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

<table>15 GHz stacked scans. From top to bottom we plot the 15 GHz stacked scans in the declination range 25° to 47.5°.  The data have been binned into 4° pixels.</table>

Advances in Astronomy

fig2

Figure 2

Figure 2: A Characterization of the Diffuse Galactic Emissions at Large Angular Scales Using the Tenerife Data 