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The Araucaria Project. The Distance of the Large Magellanic Cloud from Near-Infrared Photom

We have obtained deep infrared $J$ and $K$ band observations of five fields located in the Large Magellanic Cloud (LMC) bar with the ESO New Technology Telescope equipped with the SOFI infrared camera. In our fields, 65 RR Lyrae stars catalogued by the OGL

TheAraucariaProject.TheDistanceoftheLargeMagellanicCloudfromNear-InfraredPhotometryofRRLyraeVariables1

OlafSzewczyk

arXiv:0804.3333v1 [astro-ph] 21 Apr 2008UniversidaddeConcepci´on,DepartamentodeFisica,AstronomyGroup,Casilla160-C,Concepci´on,ChileWarsawUniversityObservatory,Al.Ujazdowskie4,00-478,Warsaw,Polandszewczyk@astro-udec.clGrzegorzPietrzy´nskiUniversidaddeConcepci´on,DepartamentodeFisica,AstronomyGroup,Casilla160-C,Concepci´on,ChileWarsawUniversityObservatory,Al.Ujazdowskie4,00-478,Warsaw,Polandpietrzyn@astrouw.edu.plWolfgangGierenUniversidaddeConcepci´on,DepartamentodeFisica,AstronomyGroup,Casilla160-C,Concepci´on,Chilewgieren@astro-udec.clJesperStormAstrophysikalischesInstitutPotsdam,AnderSternwarte16,D-14482Potsdam,Germany

jstorm@aip.de

AlistairWalker

CerroTololoInter-AmericanObservatory,Casilla603,LaSerena,Chile

awalker@ctio.noao.edu

LucaRizzi

JointAstronomyCentre,66N.A’ohokuPl.,Hilo,Hawaii,96720

luca@ifa.hawaii.edu

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