&system mp=11.044 zp=3  mt=208 zt=82 elab=770 esep=0.37  polar=E1 /
&thgrid thmin=0.03 thmax=5.01 nth=300 thres=0.44 thgr=2.34  ifgaus=T /
&egrid  ermin=0.01  ermax=5.0 ner=200 foldtype=1 resfact=0.19 /
dBdE.dat


# INPUT DESCRIPTION -------------------------------------------------------
  o SYSTEM namelist: 
    mp, mt= projectile/target masses (in amu units)
    zp, zt= projectile/target charges 
    elab=Incident (LAB) energy
    polar = multipolarity (E1 so far)
   
  o THGRID namelist:
    thmin, thmax, nth: min, max and number of angles
    thres = angular resolution (for convolution)
    thgr  = grazing angle
    ifgaus: if TRUE, perform convolution with Gaussian functions
            if FALSE, perform convolution with Poissons

  o EGRID namelist:
    ermin, ermax, ner: min, max, and number of relative energies
    ifgausen= same as ifgaus for energy convolution
    foldtype= 0 for constant sigma=resfact
              1 for sigma=resfact*sqrt(Erel)     Erel in MeV
              2 for sigma read in external file fileres
    resfact= energy resolution (definition depends on foldtype)
    fileres= external files with sigma values
    
  o Filename with dB/dE distribution in UNIFORM grid for relative energy (units of e2 fm^(2*lambda) )

# MAIN OUTPUT FILES ----------------------------------------------------------
  o dsdw.out: angular distribution, dsigma/dOmega (mb/sr), integrated in energy, from ermin to ermax
  o dsde.out: differential energy distribution (dsigma/dE), in mb/MeV, integrated in angle, from thmin to thmax.
  o dnde.out: number of "equivalent photons" as a function of the continuum energy. 

  If convolution with experimental resolution is used, also:
   
  o dsdwf.out: convoluted angular distribution 
  o dsdef.out: convoluted energy distribution




