumed to be in expr_unit expressed in dest_unit. This is a variant of the two-argument gavo_specconv for when the unit of expr is not known to the ADQL translator, either because it because it is a literal or because it does not look like a spectral unit. Examples:: gavo_specconv(656, 'nm', 'J') BETWEEN spectral_start AND spectral_end gavo_specconv(arccos(phi)*incidence, 'Hz', 'eV') Clearly, overriding known units is likely to yield bad results; the translator therefore warns if an existing unit is overridden with a different unit.

gavo_to_jd(d TIMESTAMP) -> DOUBLE PRECISION

The function converts a postgres timestamp to julian date. This is naive; no corrections for timezones, let alone time scales or the like are done; you can thus not expect this to be good to second-precision unless you are careful in the construction of the timestamp.

gavo_to_mjd(d TIMESTAMP) -> DOUBLE PRECISION

The function converts a postgres timestamp to modified julian date. This is naive; no corrections for timezones, let alone time scales or the like are done; you can thus not expect this to be good to second-precision unless you are careful in the construction of the timestamp.

gavo_transform(from_sys TEXT, to_sys TEXT, geo GEOMETRY) -> GEOMETRY

The function transforms ADQL geometries between various reference systems. geo can be a POINT, a CIRCLE, or a POLYGON, and the function will return a geometry of the same type. In the current implementation, from_sys and to_sys must be literal strings (i.e., they cannot be computed through expressions or be taken from database columns). All transforms are just simple rotations, which is only a rough approximation to the actual relationships between reference systems (in particular between FK4 and ICRS-based ones). Note that, in particular, the epoch is not changed (i.e., no proper motions are applied). We currently support the following reference frames: ICRS, FK5 (which is treated as ICRS), FK4 (for B1950. without epoch-dependent corrections), GALACTIC. Reference frame names are case-sensitive.

gavo_vocmatch(vocname TEXT, term TEXT, matchagainst TEXT) -> INTEGER

returns 1 if matchagainst is term or narrower in the IVOA vocabulary vocname, 0 otherwise. This is intended for semantic querying. For instance, gavo_vocmatch('datalink/core', 'calibration', semantics) would be 1 if semantics is any of calibration, bias, dark, or flat. For RDF-flavoured vocabularies (strict trees), term will expand to the entire branch rooted in term. For SKOS-flavoured vocabularies (where narrower is not transitive), only directly narrower terms will be included. Both the term and the vocabulary name must be string literals (i.e., constants). matchagainst can be any string-valued expression.

ivo_apply_pm(ra DOUBLE PRECISION, dec DOUBLE PRECISION, pmra DOUBLE PRECISION, pmde DOUBLE PRECISON, epdist DOUBLE PRECISION) -> POINT

Returns a POINT (in the UNDEFINED reference frame) for the position an object at ra/dec with proper motion pmra/pmde has after epdist years. positions must be in degrees, PMs in should be in julian years (i.e., proper motions are expected in degrees/year). pmra is assumed to contain cos(delta). This function goes through the tangential plane. Since it does not have information on distance and radial velocity, it cannot reconstruct the true space motion, and hence its results will degrade over time.

ivo_hashlist_has(hashlist TEXT, item TEXT) -> INTEGER

The function takes two strings; the first is a list of words not containing the hash sign (#), concatenated by hash signs, the second is a word not containing the hash sign. It returns 1 if, compared case-insensitively, the second argument is in the list of words coded in the first argument. The behaviour in case the the second argument contains a hash sign is unspecified.

ivo_hasword(haystack TEXT, needle TEXT) -> INTEGER

gavo_hasword returns 1 if needle shows up in haystack, 0 otherwise. This is for "google-like"-searches in text-like fields. In word, you can actually employ a fairly complex query language; see https://www.postgresql.org/docs/current/textsearch.html for details.

ivo_healpix_center(hpxOrder INTEGER, hpxIndex BIGINT) -> POINT

returns a POINT corresponding to the center of the healpix with the given index at the given order.

ivo_healpix_index(order INTEGER, ra DOUBLE PRECISION, dec DOUBLE PRECISION) -> BIGINT

Returns the index of the (nest) healpix with order containing the spherical point (ra, dec). An alternative, 2-argument form ivo_healpix_index(order INTEGER, p POINT) -> BIGINT is also available.

ivo_interval_has(val NUMERIC, iv INTERVAL) -> INTEGER

The function returns 1 if the interval iv contains val, 0 otherwise. The lower limit is always included in iv, behaviour on the upper limit is column-specific.

ivo_interval_overlaps(l1 NUMERIC, h1 NUMERIC, l2 NUMERIC, h2 NUMERIC) -> INTEGER

The function returns 1 if the interval [l1...h1] overlaps with the interval [l2...h2]. For the purposes of this function, the case l1=h2 or l2=h1 is treated as overlap. The function returns 0 for non-overlapping intervals.

ivo_nocasematch(value TEXT, pattern TEXT) -> INTEGER

ivo_nocasematch returns 1 if pattern matches value, 0 otherwise. pattern is defined as for the SQL LIKE operator, but the match is performed case-insensitively. This function in effect provides a surrogate for the ILIKE SQL operator that is missing from ADQL. On this site, this is actually implemented using python's and SQL's LOWER, so for everything except ASCII, your milage will vary.

ivo_string_agg(expression TEXT, delimiter TEXT) -> TEXT

An aggregate function returning all values of expression within a GROUP contcatenated with delimiter

BOX

POINT

CIRCLE

POLYGON

REGION

CENTROID

COORD1

COORD2

DISTANCE

CONTAINS

INTERSECTS

AREA

LOWER

ILIKE

OFFSET

CAST

IN_UNIT

WITH

TABLESAMPLE

Written after a table reference, TABLESAMPLE(10) will make the database only use 10% of the rows; these are `somewhat random' in that the system will use random blocks. This should be good enough when just testing queries (and much better than using TOP n).

MOC

A geometry function creating MOCs. It either takes a string argument with an ASCII MOC ('4/13 17-18 8/3002'), or an order and another geometry.

COALESCE

This is the standard SQL COALESCE for providing defaults in case of NULL values.

UNION

EXCEPT

INTERSECT

text/tab-separated-valuestsvtext/plaintxttext/csvcsv_baretext/csv;header=presentcsvapplication/jsonjsonapplication/geo+jsongeojsonapplication/x-votable+xmlvotableapplication/x-votable+xml;serialization=BINARY2votable/b2votableb2application/x-votable+xml;serialization=TABLEDATAtext/xmlvotable/tdvotabletdapplication/x-votable+xml;serialization=TABLEDATA;version=1.1text/xmlvotabletd1.1application/x-votable+xml;version=1.1text/xmlvotable1.1application/x-votable+xml;serialization=TABLEDATA;version=1.2text/xmlvotabletd1.2application/x-votable+xml;serialization=TABLEDATA;version=1.5vodmlapplication/x-votable+xml;version=1.5vodmlbtext/htmlhtmlapplication/fitsfits1728003600200002000000020000000https://dachs.oca.eu/__system__/tap/run/availabilityhttps://dachs.oca.eu/__system__/tap/run/capabilitieshttps://dachs.oca.eu/__system__/tap/run/tableMetadatahttps://dachs.oca.eu/__system__/tap/run/examplesmp3c_best_epn This service publishes average values of various physical properties for minor bodies. It mirrors part of the data reported by the Minor Planet Physical Properties Catalogue (MP3C) user-friendly interface at https://mp3c.oca.eu/. Quantities include masses, diameters, albedos and orbital parameters.mp3c_best_epn.epn_core This service publishes average values of various physical properties for minor bodies. It mirrors part of the data reported by the Minor Planet Physical Properties Catalogue (MP3C) user-friendly interface at https://mp3c.oca.eu/. Quantities include masses, diameters, albedos and orbital parameters.ivo://ivoa.net/std/epntap#table-2.01200000granule_uidInternal table row index, which must be unique within the table. Can be alphanumeric.meta.idchargranule_gidCommon to granules of same type (e.g. same map projection, or geometry data products). Can be alphanumeric.meta.idcharobs_idAssociates granules derived from the same data (e.g. various representations/processing levels). Can be alphanumeric, may be the ID of original observation.meta.id;obschardataproduct_typeThe high-level organization of the data product, from a controlled vocabulary (e.g., 'im' for image, sp for spectrum). Multiple terms may be used, separated by # characters.meta.code.classcharnullabletarget_nameStandard IAU name of target (from a list related to target class), case sensitivemeta.id;srccharnullabletarget_classType of target, from a controlled vocabulary.src.classcharnullabletime_minAcquisition start time (in JD), as UTC at time_refpositiondtime.start;obsdoublenullabletime_maxAcquisition stop time (in JD), as UTC at time_refpositiondtime.end;obsdoublenullabletime_sampling_step_minSampling time for measurements of dynamical phenomena, lower limit.stime.resolution;stat.mindoublenullabletime_sampling_step_maxSampling time for measurements of dynamical phenomena, upper limitstime.resolution;stat.maxdoublenullabletime_exp_minIntegration time of the measurement, lower limit.stime.duration;obs.exposure;stat.mindoublenullabletime_exp_maxIntegration time of the measurement, upper limitstime.duration;obs.exposure;stat.maxdoublenullablespectral_range_minSpectral range (frequency), lower limit.Hzem.freq;stat.mindoublenullablespectral_range_maxSpectral range (frequency), upper limitHzem.freq;stat.maxdoublenullablespectral_sampling_step_minSpectral sampling step, lower limit.Hzem.freq;spect.binSize;stat.mindoublenullablespectral_sampling_step_maxSpectral sampling step, upper limitHzem.freq;spect.binSize;stat.maxdoublenullablespectral_resolution_minSpectral resolution, lower limit.spect.resolution;stat.mindoublenullablespectral_resolution_maxSpectral resolution, upper limitspect.resolution;stat.maxdoublenullablec1min(This data collection does not give coordinates)doublenullablec1max(This data collection does not give coordinates)doublenullablec2min(This data collection does not give coordinates)doublenullablec2max(This data collection does not give coordinates)doublenullablec3min(This data collection does not give coordinates)doublenullablec3max(This data collection does not give coordinates)doublenullables_regionObsCore-like footprint, valid for celestial, spherical, or body-fixed framespos.outline;obs.fieldcharnullablec1_resol_min(This data collection does not give coordinates)doublenullablec1_resol_max(This data collection does not give coordinates)doublenullablec2_resol_min(This data collection does not give coordinates)doublenullablec2_resol_max(This data collection does not give coordinates)doublenullablec3_resol_min(This data collection does not give coordinates)doublenullablec3_resol_max(This data collection does not give coordinates)doublenullablespatial_frame_typeFlavor of coordinate system, defines the nature of coordinates. From a controlled vocabulary, where 'none' means undefined.meta.code.class;pos.framecharnullableincidence_minIncidence angle (solar zenithal angle) during data acquisition, lower limit.degpos.incidenceAng;stat.mindoublenullableincidence_maxIncidence angle (solar zenithal angle) during data acquisition, upper limitdegpos.incidenceAng;stat.maxdoublenullableemergence_minEmergence angle during data acquisition, lower limit.degpos.emergenceAng;stat.mindoublenullableemergence_maxEmergence angle during data acquisition, upper limitdegpos.emergenceAng;stat.maxdoublenullablephase_minPhase angle during data acquisition, lower limit.degpos.phaseAng;stat.mindoublenullablephase_maxPhase angle during data acquisition, upper limitdegpos.phaseAng;stat.maxdoublenullableinstrument_host_nameStandard name of the observatory or spacecraftmeta.id;instr.obstycharnullableinstrument_nameStandard name of instrumentmeta.id;instrcharnullablemeasurement_typeUCD(s) defining the data, with multiple entries separated by hash (#) characters.meta.ucdcharnullableprocessing_levelDataset-related encoding, or simplified CODMAC calibration levelmeta.calibLevelintcreation_dateDate of first entry of this granuletime.creationcharnullablemodification_dateDate of last modification (used to handle mirroring)time.processingcharnullablerelease_dateStart of public access periodtime.releasecharnullableservice_titleTitle of resource (an acronym really, will be used to handle multiservice results)meta.titlecharnullablealt_target_nameProvides alternative target name if more common (e.g. comets); multiple identifiers can be separated by hashesmeta.id;srccharnullablemassMass of objectkgphys.massdoublenullablediameterTarget diameter, or equivalent diameter for binary objectskmphys.size.diameterdoublenullablesemi_major_axisAUphys.size.smajAxisdoublenullableinclinationOrbit inclinationsrc.orbital.inclinationdoublenullableeccentricityOrbit eccentricitysrc.orbital.eccentricitydoublenullablemagnitudeAbsolute magnitude. For small bodies, from HG magnitude systemmagphys.magAbsdoublenullablealbedoTarget albedophys.albedodoublenullablepublisherA short string identifying the entity running the data service usedmeta.curationcharnullableproducer_nameData producer name, especially in compilations of experimental datameta.notecharnullableparentNumber of target parent (asteroid family number)meta.id.parentintnullableparent_nameName of target parent (asteroid family)meta.id.parentcharnullablemass_errorMass of object errorkgstat.error;phys.massfloatnullablediameter_errorTarget diameter errorkmstat.error;phys.size.diameterfloatnullablesemi_major_axis_errorOrbital proper semimajor axis errorAUstat.error;phys.size.smajAxisfloatnullableinclination_errorOrbit proper inclination errordegstat.error;src.orbital.inclinationfloatnullablemagnitude_errorAbsolute magnitude error, from HG magnitude systemmagstat.error;phys.magAbsfloatnullableslope_parameterSlope parameter (surge in brightness), observed when the body is near oppositionfloatnullableslope_parameter_errorError of slope parameter (surge in brightness), observed when the body is near oppositionfloatnullableeccentricity_errorOrbit eccentricitystat.error;src.orbital.eccentricityfloatnullablealbedo_errorTarget albedo errorstat.error;phys.albedofloatnullableexternal_linkLink to a web page providing more details on the granulemeta.ref.urlcharmp3c_main This service publishes minor body data, including orbits, masses, diameters, albedos, families and magnitudes. The tables have the same format as those used by the Minor Planet Physical Properties Catalogue (MP3C) user-friendly interface at https://mp3c.oca.eu/ and let you run more complex queries than the web interface.mp3c_main.version Provides information on the database version stored under this schema.versionVersion of this database.id_versioncharindexedprimarydate_createdDate of creation of the database. Since we never update the database but recreate it when updating the data, this field also represents the "date of last update".time.creationcharmp3c_gen_db_revisionRevision number (commit hash) of the mp3c-gen-db project used to generate this database.meta.idcharsources_hashesJSON representing the checksums of all input files fed to the mp3c-gen-db project and used to generate this database.meta.codecharmp3c_main.name Lists all possible names of referenced minor bodies.bidBody ID representing an asteroid or dwarf planet across tables. Useful for JOIN queries. Body IDs are consistent only within a given version of the database and may change with time.meta.idintnameName of body (asteroid or dwarf planet). May be an alternative designation.meta.idcharindexedprimarypriorityPriority given to the name. Low values indicate higher precedence and the name with lowest value defines the main body name.meta.codeintmp3c_main.body Minor body objects with their primary names.bidBody ID representing an asteroid or dwarf planet across tables. Useful for JOIN queries. Body IDs are consistent only within a given version of the database and may change with time.meta.idintindexedprimarynameMain name of body (asteroid or dwarf planet) as attributed by the name with lowest priority index in the "name" table of all body designations.meta.idcharmp3c_main.mpcorb Minor Planet Center (MPC) data.numberMPC body numbermeta.idintnullablenameName of body (asteroid or dwarf planet). May be an alternative designation.meta.idcharbidBody ID representing an asteroid or dwarf planet across tables. Useful for JOIN queries. Body IDs are consistent only within a given version of the database and may change with time.meta.idintindexedprimaryaMPC orbit semi-major axis.AUphys.size.smajAxisfloateMPC orbit eccentricity.src.orbital.eccentricityfloatiMPC orbit inclination, J2000.0.degsrc.orbital.inclinationfloatsin_iMPC orbit sine of inclination.floatperihelionMPC orbit argument of perihelion.degsrc.orbital.periastronfloatnodeMPC longitude of the ascending node, J2000.0degsrc.orbital.nodefloatmMPC mean anomaly at epoch.src.orbital.meananomalyfloatnMPC mean daily motion.deg/dsrc.orbital.meananomalyfloatepochMPC epoch (terrestrial time, TT).time.epochfloatn_obsMPC number of observations.meta.number;obsintn_oppMPC number of oppositions.meta.numberintmultiopp_year_first_observedMPC year first observed.timeintnullablemultiopp_year_last_observedMPC year last observed.timeintnullablesingleopp_arc_lengthMPC arc length for single-opposition orbits.dtimeintnullablermsMPC RMS residual.stat.fit.residualfloatnullablemp3c_main.prop_mass Mass measurements with bibliographic sources.idRow identifier.meta.idintindexedprimarybidBody ID representing an asteroid or dwarf planet across tables. Useful for JOIN queries. Body IDs are consistent only within a given version of the database and may change with time.meta.idintmpc_numMPC body numbermeta.idintnullablenameName of body (asteroid or dwarf planet). May be an alternative designation.meta.idcharvalMass of body.kgphys.massfloatunc_loLower uncertainty on mass of body.kgstat.error;phys.massfloatnullableunc_upUpper uncertainty on mass of body.kgstat.error;phys.massfloatnullableauthorAuthor of measurement.meta.bib.authorcharrefBibliographic reference for the measurement.meta.bibcharmethodMethod used for the measurement.meta.codecharnullableref_urlBibliographic reference URL for the measurement.meta.ref.urlcharmp3c_main.prop_diameter Diameter measurements with bibliographic sources.idRow identifier.meta.idintindexedprimarybidBody ID representing an asteroid or dwarf planet across tables. Useful for JOIN queries. Body IDs are consistent only within a given version of the database and may change with time.meta.idintmpc_numMPC body numbermeta.idintnullablenameName of body (asteroid or dwarf planet). May be an alternative designation.meta.idcharvalDiameter of body.kmphys.size.diameterfloatunc_loLower uncertainty on diameter of body.kmstat.error;phys.size.diameterfloatnullableunc_upUpper uncertainty on diameter of body.kmstat.error;phys.size.diameterfloatnullableauthorAuthor of measurement.meta.bib.authorcharrefBibliographic reference for the measurement.meta.bibcharmethodMethod used for the measurement.meta.codecharnullableref_urlBibliographic reference URL for the measurement.meta.ref.urlcharmp3c_main.prop_albedo Albedo measurements with bibliographic sources.idRow identifier.meta.idintindexedprimarybidBody ID representing an asteroid or dwarf planet across tables. Useful for JOIN queries. Body IDs are consistent only within a given version of the database and may change with time.meta.idintmpc_numMPC body numbermeta.idintnullablenameName of body (asteroid or dwarf planet). May be an alternative designation.meta.idcharvalGeometric visible albedo of body.phys.albedofloatunc_loLower uncertainty on geometric visible albedo of body.stat.error;phys.albedofloatnullableunc_upUpper uncertainty on geometric visible albedo of body.stat.error;phys.albedofloatnullableauthorAuthor of measurement.meta.bib.authorcharrefBibliographic reference for the measurement.meta.bibcharmethodMethod used for the measurement.meta.codecharnullableref_urlBibliographic reference URL for the measurement.meta.ref.urlcharmp3c_main.prop_h Magnitude measurements (H parameter of HG system) with bibliographic sources.idRow identifier.meta.idintindexedprimarybidBody ID representing an asteroid or dwarf planet across tables. Useful for JOIN queries. Body IDs are consistent only within a given version of the database and may change with time.meta.idintmpc_numMPC body numbermeta.idintnullablenameName of body (asteroid or dwarf planet). May be an alternative designation.meta.idcharvalAbsolute magnitude of body (HG system).magphys.magAbsfloatunc_loLower uncertainty on absolute magnitude of body (HG system).magstat.error;phys.magAbsfloatnullableunc_upUpper uncertainty on absolute magnitude of body (HG system).magstat.error;phys.magAbsfloatnullableauthorAuthor of measurement.meta.bib.authorcharrefBibliographic reference for the measurement.meta.bibcharmethodMethod used for the measurement.meta.codecharnullableref_urlBibliographic reference URL for the measurement.meta.ref.urlcharmp3c_main.prop_g Slope parameter of the magnitude measurements (G parameter of HG system) with bibliographic sources.idRow identifier.meta.idintindexedprimarybidBody ID representing an asteroid or dwarf planet across tables. Useful for JOIN queries. Body IDs are consistent only within a given version of the database and may change with time.meta.idintmpc_numMPC body numbermeta.idintnullablenameName of body (asteroid or dwarf planet). May be an alternative designation.meta.idcharvalSlope parameter of magnitude of body (HG system).arith.gradfloatunc_loLower uncertainty on slope parameter of magnitude of body (HG system).stat.error;arith.gradfloatnullableunc_upUpper uncertainty on slope parameter of magnitude of body (HG system).stat.error;arith.gradfloatnullableauthorAuthor of measurement.meta.bib.authorcharrefBibliographic reference for the measurement.meta.bibcharmethodMethod used for the measurement.meta.codecharnullableref_urlBibliographic reference URL for the measurement.meta.ref.urlcharmp3c_main.prop_family Family (parent bodies) measurements with bibliographic sources.idRow identifier.meta.idintindexedprimarybidBody ID representing an asteroid or dwarf planet across tables. Useful for JOIN queries. Body IDs are consistent only within a given version of the database and may change with time.meta.idintmpc_numMPC body numbermeta.idintnullablenameName of body (asteroid or dwarf planet). May be an alternative designation.meta.idcharparentParent body of body attributed by MP3C based on author's family.meta.idintparent_nameParent body name of body attributed by MP3C based on author's family.meta.idcharfamily_idAuthor's ID of the family in which the body has been classified.meta.idcharfamily_nameAuthor's name of family in which the body has been classified.meta.idcharc_paramC_j parameter that helps to identify potential interlopers in a family. A large absolute value means more chance that the body is in reality not part of the attributed family. For example, for the Nesvorny families, C_j is defined as C_j = 10^(-H_j/5) (a_j - a_center)/C_0, with H the absolute magnitude, a the proper semimajor axis of a member, a_center the family center, C_0 the best fit to the V-shape envelope of the family, and index j runs over individual bodies.meta.numberfloatnullableauthorAuthor of measurement.meta.bib.authorcharrefBibliographic reference for the measurement.meta.bibcharmethodMethod used for the measurement.meta.codecharnullableref_urlBibliographic reference URL for the measurement.meta.ref.urlcharmp3c_main.prop_proper_elements Proper elements measurements with bibliographic sources.idRow identifier.meta.idintindexedprimarybidBody ID representing an asteroid or dwarf planet across tables. Useful for JOIN queries. Body IDs are consistent only within a given version of the database and may change with time.meta.idintmpc_numMPC body numbermeta.idintnullablenameName of body (asteroid or dwarf planet). May be an alternative designation.meta.idchara_pProper semi-major axis of body orbit.AUphys.size.smajAxisfloate_pProper eccentricity of body orbit.src.orbital.eccentricityfloatsin_i_pSine of proper inclination of body orbit.floatauthorAuthor of measurement.meta.bib.authorcharrefBibliographic reference for the measurement.meta.bibcharmethodMethod used for the measurement.meta.codecharnullableref_urlBibliographic reference URL for the measurement.meta.ref.urlcharmp3c_main.best Best values for all physical properties of the minor bodies. For example, when a body has several mass measurements in the prop_mass table, we report here an average mass.bidBody ID representing an asteroid or dwarf planet across tables. Useful for JOIN queries. Body IDs are consistent only within a given version of the database and may change with time.meta.idintindexedprimaryparentBest parent body number (family) of body.meta.idintnullableparent_nameBest parent body name (family) of body.meta.idcharmassBest mass of body.kgphys.massfloatnullablemass_errError on best mass of body.kgstat.error;phys.massfloatnullablediameterBest diameter of body.kmphys.size.diameterfloatnullablediameter_errError on best diameter of body.kmstat.error;phys.size.diameterfloatnullableinverse_diameterBest inverse of diameter of body.km**-1floatnullableinverse_diameter_errError on best inverse of diameter of body.km**-1stat.errorfloatnullablealbedoBest geometric visible albedo of body.phys.albedofloatnullablealbedo_errError on est geometric visible albedo of body.stat.error;phys.albedofloatnullablegBest slope parameter of magnitude of body (HG system).arith.gradfloatnullableg_errError on best slope parameter of magnitude of body (HG system).stat.error;arith.gradfloatnullablehBest absolute magnitude of body (HG system).magphys.magAbsfloatnullableh_errError on best absolute magnitude of body (HG system).magstat.error;phys.magAbsfloatnullablea_pBest proper semi-major axis of body orbit.AUphys.size.smajAxisfloatnullablea_p_errError on best proper semi-major axis of body orbit.AUstat.error;phys.size.smajAxisfloatnullablee_pBest proper eccentricity of body orbit.src.orbital.eccentricityfloatnullablee_p_errError on best proper eccentricity of body orbit.stat.error;src.orbital.eccentricityfloatnullablei_pBest proper inclination of body orbit.degsrc.orbital.inclinationfloatnullablei_p_errError on best proper inclination of body orbit.degstat.error;src.orbital.inclinationfloatnullablesin_i_pSine of proper inclination of body orbit.floatnullablesin_i_p_errError on sine of proper inclination of body orbit.stat.errorfloatnullabletap_schema OCA Data Center's Table Access Protocol (TAP) service with table metadata.tap_schema.schemasSchemas containing tables available for ADQL querying.schema_nameFully qualified schema namecharindexedprimarydescriptionBrief description of the schemaunicodeCharnullableutypeutype if schema corresponds to a data modelcharnullableschema_indexSuggested position this schema should take in a sorted list of schemas from this data center.intnullabletap_schema.tablesTables available for ADQL querying.schema_nameFully qualified schema namecharnullabletable_nameFully qualified table namecharindexedprimarytable_typeOne of: table, viewcharnullabledescriptionBrief description of the tableunicodeCharnullableutypeutype if the table corresponds to a data modelcharnullabletable_indexSuggested position this table should take in a sorted list of tables from this data centerintnullablesourcerdId of the originating rd (local information)charnullabletap_schema.schemasschema_nameschema_nametap_schema.columnsColumns in tables available for ADQL querying.table_nameFully qualified table namecharindexedprimarycolumn_nameColumn namecharindexedprimarydescriptionBrief description of columnunicodeCharnullableunitUnit in VO standard formatcharnullableucdUCD of column if anycharnullableutypeUtype of column if anycharnullabledatatypeADQL datatypecharnullablearraysizeArraysize in VOTable notationcharnullablextypeVOTable extended type information (for special interpretation of data content, e.g., timestamps or points)charnullable"size"Legacy length (ignore if you can).intnullableprincipalIs column principal?intindexedIs there an index on this column?intstdIs this a standard column?intsourcerdId of the originating rd (local information)charnullablecolumn_index1-based index of the column in database order.shortnullabletap_schema.tablestable_nametable_nametap_schema.keysForeign key relationships between tables available for ADQL querying.key_idUnique key identifiercharindexedprimaryfrom_tableFully qualified table namecharnullabletarget_tableFully qualified table namecharnullabledescriptionDescription of this keyunicodeCharnullableutypeUtype of this keycharnullablesourcerdId of the originating rd (local information)charnullabletap_schema.tablesfrom_tabletable_nametap_schema.tablestarget_tabletable_nametap_schema.key_columnsColumns participating in foreign key relationships between tables available for ADQL querying.key_idKey identifier from TAP_SCHEMA.keyscharnullablefrom_columnKey column name in the from tablecharnullabletarget_columnKey column in the target tablecharnullablesourcerdId of the originating rd (local information)charnullabletap_schema.keyskey_idkey_idtap_schema.groupsColumns that are part of groups within tables available for ADQL querying.table_nameFully qualified table namecharnullablecolumn_nameName of a column belonging to the groupcharnullablecolumn_utypeutype the column withing the groupcharnullablegroup_nameName of the groupcharnullablegroup_utypeutype of the groupcharnullablesourcerdId of the originating rd (local information)charnullabletap_schema.tablestable_nametable_namevossp The VO-IMCCE project is born in 2003. The first step was to make an interconnection between the VizieR service (CDS) and the service of calculation of asteroid ephemerides of the IMCCE. In 2004, we began the development of tools and services in the framework of the Virtual observatory. In 2005 the first version of the SkyBoT service is born to answer the simple question: which solar system bodies are visible in a given area of the sky at a given epoch? The service was put in production in January 2006 through a Web service, through the VO portal Aladin (CDS), and through various softwares, such as Audela and the WCS tools. A few months later, the Miriade services came out to provide new computing services of solar system body ephemerides.vossp.ssobft The ssoBFT is a broad and flat table that compiles all the property values of all the SSOs. It is intended to people who want to make statistics or plots on SSO properties.1455526"sso_id"Unique identifier of the SSOmeta.id;meta.mainunicodeCharnullable"sso_number"IAU number of the SSOmeta.idintnullable"sso_name"Official name or provisional designation of the SSOmeta.idunicodeCharnullable"sso_type"Type of SSO (planet, satellite, asteroid, dwarf planet, comet)src.classcharnullable"sso_class"Dynamical population the SSO belongs tometa.code.classcharnullable"ssocard"unicodeCharnullable"orbital_elements.ref_epoch"Reference epoch of osculationdtime.epoch;src.orbitalfloatnullable"orbital_elements.number_observation"Number of observations used to compute the orbitmeta.number;obsintnullable"orbital_elements.orbital_arc"Orbital arc spanned by observations used in orbit computationdtime.duration;src.orbitalintnullable"orbital_elements.ceu.value"Absolute value of the current 1-sigma ephemeris uncertainty (CEU)arcsecstat.rms;src.orbitalfloatindexednullable"orbital_elements.ceu.error.min"Absolute value of the current 1-sigma ephemeris uncertainty (CEU)arcsecstat.rms;src.orbitalfloatindexednullable"orbital_elements.ceu.error.max"Absolute value of the current 1-sigma ephemeris uncertainty (CEU)arcsecstat.rms;src.orbitalfloatindexednullable"orbital_elements.ceu_rate.value"Rate of change of the absolute value of the current 1-sigma ephemeris uncertainty (CEU)arcsec/dstat.rms;arith.ratefloatnullable"orbital_elements.ceu_rate.error.min"Rate of change of the absolute value of the current 1-sigma ephemeris uncertainty (CEU)arcsec/dstat.rms;arith.ratefloatnullable"orbital_elements.ceu_rate.error.max"Rate of change of the absolute value of the current 1-sigma ephemeris uncertainty (CEU)arcsec/dstat.rms;arith.ratefloatnullable"orbital_elements.semi_major_axis.value"Semi-major axis of the orbitaupos.distance;src.orbitalfloatindexednullable"orbital_elements.semi_major_axis.error.min"Semi-major axis of the orbitaupos.distance;src.orbitalfloatindexednullable"orbital_elements.semi_major_axis.error.max"Semi-major axis of the orbitaupos.distance;src.orbitalfloatindexednullable"orbital_elements.semi_major_axis.ratio.value"Semi-major axis of the orbitaupos.distance;src.orbitalfloatnullable"orbital_elements.semi_major_axis.ratio.error.min"Semi-major axis of the orbitaupos.distance;src.orbitalfloatnullable"orbital_elements.semi_major_axis.ratio.error.max"Semi-major axis of the orbitaupos.distance;src.orbitalfloatnullable"orbital_elements.eccentricity.value"Eccentricity of the orbitsrc.orbital.eccentricityfloatindexednullable"orbital_elements.eccentricity.error.min"Eccentricity of the orbitsrc.orbital.eccentricityfloatindexednullable"orbital_elements.eccentricity.error.max"Eccentricity of the orbitsrc.orbital.eccentricityfloatindexednullable"orbital_elements.inclination.value"Inclination of the orbitdegsrc.orbital.inclinationfloatindexednullable"orbital_elements.inclination.error.min"Inclination of the orbitdegsrc.orbital.inclinationfloatindexednullable"orbital_elements.inclination.error.max"Inclination of the orbitdegsrc.orbital.inclinationfloatindexednullable"orbital_elements.inclination.ref_plane"Inclination of the orbitdegsrc.orbital.inclinationfloatnullable"orbital_elements.node_longitude.value"Longitude of the ascending node of the orbitdegsrc.orbital.nodefloatindexednullable"orbital_elements.node_longitude.error.min"Longitude of the ascending node of the orbitdegsrc.orbital.nodefloatindexednullable"orbital_elements.node_longitude.error.max"Longitude of the ascending node of the orbitdegsrc.orbital.nodefloatindexednullable"orbital_elements.periapsis_argument.value"Argument of periapsis of the orbitdegsrc.orbital.periastronfloatindexednullable"orbital_elements.periapsis_argument.error.min"Argument of periapsis of the orbitdegsrc.orbital.periastronfloatindexednullable"orbital_elements.periapsis_argument.error.max"Argument of periapsis of the orbitdegsrc.orbital.periastronfloatindexednullable"orbital_elements.pericenter_date.value"Date of passage to the pericenterdtime.epoch;src.orbital.periastronfloatnullable"orbital_elements.pericenter_date.error.min"Date of passage to the pericenterdtime.epoch;src.orbital.periastronfloatnullable"orbital_elements.pericenter_date.error.max"Date of passage to the pericenterdtime.epoch;src.orbital.periastronfloatnullable"orbital_elements.mean_anomaly.value"Angle between lines drawn from the Sun to the periapsis and to a point moving on the orbit at a uniform rate corresponding to the period of revolution of the SSOdegsrc.orbital.meanAnomalyfloatnullable"orbital_elements.mean_anomaly.error.min"Angle between lines drawn from the Sun to the periapsis and to a point moving on the orbit at a uniform rate corresponding to the period of revolution of the SSOdegsrc.orbital.meanAnomalyfloatnullable"orbital_elements.mean_anomaly.error.max"Angle between lines drawn from the Sun to the periapsis and to a point moving on the orbit at a uniform rate corresponding to the period of revolution of the SSOdegsrc.orbital.meanAnomalyfloatnullable"orbital_elements.mean_motion.value"Mean angular velocity required for the body to complete one orbitdeg/dsrc.orbital.meanMotionfloatnullable"orbital_elements.mean_motion.error.min"Mean angular velocity required for the body to complete one orbitdeg/dsrc.orbital.meanMotionfloatnullable"orbital_elements.mean_motion.error.max"Mean angular velocity required for the body to complete one orbitdeg/dsrc.orbital.meanMotionfloatnullable"orbital_elements.orbital_period.value"Amount of time the SSO takes to complete one orbitdtime.period.revolutionfloatindexednullable"orbital_elements.orbital_period.error.min"Amount of time the SSO takes to complete one orbitdtime.period.revolutionfloatindexednullable"orbital_elements.orbital_period.error.max"Amount of time the SSO takes to complete one orbitdtime.period.revolutionfloatindexednullable"orbital_elements.author"Name of the orbit computermeta.bib.authorcharnullable"orbital_elements.periapsis_distance.value"Nearest point of the orbit around the primary bodyaupos.distance;src.orbital;stat.minfloatindexednullable"orbital_elements.periapsis_distance.error.min"Nearest point of the orbit around the primary bodyaupos.distance;src.orbital;stat.minfloatindexednullable"orbital_elements.periapsis_distance.error.max"Nearest point of the orbit around the primary bodyaupos.distance;src.orbital;stat.minfloatindexednullable"orbital_elements.apoapsis_distance.value"Farthest point of the orbit around the primary bodyaupos.distance;src.orbital;stat.maxfloatindexednullable"orbital_elements.apoapsis_distance.error.min"Farthest point of the orbit around the primary bodyaupos.distance;src.orbital;stat.maxfloatindexednullable"orbital_elements.apoapsis_distance.error.max"Farthest point of the orbit around the primary bodyaupos.distance;src.orbital;stat.maxfloatindexednullable"proper_elements.proper_semi_major_axis.value"Proper semi-major axis of the orbitaupos.distance;src.orbitalfloatindexednullable"proper_elements.proper_semi_major_axis.error.min"Proper semi-major axis of the orbitaupos.distance;src.orbitalfloatindexednullable"proper_elements.proper_semi_major_axis.error.max"Proper semi-major axis of the orbitaupos.distance;src.orbitalfloatindexednullable"proper_elements.proper_eccentricity.value"Proper eccentricity of the orbitsrc.orbital.eccentricityfloatindexednullable"proper_elements.proper_eccentricity.error.min"Proper eccentricity of the orbitsrc.orbital.eccentricityfloatindexednullable"proper_elements.proper_eccentricity.error.max"Proper eccentricity of the orbitsrc.orbital.eccentricityfloatindexednullable"proper_elements.proper_inclination.value"Proper inclination of the orbitdegsrc.orbital.inclinationfloatindexednullable"proper_elements.proper_inclination.error.min"Proper inclination of the orbitdegsrc.orbital.inclinationfloatindexednullable"proper_elements.proper_inclination.error.max"Proper inclination of the orbitdegsrc.orbital.inclinationfloatindexednullable"proper_elements.proper_sine_inclination.value"Sine of proper inclination of the orbitfloatindexednullable"proper_elements.proper_sine_inclination.error.min"Sine of proper inclination of the orbitfloatindexednullable"proper_elements.proper_sine_inclination.error.max"Sine of proper inclination of the orbitfloatindexednullable"proper_elements.proper_frequency_mean_motion.value"Proper frequency of mean motion of the orbitdeg/yrsrc.orbital.meanMotion;arith.variationfloatnullable"proper_elements.proper_frequency_mean_motion.error.min"Proper frequency of mean motion of the orbitdeg/yrsrc.orbital.meanMotion;arith.variationfloatnullable"proper_elements.proper_frequency_mean_motion.error.max"Proper frequency of mean motion of the orbitdeg/yrsrc.orbital.meanMotion;arith.variationfloatnullable"proper_elements.proper_frequency_perihelion_longitude.value"Proper frequency of perihelion longitude of the orbitarcsec/yrsrc.orbital.periastron;arith.variationfloatnullable"proper_elements.proper_frequency_perihelion_longitude.error.min"Proper frequency of perihelion longitude of the orbitarcsec/yrsrc.orbital.periastron;arith.variationfloatnullable"proper_elements.proper_frequency_perihelion_longitude.error.max"Proper frequency of perihelion longitude of the orbitarcsec/yrsrc.orbital.periastron;arith.variationfloatnullable"proper_elements.proper_frequency_nodal_longitude.value"Proper frequency of the longitude of the ascending node of the orbitarcsec/yrsrc.orbital.node;arith.variationfloatnullable"proper_elements.proper_frequency_nodal_longitude.error.min"Proper frequency of the longitude of the ascending node of the orbitarcsec/yrsrc.orbital.node;arith.variationfloatnullable"proper_elements.proper_frequency_nodal_longitude.error.max"Proper frequency of the longitude of the ascending node of the orbitarcsec/yrsrc.orbital.node;arith.variationfloatnullable"proper_elements.lyapunov_time"Lyapunov timekyrstat.lyapunovfloatnullable"proper_elements.integration_time"Time span of the integration to compute the proper elementsMyrtime.intervalfloatnullable"tisserand_parameters.Jupiter.value"Tisserand parameter with respect to Jupitersrc.orbital.Tisserandfloatnullable"tisserand_parameters.Jupiter.error.min"Tisserand parameter with respect to Jupitersrc.orbital.Tisserandfloatnullable"tisserand_parameters.Jupiter.error.max"Tisserand parameter with respect to Jupitersrc.orbital.Tisserandfloatnullable"tisserand_parameters.Saturn.value"Tisserand parameter with respect to Saturnsrc.orbital.Tisserandfloatnullable"tisserand_parameters.Saturn.error.min"Tisserand parameter with respect to Saturnsrc.orbital.Tisserandfloatnullable"tisserand_parameters.Saturn.error.max"Tisserand parameter with respect to Saturnsrc.orbital.Tisserandfloatnullable"tisserand_parameters.Uranus.value"Tisserand parameter with respect to Uranussrc.orbital.Tisserandfloatnullable"tisserand_parameters.Uranus.error.min"Tisserand parameter with respect to Uranussrc.orbital.Tisserandfloatnullable"tisserand_parameters.Uranus.error.max"Tisserand parameter with respect to Uranussrc.orbital.Tisserandfloatnullable"tisserand_parameters.Neptune.value"Tisserand parameter with respect to Neptunesrc.orbital.Tisserandfloatnullable"tisserand_parameters.Neptune.error.min"Tisserand parameter with respect to Neptunesrc.orbital.Tisserandfloatnullable"tisserand_parameters.Neptune.error.max"Tisserand parameter with respect to Neptunesrc.orbital.Tisserandfloatnullable"family.family_number"IAU number of the family largest membermeta.idintindexednullable"family.family_name"Name of the family largest membermeta.id;meta.maincharindexednullable"family.family_status"Status within the family (member of the core, halo, or diffuse halo)meta.code.statuscharnullable"pair.sibling_number"IAU number of the sibling SSOmeta.idintindexednullable"pair.sibling_name"Name of the sibling SSOmeta.id;meta.maincharindexednullable"pair.distance"Distance between the orbits (SSO and sibling)m/spos.distance;src.orbitalfloatindexednullable"pair.age.value"Estimated age of the pairkyrtime.agefloatindexednullable"pair.age.error.min"Estimated age of the pairkyrtime.agefloatindexednullable"pair.age.error.max"Estimated age of the pairkyrtime.agefloatindexednullable"moid.Mercury.value"Minimum orbit intersection distance with respect to Mercuryausrc.orbital;stat.min;pos.distancefloatnullable"moid.Mercury.error.min"Minimum orbit intersection distance with respect to Mercuryausrc.orbital;stat.min;pos.distancefloatnullable"moid.Mercury.error.max"Minimum orbit intersection distance with respect to Mercuryausrc.orbital;stat.min;pos.distancefloatnullable"moid.Venus.value"Minimum orbit intersection distance with respect to Venusausrc.orbital;stat.min;pos.distancefloatnullable"moid.Venus.error.min"Minimum orbit intersection distance with respect to Venusausrc.orbital;stat.min;pos.distancefloatnullable"moid.Venus.error.max"Minimum orbit intersection distance with respect to Venusausrc.orbital;stat.min;pos.distancefloatnullable"moid.EMB.value"Minimum orbit intersection distance with respect to Earth-Moon barycenterausrc.orbital;stat.min;pos.distancefloatnullable"moid.EMB.error.min"Minimum orbit intersection distance with respect to Earth-Moon barycenterausrc.orbital;stat.min;pos.distancefloatnullable"moid.EMB.error.max"Minimum orbit intersection distance with respect to Earth-Moon barycenterausrc.orbital;stat.min;pos.distancefloatnullable"moid.Mars.value"Minimum orbit intersection distance with respect to Marsausrc.orbital;stat.min;pos.distancefloatnullable"moid.Mars.error.min"Minimum orbit intersection distance with respect to Marsausrc.orbital;stat.min;pos.distancefloatnullable"moid.Mars.error.max"Minimum orbit intersection distance with respect to Marsausrc.orbital;stat.min;pos.distancefloatnullable"moid.Jupiter.value"Minimum orbit intersection distance with respect to Jupiterausrc.orbital;stat.min;pos.distancefloatnullable"moid.Jupiter.error.min"Minimum orbit intersection distance with respect to Jupiterausrc.orbital;stat.min;pos.distancefloatnullable"moid.Jupiter.error.max"Minimum orbit intersection distance with respect to Jupiterausrc.orbital;stat.min;pos.distancefloatnullable"moid.Saturn.value"Minimum orbit intersection distance with respect to Saturnausrc.orbital;stat.min;pos.distancefloatnullable"moid.Saturn.error.min"Minimum orbit intersection distance with respect to Saturnausrc.orbital;stat.min;pos.distancefloatnullable"moid.Saturn.error.max"Minimum orbit intersection distance with respect to Saturnausrc.orbital;stat.min;pos.distancefloatnullable"moid.Uranus.value"Minimum orbit intersection distance with respect to Uranusausrc.orbital;stat.min;pos.distancefloatnullable"moid.Uranus.error.min"Minimum orbit intersection distance with respect to Uranusausrc.orbital;stat.min;pos.distancefloatnullable"moid.Uranus.error.max"Minimum orbit intersection distance with respect to Uranusausrc.orbital;stat.min;pos.distancefloatnullable"moid.Neptune.value"Minimum orbit intersection distance with respect to Neptuneausrc.orbital;stat.min;pos.distancefloatnullable"moid.Neptune.error.min"Minimum orbit intersection distance with respect to Neptuneausrc.orbital;stat.min;pos.distancefloatnullable"moid.Neptune.error.max"Minimum orbit intersection distance with respect to Neptuneausrc.orbital;stat.min;pos.distancefloatnullable"source_regions.hun.value"Probability that the SSO is derived from Hungaria populationstat.probabilityfloatindexednullable"source_regions.hun.error.min"Probability that the SSO is derived from Hungaria populationstat.probabilityfloatindexednullable"source_regions.hun.error.max"Probability that the SSO is derived from Hungaria populationstat.probabilityfloatindexednullable"source_regions.nu6.value"Probability that the SSO is derived from the ν_6 secular resonance with Saturnstat.probabilityfloatindexednullable"source_regions.nu6.error.min"Probability that the SSO is derived from the ν_6 secular resonance with Saturnstat.probabilityfloatindexednullable"source_regions.nu6.error.max"Probability that the SSO is derived from the ν_6 secular resonance with Saturnstat.probabilityfloatindexednullable"source_regions.pho.value"Probability that the SSO is derived from Phocaea populationstat.probabilityfloatindexednullable"source_regions.pho.error.min"Probability that the SSO is derived from Phocaea populationstat.probabilityfloatindexednullable"source_regions.pho.error.max"Probability that the SSO is derived from Phocaea populationstat.probabilityfloatindexednullable"source_regions.mm31.value"Probability that the SSO is derived from the 3:1 mean motion resonancestat.probabilityfloatindexednullable"source_regions.mm31.error.min"Probability that the SSO is derived from the 3:1 mean motion resonancestat.probabilityfloatindexednullable"source_regions.mm31.error.max"Probability that the SSO is derived from the 3:1 mean motion resonancestat.probabilityfloatindexednullable"source_regions.mm52.value"Probability that the SSO is derived from the 5:2 mean motion resonancestat.probabilityfloatindexednullable"source_regions.mm52.error.min"Probability that the SSO is derived from the 5:2 mean motion resonancestat.probabilityfloatindexednullable"source_regions.mm52.error.max"Probability that the SSO is derived from the 5:2 mean motion resonancestat.probabilityfloatindexednullable"source_regions.mm21.value"Probability that the SSO is derived from the 2:1 mean motion resonancestat.probabilityfloatindexednullable"source_regions.mm21.error.min"Probability that the SSO is derived from the 2:1 mean motion resonancestat.probabilityfloatindexednullable"source_regions.mm21.error.max"Probability that the SSO is derived from the 2:1 mean motion resonancestat.probabilityfloatindexednullable"source_regions.jfc.value"Probability that the SSO is derived from the Jupiter Family Comet regionstat.probabilityfloatindexednullable"source_regions.jfc.error.min"Probability that the SSO is derived from the Jupiter Family Comet regionstat.probabilityfloatindexednullable"source_regions.jfc.error.max"Probability that the SSO is derived from the Jupiter Family Comet regionstat.probabilityfloatindexednullable"delta_v.delta_v"Best total velocity range to rendezvous with targetkm/sphys.velocfloatindexednullable"delta_v.transfer_time"Best flight time to rendezvous with targetdtime.durationfloatindexednullable"delta_v.n_burns"Number of burns corresponding to the best Delta-Vmeta.idintindexednullable"yarkovsky.dadt.value"Semi-major axis drift induced by the Yarkovsky effect1e-4au/Myrarith.rate;pos.distance;src.orbitalfloatindexednullable"yarkovsky.dadt.error.min"Semi-major axis drift induced by the Yarkovsky effect1e-4au/Myrarith.rate;pos.distance;src.orbitalfloatindexednullable"yarkovsky.dadt.error.max"Semi-major axis drift induced by the Yarkovsky effect1e-4au/Myrarith.rate;pos.distance;src.orbitalfloatindexednullable"yarkovsky.A2.value"Radial acceleration induced by the Yarkovsky effect1e-15au/d**2phys.accelerationfloatnullable"yarkovsky.A2.error.min"Radial acceleration induced by the Yarkovsky effect1e-15au/d**2phys.accelerationfloatnullable"yarkovsky.A2.error.max"Radial acceleration induced by the Yarkovsky effect1e-15au/d**2phys.accelerationfloatnullable"yarkovsky.snr"Signal-to-noise ratio of Yarkovsky detectionstat.snrfloatnullable"yarkovsky.S"Yarkovsky sensitivity parameterstat.paramfloatnullable"absolute_magnitude.value"Absolute magnitude of the SSOmagphys.magAbsfloatindexednullable"absolute_magnitude.error.min"Absolute magnitude of the SSOmagphys.magAbsfloatindexednullable"absolute_magnitude.error.max"Absolute magnitude of the SSOmagphys.magAbsfloatindexednullable"diameter.value"Volume-equivalent diameterkmphys.size.diameterfloatindexednullable"diameter.error.min"Volume-equivalent diameterkmphys.size.diameterfloatindexednullable"diameter.error.max"Volume-equivalent diameterkmphys.size.diameterfloatindexednullable"diameter.ratio.value"Volume-equivalent diameterkmphys.size.diameterfloatnullable"diameter.ratio.error.min"Volume-equivalent diameterkmphys.size.diameterfloatnullable"diameter.ratio.error.max"Volume-equivalent diameterkmphys.size.diameterfloatnullable"diameter.reference.value"Volume-equivalent diameterkmphys.size.diameterfloatnullable"diameter.reference.error.min"Volume-equivalent diameterkmphys.size.diameterfloatnullable"diameter.reference.error.max"Volume-equivalent diameterkmphys.size.diameterfloatnullable"albedo.value"Geometrical albedo in V bandphys.albedofloatindexednullable"albedo.error.min"Geometrical albedo in V bandphys.albedofloatindexednullable"albedo.error.max"Geometrical albedo in V bandphys.albedofloatindexednullable"albedo.type"Type of albedometa.note;phys.albedocharnullable"mass.value"Mass of the SSOkgphys.massfloatindexednullable"mass.error.min"Mass of the SSOkgphys.massfloatindexednullable"mass.error.max"Mass of the SSOkgphys.massfloatindexednullable"mass.ratio.value"Mass of the SSOkgphys.massfloatnullable"mass.ratio.error.min"Mass of the SSOkgphys.massfloatnullable"mass.ratio.error.max"Mass of the SSOkgphys.massfloatnullable"density.value"Volumetric mass densitykg/m**3phys.densityfloatindexednullable"density.error.min"Volumetric mass densitykg/m**3phys.densityfloatindexednullable"density.error.max"Volumetric mass densitykg/m**3phys.densityfloatindexednullable"hill_sphere_radius.value"Radius of the gravitational sphere of influence of the SSOauphys.size.radiusfloatindexednullable"hill_sphere_radius.error.min"Radius of the gravitational sphere of influence of the SSOauphys.size.radiusfloatindexednullable"hill_sphere_radius.error.max"Radius of the gravitational sphere of influence of the SSOauphys.size.radiusfloatindexednullable"taxonomy.class"Taxonomic classsrc.class.colorcharindexednullable"taxonomy.complex"Taxonomic complexsrc.class.colorcharindexednullable"taxonomy.waverange"Wavelength range used for the taxonomic classificationcharindexednullable"taxonomy.scheme"Taxonomic classification schemecharindexednullable"taxonomy.technique"Method used to determine the taxonomycharnullable"thermal_inertia.value"Equivalent thermal inertia at 1 auJ.s**(-1/2).K**-1.m**-2phys.thermalInertiafloatindexednullable"thermal_inertia.error.min"Equivalent thermal inertia at 1 auJ.s**(-1/2).K**-1.m**-2phys.thermalInertiafloatindexednullable"thermal_inertia.error.max"Equivalent thermal inertia at 1 auJ.s**(-1/2).K**-1.m**-2phys.thermalInertiafloatindexednullable"colors.g-i.color.value"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.g-i.color.error.min"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.g-i.color.error.max"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.g-i.facility"Observing facility that provided the observationsmeta.id;instr.obstycharnullable"colors.g-i.observer"IAU code of the observermeta.id;instr.obstycharnullable"colors.g-i.epoch"Julian date of the observationdtime.epochfloatnullable"colors.g-i.delta_time"Time difference between the acquisition time of the two filtersstime.durationfloatnullable"colors.g-i.id_filter_1"Unique identifier of the first filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.g-i.id_filter_2"Unique identifier of the second filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.g-i.phot_sys"Reference photometric system (Vega, AB, or ST)charnullable"colors.g-i.technique"Method used to determine the colorcharnullable"colors.g-r.color.value"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.g-r.color.error.min"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.g-r.color.error.max"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.g-r.facility"Observing facility that provided the observationsmeta.id;instr.obstycharnullable"colors.g-r.observer"IAU code of the observermeta.id;instr.obstycharnullable"colors.g-r.epoch"Julian date of the observationdtime.epochfloatnullable"colors.g-r.delta_time"Time difference between the acquisition time of the two filtersstime.durationfloatnullable"colors.g-r.id_filter_1"Unique identifier of the first filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.g-r.id_filter_2"Unique identifier of the second filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.g-r.phot_sys"Reference photometric system (Vega, AB, or ST)charnullable"colors.g-r.technique"Method used to determine the colorcharnullable"colors.g-z.color.value"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.g-z.color.error.min"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.g-z.color.error.max"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.g-z.facility"Observing facility that provided the observationsmeta.id;instr.obstycharnullable"colors.g-z.observer"IAU code of the observermeta.id;instr.obstycharnullable"colors.g-z.epoch"Julian date of the observationdtime.epochfloatnullable"colors.g-z.delta_time"Time difference between the acquisition time of the two filtersstime.durationfloatnullable"colors.g-z.id_filter_1"Unique identifier of the first filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.g-z.id_filter_2"Unique identifier of the second filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.g-z.phot_sys"Reference photometric system (Vega, AB, or ST)charnullable"colors.g-z.technique"Method used to determine the colorcharnullable"colors.i-z.color.value"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.i-z.color.error.min"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.i-z.color.error.max"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.i-z.facility"Observing facility that provided the observationsmeta.id;instr.obstycharnullable"colors.i-z.observer"IAU code of the observermeta.id;instr.obstycharnullable"colors.i-z.epoch"Julian date of the observationdtime.epochfloatnullable"colors.i-z.delta_time"Time difference between the acquisition time of the two filtersstime.durationfloatnullable"colors.i-z.id_filter_1"Unique identifier of the first filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.i-z.id_filter_2"Unique identifier of the second filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.i-z.phot_sys"Reference photometric system (Vega, AB, or ST)charnullable"colors.i-z.technique"Method used to determine the colorcharnullable"colors.r-i.color.value"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.r-i.color.error.min"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.r-i.color.error.max"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.r-i.facility"Observing facility that provided the observationsmeta.id;instr.obstycharnullable"colors.r-i.observer"IAU code of the observermeta.id;instr.obstycharnullable"colors.r-i.epoch"Julian date of the observationdtime.epochfloatnullable"colors.r-i.delta_time"Time difference between the acquisition time of the two filtersstime.durationfloatnullable"colors.r-i.id_filter_1"Unique identifier of the first filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.r-i.id_filter_2"Unique identifier of the second filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.r-i.phot_sys"Reference photometric system (Vega, AB, or ST)charnullable"colors.r-i.technique"Method used to determine the colorcharnullable"colors.r-z.color.value"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.r-z.color.error.min"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.r-z.color.error.max"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.r-z.facility"Observing facility that provided the observationsmeta.id;instr.obstycharnullable"colors.r-z.observer"IAU code of the observermeta.id;instr.obstycharnullable"colors.r-z.epoch"Julian date of the observationdtime.epochfloatnullable"colors.r-z.delta_time"Time difference between the acquisition time of the two filtersstime.durationfloatnullable"colors.r-z.id_filter_1"Unique identifier of the first filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.r-z.id_filter_2"Unique identifier of the second filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.r-z.phot_sys"Reference photometric system (Vega, AB, or ST)charnullable"colors.r-z.technique"Method used to determine the colorcharnullable"colors.u-g.color.value"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.u-g.color.error.min"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.u-g.color.error.max"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.u-g.facility"Observing facility that provided the observationsmeta.id;instr.obstycharnullable"colors.u-g.observer"IAU code of the observermeta.id;instr.obstycharnullable"colors.u-g.epoch"Julian date of the observationdtime.epochfloatnullable"colors.u-g.delta_time"Time difference between the acquisition time of the two filtersstime.durationfloatnullable"colors.u-g.id_filter_1"Unique identifier of the first filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.u-g.id_filter_2"Unique identifier of the second filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.u-g.phot_sys"Reference photometric system (Vega, AB, or ST)charnullable"colors.u-g.technique"Method used to determine the colorcharnullable"colors.u-i.color.value"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.u-i.color.error.min"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.u-i.color.error.max"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.u-i.facility"Observing facility that provided the observationsmeta.id;instr.obstycharnullable"colors.u-i.observer"IAU code of the observermeta.id;instr.obstycharnullable"colors.u-i.epoch"Julian date of the observationdtime.epochfloatnullable"colors.u-i.delta_time"Time difference between the acquisition time of the two filtersstime.durationfloatnullable"colors.u-i.id_filter_1"Unique identifier of the first filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.u-i.id_filter_2"Unique identifier of the second filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.u-i.phot_sys"Reference photometric system (Vega, AB, or ST)charnullable"colors.u-i.technique"Method used to determine the colorcharnullable"colors.u-r.color.value"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.u-r.color.error.min"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.u-r.color.error.max"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.u-r.facility"Observing facility that provided the observationsmeta.id;instr.obstycharnullable"colors.u-r.observer"IAU code of the observermeta.id;instr.obstycharnullable"colors.u-r.epoch"Julian date of the observationdtime.epochfloatnullable"colors.u-r.delta_time"Time difference between the acquisition time of the two filtersstime.durationfloatnullable"colors.u-r.id_filter_1"Unique identifier of the first filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.u-r.id_filter_2"Unique identifier of the second filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.u-r.phot_sys"Reference photometric system (Vega, AB, or ST)charnullable"colors.u-r.technique"Method used to determine the colorcharnullable"colors.J-K.color.value"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.J-K.color.error.min"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.J-K.color.error.max"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.J-K.facility"Observing facility that provided the observationsmeta.id;instr.obstycharnullable"colors.J-K.observer"IAU code of the observermeta.id;instr.obstycharnullable"colors.J-K.epoch"Julian date of the observationdtime.epochfloatnullable"colors.J-K.delta_time"Time difference between the acquisition time of the two filtersstime.durationfloatnullable"colors.J-K.id_filter_1"Unique identifier of the first filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.J-K.id_filter_2"Unique identifier of the second filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.J-K.phot_sys"Reference photometric system (Vega, AB, or ST)charnullable"colors.J-K.technique"Method used to determine the colorcharnullable"colors.J-Ks.color.value"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.J-Ks.color.error.min"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.J-Ks.color.error.max"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.J-Ks.facility"Observing facility that provided the observationsmeta.id;instr.obstycharnullable"colors.J-Ks.observer"IAU code of the observermeta.id;instr.obstycharnullable"colors.J-Ks.epoch"Julian date of the observationdtime.epochfloatnullable"colors.J-Ks.delta_time"Time difference between the acquisition time of the two filtersstime.durationfloatnullable"colors.J-Ks.id_filter_1"Unique identifier of the first filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.J-Ks.id_filter_2"Unique identifier of the second filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.J-Ks.phot_sys"Reference photometric system (Vega, AB, or ST)charnullable"colors.J-Ks.technique"Method used to determine the colorcharnullable"colors.Y-J.color.value"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.Y-J.color.error.min"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.Y-J.color.error.max"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.Y-J.facility"Observing facility that provided the observationsmeta.id;instr.obstycharnullable"colors.Y-J.observer"IAU code of the observermeta.id;instr.obstycharnullable"colors.Y-J.epoch"Julian date of the observationdtime.epochfloatnullable"colors.Y-J.delta_time"Time difference between the acquisition time of the two filtersstime.durationfloatnullable"colors.Y-J.id_filter_1"Unique identifier of the first filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.Y-J.id_filter_2"Unique identifier of the second filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.Y-J.phot_sys"Reference photometric system (Vega, AB, or ST)charnullable"colors.Y-J.technique"Method used to determine the colorcharnullable"colors.Y-K.color.value"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.Y-K.color.error.min"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.Y-K.color.error.max"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.Y-K.facility"Observing facility that provided the observationsmeta.id;instr.obstycharnullable"colors.Y-K.observer"IAU code of the observermeta.id;instr.obstycharnullable"colors.Y-K.epoch"Julian date of the observationdtime.epochfloatnullable"colors.Y-K.delta_time"Time difference between the acquisition time of the two filtersstime.durationfloatnullable"colors.Y-K.id_filter_1"Unique identifier of the first filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.Y-K.id_filter_2"Unique identifier of the second filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.Y-K.phot_sys"Reference photometric system (Vega, AB, or ST)charnullable"colors.Y-K.technique"Method used to determine the colorcharnullable"colors.Y-Ks.color.value"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.Y-Ks.color.error.min"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.Y-Ks.color.error.max"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.Y-Ks.facility"Observing facility that provided the observationsmeta.id;instr.obstycharnullable"colors.Y-Ks.observer"IAU code of the observermeta.id;instr.obstycharnullable"colors.Y-Ks.epoch"Julian date of the observationdtime.epochfloatnullable"colors.Y-Ks.delta_time"Time difference between the acquisition time of the two filtersstime.durationfloatnullable"colors.Y-Ks.id_filter_1"Unique identifier of the first filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.Y-Ks.id_filter_2"Unique identifier of the second filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.Y-Ks.phot_sys"Reference photometric system (Vega, AB, or ST)charnullable"colors.Y-Ks.technique"Method used to determine the colorcharnullable"colors.c-o.color.value"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.c-o.color.error.min"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.c-o.color.error.max"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.c-o.facility"Observing facility that provided the observationsmeta.id;instr.obstycharnullable"colors.c-o.observer"IAU code of the observermeta.id;instr.obstycharnullable"colors.c-o.epoch"Julian date of the observationdtime.epochfloatnullable"colors.c-o.delta_time"Time difference between the acquisition time of the two filtersstime.durationfloatnullable"colors.c-o.id_filter_1"Unique identifier of the first filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.c-o.id_filter_2"Unique identifier of the second filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.c-o.phot_sys"Reference photometric system (Vega, AB, or ST)charnullable"colors.c-o.technique"Method used to determine the colorcharnullable"colors.u-z.color.value"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.u-z.color.error.min"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.u-z.color.error.max"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.u-z.facility"Observing facility that provided the observationsmeta.id;instr.obstycharnullable"colors.u-z.observer"IAU code of the observermeta.id;instr.obstycharnullable"colors.u-z.epoch"Julian date of the observationdtime.epochfloatnullable"colors.u-z.delta_time"Time difference between the acquisition time of the two filtersstime.durationfloatnullable"colors.u-z.id_filter_1"Unique identifier of the first filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.u-z.id_filter_2"Unique identifier of the second filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.u-z.phot_sys"Reference photometric system (Vega, AB, or ST)charnullable"colors.u-z.technique"Method used to determine the colorcharnullable"colors.v-g.color.value"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.v-g.color.error.min"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.v-g.color.error.max"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.v-g.facility"Observing facility that provided the observationsmeta.id;instr.obstycharnullable"colors.v-g.observer"IAU code of the observermeta.id;instr.obstycharnullable"colors.v-g.epoch"Julian date of the observationdtime.epochfloatnullable"colors.v-g.delta_time"Time difference between the acquisition time of the two filtersstime.durationfloatnullable"colors.v-g.id_filter_1"Unique identifier of the first filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.v-g.id_filter_2"Unique identifier of the second filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.v-g.phot_sys"Reference photometric system (Vega, AB, or ST)charnullable"colors.v-g.technique"Method used to determine the colorcharnullable"colors.v-i.color.value"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.v-i.color.error.min"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.v-i.color.error.max"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.v-i.facility"Observing facility that provided the observationsmeta.id;instr.obstycharnullable"colors.v-i.observer"IAU code of the observermeta.id;instr.obstycharnullable"colors.v-i.epoch"Julian date of the observationdtime.epochfloatnullable"colors.v-i.delta_time"Time difference between the acquisition time of the two filtersstime.durationfloatnullable"colors.v-i.id_filter_1"Unique identifier of the first filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.v-i.id_filter_2"Unique identifier of the second filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.v-i.phot_sys"Reference photometric system (Vega, AB, or ST)charnullable"colors.v-i.technique"Method used to determine the colorcharnullable"colors.v-r.color.value"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.v-r.color.error.min"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.v-r.color.error.max"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.v-r.facility"Observing facility that provided the observationsmeta.id;instr.obstycharnullable"colors.v-r.observer"IAU code of the observermeta.id;instr.obstycharnullable"colors.v-r.epoch"Julian date of the observationdtime.epochfloatnullable"colors.v-r.delta_time"Time difference between the acquisition time of the two filtersstime.durationfloatnullable"colors.v-r.id_filter_1"Unique identifier of the first filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.v-r.id_filter_2"Unique identifier of the second filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.v-r.phot_sys"Reference photometric system (Vega, AB, or ST)charnullable"colors.v-r.technique"Method used to determine the colorcharnullable"colors.v-z.color.value"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.v-z.color.error.min"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.v-z.color.error.max"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.v-z.facility"Observing facility that provided the observationsmeta.id;instr.obstycharnullable"colors.v-z.observer"IAU code of the observermeta.id;instr.obstycharnullable"colors.v-z.epoch"Julian date of the observationdtime.epochfloatnullable"colors.v-z.delta_time"Time difference between the acquisition time of the two filtersstime.durationfloatnullable"colors.v-z.id_filter_1"Unique identifier of the first filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.v-z.id_filter_2"Unique identifier of the second filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.v-z.phot_sys"Reference photometric system (Vega, AB, or ST)charnullable"colors.v-z.technique"Method used to determine the colorcharnullable"colors.H-K.color.value"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.H-K.color.error.min"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.H-K.color.error.max"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.H-K.facility"Observing facility that provided the observationsmeta.id;instr.obstycharnullable"colors.H-K.observer"IAU code of the observermeta.id;instr.obstycharnullable"colors.H-K.epoch"Julian date of the observationdtime.epochfloatnullable"colors.H-K.delta_time"Time difference between the acquisition time of the two filtersstime.durationfloatnullable"colors.H-K.id_filter_1"Unique identifier of the first filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.H-K.id_filter_2"Unique identifier of the second filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.H-K.phot_sys"Reference photometric system (Vega, AB, or ST)charnullable"colors.H-K.technique"Method used to determine the colorcharnullable"colors.H-Ks.color.value"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.H-Ks.color.error.min"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.H-Ks.color.error.max"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.H-Ks.facility"Observing facility that provided the observationsmeta.id;instr.obstycharnullable"colors.H-Ks.observer"IAU code of the observermeta.id;instr.obstycharnullable"colors.H-Ks.epoch"Julian date of the observationdtime.epochfloatnullable"colors.H-Ks.delta_time"Time difference between the acquisition time of the two filtersstime.durationfloatnullable"colors.H-Ks.id_filter_1"Unique identifier of the first filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.H-Ks.id_filter_2"Unique identifier of the second filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.H-Ks.phot_sys"Reference photometric system (Vega, AB, or ST)charnullable"colors.H-Ks.technique"Method used to determine the colorcharnullable"colors.J-H.color.value"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.J-H.color.error.min"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.J-H.color.error.max"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.J-H.facility"Observing facility that provided the observationsmeta.id;instr.obstycharnullable"colors.J-H.observer"IAU code of the observermeta.id;instr.obstycharnullable"colors.J-H.epoch"Julian date of the observationdtime.epochfloatnullable"colors.J-H.delta_time"Time difference between the acquisition time of the two filtersstime.durationfloatnullable"colors.J-H.id_filter_1"Unique identifier of the first filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.J-H.id_filter_2"Unique identifier of the second filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.J-H.phot_sys"Reference photometric system (Vega, AB, or ST)charnullable"colors.J-H.technique"Method used to determine the colorcharnullable"colors.Y-H.color.value"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.Y-H.color.error.min"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.Y-H.color.error.max"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.Y-H.facility"Observing facility that provided the observationsmeta.id;instr.obstycharnullable"colors.Y-H.observer"IAU code of the observermeta.id;instr.obstycharnullable"colors.Y-H.epoch"Julian date of the observationdtime.epochfloatnullable"colors.Y-H.delta_time"Time difference between the acquisition time of the two filtersstime.durationfloatnullable"colors.Y-H.id_filter_1"Unique identifier of the first filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.Y-H.id_filter_2"Unique identifier of the second filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.Y-H.phot_sys"Reference photometric system (Vega, AB, or ST)charnullable"colors.Y-H.technique"Method used to determine the colorcharnullable"colors.u-v.color.value"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.u-v.color.error.min"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.u-v.color.error.max"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.u-v.facility"Observing facility that provided the observationsmeta.id;instr.obstycharnullable"colors.u-v.observer"IAU code of the observermeta.id;instr.obstycharnullable"colors.u-v.epoch"Julian date of the observationdtime.epochfloatnullable"colors.u-v.delta_time"Time difference between the acquisition time of the two filtersstime.durationfloatnullable"colors.u-v.id_filter_1"Unique identifier of the first filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.u-v.id_filter_2"Unique identifier of the second filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.u-v.phot_sys"Reference photometric system (Vega, AB, or ST)charnullable"colors.u-v.technique"Method used to determine the colorcharnullable"colors.V-I.color.value"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.V-I.color.error.min"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.V-I.color.error.max"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.V-I.facility"Observing facility that provided the observationsmeta.id;instr.obstycharnullable"colors.V-I.observer"IAU code of the observermeta.id;instr.obstycharnullable"colors.V-I.epoch"Julian date of the observationdtime.epochfloatnullable"colors.V-I.delta_time"Time difference between the acquisition time of the two filtersstime.durationfloatnullable"colors.V-I.id_filter_1"Unique identifier of the first filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.V-I.id_filter_2"Unique identifier of the second filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.V-I.phot_sys"Reference photometric system (Vega, AB, or ST)charnullable"colors.V-I.technique"Method used to determine the colorcharnullable"colors.V-R.color.value"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.V-R.color.error.min"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.V-R.color.error.max"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.V-R.facility"Observing facility that provided the observationsmeta.id;instr.obstycharnullable"colors.V-R.observer"IAU code of the observermeta.id;instr.obstycharnullable"colors.V-R.epoch"Julian date of the observationdtime.epochfloatnullable"colors.V-R.delta_time"Time difference between the acquisition time of the two filtersstime.durationfloatnullable"colors.V-R.id_filter_1"Unique identifier of the first filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.V-R.id_filter_2"Unique identifier of the second filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.V-R.phot_sys"Reference photometric system (Vega, AB, or ST)charnullable"colors.V-R.technique"Method used to determine the colorcharnullable"colors.B-V.color.value"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.B-V.color.error.min"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.B-V.color.error.max"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.B-V.facility"Observing facility that provided the observationsmeta.id;instr.obstycharnullable"colors.B-V.observer"IAU code of the observermeta.id;instr.obstycharnullable"colors.B-V.epoch"Julian date of the observationdtime.epochfloatnullable"colors.B-V.delta_time"Time difference between the acquisition time of the two filtersstime.durationfloatnullable"colors.B-V.id_filter_1"Unique identifier of the first filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.B-V.id_filter_2"Unique identifier of the second filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.B-V.phot_sys"Reference photometric system (Vega, AB, or ST)charnullable"colors.B-V.technique"Method used to determine the colorcharnullable"colors.R-I.color.value"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.R-I.color.error.min"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.R-I.color.error.max"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.R-I.facility"Observing facility that provided the observationsmeta.id;instr.obstycharnullable"colors.R-I.observer"IAU code of the observermeta.id;instr.obstycharnullable"colors.R-I.epoch"Julian date of the observationdtime.epochfloatnullable"colors.R-I.delta_time"Time difference between the acquisition time of the two filtersstime.durationfloatnullable"colors.R-I.id_filter_1"Unique identifier of the first filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.R-I.id_filter_2"Unique identifier of the second filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.R-I.phot_sys"Reference photometric system (Vega, AB, or ST)charnullable"colors.R-I.technique"Method used to determine the colorcharnullable"colors.B-R.color.value"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.B-R.color.error.min"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.B-R.color.error.max"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.B-R.facility"Observing facility that provided the observationsmeta.id;instr.obstycharnullable"colors.B-R.observer"IAU code of the observermeta.id;instr.obstycharnullable"colors.B-R.epoch"Julian date of the observationdtime.epochfloatnullable"colors.B-R.delta_time"Time difference between the acquisition time of the two filtersstime.durationfloatnullable"colors.B-R.id_filter_1"Unique identifier of the first filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.B-R.id_filter_2"Unique identifier of the second filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.B-R.phot_sys"Reference photometric system (Vega, AB, or ST)charnullable"colors.B-R.technique"Method used to determine the colorcharnullable"colors.V-Z.color.value"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.V-Z.color.error.min"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.V-Z.color.error.max"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.V-Z.facility"Observing facility that provided the observationsmeta.id;instr.obstycharnullable"colors.V-Z.observer"IAU code of the observermeta.id;instr.obstycharnullable"colors.V-Z.epoch"Julian date of the observationdtime.epochfloatnullable"colors.V-Z.delta_time"Time difference between the acquisition time of the two filtersstime.durationfloatnullable"colors.V-Z.id_filter_1"Unique identifier of the first filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.V-Z.id_filter_2"Unique identifier of the second filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.V-Z.phot_sys"Reference photometric system (Vega, AB, or ST)charnullable"colors.V-Z.technique"Method used to determine the colorcharnullable"colors.Z-J.color.value"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.Z-J.color.error.min"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.Z-J.color.error.max"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.Z-J.facility"Observing facility that provided the observationsmeta.id;instr.obstycharnullable"colors.Z-J.observer"IAU code of the observermeta.id;instr.obstycharnullable"colors.Z-J.epoch"Julian date of the observationdtime.epochfloatnullable"colors.Z-J.delta_time"Time difference between the acquisition time of the two filtersstime.durationfloatnullable"colors.Z-J.id_filter_1"Unique identifier of the first filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.Z-J.id_filter_2"Unique identifier of the second filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.Z-J.phot_sys"Reference photometric system (Vega, AB, or ST)charnullable"colors.Z-J.technique"Method used to determine the colorcharnullable"colors.U-B.color.value"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.U-B.color.error.min"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.U-B.color.error.max"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.U-B.facility"Observing facility that provided the observationsmeta.id;instr.obstycharnullable"colors.U-B.observer"IAU code of the observermeta.id;instr.obstycharnullable"colors.U-B.epoch"Julian date of the observationdtime.epochfloatnullable"colors.U-B.delta_time"Time difference between the acquisition time of the two filtersstime.durationfloatnullable"colors.U-B.id_filter_1"Unique identifier of the first filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.U-B.id_filter_2"Unique identifier of the second filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.U-B.phot_sys"Reference photometric system (Vega, AB, or ST)charnullable"colors.U-B.technique"Method used to determine the colorcharnullable"colors.R-z.color.value"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.R-z.color.error.min"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.R-z.color.error.max"Difference in magnitude measured through two different filtersphot.colorfloatnullable"colors.R-z.facility"Observing facility that provided the observationsmeta.id;instr.obstycharnullable"colors.R-z.observer"IAU code of the observermeta.id;instr.obstycharnullable"colors.R-z.epoch"Julian date of the observationdtime.epochfloatnullable"colors.R-z.delta_time"Time difference between the acquisition time of the two filtersstime.durationfloatnullable"colors.R-z.id_filter_1"Unique identifier of the first filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.R-z.id_filter_2"Unique identifier of the second filter, see SVO filter servicemeta.id;instr.filtercharnullable"colors.R-z.phot_sys"Reference photometric system (Vega, AB, or ST)charnullable"colors.R-z.technique"Method used to determine the colorcharnullable"spins.1.period.value"Synodic or sidereal period of rotationhtime.period.rotationfloatnullable"spins.1.period.error.min"Synodic or sidereal period of rotationhtime.period.rotationfloatnullable"spins.1.period.error.max"Synodic or sidereal period of rotationhtime.period.rotationfloatnullable"spins.1.period_type"Type of the period of rotation (synodic or sidereal)meta.code;time.period.rotationcharnullable"spins.1.period_flag"Quality flag of the period of rotationmeta.codecharnullable"spins.1.t0"Reference epoch for the spin coordinatesdtime.epochfloatnullable"spins.1.W0"Rotational phase at reference epochdegtime.phasefloatnullable"spins.1.Wp"Rotational velocitydeg/dphys.veloc.rotatfloatnullable"spins.1.obliquity"Obliquity of the spin axisdegphys.obliquityfloatnullable"spins.1.RA0.value"Right ascension of the spin axis (EQJ2000)degpos.eq.rafloatnullable"spins.1.RA0.error.min"Right ascension of the spin axis (EQJ2000)degpos.eq.rafloatnullable"spins.1.RA0.error.max"Right ascension of the spin axis (EQJ2000)degpos.eq.rafloatnullable"spins.1.DEC0.value"Declination of the spin axis (EQJ2000)degpos.eq.decfloatnullable"spins.1.DEC0.error.min"Declination of the spin axis (EQJ2000)degpos.eq.decfloatnullable"spins.1.DEC0.error.max"Declination of the spin axis (EQJ2000)degpos.eq.decfloatnullable"spins.1.long.value"Longitude of the spin axis (ECJ2000)degpos.ecliptic.lonfloatnullable"spins.1.long.error.min"Longitude of the spin axis (ECJ2000)degpos.ecliptic.lonfloatnullable"spins.1.long.error.max"Longitude of the spin axis (ECJ2000)degpos.ecliptic.lonfloatnullable"spins.1.lat.value"Latitude of the spin axis (ECJ2000)degpos.ecliptic.latfloatnullable"spins.1.lat.error.min"Latitude of the spin axis (ECJ2000)degpos.ecliptic.latfloatnullable"spins.1.lat.error.max"Latitude of the spin axis (ECJ2000)degpos.ecliptic.latfloatnullable"spins.1.technique"Method used to determine the spincharnullable"spins.2.period.value"Synodic or sidereal period of rotationhtime.period.rotationfloatnullable"spins.2.period.error.min"Synodic or sidereal period of rotationhtime.period.rotationfloatnullable"spins.2.period.error.max"Synodic or sidereal period of rotationhtime.period.rotationfloatnullable"spins.2.period_type"Type of the period of rotation (synodic or sidereal)meta.code;time.period.rotationcharnullable"spins.2.period_flag"Quality flag of the period of rotationmeta.codecharnullable"spins.2.t0"Reference epoch for the spin coordinatesdtime.epochfloatnullable"spins.2.W0"Rotational phase at reference epochdegtime.phasefloatnullable"spins.2.Wp"Rotational velocitydeg/dphys.veloc.rotatfloatnullable"spins.2.obliquity"Obliquity of the spin axisdegphys.obliquityfloatnullable"spins.2.RA0.value"Right ascension of the spin axis (EQJ2000)degpos.eq.rafloatnullable"spins.2.RA0.error.min"Right ascension of the spin axis (EQJ2000)degpos.eq.rafloatnullable"spins.2.RA0.error.max"Right ascension of the spin axis (EQJ2000)degpos.eq.rafloatnullable"spins.2.DEC0.value"Declination of the spin axis (EQJ2000)degpos.eq.decfloatnullable"spins.2.DEC0.error.min"Declination of the spin axis (EQJ2000)degpos.eq.decfloatnullable"spins.2.DEC0.error.max"Declination of the spin axis (EQJ2000)degpos.eq.decfloatnullable"spins.2.long.value"Longitude of the spin axis (ECJ2000)degpos.ecliptic.lonfloatnullable"spins.2.long.error.min"Longitude of the spin axis (ECJ2000)degpos.ecliptic.lonfloatnullable"spins.2.long.error.max"Longitude of the spin axis (ECJ2000)degpos.ecliptic.lonfloatnullable"spins.2.lat.value"Latitude of the spin axis (ECJ2000)degpos.ecliptic.latfloatnullable"spins.2.lat.error.min"Latitude of the spin axis (ECJ2000)degpos.ecliptic.latfloatnullable"spins.2.lat.error.max"Latitude of the spin axis (ECJ2000)degpos.ecliptic.latfloatnullable"spins.2.technique"Method used to determine the spincharnullable"spins.3.period.value"Synodic or sidereal period of rotationhtime.period.rotationfloatnullable"spins.3.period.error.min"Synodic or sidereal period of rotationhtime.period.rotationfloatnullable"spins.3.period.error.max"Synodic or sidereal period of rotationhtime.period.rotationfloatnullable"spins.3.period_type"Type of the period of rotation (synodic or sidereal)meta.code;time.period.rotationcharnullable"spins.3.period_flag"Quality flag of the period of rotationmeta.codecharnullable"spins.3.t0"Reference epoch for the spin coordinatesdtime.epochfloatnullable"spins.3.W0"Rotational phase at reference epochdegtime.phasefloatnullable"spins.3.Wp"Rotational velocitydeg/dphys.veloc.rotatfloatnullable"spins.3.obliquity"Obliquity of the spin axisdegphys.obliquityfloatnullable"spins.3.RA0.value"Right ascension of the spin axis (EQJ2000)degpos.eq.rafloatnullable"spins.3.RA0.error.min"Right ascension of the spin axis (EQJ2000)degpos.eq.rafloatnullable"spins.3.RA0.error.max"Right ascension of the spin axis (EQJ2000)degpos.eq.rafloatnullable"spins.3.DEC0.value"Declination of the spin axis (EQJ2000)degpos.eq.decfloatnullable"spins.3.DEC0.error.min"Declination of the spin axis (EQJ2000)degpos.eq.decfloatnullable"spins.3.DEC0.error.max"Declination of the spin axis (EQJ2000)degpos.eq.decfloatnullable"spins.3.long.value"Longitude of the spin axis (ECJ2000)degpos.ecliptic.lonfloatnullable"spins.3.long.error.min"Longitude of the spin axis (ECJ2000)degpos.ecliptic.lonfloatnullable"spins.3.long.error.max"Longitude of the spin axis (ECJ2000)degpos.ecliptic.lonfloatnullable"spins.3.lat.value"Latitude of the spin axis (ECJ2000)degpos.ecliptic.latfloatnullable"spins.3.lat.error.min"Latitude of the spin axis (ECJ2000)degpos.ecliptic.latfloatnullable"spins.3.lat.error.max"Latitude of the spin axis (ECJ2000)degpos.ecliptic.latfloatnullable"spins.3.technique"Method used to determine the spincharnullable"spins.4.period.value"Synodic or sidereal period of rotationhtime.period.rotationfloatnullable"spins.4.period.error.min"Synodic or sidereal period of rotationhtime.period.rotationfloatnullable"spins.4.period.error.max"Synodic or sidereal period of rotationhtime.period.rotationfloatnullable"spins.4.period_type"Type of the period of rotation (synodic or sidereal)meta.code;time.period.rotationcharnullable"spins.4.period_flag"Quality flag of the period of rotationmeta.codecharnullable"spins.4.t0"Reference epoch for the spin coordinatesdtime.epochfloatnullable"spins.4.W0"Rotational phase at reference epochdegtime.phasefloatnullable"spins.4.Wp"Rotational velocitydeg/dphys.veloc.rotatfloatnullable"spins.4.obliquity"Obliquity of the spin axisdegphys.obliquityfloatnullable"spins.4.RA0.value"Right ascension of the spin axis (EQJ2000)degpos.eq.rafloatnullable"spins.4.RA0.error.min"Right ascension of the spin axis (EQJ2000)degpos.eq.rafloatnullable"spins.4.RA0.error.max"Right ascension of the spin axis (EQJ2000)degpos.eq.rafloatnullable"spins.4.DEC0.value"Declination of the spin axis (EQJ2000)degpos.eq.decfloatnullable"spins.4.DEC0.error.min"Declination of the spin axis (EQJ2000)degpos.eq.decfloatnullable"spins.4.DEC0.error.max"Declination of the spin axis (EQJ2000)degpos.eq.decfloatnullable"spins.4.long.value"Longitude of the spin axis (ECJ2000)degpos.ecliptic.lonfloatnullable"spins.4.long.error.min"Longitude of the spin axis (ECJ2000)degpos.ecliptic.lonfloatnullable"spins.4.long.error.max"Longitude of the spin axis (ECJ2000)degpos.ecliptic.lonfloatnullable"spins.4.lat.value"Latitude of the spin axis (ECJ2000)degpos.ecliptic.latfloatnullable"spins.4.lat.error.min"Latitude of the spin axis (ECJ2000)degpos.ecliptic.latfloatnullable"spins.4.lat.error.max"Latitude of the spin axis (ECJ2000)degpos.ecliptic.latfloatnullable"spins.4.technique"Method used to determine the spincharnullable