Two versions of the reduced SpUDS MIPS 24 micron imaging are available

spuds_24_Emos_*.fits     - 24um map, with pixel scale of 2.49"/pixel 
                         (i.e., the instrument pixel scale) and a flux
                         conversion factor of 6.60 uJy/DN.

spuds_24_Emos0.5_*.fits  - 24um map, with pixel scale of 1.245"/pixel, 
                         and a flux conversion factor of 1.6 uJy/DN.

The second map offers a better spatial resolution, and this is the map 
we should use in most cases.  However, please be warned that this map 
gives signal-to-noise ratios slightly better than what they should be.  
This is because the pixel sub-sampling introduces some amount of data 
smoothing in the process.  Therefore, if we want to define the depth of 
this 24um data properly, the first map (i.e., with no pixel 
sub-sampling) should be used.  The zero-point for photometry is 
4 times larger for the first map because surface brightness, not flux, 
was preserved in the sub-sampling process.

There are a number of streaks of streaks in the map produced by asteroids.

In both cases, the *_sci.fits file is the data image and *_err.fits file
is the error image.