The Period-Luminosity Relation of RR Lyrae Stars in the SDSS Photometric System

dc.date.accessioned2020-03-11T20:25:54Z
dc.date.accessioned2022-10-18T22:40:07Z
dc.date.available2020-03-11T20:25:54Z
dc.date.available2022-10-18T22:40:07Z
dc.date.created2020-03-11T20:25:54Z
dc.date.issued2008
dc.identifierhttp://hdl.handle.net/10533/237916
dc.identifier15010003
dc.identifierWOS:000262862200012
dc.identifierno scielo
dc.identifiereid=2-s2.0-55249119313
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/4469255
dc.description.abstractWe provide the first detailed study of the RR Lyrae period-luminosity (PL) relation in the ugriz bandpasses of the Sloan Digital Sky Survey (SDSS) filter system. We argue that tight, simple PL relations are not present in the SDSS filters, except for the
dc.languageeng
dc.relationhttps://doi.org/10.1086/591231
dc.relation10.1086/591231
dc.rightsinfo:eu-repo/semantics/openAccess
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 Chile
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.titleThe Period-Luminosity Relation of RR Lyrae Stars in the SDSS Photometric System
dc.typeArticulo


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