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After IRAS, IR correlation functions have been mainly estimated based on deep surveys.
Finally, the properties of the X-ray sources populating the deep surveys will be described and compared with the predictions of the most recent synthesis models.
With reasonable assumptions, however, we can make predictions for the source populations that we should detect in the AXAF and XMM deep surveys.
Optical and near-infrared (NIR) deep surveys have been very powerful for detecting very faint sources in the high-redshift (z) universe.
In the near- and mid-infrared regions, wide and deep surveys of pre-selected sky areas will be made with large low-noise arrays.
Deep surveys at mid-infrared through submillimeter wavelengths indicate that a substantial fraction of the total luminosity output from galaxies at high redshift (z>1) emerges at wavelengths 30 300 μm.
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The patch, known as the southern GOODS field, for Great Observatories Origins Deep Survey, has been observed by a variety of telescopes and satellites, including Hubble in 2004.
The ultra deep survey surpasses two earlier surveys, known as the Hubble Deep Fields, which revealed thousands of new galaxies dating back as far as when the universe was only a billion years old.
One such collaboration is GOODS, or the Great Observatories Origins Deep Survey, in which Spitzer worked with Chandra and Hubble to look in detail at a small patch of sky.
Just like archeologists who find older artifacts by digging deeper, astronomers use "deep" surveys--during which a telescope looks at one patch of sky for a long time to gather the most possible light--to look back to the distant past.
Related sites The paper (PDF) Paolo Padovani Astrophysical Virtual Observatory The Great Observatories Origins Deep Survey.
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