J/A+A/679/A60ivo://CDS.VizieR/J/A+A/679/A60doi:10.26093/cds/vizier.36790060CDSMarciniak A.Durech J.Choukroun A.Hanus J.Ogloza W.Szakats R.,Molnar L.Pal A.Monteiro F.Frappa E.Beisker W.Pavlov H.Moore J.,Adomaviciene R.Aikawa R.Andersson S.Antonini P.Argentin Y.,Asai A.Assoignon P.Barton J.Baruffetti P.Bath K.L.Behrend R.,Benedyktowicz L.Bernasconi L.Biguet G.Billiani M.Blazewicz D.,Boninsegna R.Borkowski M.Bosch J.Brazill S.Bronikowska M.Bruno A.,Butkiewicz-Bak M.Caron J.Casalnuovo G.Castellani J.J.Ceravolo P.,Conjat M.Delincak P.Delpau J.Demeautis C.Demirkol A.Drozdz M.,Duffard R.Durandet C.Eisfeldt D.Evangelista M.Fauvaud S.,Fauvaud M.Ferrais M.Filipek M.Fini P.Fukui K.Gahrken B.Geier S.,George T.Goffin B.Golonka J.Goto T.Grice J.Guhl K.Halir K.,Hanna W.Harman M.Hashimoto A.Hasubick W.Higgins D.Higuchi M.,Hirose T.Hirsch R.Hofschulz O.Horaguchi T.Horbowicz J.Ida M.,Ignacz B.Ishida M.Isobe K.Jehin E.Joachimczyk B.Jones A.Juan J.,Kaminski K.Kaminska M.K.Kankiewicz P.Kasebe H.Kattentidt B.,Kim D.-H.Kim M.-J.Kitazaki K.Klotz A.Komraus M.Konstanciak I.,Konyves - Toth R.Kouno K.Kowald E.Krajewski J.Krannich G.,Kreutzer A.Kryszczynska A.Kubanek J.Kudak V.Kugel F.Kukita R.,Kulczak P.Lazzaro D.Licandro J.Livet F.Maley P.Manago N.,Manek J.Manna A.Matsushita H.Meister S.Mesquita W.Messner S.,Michelet J.Michimani J.Mieczkowska I.Morales N.Motylinski M.,Murawiecka M.Newman J.Nikitin V.Nishimura M.Oey J.Oszkiewicz D.,Owada M.Pakstiene E.Pawlowski M.Pereira W.Perig V.Perla J.,Pilcher F.Podlewska-Gaca E.Polak J.Polakis T.Polinska M.,Popowicz A.Richard F.Rives J.J.Rodrigues T.Roginski L.Rondon E.,Rottenborn M.Schafer R.Schnabel C.Schreurs O.Selva A.Simon M.,Skiff B.Skrutskie M.Skrzypek J.Sobkowiak K.Sonbas E.Sposetti S.,Stuart P.Szyszka K.Terakubo K.Thomas W.Trela P.Uchiyama S.,Urbanik M.Vaudescal G.Venable R.Watanabe Ha.Watanabe Hi.,Winiarski M.Wroblewski R.Yamamura H.Yamashita M.Yoshihara H.,Zawilski M.Zeleny P.Zejmo M.Zukowski K.Zywica S.2024-11-06T20:06:17Z2023-11-07T09:34:04ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frsolar-systemasteroidsphotometryvisible-astronomyAs evidenced by recent survey results, the majority of asteroids are slow rotators (spin periods longer than 12h), but lack spin and shape models because of selection bias. This bias is skewing our overall understanding of the spins, shapes, and sizes of asteroids, as well as of their other properties. Also, diameter determinations for large (>60km) and medium-sized asteroids (between 30 and 60km) often vary by over 30% for multiple reasons. Our long-term project is focused on a few tens of slow rotators with periods of up to 60 h. We aim to obtain their full light curves and reconstruct their spins and shapes. We also precisely scale the models, typically with an accuracy of a few percent. We used wide sets of dense light curves for spin and shape reconstructions via light-curve inversion. Precisely scaling them with thermal data was not possible here because of poor infrared datasets: large bodies tend to saturate in WISE mission detectors. Therefore, we recently also launched a special campaign among stellar occultation observers, both in order to scale these models and to verify the shape solutions, often allowing us to break the mirror pole ambiguity. The presented scheme resulted in shape models for 16 slow rotators, most of them for the first time. Fitting them to chords from stellar occultation timings resolved previous inconsistencies in size determinations. For around half of the targets, this fitting also allowed us to identify a clearly preferred pole solution from the pair of two mirror pole solutions, thus removing the ambiguity inherent to light-curve inversion. We also address the influence of the uncertainty of the shape models on the derived diameters. Overall, our project has already provided reliable models for around 50 slow rotators. Such well-determined and scaled asteroid shapes will, for example, constitute a solid basis for precise density determinations when coupled with mass information. Spin and shape models in general continue to fill the gaps caused by various biases.2023A&A...679A..60Mhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/679/A60CatalogResearchIsServedByTAP VizieR generic servicerelated-toB/astorb : Orbits of Minor Planets (Bowell+ 2014)J/A+A/654/A87 : Properties of slowly rotating asteroids (Marciniak+ 2021)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/679/A60https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/679/A60http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/679/A60https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/679/A60https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/679/A60http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/679/A60GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultJ/A+A/679/A60/table1Spin parameters and sizes of asteroid models obtained in this workE_Dm? Error on Dm (upper value)kmstat.error;stat.maxintnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintLCShow the light curvesmeta.ref.urlcharAsteroidAsteroid namemeta.id;meta.maincharMethodMethodmeta.notecharlambdapPole ecliptic longitude (J2000)degpos.ecliptic.loninte_lambdapPole ecliptic longitude errordegstat.errorintbetapPole ecliptic latitude (J2000)degpos.ecliptic.latinte_betapPole ecliptic latitude errordegstat.errorintPPole sidereal rotation periodhtime.perioddoublee_PPole sidereal rotation period errorhstat.errordoubleObs-spanObserving span in calendar yearsyrtime.intervalcharNappNumber of apparitionsmeta.numberintNlcNumber of light curvesmeta.numberintDPole Pole volume equivalent diameterkmmeta.bib.volumeintE_DPole Error on D (upper value)kmstat.error;stat.maxinte_DPole Error on D (lower value)kmstat.errorintDRMS? Pole RMS residual from the stellar occultation fittingkmstat.fit.residualintnullablelambdapm? Mirror pole ecliptic longitude (J2000)degpos.ecliptic.lonintnullablee_lambdapm? Mirror pole ecliptic longitude errordegstat.errorintnullablebetapm? Mirror pole ecliptic latitude (J2000)degpos.ecliptic.latintnullablee_betapm? Mirror pole ecliptic latitude errordegstat.errorintnullablePm? Mirror pole Sidereal rotation periodhtime.perioddoublenullablee_Pm? Mirror pole Sidereal rotation period errorhstat.errordoublenullableDm? Mirror pole volume equivalent diameterkmmeta.bib.volumeintnullablee_Dm? Error on Dm (lower value)kmstat.errorintnullableDRMSm? Mirror pole RMS residual from the stellar occultation fittingkmstat.fit.residualintnullableFileNameName of the file with light curve datameta.id;meta.filecharJ/A+A/679/A60/70lcsAsteroid 70 Panopaea individual lightcurvesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintJDJD epoch corrected for the light-time corresponding to the Earth-asteroid distancedtime.epochdoublebrRelative brightness in intensity units, mean brightness of each lightcurve is unityphot.magdoubleSxx component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.x;pos.heliocentricdoubleSyy component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.y;pos.heliocentricdoubleSzz component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.z;pos.heliocentricdoubleExx component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.xdoubleEyy component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.dirCosdoubleEzz component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.zdoubleJ/A+A/679/A60/275lcsAsteroid 275 Sapientia individual lightcurvesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSxx component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.x;pos.heliocentricdoubleSyy component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.y;pos.heliocentricdoubleJDJD epoch corrected for the light-time corresponding to the Earth-asteroid distancedtime.epochdoublebrRelative brightness in intensity units, mean brightness of each lightcurve is unityphot.magdoubleSzz component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.z;pos.heliocentricdoubleExx component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.xdoubleEyy component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.dirCosdoubleEzz component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.zdoubleJ/A+A/679/A60/286lcsAsteroid 286 Iclea individual lightcurvesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintJDJD epoch corrected for the light-time corresponding to the Earth-asteroid distancedtime.epochdoublebrRelative brightness in intensity units, mean brightness of each lightcurve is unityphot.magdoubleSxx component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.x;pos.heliocentricdoubleSyy component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.y;pos.heliocentricdoubleSzz component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.z;pos.heliocentricdoubleExx component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.xdoubleEyy component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.dirCosdoubleEzz component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.zdoubleJ/A+A/679/A60/326lcsAsteroid 326 Tamara individual lightcurvesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintJDJD epoch corrected for the light-time corresponding to the Earth-asteroid distancedtime.epochdoublebrRelative brightness in intensity units, mean brightness of each lightcurve is unityphot.magdoubleSxx component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.x;pos.heliocentricdoubleSyy component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.y;pos.heliocentricdoubleSzz component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.z;pos.heliocentricdoubleExx component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.xdoubleEyy component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.dirCosdoubleEzz component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.zdoubleJ/A+A/679/A60/412lcsAsteroid 412 Elisabetha individual lightcurvesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintJDJD epoch corrected for the light-time corresponding to the Earth-asteroid distancedtime.epochdoublebrRelative brightness in intensity units, mean brightness of each lightcurve is unityphot.magdoubleSxx component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.x;pos.heliocentricdoubleSyy component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.y;pos.heliocentricdoubleSzz component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.z;pos.heliocentricdoubleExx component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.xdoubleEyy component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.dirCosdoubleEzz component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.zdoubleJ/A+A/679/A60/426lcsAsteroid 426 Hippo individual lightcurvesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintJDJD epoch corrected for the light-time corresponding to the Earth-asteroid distancedtime.epochdoublebrRelative brightness in intensity units, mean brightness of each lightcurve is unityphot.magdoubleSxx component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.x;pos.heliocentricdoubleSyy component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.y;pos.heliocentricdoubleSzz component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.z;pos.heliocentricdoubleExx component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.xdoubleEyy component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.dirCosdoubleEzz component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.zdoubleJ/A+A/679/A60/439lcsAsteroid 439 Ohio individual lightcurvesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintJDJD epoch corrected for the light-time corresponding to the Earth-asteroid distancedtime.epochdoublebrRelative brightness in intensity units, mean brightness of each lightcurve is unityphot.magdoubleSxx component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.x;pos.heliocentricdoubleSyy component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.y;pos.heliocentricdoubleSzz component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.z;pos.heliocentricdoubleExx component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.xdoubleEyy component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.dirCosdoubleEzz component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.zdoubleJ/A+A/679/A60/464lcsAsteroid 464 Megaira individual lightcurvesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintJDJD epoch corrected for the light-time corresponding to the Earth-asteroid distancedtime.epochdoublebrRelative brightness in intensity units, mean brightness of each lightcurve is unityphot.magdoubleSxx component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.x;pos.heliocentricdoubleSyy component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.y;pos.heliocentricdoubleSzz component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.z;pos.heliocentricdoubleExx component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.xdoubleEyy component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.dirCosdoubleEzz component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.zdoubleJ/A+A/679/A60/476lcsAsteroid 476 Hedwig individual lightcurvesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintJDJD epoch corrected for the light-time corresponding to the Earth-asteroid distancedtime.epochdoublebrRelative brightness in intensity units, mean brightness of each lightcurve is unityphot.magdoubleSxx component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.x;pos.heliocentricdoubleSyy component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.y;pos.heliocentricdoubleSzz component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.z;pos.heliocentricdoubleExx component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.xdoubleEyy component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.dirCosdoubleEzz component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.zdoubleJ/A+A/679/A60/524lcsAsteroid 524 Fidelio individual lightcurvesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintJDJD epoch corrected for the light-time corresponding to the Earth-asteroid distancedtime.epochdoublebrRelative brightness in intensity units, mean brightness of each lightcurve is unityphot.magdoubleSxx component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.x;pos.heliocentricdoubleSyy component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.y;pos.heliocentricdoubleSzz component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.z;pos.heliocentricdoubleExx component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.xdoubleEyy component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.dirCosdoubleEzz component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.zdoubleJ/A+A/679/A60/530lcsAsteroid 530 Turandot individual lightcurvesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintJDJD epoch corrected for the light-time corresponding to the Earth-asteroid distancedtime.epochdoublebrRelative brightness in intensity units, mean brightness of each lightcurve is unityphot.magdoubleSxx component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.x;pos.heliocentricdoubleSyy component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.y;pos.heliocentricdoubleSzz component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.z;pos.heliocentricdoubleExx component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.xdoubleEyy component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.dirCosdoubleEzz component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.zdoubleJ/A+A/679/A60/551lcsAsteroid 551 Ortrud individual lightcurvesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintJDJD epoch corrected for the light-time corresponding to the Earth-asteroid distancedtime.epochdoublebrRelative brightness in intensity units, mean brightness of each lightcurve is unityphot.magdoubleSxx component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.x;pos.heliocentricdoubleSyy component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.y;pos.heliocentricdoubleSzz component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.z;pos.heliocentricdoubleExx component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.xdoubleEyy component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.dirCosdoubleEzz component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.zdoubleJ/A+A/679/A60/566lcsAsteroid 566 Stereoskopia individual lightcurvesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintJDJD epoch corrected for the light-time corresponding to the Earth-asteroid distancedtime.epochdoublebrRelative brightness in intensity units, mean brightness of each lightcurve is unityphot.magdoubleSxx component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.x;pos.heliocentricdoubleSyy component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.y;pos.heliocentricdoubleSzz component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.z;pos.heliocentricdoubleExx component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.xdoubleEyy component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.dirCosdoubleEzz component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.zdoubleJ/A+A/679/A60/657lcsAsteroid 657 Gunlod individual lightcurvesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintJDJD epoch corrected for the light-time corresponding to the Earth-asteroid distancedtime.epochdoublebrRelative brightness in intensity units, mean brightness of each lightcurve is unityphot.magdoubleSxx component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.x;pos.heliocentricdoubleSyy component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.y;pos.heliocentricdoubleSzz component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.z;pos.heliocentricdoubleExx component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.xdoubleEyy component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.dirCosdoubleEzz component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.zdoubleJ/A+A/679/A60/738lcsAsteroid 738 Alagasta individual lightcurvesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintJDJD epoch corrected for the light-time corresponding to the Earth-asteroid distancedtime.epochdoublebrRelative brightness in intensity units, mean brightness of each lightcurve is unityphot.magdoubleSxx component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.x;pos.heliocentricdoubleSyy component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.y;pos.heliocentricdoubleSzz component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.z;pos.heliocentricdoubleExx component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.xdoubleEyy component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.dirCosdoubleEzz component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.zdoubleJ/A+A/679/A60/806lcsAsteroid 806 Gyldenia individual lightcurvesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintJDJD epoch corrected for the light-time corresponding to the Earth-asteroid distancedtime.epochdoublebrRelative brightness in intensity units, mean brightness of each lightcurve is unityphot.magdoubleSxx component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.x;pos.heliocentricdoubleSyy component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.y;pos.heliocentricdoubleSzz component of the vector from the asteroid to the Sun in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.z;pos.heliocentricdoubleExx component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.xdoubleEyy component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.dirCosdoubleEzz component of the vector from the asteroid to the Earth in J2000 ecliptic Cartesian coordinatesAUpos.cartesian.zdouble