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NASA NTRS · 20080032522

Detector Modeling and CMB Polarimetry Technology Development at GSFC

Abstract

Pixel size limits the resolution in the focal plane. This should be accounted for in optical design. Alternatively, this reduces the effective number of independent detectors. Polarization and scattering are intrinsically related, and both are more severe at low pnambda. Future work: Quantification of the pixel cross-coupling- calculate a theoretical covariance matrix to predict performance of future detector arrays.

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BibTeXRIS

Chuss, David T., Wollack, Edward J., Moseley, S. Harvey, Withington, Stafford, Saklatvala, George. 2007-12-03. Detector Modeling and CMB Polarimetry Technology Development at GSFC. https://ntrs.nasa.gov/citations/20080032522

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