11 MAY 2015 

New line lists for B and for 10B and 11B.  Telluric isotopic abundances 
are included so that the combined spectrum reproduces the natural B 
spectra
10B = 0.199, log10 -0.701 
11B = 0.801, log10 -0.096
For astrophysical work the isotopic abundances must be determined. 
The doppler widths are significantly different.
Mass 10B = 10.012937
Mass 11B = 11.009305

Filenames
*050010* = 10B
*050011* = 11B
*0500*Z =  B
*0500  = 10B + 11B

GFEMQ0500.ALL is the final result for use in spectrum synthesis.