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We present the AEGIS-X survey, a series of deep Chandra ACIS-I observationsof the Extended Groth Strip. The survey comprises pointings at 8 separatepositions, each with nominal exposure 200ks, covering a total area ofapproximately 0.67 deg2 in a strip of length 2 degrees. We describe in detailan updated version of our data reduction and point source detection algorithmsused to analyze these data. A total of 1325 band-merged sources have been foundto a Poisson probability limit of 4e-6, with limiting fluxes of 5.3e-17erg/cm2/s in the soft (0.5-2 keV) band and 3.8e-16 erg/cm2/s in the hard (2-10keV) band. We present simulations verifying the validity of our sourcedetection procedure and showing a very small, <1.5%, contamination rate fromspurious sources. Optical/NIR counterparts have been identified from the DEEP2,CFHTLS, and Spitzer/IRAC surveys of the same region. Using a likelihood ratiomethod, we find optical counterparts for 76% of our sources, complete toR(AB)=24.1, and, of the 66% of the sources that have IRAC coverage, 94% have acounterpart to a limit of 0.9 microJy at 3.6 microns (m(AB)=23.8). Afteraccounting for (small) positional offsets in the 8 Chandra fields, theastrometric accuracy of the Chandra positions is found to be 0.8 arcsec RMS,however this number depends both on the off-axis angle and the number ofdetected counts for a given source. All the data products described in thispaper are made available via a public website.

AEGIS-X: The Chandra Deep Survey of the Extended Groth Strip