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AEGIS, or the All-Wavelength Extended Groth Strip International Survey, is a multi-wavelength astronomical survey of a patch of the sky with low extinction and zodiacal scattering. The purpose of the survey is to study the physical processes and evolution of galaxies at redshift z ~ 1. As of February 2011 more than 80 research papers have been published based on data from the survey.〔(AEGIS Papers ) retrieved February 10, 2011〕 ==Observatories== AEGIS makes use of multiple terrestrial and space based observatories to conduct the survey. These observatories make overlapping scans of the survey area.〔(EGS Coverage )〕 The primary telescopes are:〔(Official Project Site )〕 *Very Large Array *Spitzer Space Telescope *Palomar Observatory *Canada-France-Hawaii Telescope *Keck Observatory *Hubble Space Telescope *GALEX *Chandra X-ray Observatory ==See also== 抄文引用元・出典: フリー百科事典『 ウィキペディア（Wikipedia）』 ■ウィキペディアで「AEGIS (astronomy)」の詳細全文を読む スポンサード リンク
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