4. DIS-09 : a Target with almost NO Dust-Scattered Starlight
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 4.01 |
Here is the correlation
between FUV and NUV with NO dust-scattered starlight removed. Now, we are not going to waste your time
by showing you the Mathematica images after removal of the tiny amount of dust-scattered starlight, but we WILL show you,
now, the effect on the correlation
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4.02 |
Our dust map from Schlegel et al. shows
only a tiny amount of dust: maximum E(B-V) is 0.035
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4.03 |
FUV correlation with E(B-V)
NUV correlation with E(B-V)
Kind of a funny bifurcation in the FUV correlation. That does NOT usually occur, but, it does occur for dis.09
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4.04 |
The time has now come to look at our Mathematica GALEX images for DIS-09. Here are the pipeline backgrounds for
FUV and
NUV (no dust-scattered starlight removed)
Here are the same two, side by side for comparison.
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4.05 |
Well, what else is there to say? Form your theory! Here is a major mystery! WHAT IS THIS DIFFUSE UV RADIATION FIELD?
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4.06 |
To assist you in forming your theory, here are:
rotating FUV and NUV images of DIS-09
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Before going on to serious analysis of what we are actually seeing, let us pause and have a
little FUN with 3D views of Target One!
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