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Table 3:

Photometry from Spitzer IRAC (3.6-8 $\mu $m) and MIPS (24-160 $\mu $m).
2MASS F3.6 F4.5 F5.8 F8.0 F24 F70 F160
  mJy mJy mJy mJy mJy mJy mJy
00465933-2527218$^{\rm ~*}$         5.29 53.1 158.0
00482481-2519270$^{\rm ~*}$         2.52 28.5 81.0
00561930-3742185 0.477   0.410   1.50 21.5 49.9
13092436+2939351   0.530   3.09      
13371806-3005123 0.676   0.898   1.57 21.4  
14080590+5414370$^{\rm ~*}$         6.57 55.4  
15163000+5614003$^{\rm ~*}$ 0.335 0.309 0.290 1.61 2.75 53.9 76.3
17512100+5652085         2.21    
17554655+6638399 0.520 0.38 0.86 2.96 4.49    
17564103+6634162 1.050 0.714 0.915 4.37 4.87    
17571162+6645220$^{\rm ~*}$ 0.455 0.337 0.645 1.66   34.6  
17574141+6648578 0.572 0.410 0.557 1.91 1.40    
17582761+6651113 0.705 0.520 0.630 3.39 2.65    
17584647+6647585 0.527 0.375 0.576 2.57 2.28    

Uncertainties are about 10% at 3.6-8 $\mu $m, and less than 30% at 24-160 $\mu $m; * Median redshift of the sample (z = 0.105) adopted.


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