Miller et al. use D band (centered on 144 GHz) data from the
ground-based MAT (Mobile Anisotropy Telescope) 1998 experiment on
Cerro Toco, Chile, to constrain CMBR anisotropy.
The window function file
were provided by E. Torbet. The first column is , which runs
from 2 to 1300 (although one is not computed to ). The next five columns are the combined D1 + D2 zero-lag
's for groups 6, 7, ..., 10. Each group is a combination of
various -point chops of D1 and D2 data; see Miller et al. for
The quoted bandtemperature values are computed for a flat bandpower spectrum.
They are from Miller et al. with 8% added in quadrature to their statistical
1 error bars to account for the 1 calibration uncertainty.
Links to the experiment webpages.
A.D. Miller, et al., ``A Measurement of the Angular Power Spectrum of the Cosmic Microwave Background from = 100 to 400", Astrophys. J. Lett. 524, L1 (1999).