The first measurements of galaxy clustering from Infrared Array Camera (IRAC) data of the Spitzer First Look Survey

We present the first results of the angular autocorrelation function of the galaxies detected by the Infrared Array Camera (IRAC) instrument in the First Look Survey (FLS) of the Spitzer Space Telescope. We detect significant signals of galaxy clustering within the survey area. The angular autocorrelation function of the galaxies detected in each of the four IRAC instrument channels is consistent with a power-law form w(theta) = Atheta(1-gamma) out to theta = 0.degrees2, with the slope ranging from gamma = 1.5 to 1.8. We estimate the correlation amplitude A to be 2.95 x 10(-3), 2.03 x 10(-3), 4.53 x 10(-3), and 2.34 x 10(-3) at theta = 1degrees for galaxies detected in the IRAC 3.6, 4.5, 5.8, and 8.0 mum instrument channels, respectively. We compare our measurements at 3.6 mum with the previous K-band measurements and discuss the implications of these results.