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Ancillary Data


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HerMES fields were chosen so as to provide the best multi-wavelength coverage over wide areas.

 


 

Ancillary Data by Wavelength

Wavelength Ancillary Data
X-ray Chandra/XMM
UV GALEX Photometry and Spectroscopy
Optical SDSS Photometry and Spectroscopy
Near-IR UKIDSS, VISTA Legacy Surveys from 2010
Mid-IR SWIRE, SDWFS, S-COSMOS, GOODS
(S)MM SCUBA, MAMBO, AzTEC, LABOCA, SCUBA2 Legacy Surveys from 2010
Radio VLA, GMRT, ATC

 

Ancillary Data by Field/Survey

(links will navigate away from the HerMES site)

 

  • SWIRE - The Spitzer Wide-area InfraRed Extragalactic survey is one of six very large programs undertaken as Legacy surveys during the first year of the Spitzer Space Telescope.
  • COSMOS - The Cosmological Evolution Survey is an HST Treasury Project to survey a 2 square degree equatorial field with the Advanced Camera for Surveys (ACS).
  • AEGIS - Targeted on a special area of the sky, called the Extended Groth Strip (EGS).
  • GOODS - Unites extremely deep observations from NASA's Great Observatories, Spitzer, Hubble, and Chandra, ESA's Herschel and XMM-Newton, and from the most powerful ground-based facilities, to survey the distant universe to the faintest flux limits across the electromagnetic spectrum.
  • SERVS
  • VIDEO
  • LOFAR - The LOw Frequency ARray is a multi-purpose sensor array is a new and innovative effort to force a breakthrough in sensitivity for astronomical observations at radio-frequencies below 250 MHz.