Gutiérrez et al. use 10 and 15 GHz data from the ground-based Tenerife experiment, in conjunction with diffuse foreground galactic contamination data, to constrain CMBR anisotropy.

The FWHM of the beam, assumed to be gaussian, is
. The zero-lag window function of the three-beam experiment is

where , is a Legendre polynomial of order , and is half of the peak-to-peak chop angle.

The first column in the window function
file
is , which runs from 2 to
130. The second column is .

The quoted bandtemperature values are from Gutiérrez et al., with 10% added
in quadrature to their statistical 1 error bars to account for the
Tenerife 1 calibration uncertainty.

**Links to the experiment webpages.**

C.M. Gutiérrez, R. Rebolo, R.A. Watson, R.D. Davies, A.W. Jones, and
A.N. Lasenby, ``The Tenerife Cosmic Microwave Background Maps:
Observations and First Analysis", *Astrophys. J.* **529**, 47 (2000).

Department of Physics, Kansas State University

Last updated: 2000-08-31