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A Variable Star Census in a Perseus Field

dc.contributor.authorPASTERNACKI, T.
dc.contributor.authorCSIZMADIA, Sz.
hal.structure.identifierInstitut de Radioprotection et de Sûreté Nucléaire [IRSN]
dc.contributor.authorCABRERA, Justo
dc.contributor.authorEIGMUELLER, P.
hal.structure.identifierDLR Institute of Planetary Research
dc.contributor.authorERIKSON, A.
dc.contributor.authorFRUTH, T.
dc.contributor.authorVON PARIS, P.
hal.structure.identifierDLR Institute of Planetary Research
dc.contributor.authorRAUER, H.
dc.contributor.authorTITZ, R.
dc.contributor.authorEISLOEFFEL, J.
hal.structure.identifierThüringer Landessternwarte Tautenburg [TLS]
dc.contributor.authorHATZES, A.
hal.structure.identifierObservatoire de Haute-Provence [OHP]
dc.contributor.authorBOER, M.
hal.structure.identifierObservatoire de Haute-Provence [OHP]
dc.contributor.authorTOURNOIS, G.
hal.structure.identifierDLR Institute of Planetary Research
dc.contributor.authorKABATH, P.
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
hal.structure.identifierObservatoire aquitain des sciences de l'univers [OASU]
hal.structure.identifierUniversité Sciences et Technologies - Bordeaux 1 [UB]
hal.structure.identifierLaboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
dc.contributor.authorHEDELT, P.
dc.contributor.authorVOSS, H.
dc.date.created2011-08-25
dc.date.issued2011
dc.identifier.issn0004-6256
dc.description.abstractEnThe Berlin Exoplanet Search Telescope is a small-aperture, wide-field telescope dedicated to time-series photometric observations. During an initial commissioning phase at the Thueringer Landessternwarte Tautenburg, Germany, and subsequent operations at the Observatoire de Haute-Provence, France, a 3.1 {\deg} x 3.1 {\deg} circumpolar field close to the galactic plane centered at ({\alpha}, {\delta}) = (02h 39m 23s, +52{\deg} 01' 46") (J 2000.0) was observed between 2001 August and 2006 December during 52 nights. From the 32129 stars observed, a subsample of 145 stars with clear stellar variability was detected out of which 125 are newly identified variable objects. For five bright objects, the system parameters were derived by modeling the light curve.
dc.language.isoen
dc.publisherAmerican Astronomical Society
dc.title.enA Variable Star Census in a Perseus Field
dc.typeArticle de revue
dc.identifier.doi10.1088/0004-6256/142/4/114
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP]
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP]
dc.identifier.arxiv1108.4863
bordeaux.journalThe Astronomical Journal
bordeaux.page114
bordeaux.volume142
bordeaux.issue4
bordeaux.peerReviewedoui
hal.identifierhal-00620199
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00620199v1
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