Title: Disk Masses and Dust Evolution of Protoplanetary Disks
       Around Brown Dwarfs
Authors: Rilinger A.M., Espaillat C.C.
Figure: Spectral Energy Distribution for GY92 141
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Byte-by-byte Description of file: datafileA2e.txt
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   Bytes Format Units   Label   Explanations
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   1-  7 F7.3   um      Wave    Wavelength
   9-  9 A1     ---     Flag    Flux upper limit flag
  11- 16 F6.3   mJy     Flux    Flux density
  18- 22 F5.3   mJy   e_Flux    ? Uncertainty in flux density (1)
  24- 54 A31    ---     Source  Filter and/or telescope of measurement
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Note (1): No flux uncertainties given for upper limit measurements.
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  0.478    0.004       PAN-STARRS/PS1:g                
  0.504    0.008 0.001 GAIA/GAIA3:Gbp                  
  0.505    0.026 0.009 GAIA/GAIA2:Gbp                  
  0.554    0.019 0.004 Johnson:V                       
  0.583    0.030 0.000 GAIA/GAIA3:G                    
  0.613    0.006 0.001 PAN-STARRS/PS1:r                
  0.623    0.030 0.000 GAIA/GAIA2:G                    
  0.673    0.032       Gaia:G                          
  0.749    0.048 0.001 PAN-STARRS/PS1:i                
  0.763    0.103 0.003 GAIA/GAIA3:Grp                  
  0.764    0.062       SDSS:i'                         
  0.773    0.105 0.002 GAIA/GAIA2:Grp                  
  0.866    0.213 0.003 PAN-STARRS/PS1:z                
  0.960    0.512 0.006 PAN-STARRS/PS1:y                
  1.251    1.220 0.050 Johnson:J                       
  1.631    1.700 0.080 Johnson:H                       
  2.192    1.850 0.220 Johnson:K                       
  3.352    1.240 0.040 WISE:W1                         
  3.552    1.550 0.080 Spitzer/IRAC:3.6                
  4.496    1.310 0.060 Spitzer/IRAC:4.5                
  4.603    1.170 0.050 WISE:W2                         
  5.735    1.340 0.080 Spitzer/IRAC:5.8                
  7.878    1.240 0.080 Spitzer/IRAC:8.0                
 11.568 <  3.150       WISE:W3                         
 22.106 < 19.500       WISE:W4                         
 23.691    0.457 0.444 Spitzer/MIPS:24                 
889.996 <  0.280       0.89mm (Testi et al. submitted)