J/ApJ/792/30ivo://CDS.VizieR/J/ApJ/792/30doi:10.26093/cds/vizier.17920030CDSMainzer A.Bauer J.Cutri R.M.Grav T.Masiero J.Beck R.,Clarkson P.Conrow T.Dailey J.Eisenhardt P.Fabinsky B.,Fajardo-Acosta S.Fowler J.Gelino C.Grillmair C.Heinrichsen I.,Kendall M.Kirkpatrick J.D.Liu F.Masci F.McCallon H.Nugent C.R.,Papin M.Rice E.Royer D.Ryan T.Sevilla P.Sonnett S.Stevenson R.,Thompson D.B.Wheelock S.Wiemer D.Wittman M.Wright E.Yan L.2017-05-23T09:29:11Z2017-04-13T10:18:32ZCDS support team

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

cds-question@unistra.frasteroidscometsinfrared-photometrysurveysNASA's Wide-field Infrared Survey Explorer (WISE) spacecraft has been brought out of hibernation and has resumed surveying the sky at 3.4 and 4.6 {mu}m. The scientific objectives of the NEOWISE reactivation mission are to detect, track, and characterize near-Earth asteroids and comets. The search for minor planets resumed on 2013 December 23, and the first new near-Earth object (NEO) was discovered 6 days later. As an infrared survey, NEOWISE detects asteroids based on their thermal emission and is equally sensitive to high and low albedo objects; consequently, NEOWISE-discovered NEOs tend to be large and dark. Over the course of its three-year mission, NEOWISE will determine radiometrically derived diameters and albedos for ~2000 NEOs and tens of thousands of Main Belt asteroids. The 32 months of hibernation have had no significant effect on the mission's performance. Image quality, sensitivity, photometric and astrometric accuracy, completeness, and the rate of minor planet detections are all essentially unchanged from the prime mission's post-cryogenic phase.2014ApJ...792...30Mhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/792/30CatalogResearchIsServedByTAP VizieR generic servicerelated-toII/311 : WISE All-Sky Data Release (Cutri+ 2012)J/A+A/375/285 : Photometric observations of 9 Near-Earth Objects (Szabo+, 2001)J/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)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/792/30https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/792/30http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/792/30https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/792/30https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/792/30http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/792/30GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tap1.143914381504295e-19 1.2934455535160846e-19InfrareddefaultJ/ApJ/792/30/table2Thermal Fit Results for the NEO Detections Reported in this WorkrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameIdentifiermeta.id;meta.maincharONameOther namemeta.idcharHH magnitudemagphot.mag;em.IR.HfloatGPhase curve slope parameterarith.grad;stat.paramfloatDDiameterkmphys.size.diameterfloate_Drms uncertainty on Dkmstat.errorfloatpVVisible albedophys.albedofloate_pVrms uncertaitny on pV (1)stat.errorfloatetaBeaming parameterstat.fit.paramfloate_etarms uncertaitny on eta (1)stat.error;phys.electron.degenfloatpIRInfrared albedophys.albedofloate_pIRrms uncertaitny on pIR (1)stat.errorfloatNobsW1Number of observations in NEOWISE W1 bandmeta.numberintNobsW2Number of observations in NEOWISE W2 bandmeta.numberintLCLight curvesmeta.ref.urlcharJ/ApJ/792/30/table1Preliminary NEOWISE magnitudes for the NEOs shown in Figure 15 at each observation's modified Julian daterecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameIdentifiermeta.id;meta.maincharMJDModified Julian Date of observationdtime.epochdoublel_3.4magThe 2{sigma} upper limit flag on 3.4mag (1)meta.code.errorchar3.4magNEOWISE 3.4 micron band magnitudemagphot.mag;em.IR.3-4umfloate_3.4mag? Uncertainty in 3.4magmagstat.errorfloatnullable4.6magNEOWISE 4.6 micron band magnitudemagphot.mag;em.IR.4-8umfloate_4.6magUncertainty in 4.6magmagstat.errorfloatFAper[0] flag for aperture radius used for photometry (2)meta.codeint