Davis, M.Guhathakurta, P.Konidaris, N.Newman, J. A.Ashby, M. L. N.Biggs, A. D.Barmby, P.Bundy, K.Chapman, S.Coil, A. L.Conselice, C.Cooper, M.Croton, D.Eisenhardt, P.Ellis, R.Faber, S.Fang, T.Fazio, G. G.Georgakakis, A.Gerke, B.Goss, W. M.Gwyn, S.Harker, J.Hopkins, A.Huang, J. -SIvison, R. J.Kassin, S. A.Kirby, E.Koekemoer, A.Koo, D. C.Laird, E.Floc'h, E. LeLin, L.Lotz, J.Marshall, P. J.Martin, D. C.Metevier, A.Moustakas, L. A.Nandra, K.Noeske, K.Papovich, C.Phillips, A. C.Rich, R. M.Rieke, G. H.Rigopoulou, D.Salim, S.Schiminovich, D.Simard, L.Smail, I.Small, T. A.Weiner, B.Willmer, C. N. A.Willner, S. P.Wilson, G.Wright, E.Yan, R.2014-03-122014-03-122007-05-01Davis, M., P. Guhathakurta, N. Konidaris, J. A. Newman, et al. 2007. "The All-wavelength Extended Groth Strip International Survey (AEGIS) Data Sets." The Astrophysical Journal 660(1): 1-L60004-637Xhttp://dx.doi.org/10.1086/517931http://hdl.handle.net/10222/45289In this the first of a series of Letters, we present a description of the panchromatic data sets that have been acquired in the Extended Groth Strip region of the sky. Our survey, the All-wavelength Extended Groth strip International Survey (AEGIS), is intended to study the physical properties and evolutionary processes of galaxies at z ~ 1. It includes the following deep, wide-field imaging data sets: Chandra/ACIS X-ray (0.5 - 10 keV), GALEX ultraviolet (1200 - 2500 Angstrom), CFHT/MegaCam Legacy Survey optical (3600 - 9000 Angstroms), CFHT/CFH12K optical (4500 - 9000 Angstroms), Hubble Space Telescope/ACS optical (4400 - 8500 Angstroms), Palomar/WIRC near-infrared (1.2 - 2.2 microns), Spitzer/IRAC mid-infrared (3.6 - 8.0 microns), Spitzer/MIPS far-infrared (24 - 70 microns), and VLA radio continuum (6 - 20 cm). In addition, this region of the sky has been targeted for extensive spectroscopy using the DEIMOS spectrograph on the Keck II 10 m telescope. Our survey is compared to other large multiwavelength surveys in terms of depth and sky coverage.article66011