Secondary UBVRI-CCD standard stars in the neighbourhood of Landolt standard stars

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dc.contributor.authorGaladí-Enríquez, Davidcat
dc.contributor.authorTrullols i Farreny, Enriccat
dc.contributor.authorJordi i Nebot, Carmecat
dc.date.accessioned2009-08-28T08:28:20Z
dc.date.available2009-08-28T08:28:20Z
dc.date.issued2000cat
dc.description.abstractA list of 681 UBVRI secondary standard stars for CCD photometry is presented. Visual magnitude ranges from 9.7 to 19.4, and the B-V colour index varies from 1.15 to 1.97. The stars are grouped into 11 different fields, each of them is generally observable in a single CCD frame. The stars are located near Landolt UBVRI equatorial standards, accessible to telescopes in both hemispheres, and mainly within the 5 - 8 hours range of right ascension. Photometry, equatorial coordinates and finding charts are provided.eng
dc.format.extent9 p.cat
dc.format.mimetypeapplication/pdfeng
dc.identifier.idgrec164580cat
dc.identifier.issn0365-0138cat
dc.identifier.urihttps://hdl.handle.net/2445/9226
dc.language.isoengeng
dc.publisherEDP Sciencescat
dc.relation.isformatofReproducció del document publicat a http://dx.doi.org/10.1051/aas:2000266cat
dc.relation.ispartofAstronomy and Astrophysics Supplement Series, 2000, vol. 146, núm. 1, p. 169-177.cat
dc.relation.requireshttp://dx.doi.org/10.1051/aas:2000266
dc.rights(c) The European Southern Observatory, 2000cat
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess
dc.sourceArticles publicats en revistes (Física Quàntica i Astrofísica)
dc.subject.classificationEstelscat
dc.subject.classificationFotometria astronòmicacat
dc.subject.otherMethods: observationaleng
dc.subject.otherTechniques: photometriceng
dc.subject.otherStars: generaleng
dc.titleSecondary UBVRI-CCD standard stars in the neighbourhood of Landolt standard starseng
dc.typeinfo:eu-repo/semantics/articleeng
dc.typeinfo:eu-repo/semantics/publishedVersion

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