4.6 Article

HerMES: The SPIRE confusion limit

Journal

ASTRONOMY & ASTROPHYSICS
Volume 518, Issue -, Pages -

Publisher

EDP SCIENCES S A
DOI: 10.1051/0004-6361/201014680

Keywords

space vehicules: instruments; surveys; submillimeter: diffuse background; submillimiter: galaxies

Funding

  1. CSA (Canada)
  2. NAOC (China)
  3. CEA, CNES, CNRS (France)
  4. ASI (Italy)
  5. MCINN (Spain)
  6. SNSB (Sweden)
  7. STFC (UK)
  8. NASA (USA)
  9. STFC [PP/E001173/1, ST/G002630/1, ST/F007019/1, ST/F002858/1, ST/H001530/1] Funding Source: UKRI
  10. Science and Technology Facilities Council [ST/F002858/1, PP/E001173/1, ST/F007019/1, ST/G002630/1, PP/E001181/1] Funding Source: researchfish
  11. UK Space Agency [ST/G003874/1, ST/G003831/1] Funding Source: researchfish

Ask authors/readers for more resources

We report on the sensitivity of SPIRE photometers on the Herschel Space Observatory. Specifically, we measure the confusion noise from observations taken during the science demonstration phase of the Herschel Multi-tiered Extragalactic Survey. Confusion noise is defined to be the spatial variation of the sky intensity in the limit of infinite integration time, and is found to be consistent among the different fields in our survey at the level of 5.8, 6.3 and 6.8 mJy/beam at 250, 350 and 500 mu m, respectively. These results, together with the measured instrument noise, may be used to estimate the integration time required for confusion limited maps, and provide a noise estimate for maps obtained by SPIRE.

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