!+
!
! bin_solve.sfit
!   An example SFIT input file for fitting composite spectra
!
! Purpose:
!=  compute Teff, log g, etc,  for both componets in a compositte spectrum
!   using lines in the wavalength range: 3800 5200
!   a high resolution echelle spectrum
!   and assuming the new (STERNE2 + LESTER) LTE model grids
!
!   :: NB the Opacity Sampling Grid will come soon. 
!
! Mode: 
!   SLV / AMOEBA ?? / HIRES
!
! Method: 
!   Read in a model atmosphere grid for the hot star
!   Read in a model atmosphere grid for the cool star
!   Read in a hires optical spectrum 
!   Uses amoeba  to find optimum model
!
!   ** WARNING **
!   This example is not yet suppplied with test data and has not 
!   been proven in action. The methods were used successfully in 
!   real applications (BI Lyncis and other sdBs)  and published.
!
!   Jeffery & Aznar Cuadrado 2001, A&A 378, 936.
!   Aznar Cuadrado & Jeffery 2002. A&A 385, 131.
!
! Version:
!   2005-Feb-07 (CSJ)
!
! Notes:
!   input for SFIT version 2.5 or later
!
!-


read_grid helium_blue 
read_grd2 kurucz_blue 

method_amoeba 
method_range 3900 5000 
method_tolerance 1.0E-3 

slv_teff1  28.6 0.2   
fix_logg1   3.64 0.0   
fix_ahe1    0.943 0.0  
fix_vsini1  0.0 0.0     
fix_rad1    1.0 0.0     
fix_vrad1   0.0 0.0  

slv_teff2   5.8 0.2  
fix_logg2   4.5 0.0  
fix_ahe2    0.0 0.0  
fix_vsini2  0.0 0.0  
slv_rad2    2.5 0.1  
fix_vrad2   0.0 0.0  


continuum_poly 3  ! define continuum with 3rd order polynomial fit 

data_spectrum './bi_lyn.dat' 
data_instrument 1.0 ! instrumental profile FWHM (Angstroms) 
data_drift 0.0 ! velocity drift during exposure (km/s) } 

solve 

end