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We present a near- to mid-infrared point source catalog of 5 photometricbands at 3.2, 7, 11, 15 and 24 um for a 10 deg2 area of the Large MagellanicCloud (LMC) obtained with the Infrared Camera (IRC) onboard the AKARIsatellite. To cover the survey area the observations were carried out at 3separate seasons from 2006 May to June, 2006 October to December, and 2007March to July.  The 10-sigma limiting magnitudes of the present survey are 17.9, 13.8, 12.4,9.9, and 8.6 mag at 3.2, 7, 11, 15 and 24 um, respectively. The photometricaccuracy is estimated to be about 0.1 mag at 3.2 um and 0.06--0.07 mag in theother bands. The position accuracy is 0.3" at 3.2, 7 and 11um and 1.0" at 15and 24 um. The sensitivities at 3.2, 7, and 24 um are roughly comparable tothose of the Spitzer SAGE LMC point source catalog, while the AKARI catalogprovides the data at 11 and 15 um, covering the mid-infrared spectral rangecontiguously. Two types of catalog are provided: a Catalog and an Archive. TheArchive contains all the detected sources, while the Catalog only includes thesources that have a counterpart in the Spitzer SAGE point source catalog. TheArchive contains about 650,000, 140,000, 97,000, 43,000, and 52,000 sources at3.2, 7, 11, 15, and 24 um, respectively. Based on the catalog, we discuss theluminosity functions at each band, the color-color diagram, and thecolor-magnitude diagram using the 3.2, 7, and 11 um band data. Stars withoutcircumstellar envelopes, dusty C-rich and O-rich stars, young stellar objects,and background galaxies are located at distinct regions in the diagrams,suggesting that the present catalog is useful for the classification of objectstowards the LMC.

AKARI Infrared Camera Survey of the Large Magellanic Cloud. I. Point Source Catalog