5.6 The Cosmic Anisotropy Telescope5 Current and future CMB 5.4 The Owen's Valley Radio

5.5 Python 

Python is located at the Amundsen-Scott South Pole Station in Antartica. It consists of a single bolometer on a 75cm telescope, operating at a frequency of 90 GHz with a tex2html_wrap_inline1847 FWHM beam. Three seasons of observations have already been analysed (Python I [47], Python II [86] and Python III [80]). The Python results can be separated into two distinct bins in tex2html_wrap_inline1617 space (one centred at tex2html_wrap_inline1851 and the other at tex2html_wrap_inline1853). The results for these two bins are tex2html_wrap_inline1855 K and tex2html_wrap_inline1857 K respectively. Python IV and V data have already been taken and the analysis should be published very shortly. Details of the IV tex2html_wrap_inline1859 season can be found in Kovac et al. (1997) [64].

5.6 The Cosmic Anisotropy Telescope5 Current and future CMB 5.4 The Owen's Valley Radio

image The Cosmic Microwave Background
Aled W. Jones and Anthony N. Lasenby
http://www.livingreviews.org/lrr-1998-11
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