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dc.contributor.authorSchanche, N.
dc.contributor.authorCameron, A. Collier
dc.contributor.authorAlmenara, J. M.
dc.contributor.authorAlsubai, K. A.
dc.contributor.authorAnderson, D. R.
dc.contributor.authorArmstrong, D. J.
dc.contributor.authorBarkaoui, K.
dc.contributor.authorBarros, S. C. C.
dc.contributor.authorBochinski, J.
dc.contributor.authorBonomo, A. S.
dc.contributor.authorBouchy, F.
dc.contributor.authorBrown, D. J. A.
dc.contributor.authorBurdanov, A.
dc.contributor.authorBusuttil, R.
dc.contributor.authorDeleuil, M.
dc.contributor.authorDelrez, L.
dc.contributor.authorFaedi, F.
dc.contributor.authorGillon, M.
dc.contributor.authorHay, K.
dc.contributor.authorHebb, L.
dc.contributor.authorHebrard, G.
dc.contributor.authorJehin, E.
dc.contributor.authorKolb, U.
dc.contributor.authorMaxted, P. F. L.
dc.contributor.authorMiller, G.
dc.contributor.authorNielsen, L. D.
dc.contributor.authorPollacco, D. L.
dc.contributor.authorPozuelos, F. J.
dc.contributor.authorQueloz, D.
dc.contributor.authorRelles, H.
dc.contributor.authorSmalley, B.
dc.contributor.authorTriaud, A. H. M. J.
dc.contributor.authorUdry, S.
dc.contributor.authorWest, R.
dc.contributor.authorWheatley, P. J.
dc.date.accessioned2019-10-01T15:30:02Z
dc.date.available2019-10-01T15:30:02Z
dc.date.issued2019-10
dc.identifier261445261
dc.identifier051260bb-5fad-407a-9971-b577e9ac5f1c
dc.identifier000484349700034
dc.identifier85076687761
dc.identifier.citationSchanche , N , Cameron , A C , Almenara , J M , Alsubai , K A , Anderson , D R , Armstrong , D J , Barkaoui , K , Barros , S C C , Bochinski , J , Bonomo , A S , Bouchy , F , Brown , D J A , Burdanov , A , Busuttil , R , Deleuil , M , Delrez , L , Faedi , F , Gillon , M , Hay , K , Hebb , L , Hebrard , G , Jehin , E , Kolb , U , Maxted , P F L , Miller , G , Nielsen , L D , Pollacco , D L , Pozuelos , F J , Queloz , D , Relles , H , Smalley , B , Triaud , A H M J , Udry , S , West , R & Wheatley , P J 2019 , ' SuperWASP dispositions and false positive catalogue ' , Monthly Notices of the Royal Astronomical Society , vol. 488 , no. 4 , pp. 4905-4915 . https://doi.org/10.1093/mnras/stz2064en
dc.identifier.issn0035-8711
dc.identifier.otherORCID: /0000-0002-8863-7828/work/62668323
dc.identifier.urihttps://hdl.handle.net/10023/18593
dc.descriptionNS acknowledges the support of the National Priorities Research Program (NPRP) grant #X-019-1-006 from the Qatar National Research Fund (a member of Qatar Foundation). ACC acknowledges support from the Science & Technology Facilities Council (STFC) consolidated grant number ST/R000824/1.en
dc.description.abstractSuperWASP, the Northern hemisphere WASP observatory, has been observing the skies from La Palma since 2004. In that time, more than 50 planets have been discovered with data contributions from SuperWASP. In the process of validating planets, many false-positive candidates have also been identified. The TESS telescope is set to begin observations of the northern sky in 2019. Similar to the WASP survey, the TESS pixel size is relatively large (13arcsec for WASP and 21arcsec for TESS), making it susceptible to many blended signals and false detections caused principally by grazing and blended stellar eclipsing binary systems. In order to reduce duplication of effort on targets, we present a catalogue of 1041 Northern hemisphere SuperWASP targets that have been rejected as planetary transits through follow-up observation.
dc.format.extent11
dc.format.extent3279281
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen
dc.subjectMethods: observationalen
dc.subjectCataloguesen
dc.subjectPlanets and satellites: detectionen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subjectDASen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleSuperWASP dispositions and false positive catalogueen
dc.typeJournal articleen
dc.contributor.sponsorScience & Technology Facilities Councilen
dc.contributor.sponsorScience & Technology Facilities Councilen
dc.contributor.institutionUniversity of St Andrews. St Andrews Centre for Exoplanet Scienceen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.identifier.doi10.1093/mnras/stz2064
dc.description.statusPeer revieweden
dc.identifier.grantnumberST/R00824/1en
dc.identifier.grantnumberST/R003203/1en


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