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

<table>From top to bottom. 408 MHz synchrotron map. Resolution: 0.85° and pixels: 0.33°. WHAM <svg height="15.4" id="M30" style="vertical-align:-3.3907pt" version="1.1" viewbox="0 0 22.4125 15.4" width="22.4125" xmlns="http://www.w3.org/2000/svg" xmlns:xlink="http://www.w3.org/1999/xlink">
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<g transform="matrix(.012,-0,0,-.012,14.975,15.187)"><path d="M545 106q-67 -118 -134 -118q-24 0 -40 37.5t-30 129.5h-2q-47 -72 -103 -119.5t-108 -47.5q-47 0 -76 45.5t-29 119.5q0 113 85 204t174 91q47 0 70 -33.5t43 -119.5h3q32 47 80 140l55 13l10 -9q-47 -80 -138 -201q17 -99 27.5 -136t22.5 -37q23 0 69 61zM333 204
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</svg> map.This map is a courtesy of the WHAM collaboration. Resolution: 1° and pixels: 1°. Combined DIRBE plus IRAS 100 <i>μ</i>m dust map. Resolution: 6 arcmin and pixels: 0.25°.</table>

Advances in Astronomy

fig4

Figure 4

Figure 4: A Characterization of the Diffuse Galactic Emissions at Large Angular Scales Using the Tenerife Data 