We carried out near- to mid-infrared imaging and spectroscopic observations of patchy areas in the Small Magellanic Cloud using the Infrared Camera aboard AKARI. Two 100arcmin^2^ areas were imaged in 3.2, 4.1, 7, 11, 15, and 24um, and also spectroscopically observed in the wavelength range continuously from 2.5 to 13.4um. The spectral resolving power, {lambda}{Delta}{lambda}, values were about 20, 50, and 50 at 3.5, 6.6, and 10.6um, respectively. Other than the two 100arcmin^2^ areas, some patchy areas were imaged and/or spectroscopically observed as well. In this paper, we overview the observations and present a list of near- to mid-infrared photometric results, which lists ~12000 near-infrared and ~1800 mid-infrared bright point sources detected in the observed areas. The 10{sigma} limits are 16.50, 16.12, 13.28, 11.26, 9.62, and 8.76 in Vega magnitudes at 3.2, 4.1, 7, 11, 15, and 24um bands, respectively.
Cone search capability for table J/PASJ/62/273/smc_akari (AKARI SMC photometry in all filters: N3 (3.2{mu}m), N4 (4.1{mu}m), S7 (7{mu}m), S11 (11{mu}m), L15 (15{mu}m), L24 (24{mu}m))
