SCOPUS 정보 검색 플랫폼

Monthly Notices of the Royal Astronomical Society

Volumn 393, Issue 2, 2009, Pages 531-537

Phase shift sequences for an adding interferometer

(3) Hyland, Peter a,c Follin, Brent b Bunn, Emory F b

a University of Wisconsin Madison (United States)

b UNIVERSITY OF RICHMOND (United States)

c MCGILL UNIVERSITY (Canada)

Author keywords

Cosmic microwave background; Techniques: interferometric; Techniques: polarimetric

Indexed keywords

INTERFEROMETERS; INTERFEROMETRY; POLARIMETERS; SIGNAL TO NOISE RATIO; SYSTEMATIC ERRORS; VISIBILITY;

BOLOMETRIC INTERFEROMETER; BOLOMETRIC INTERFEROMETRY; COSMIC MICROWAVE BACKGROUND POLARIMETRIES; COSMIC MICROWAVES BACKGROUND; MODE SIGNALS; ORTHOGONALITY; SHIFT SEQUENCES; SYSTEMATIC METHOD; TECHNIQUE: INTERFEROMETRIC; TECHNIQUES: POLARIMETRIC;

COSMOLOGY;

EID: 60249097878 PISSN: 00358711 EISSN: 13652966 Source Type: Journal
DOI: 10.1111/j.1365-2966.2008.14194.x Document Type: Article

Times cited : (7)

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