Subrahmanyan et al. (1998 [ATCA1], 2000 [ATCA2]) use 8.7 GHz data from
the ground-based ATCA (Australia Telescope Compact Array) experiment,
in conjunction with foreground contamination data, to constrain CMBR
The window function was provided by R. Subrahmanyan. The first column in the
window function file
is , which runs from 2 to 9999. The second and
third columns are the ATCA1 and ATCA2 zero-lag 's.
The quoted bandtemperature values are from Subrahmanyan et al. (1998, 2000).
They were computed assuming a flat bandpower spectrum.
Link to the experiment webpage.
R. Subrahmanyan, M.J. Kesteven, R.D. Ekers, M. Sinclair, and J. Silk, ``The
Australia Telescope Search for Cosmic Microwave Background Anisotropy",
MNRAS 298, 1189 (1998).
R. Subrahmanyan, M.J. Kesteven, R.D. Ekers, M. Sinclair, and J. Silk, ``An Australia Telescope Survey for CMB Anisotropies",astro-ph/0002467.