alerce_tap.lsst_ivo://x-unregistred/alerce_tap/multisurvey_lowercase/lsst_ss_detectionALeRCE (Automatic Learning for the Rapid Classification of Events)ALeRCE Teamhttps://tap.alerce.online/favicon.png2026-04-11T22:13:50ZALeRCE Team

Beauchef 851, Edificio Norte, piso 6. Santiago, Chile.

alerce.broker@gmail.comastronomy, objectssurveystransientstime-series Individual LSST detections associated with solar system objects, including observing geometry (phase angle, elongation, ranges), ephemeris predictions, ephemeris offsets (O-C residuals), and heliocentric/topocentric state vectors in ICRS coordinates.http://tap.alerce.online/tableinfo/alerce_tap.lsst_ss_detectionalerce_tap Multi-survey astronomical object catalog containing astrometric and statistical information from multiple surveys. This table provides aggregated properties for astronomical objects including position, detection statistics, and temporal coverage.alerce_tap.lsst_ss_detection Individual LSST detections associated with solar system objects, including observing geometry (phase angle, elongation, ranges), ephemeris predictions, ephemeris offsets (O-C residuals), and heliocentric/topocentric state vectors in ICRS coordinates.measurement_idUnique identifier of this DIA source observationmeta.idlongindexedprimaryssobjectidLSST solar system object identifiermeta.id;srclongindexedprimarydesignationUnpacked primary provisional designation for this solar system objectmeta.id;srccharnullableecllambdaEcliptic longitudedegpos.ecliptic.londoubleeclbetaEcliptic latitudedegpos.ecliptic.latdoublegallonGalactic longitudedegpos.galactic.londoublegallatGalactic latitudedegpos.galactic.latdoubleelongationSolar elongation, the angular separation of the object from the Sun on the celestial spheredegpos.angDistancefloatnullablephaseanglePhase angle, the angle between the Sun and observer as seen from the objectdegpos.phaseAngfloatnullabletoporangeTopocentric range, the distance from the observer to the objectAUphys.distancefloatnullabletoporangerateTopocentric range rate, the radial velocity of the object relative to the observerAU/dphys.velocfloatnullableheliorangeHeliocentric range, the distance from the Sun to the objectAUphys.distancefloatnullableheliorangerateHeliocentric range rate, the radial velocity of the object relative to the SunAU/dphys.velocfloatnullableephraPredicted ICRS right ascension computed from orbit propagation at observation timedegpos.eq.ra;meta.modelled;pos.ephemdoublenullableephdecPredicted ICRS declination computed from orbit propagation at observation timedegpos.eq.dec;meta.modelled;pos.ephemdoublenullableephvmagPredicted V-band magnitude computed from orbit propagation at observation timemagphot.mag;em.opt.V;meta.modelled;pos.ephemfloatnullableephratePredicted total angular rate of motion on the skyarcsec/hpos.pm;pos.ephemfloatnullableephrateraPredicted angular rate of motion along right ascensionarcsec/hpos.pm;pos.eq.ra;pos.ephemfloatnullableephratedecPredicted angular rate of motion along declinationarcsec/hpos.pm;pos.eq.dec;pos.ephemfloatnullableephoffsetTotal angular offset between observed and predicted position on the celestial spherearcsecpos.angDistance;stat.fit.omcfloatnullableephoffsetraAngular offset in right ascension between observed and predicted position (observed minus predicted)degpos.eq.ra;stat.fit.omcdoublenullableephoffsetdecAngular offset in declination between observed and predicted position (observed minus predicted)degpos.eq.dec;stat.fit.omcdoublenullableephoffsetalongtrackAngular offset along the direction of motion between observed and predicted positionarcsecpos.angDistance;stat.fit.omcfloatnullableephoffsetcrosstrackAngular offset perpendicular to the direction of motion between observed and predicted positionarcsecpos.angDistance;stat.fit.omcfloatnullablehelio_xHeliocentric X position component in ICRS reference frameAUpos.cartesian.x;pos.heliocentricfloatnullablehelio_yHeliocentric Y position component in ICRS reference frameAUpos.cartesian.y;pos.heliocentricfloatnullablehelio_zHeliocentric Z position component in ICRS reference frameAUpos.cartesian.z;pos.heliocentricfloatnullablehelio_vxHeliocentric velocity component along X axis in ICRS reference frameAU/dphys.veloc;pos.cartesian.x;pos.heliocentricfloatnullablehelio_vyHeliocentric velocity component along Y axis in ICRS reference frameAU/dphys.veloc;pos.cartesian.y;pos.heliocentricfloatnullablehelio_vzHeliocentric velocity component along Z axis in ICRS reference frameAU/dphys.veloc;pos.cartesian.z;pos.heliocentricfloatnullablehelio_vtotHeliocentric total velocity magnitudeAU/dphys.veloc;pos.heliocentricfloatnullabletopo_xTopocentric X position component in ICRS reference frame relative to the observerAUpos.cartesian.xfloatnullabletopo_yTopocentric Y position component in ICRS reference frame relative to the observerAUpos.cartesian.yfloatnullabletopo_zTopocentric Z position component in ICRS reference frame relative to the observerAUpos.cartesian.zfloatnullabletopo_vxTopocentric velocity component along X axis in ICRS reference frameAU/dphys.veloc;pos.cartesian.xfloatnullabletopo_vyTopocentric velocity component along Y axis in ICRS reference frameAU/dphys.veloc;pos.cartesian.yfloatnullabletopo_vzTopocentric velocity component along Z axis in ICRS reference frameAU/dphys.veloc;pos.cartesian.zfloatnullabletopo_vtotTopocentric total velocity magnitudeAU/dphys.velocfloatnullablediadistancerankRanking based on the distance between this DIA source and the predicted position of the solar system object, with 1 being the closest matchmeta.code.classintnullablecreated_dateDate record was createdtime.creationcharnullable