The Fornax Project

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dc.catalogadorpau
dc.contributor.authorClementini, G.
dc.contributor.authorGreco, C.
dc.contributor.authorHeld, E. V.
dc.contributor.authorPoretti, E.
dc.contributor.authorCatelan, Marcio
dc.contributor.authorDell'Arciprete, L.
dc.contributor.authorGullieuszik, M.
dc.contributor.authorMaio, M.
dc.contributor.authorRizzi, L.
dc.contributor.authorSmith, H. A.
dc.contributor.authorPritzl, B. J.
dc.contributor.authorRest, A.
dc.contributor.authorDe Lee, N.
dc.date.accessioned2024-03-05T15:14:39Z
dc.date.available2024-03-05T15:14:39Z
dc.date.issued2006
dc.description.abstractThe Fornax Project aims at mapping the classical instability strip of the Fornax dwarf spheroidal galaxy, from the faint Dwarf Cepheids (V ∼ 24-25 mag) to the bright Anomalous Cepheids (V ∼ 19 mag). To achieve this goal, deep B,V time-series photometry of the galaxy has been obtained with the Wide Field Imagers (WFIs) of the ESO 2.2 m and CTIO 4 m telescopes, and the Clay camera at the Magellan 6.5 m telescope. Preliminary results are presented on the Oosterhoff classification of the RR Lyrae stars identified in a northern portion of Fornax field and in three of its globular clusters....
dc.fuente.origenORCID
dc.identifier.urihttps://articles.adsabs.harvard.edu/full/2006MmSAI..77..249C
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/83998
dc.information.autorucInstituto de Astrofísica; Catelan , Marcio; 0000-0001-6003-8877; 1001556
dc.language.isoen
dc.nota.accesoContenido completo
dc.rightsacceso abierto
dc.titleThe Fornax Project
dc.typeartículo
sipa.codpersvinculados1001556
sipa.trazabilidadORCID;2024-01-22
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