Journal article
High sensitivity measurements of the CMB power spectrum with the extended Very Small Array
- Abstract:
-
We present deep Ka-band ($\nu \approx 33$ GHz) observations of the CMB made with the extended Very Small Array (VSA). This configuration produces a naturally weighted synthesized FWHM beamwidth of $\sim 11$ arcmin which covers an $\ell$-range of 300 to 1500. On these scales, foreground extragalactic sources can be a major source of contamination to the CMB anisotropy. This problem has been alleviated by identifying sources at 15 GHz with the Ryle Telescope and then monitoring these sources at...
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- Publisher copy:
- 10.1111/j.1365-2966.2004.08206.x
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Authors
Bibliographic Details
- Journal:
- Mon.Not.Roy.Astron.Soc.
- Volume:
- 353
- Pages:
- 732
- Publication date:
- 2004-02-20
- DOI:
- URN:
-
uuid:c954b36a-b8ec-43f3-a569-940607fc9174
- Source identifiers:
-
25985
- Local pid:
- pubs:25985
Item Description
- Keywords:
Terms of use
- Copyright date:
- 2004
- Notes:
- 16 pages. Accepted in MNRAS (minor revisions)
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