These figures show the apertures selected.<br>

<pre><img SRC="n7331_apertures.gif"><img SRC="n5194_apertures.gif"><img SRC="n3031_apertures.gif"></pre>
<hr>

These figures show the Dale/Helou SED model fits to the various regions.<br>

N7331
<pre><img SRC="p1n7331.gif"><img SRC="p2n7331.gif"></pre>
<pre><img SRC="p3n7331.gif"></pre>
<hr>
N5194
<pre><img SRC="p1n5194.gif"><img SRC="p2n5194.gif"></pre>
<pre><img SRC="p3n5194.gif"><img SRC="p4n5194.gif"></pre>
<pre><img SRC="p5n5194.gif"></pre>
<hr>
N3031
<pre><img SRC="p1n3031.gif"><img SRC="p2n3031.gif"></pre>
<pre><img SRC="p3n3031.gif"><img SRC="p4n3031.gif"></pre>
<pre><img SRC="p5n3031.gif"><img SRC="p6n3031.gif"></pre>
<pre><img SRC="p7n3031.gif"><img SRC="p8n3031.gif"></pre>
<hr>

Plot of fitted far-infrared color vs H-alpha SFR (areal) density
<pre><img SRC="a2.gif"></pre>
<hr>
Plot of fitted mid-to-far-infrared color vs H-alpha SFR (areal) density
<pre><img SRC="a3.gif"></pre>
<hr>
Plot of Spitzer color-color diagram, plus overlay of Dale SED model
<pre><img SRC="cc.gif"></pre>
<hr>
Plot of fitted far-infrared color vs HI Surface Brightness
<pre><img SRC="h1.gif"></pre>
<hr>
Plot of H-alpha SFR (areal) density vs  HI Surface Brightness
<pre><img SRC="h1ha.gif"></pre>
<hr>
Plot of fitted far-infrared-to-radio ratio vs Radio flux density
<pre><img SRC="qTIR.gif"></pre>
<hr>
Plot of IRAS+Spitzer+SCUBA SINGS SEDs (fitted to MIPS)
<pre><img SRC="p1.gif"></pre>
<hr>

<br>
<hr>
Last updated 23 Jul 2004