The PYTHON Microwave Background Anisotropy Experiment: Instrumentation and Analysis

Details The PYTHON Microwave Background Anisotropy Experiment: Instrumentation and Analysis The PYTHON Microwave Background Anisotropy Experiment: Instrumentation and Analysis

May 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aas...182.7701r&link_type=abstract

American Astronomical Society, 182nd AAS Meeting, #77.01D; Bulletin of the American Astronomical Society, Vol. 25, p.927

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

We will discuss the instrumentation and data analysis for the PYTHON microwave background anisotropy experiment. This instrument was used at the South Pole from 1/1 to 1/15 1993 for observations of the microwave sky at a frequency of 90 GHz. The telescope has a FWHM beam of 45', and a chop of 2.75(deg) . This work was supported by The Center for Astrophysics in Antarctica, PYI grant NSF AST-9057089, the James S. McDonnell Foundation, and NASA grant NGT-50622.

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