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
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
space (one centred at
and the other at
). The results for these two bins are
K and
K respectively. Python IV and V data have already been taken and
the analysis should be published very shortly. Details of the IV
season can be found in Kovac
et al.
(1997) [64].