J/AJ/166/152ivo://CDS.VizieR/J/AJ/166/152doi:10.26093/cds/vizier.51660152CDSMcNeill A.Gowanlock M.Mommert M.Trilling D.E.Llama J.Paddock N.2024-11-06T20:17:50Z2023-09-08T15:31:11ZCDS support team

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

cds-question@unistra.frsolar-systemasteroidsphotometryvisible-astronomyWe present photometric data for minor planets observed by the Transiting Exoplanet Survey Satellite during its Cycle 1 operations. In total we extracted usable detections for 37965 objects. We present an examination of the reliability of the rotation period and lightcurve amplitudes derived from each object based upon the number of detections and the normalised Lomb-Scargle power of our period fitting and compare and contrast our results with previous similar works. We show that for objects with 200 or more photometric detections and a derived normalised, generalised Lomb-Scargle power greater than 0.2 we have an 85% confidence in that period - this encompasses 3492 rotation periods we consider to be highly reliable. We independently examine a series of periods first reported by Pal et al. (2020ApJS..247...26P) - periods derived in both works found to have similar results should be considered reliable. Additionally we demonstrate the need to properly account for the true proportion of slow rotators (P>100h) when inferring shape distribution from sparse photometry.2023AJ....166..152Mhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/166/152CatalogResearchIsServedByTAP VizieR generic servicerelated-toB/astorb : Orbits of Minor Planets (Bowell+ 2014)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/166/152https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/166/152http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/166/152https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/166/152https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/166/152http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/166/152GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultJ/AJ/166/152/finalFinal table LCDB quality flag truerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintLCShow the light curvemeta.ref.urlcharObjectId Minor Planet Center IDmeta.id;meta.maincharAmpPeak-to-trough light curve amplitudemagsrc.var.amplitudedoubleNObsNumber of individual observationsmeta.numberintLSNormNormalised signal power of the peak of Lomb-Scargle periodogramphot.flux;arith.ratiofloatProtRotational periodhtime.perioddoubleCVexactConfidence value that the derived period is correct to within 3%stat.fit.goodnessfloatCValiasConfidence value that the derived period is correct to within 3% or is different by a factor of 2.stat.fit.goodnessfloatJ/AJ/166/152/gt200ptsTESS results, gt200pts (table 1)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintLCShow the light curvemeta.ref.urlcharObjectMinor Planet Center IDmeta.id;meta.maincharProtRotation periodhtime.perioddoublee_ProtUncertainty on rotational periodhstat.errordoubleAmpLight curve amplitudemagsrc.var.amplitudedoubleCVexactConfidence value that the derived period is correct to within 3%stat.fit.goodnessfloatCValiasConfidence value that the derived period is correct to within 3% or is different by a factor of 2.stat.fit.goodnessfloatMatch?[Y/N/-] Result is considered a match to the independent work of Pal et al. (2020ApJS..247...26P)meta.codecharJ/AJ/166/152/3scycle13sigma Cycle1 light curves for 37965 objectsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintObjectMinor Planet Center IDmeta.id;meta.maincharMJDModified Julian Date of observationdtime.epochdoubleindexedrelhTime of observation in hours where earliest observation of a given object is t=0htime.epochdoublemagThe instrumental magnitude of the object at this time-stamp (1)magphot.mag;em.optdoublee_magUncertainty in instrumental magnitudemagstat.error;phot.magdouble