A Characterization of the Diffuse Galactic Emissions at Large Angular Scales Using the Tenerife Data

<table>10 GHz stacked scans. From top to bottom we plot the stacked scans for the 10 GHz radiometer from declination 30° to 45°. The data have been binned into 4° pixels.</table>

Advances in Astronomy

fig1

Figure 1

Figure 1: A Characterization of the Diffuse Galactic Emissions at Large Angular Scales Using the Tenerife Data 