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FLS: Extragalactic Component


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Data Access through IRSA: Spatial searches on collected data sets (images, spectra, etc.) are available as follows:

Other Updates:


The extragalactic component of the FLS includes:

  • A 4 square degree imaging survey with IRAC and MIPS to a shallow depth of about one minute per pixel on the sky
  • Within the above area, a MIPS/IRAC verification survey of about 0.2 square degrees or less, with ten times the integration time.
  • Incorporation of ancillary data recommended, primarily for identification purposes.
The detailed design requirements are available online.

Survey Components:

A Selection of Related Refereed Papers

For a more complete list of Spitzer papers, please see our Spitzer Publications Archive. Go back to FLS page.


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This file was last modified on Mon Apr 23 16:48:25 2007.

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