4.7 Article

The C-Band All-Sky Survey (C-BASS): digital backend for the northern survey

Journal

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 484, Issue 4, Pages 5377-5388

Publisher

OXFORD UNIV PRESS
DOI: 10.1093/mnras/stz313

Keywords

instrumentation: polarimeters; methods: data analysis; radio continuum: general

Funding

  1. National Science Foundation (NSF) [AST-0607857, AST-1010024, AST-1212217, AST-1616227]
  2. NASA award [NNX15AF06G]
  3. STFC
  4. Royal Society
  5. University of Oxford
  6. ERC [307209]
  7. Dorothy Hodgkin Award
  8. W.M. Keck Institute for Space Studies Postdoctoral Fellowship at Caltech
  9. NASA [804074, NNX15AF06G] Funding Source: Federal RePORTER
  10. STFC [ST/K00106X/1, ST/N000919/1, ST/P000649/1] Funding Source: UKRI

Ask authors/readers for more resources

The C-Band All-Sky Survey (C-BASS) is an all-sky full-polarization survey at a frequency of 5 GHz, designed to provide data complementary to the all-sky surveys of WMAP and Planck and future CMB B-mode polarization imaging surveys. We describe the design and performance of the digital backend used for the northern part of the survey. In particular, we describe the features that efficiently implement the demodulation and filtering required to suppress contaminating signals in the time-ordered data, and the capability for real-time correction of detector non-linearity and receiver balance.

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