SWIRE <a href=http://www.ipac.caltech.edu/SWIRE/>homepage</a> 

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<pre>Lockman Hole: The entire field is covered in r' to ~23.8, and a subset to g'~26, r'~25, i'~24.</pre>  
<pre>This subset is shown by the red squares in the  <a href=lock_opt_fin.jpg>accompanying jpeg</a>. </pre>
<pre>In addition we have U band and deeper gri covering the Chandra Xray field to the N.</pre>
<pre>See the grid of small magenta squares.  This is about 1 sq deg.</pre>

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See the <a href=lock_may.jpg>MIPS scans</a> in the Lockman Hole, and the GTO field to the east (yellow).</pre>   
<pre>These data are embargoed from us (and everyone) for a year+, because the GTO data are proprietary.</pre>    
<pre>You may want to consider aiming your observations to coincide with this GTO field.</pre>
<pre>The pro is that the Spitzer data are quite a lot deeper than ours, over 0.4x1 deg.</pre>
<pre>The con is you won't get the SWIRE or the GTO data till late summer 2005 (or so).

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<pre>See <a href=en1_04jan.jpg> </a>ELAIS N1</pre>
<pre>Optical depths (5 sigma; point source) are: U 23.3; g 24.7; r 23.8; i 23.0; z 21.7.  These are from the INT Wide Field Survey.</pre>   
<pre>The attached jpeg shows our MIPS (red) & IRAC (blue/violet) AORs along with the ISO field (pink) and INTWFS field (magenta).</pre> 

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<pre>See <a href=en2_galex.jpg> </a>ELAIS N2</pre>