Abstract
We look at anticipated science results achievable with QUaD, a ground-based experiment to measure the polarization of the CMB from the South Pole, and describe the features that will enable it to measure this weak polarized signal. We show that QUaD can make a high resolution measurement of the polarization signals on small angular scales. This will lead to tighter constraints on the key cosmological parameters and could also put new limits on the inflationary model.
Original language | English |
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Pages (from-to) | 84-94 |
Number of pages | 10 |
Journal | Proceedings of SPIE - The International Society for Optical Engineering |
Volume | 5489 |
Issue number | 1 |
DOIs | |
Publication status | Published - 2004 |
Keywords
- Cosmic microwave background
- Cosmology
- Polarization
- Sub-mm telescope