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

Figure 7

Correlation between the foreground templates. From top to bottom, we plot synchrotron versus dust, free-free versus dust and free-free versus synchrotron. The correlation is presented for 𝑏>20, 𝑏>30, and 𝑏>40 ((a), (b), and (c), resp.).

(a)

(b)

(c)