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Davis, M; Guhathakurta, P; Konidaris, N. P; Newman, J. A; Ashby, M. L. N; Biggs, A. D; Barmby, P; Bundy, K; Chapman, S. C; Coil, A. L; Conselice, C. J; Cooper, M. C; Croton, D. J; Eisenhardt, P. R. M; Ellis, R. S; Faber, S. M; Fang, T; Fazio, G. G; Georgakakis, A; Gerke, B. F; Goss, W. M; Gwyn, S; Harker, J; Hopkins, A. M; Huang, J.-S; Ivison, R. J; Kassin, S. A; Kirby, E. N; Koekemoer, A. M; Koo, D. C; Laird, E. S; Le Floc’h, E; Lin, L; Lotz, J. M; Marshall, P. J; Martin, D. C; Metevier, A. J; Moustakas, L. A; Nandra, K; Noeske, K. G; 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. J; Willmer, C. N. A; Willner, S. P; Wilson, G; Wright, E. L; Yan, R
Astrophysical journal/The Astrophysical journal, 05/2007, Volume: 660, Issue: 1Journal Article
In this the first of a series of Letters, we present a panchromatic data set in the Extended Groth Strip region of the sky. Our survey, the All-Wavelength Extended Groth Strip International Survey (AEGIS), aims to study the physical properties and evolutionary processes of galaxies at z 6 1. It includes the following deep, wide-field imaging data sets: Chandra/ACIS X-ray, GALEX ultraviolet, CFHT/MegaCam Legacy Survey optical, CFHT/CFH12K optical, Hubble Space Telescope/ACS optical and NICMOS near-infrared, Palomar/WIRC near-infrared, Spitzer/IRAC mid-infrared, Spitzer/MIPS far-infrared, and VLA radio continuum. In addition, mis region of the sky has been targeted for extensive spectroscopy using the Deep Imaging Multi-Object Spectrograph (DEIMOS) on the Keck II 10 m telescope. Our survey is compared to other large multiwavelength surveys in terms of depth and sky coverage.
