Anisotropy in the microwave sky: latest results from PYTHON

Details Anisotropy in the microwave sky: latest results from PYTHON Anisotropy in the microwave sky: latest results from PYTHON

Dec 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994aas...18511806r&link_type=abstract

American Astronomical Society, 185th AAS Meeting, #118.06; Bulletin of the American Astronomical Society, Vol. 26, p.1516

Astronomy and Astrophysics

Astronomy

Scientific paper

We will report results from the second season of observations with Python, a system designed to search for degree-scale anisotropies in the Cosmic Microwave Background. The instrument, which has an array of four bolometric detectors in its focal plane, is sensitive to radiation centered at lambda = 3.3 mm. Significant fluctuations (Delta T_{RJ,rms} ~ 70mu K) were found in the first seasons observations at the South Pole, January 1993. The same fields were reobserved during December 1993; we will report on the correlation between these two data sets. Additionally, results from a second set of fields will be given.

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