| 翻訳と辞書 |
| Great Observatories Origins Deep Survey ： ウィキペディア英語版 |
Great Observatories Origins Deep Survey
The Great Observatories Origins Deep Survey or GOODS is an astronomical survey combining deep observations from three of NASA's Great Observatories: the Hubble Space Telescope, the Spitzer Space Telescope and the Chandra X-ray Observatory along with data from other space-based telescopes, such as XMM Newton, and some of the worlds most powerful ground-based telescopes. GOODS is intended to enable astronomers to study the formation and evolution of galaxies in the distant (and hence early) universe.
GOODS consists of optical and near-infrared imaging taken with the Advanced Camera for Surveys on the Hubble Space Telescope, the Very Large Telescope and the 4-m telescope at Kitt Peak National Observatory; infrared data from the Spitzer Space Telescope. These are added to pre-existing x-ray data from the Chandra X-ray Observatory and ESAs XMM-Newton. two fields of 10' by 16'; one centered on the Hubble Deep Field North (12h 36m 55s, +62° 14m 15s) and the other on the Chandra Deep Field South (3h 32m 30s, -27° 48m 20s). The two GOODS fields are the most data-rich areas of the sky in terms of depth and wavelength coverage.
==Instruments==
GOODS consists of data from the following space-based observatories:
*The Hubble Space Telescope (optical imaging with the Advanced Camera for Surveys)
*The Spitzer Space Telescope (infrared imaging)
*The Chandra X-Ray Observatory (X-ray)
*XMM-Newton (an X-ray telescope belonging to the European Space Agency)
*The Herschel Space Observatory (an infrared telescope belonging to the ESA)
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「Great Observatories Origins Deep Survey」の詳細全文を読む
スポンサード リンク
| 翻訳と辞書 : 翻訳のためのインターネットリソース |
Copyright(C) kotoba.ne.jp 1997-2016. All Rights Reserved.
|
|