J/AJ/156/60ivo://CDS.VizieR/J/AJ/156/60doi:10.26093/cds/vizier.51560060CDSMasiero J.R.Redwing E.Mainzer A.K.Bauer J.M.Cutri R.M.Grav T.,Kramer E.Nugent C.R.Sonnett S.Wright E.L.2019-02-25T11:46:55Z2019-02-05T07:53:11ZCDS support team

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

cds-question@unistra.frsolar-systemasteroidsinfrared-photometrygalaxy-classification-systemssurveysAutomated asteroid detection routines set requirements on the number of detections, signal-to-noise ratio, and the linearity of the expected motion in order to balance completeness, reliability, and time delay after data acquisition when identifying moving object tracklets. However, when the full-frame data from a survey are archived, they can be searched later for asteroids that were below the initial detection thresholds. We have conducted such a search of the first three years of the reactivated Near-Earth Object Wide-field Infrared Survey Explorer data, looking for near-Earth objects discovered by ground-based surveys that have previously unreported thermal infrared data. Using these measurements, we can then perform thermal modeling to measure the diameters and albedos of these objects. We present new physical properties for 116 Near-Earth Objects found in this search.2018AJ....156...60Mhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/156/60CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/ApJ/743/156 : NEOWISE observations of NEOs: preliminary resultsJ/ApJ/760/L12 : WISE/NEOWISE NEOs preliminary thermal fits (Mainzer+, 2012)J/ApJ/784/110 : NEOWISE observations of 105 near-Earth objects (Mainzer+, 2014)J/ApJ/814/117 : NEOWISE Reactivation mission: 1st yr data (Nugent+, 2015)J/AJ/152/63 : NEOWISE reactivation mission: 2nd yr data (Nugent+, 2016)J/AJ/154/168 : NEOWISE: thermal model fits for NEOs and MBAs (Masiero+, 2017)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/156/60https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/156/60http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/156/60https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/156/60https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/156/60http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/156/60GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapInfraredOpticaldefaultJ/AJ/156/60/table1Thermal model fits for short-arc NEOs observed in the first three years of the NEOWISE reactivation surveyrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameName in Minor Planet Center-packed (MPC) formatmeta.id;meta.maincharHMag[18.7/26.8] Absolute visual magnitudemagphys.magAbs;em.IR.HfloatG[0.15/0.15] Photometric slope parameterarith.grad;stat.paramfloatDiam[0.008/1.403] Diameterkmphys.size.diameterfloate_Diam[0.002/0.23] Uncertainty in Diamkmstat.errorfloatDcorr[0.007/1.305] Phase-corrected diameter using the equations from Mommert et al. (2018AJ....155...74M)kmphys.size.diameterfloatlogpV[-1.99/-0.23] Log of the visible-light albedophys.albedofloate_logpV[0.08/0.57] Uncertainty in logpVstat.errorfloatlogpVcor[-1.89/-0.1] Phase-corrected visible-light albedo using the equations from Mommert et al. (2018AJ....155...74M)phys.albedofloatBeam[0.54/3.14] Beaming parameter {eta}stat.fit.paramfloate_Beam[0.06/1] Uncertainty in Beamstat.errorfloatNW1[0/7] Number of detections in the W1 bandpassmeta.numberintNW2[1/13] Number of detections in the W2 bandpassmeta.numberintPhase[52.31/90.16] Phase angledegpos.phaseAngfloatFitted[0/1]? Fitted beaming flag (1)meta.codeintnullable