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dc.contributor.authorBlomme, J.
dc.contributor.authorSarro, L. M.
dc.contributor.authorO’Donovan, F. T.
dc.contributor.authorDebosscher, J.
dc.contributor.authorBrown, T.
dc.contributor.authorLopez, M.
dc.contributor.authorDubath, P.
dc.contributor.authorRimoldini, L.
dc.contributor.authorCharbonneau, D.
dc.contributor.authorDunham, E.
dc.contributor.authorMandushev, G.
dc.contributor.authorCiardi, D. R.
dc.contributor.authorDe Ridder, J.
dc.contributor.authorAerts, C.
dc.date.accessioned2019-09-27T13:19:31Z
dc.date.issued2011
dc.identifier.citationBlomme, J., L. M. Sarro, F. T. O’Donovan, J. Debosscher, T. Brown, M. Lopez, P. Dubath, et al. 2011. “Improved Methodology for the Automated Classification of Periodic Variable Stars.” Monthly Notices of the Royal Astronomical Society 418 (1): 96–106. https://doi.org/10.1111/j.1365-2966.2011.19466.x.
dc.identifier.issn0035-8711
dc.identifier.issn1365-2966
dc.identifier.urihttp://nrs.harvard.edu/urn-3:HUL.InstRepos:41417397*
dc.description.abstractWe present a novel automated methodology to detect and classify periodic variable stars in a large data base of photometric time series. The methods are based on multivariate Bayesian statistics and use a multistage approach. We applied our method to the ground-based data of the Trans-Atlantic Exoplanet Survey (TrES) Lyr1 field, which is also observed by the Kepler satellite, covering similar to 26 000 stars. We found many eclipsing binaries as well as classical non-radial pulsators, such as slowly pulsating B stars, ? Doradus, beta Cephei and d Scuti stars. Also a few classical radial pulsators were found.
dc.language.isoen_US
dc.publisherOxford University Press
dash.licenseLAA
dc.titleImproved methodology for the automated classification of periodic variable stars
dc.typeJournal Article
dc.description.versionVersion of Record
dc.relation.journalMonthly Notices of the Royal Astronomical Society
dash.depositing.authorCharbonneau, David::a0e3ca75d3fb8511f2f554ed69428108::600
dc.date.available2019-09-27T13:19:31Z
dash.workflow.comments1Science Serial ID 66525
dc.identifier.doi10.1111/j.1365-2966.2011.19466.x
dash.source.volume418;1
dash.source.page96-106


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